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Do you love twilight? The 3 stages explained

Eight photos with a bright dot lower in each from left to right, on gradually darkening backgrounds.
View at EarthSky Community Photos. | Soumyadeep Mukherjee shared this composite image from photos he took at Singalila National Park in India. Soumyadeep wrote: “There are some images, which, after you create, make you happy. This is one of them. The image shows Venus in the varying backgrounds of twilight colors. As twilight progresses, the background stars, the Sagittarius arm and nebulae are slowly revealed. The change in colors and background within the same twilight period ranged around 26 minutes during this period and latitude.” Thank you, Soumyadeep!

Twilight is that magical time of day when a glow pervades the air, even though the sun is below the horizon. Earth’s atmosphere scatters the sun’s rays to create the colors of twilight. On worlds with no atmospheres, such as the moon, the sky falls instantly dark after the sun sets.

And, if you could see twilight from outer space, you’d find that it isn’t marked by a sharp boundary on Earth’s surface. Instead, the shadow line on Earth – sometimes called the terminator line – is spread over a fairly wide area on the surface and shows the gradual transition to darkness we all experience as night falls.

Astronomers – those experts on nighttime – recognize three stages of twilight. Keep reading or watch a video to hear about the intricacies of civil, nautical and astronomical twilight, below.

Stage 1: Civil twilight

Let’s consider the stages of twilight as occurring after sunset. Keep in mind that they would reverse their order at sunrise. Civil twilight begins the moment the sun slips below the horizon. The official definition of civil twilight is the time from when the sun disappears until the sun’s center is 6 degrees below the horizon. A measurement of 6 degrees of sky is a bit more than three fingers held at arm’s length.

During civil twilight, there’s enough light to see, but people turn on their lights to drive a car, and the streetlights are starting to come on. The brightest planets appear during civil twilight.

For mid latitudes, civil twilight lasts a bit longer in summer and winter and is a bit shorter in spring and fall. In spring and fall, the sun rises and sets more directly in the east and west. Therefore, it makes a straighter path downward (or upward), reaching the 6 degree mark in a shorter period of time. In summer and winter, the sun arcs across the sky, cutting across the horizon at an angle. This angle is more pronounced in summer, which is why civil twilight lasts the longest in summer. Civil twilight in mid latitudes can last, on average, 1/2 hour.

Compare this to tropical regions. At the equator, the length of civil twilight hardly varies. The sun around the equator makes a path across the sky that cuts cleanly down toward the horizon at sunset in a nearly perpendicular fashion. Therefore, the sun and its rays disappear faster, giving equatorial regions a shorter twilight than higher latitudes. Near the poles, twilight times last much longer.

Diagram: 3 wedge-shaped areas, from light to dark blue, labeled with twilight types, between day and night on a circle.
The 3 types of twilight. Image via TWCarlson/ Wikimedia Commons (CC BY-SA 4.0).

Stage 2: Nautical twilight

In the evening, nautical twilight takes over where civil twilight ends. The definition of nautical twilight is the time period when the center of the sun is 6 degrees below the horizon to 12 degrees below the horizon. You can remember the name “nautical” because it ends when the distant line between sea and sky is no longer distinguishable. Also, more bright stars appear during this time, which was important in the early days of navigation. When nautical twilight began, sailors could use the stars as directional cues.

During nautical twilight, terrestrial objects are visible, but you need artificial lights to carry on outdoor activities.

For polar regions, the summer sun does not get more than 12 degrees below the horizon. Therefore, these regions have nautical twilight all night long, never reaching astronomical twilight or total darkness. For mid latitudes, nautical twilight can last from about 1/2 hour in spring, winter and fall, to about 45 minutes in summer.

Stage 3: Astronomical twilight

The darkest twilight stage is astronomical twilight. The definition of astronomical twilight is the period of time when the center of the sun is 12 degrees below the horizon to 18 degrees below the horizon. You probably don’t even notice any illumination left in the sky at this time.

For stargazers, this is the time when fainter stars, clusters and other sky objects appear and become good observing targets.

In mid latitudes, astronomical twilight can last about 1/2 hour from fall through spring but up to an hour in summer. Astronomical twilight begins about an hour to 1 1/2 hours after sunset for mid latitudes. So, as a rule of thumb, if you’d like to observe something in the night sky that isn’t particularly bright, you should wait about 90 minutes after sunset before you start observing.

Twilight photo gallery

Partial view of Earth from orbit showing fading colors from light side to dark side.
Twilight on Earth, viewed from space. Astronauts aboard the International Space Station captured this photo – a single digital frame – in June 2001. On the right, you see Earth illuminated by the sun. On the left, it’s nighttime. Between, washed in subtle colors, is the realm of twilight. Image via ISS Expedition 2 Crew/ Gateway to Astronaut Photography of Earth/ NASA.
Dark foreground hills, orange sky fading to yellow and blue above, with a sliver of a moon.
View at EarthSky Community Photos. | John Ashley of Amado, Arizona, caputured this image on July 6, 2024, and wrote: “A 1% crescent moon sets through twilight haze beyond the large telescopes (left horizon) at Kitt Peak National Observatory (43 miles from the camera) just after sunset on Saturday, July 7, 2024.” Thank you, John!
Brilliant yellow sunset sky fading to partly-cloudy orange above, with dark buildings and trees in foreground.
View at EarthSky Community Photos. | Pat Fogg in Claresholm, Alberta, Canada, captured this image of early twilight on June 23, 2023. Pat wrote: “Sunset looking west to the Porcupine Hills.” Thank you, Pat!

Bottom line: Twilight is that magical time between sunlight and darkness. Astronomers, the experts on nighttime, recognize three stages of twilight.

The post Do you love twilight? The 3 stages explained first appeared on EarthSky.



from EarthSky https://ift.tt/Qatvbxw
Eight photos with a bright dot lower in each from left to right, on gradually darkening backgrounds.
View at EarthSky Community Photos. | Soumyadeep Mukherjee shared this composite image from photos he took at Singalila National Park in India. Soumyadeep wrote: “There are some images, which, after you create, make you happy. This is one of them. The image shows Venus in the varying backgrounds of twilight colors. As twilight progresses, the background stars, the Sagittarius arm and nebulae are slowly revealed. The change in colors and background within the same twilight period ranged around 26 minutes during this period and latitude.” Thank you, Soumyadeep!

Twilight is that magical time of day when a glow pervades the air, even though the sun is below the horizon. Earth’s atmosphere scatters the sun’s rays to create the colors of twilight. On worlds with no atmospheres, such as the moon, the sky falls instantly dark after the sun sets.

And, if you could see twilight from outer space, you’d find that it isn’t marked by a sharp boundary on Earth’s surface. Instead, the shadow line on Earth – sometimes called the terminator line – is spread over a fairly wide area on the surface and shows the gradual transition to darkness we all experience as night falls.

Astronomers – those experts on nighttime – recognize three stages of twilight. Keep reading or watch a video to hear about the intricacies of civil, nautical and astronomical twilight, below.

Stage 1: Civil twilight

Let’s consider the stages of twilight as occurring after sunset. Keep in mind that they would reverse their order at sunrise. Civil twilight begins the moment the sun slips below the horizon. The official definition of civil twilight is the time from when the sun disappears until the sun’s center is 6 degrees below the horizon. A measurement of 6 degrees of sky is a bit more than three fingers held at arm’s length.

During civil twilight, there’s enough light to see, but people turn on their lights to drive a car, and the streetlights are starting to come on. The brightest planets appear during civil twilight.

For mid latitudes, civil twilight lasts a bit longer in summer and winter and is a bit shorter in spring and fall. In spring and fall, the sun rises and sets more directly in the east and west. Therefore, it makes a straighter path downward (or upward), reaching the 6 degree mark in a shorter period of time. In summer and winter, the sun arcs across the sky, cutting across the horizon at an angle. This angle is more pronounced in summer, which is why civil twilight lasts the longest in summer. Civil twilight in mid latitudes can last, on average, 1/2 hour.

Compare this to tropical regions. At the equator, the length of civil twilight hardly varies. The sun around the equator makes a path across the sky that cuts cleanly down toward the horizon at sunset in a nearly perpendicular fashion. Therefore, the sun and its rays disappear faster, giving equatorial regions a shorter twilight than higher latitudes. Near the poles, twilight times last much longer.

Diagram: 3 wedge-shaped areas, from light to dark blue, labeled with twilight types, between day and night on a circle.
The 3 types of twilight. Image via TWCarlson/ Wikimedia Commons (CC BY-SA 4.0).

Stage 2: Nautical twilight

In the evening, nautical twilight takes over where civil twilight ends. The definition of nautical twilight is the time period when the center of the sun is 6 degrees below the horizon to 12 degrees below the horizon. You can remember the name “nautical” because it ends when the distant line between sea and sky is no longer distinguishable. Also, more bright stars appear during this time, which was important in the early days of navigation. When nautical twilight began, sailors could use the stars as directional cues.

During nautical twilight, terrestrial objects are visible, but you need artificial lights to carry on outdoor activities.

For polar regions, the summer sun does not get more than 12 degrees below the horizon. Therefore, these regions have nautical twilight all night long, never reaching astronomical twilight or total darkness. For mid latitudes, nautical twilight can last from about 1/2 hour in spring, winter and fall, to about 45 minutes in summer.

Stage 3: Astronomical twilight

The darkest twilight stage is astronomical twilight. The definition of astronomical twilight is the period of time when the center of the sun is 12 degrees below the horizon to 18 degrees below the horizon. You probably don’t even notice any illumination left in the sky at this time.

For stargazers, this is the time when fainter stars, clusters and other sky objects appear and become good observing targets.

In mid latitudes, astronomical twilight can last about 1/2 hour from fall through spring but up to an hour in summer. Astronomical twilight begins about an hour to 1 1/2 hours after sunset for mid latitudes. So, as a rule of thumb, if you’d like to observe something in the night sky that isn’t particularly bright, you should wait about 90 minutes after sunset before you start observing.

Twilight photo gallery

Partial view of Earth from orbit showing fading colors from light side to dark side.
Twilight on Earth, viewed from space. Astronauts aboard the International Space Station captured this photo – a single digital frame – in June 2001. On the right, you see Earth illuminated by the sun. On the left, it’s nighttime. Between, washed in subtle colors, is the realm of twilight. Image via ISS Expedition 2 Crew/ Gateway to Astronaut Photography of Earth/ NASA.
Dark foreground hills, orange sky fading to yellow and blue above, with a sliver of a moon.
View at EarthSky Community Photos. | John Ashley of Amado, Arizona, caputured this image on July 6, 2024, and wrote: “A 1% crescent moon sets through twilight haze beyond the large telescopes (left horizon) at Kitt Peak National Observatory (43 miles from the camera) just after sunset on Saturday, July 7, 2024.” Thank you, John!
Brilliant yellow sunset sky fading to partly-cloudy orange above, with dark buildings and trees in foreground.
View at EarthSky Community Photos. | Pat Fogg in Claresholm, Alberta, Canada, captured this image of early twilight on June 23, 2023. Pat wrote: “Sunset looking west to the Porcupine Hills.” Thank you, Pat!

Bottom line: Twilight is that magical time between sunlight and darkness. Astronomers, the experts on nighttime, recognize three stages of twilight.

The post Do you love twilight? The 3 stages explained first appeared on EarthSky.



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New type of supernova, as a black hole triggers a star explosion

New type of supernova: A smaller, black sphere at center surrounded by a large, bright disk with a big blue sphere in it.
View larger. | Artist’s concept of a new type of supernova, showing the explosive interaction between a black hole and a massive nearby star (blue). As the separation between the star and the black hole decreased, the black hole’s intense gravity pulled gas and dust off the star into a disk. Meanwhile, the star’s outer layers were expanding, trying to swallow the hole. Ultimately, gravitational stress from the black hole triggered the star’s explosion. Collisions between the stellar explosion and shells of material from earlier interactions – located above and below the disk – powered a dramatic re-brightening event. Image via Melissa Weiss/ CfA.
  • A massive star and its black hole companion circled each other – closer and closer – as the star’s outer layers were expanding, trying to swallow the hole, while the hole was siphoning material off the star.
  • The star became unstable and exploded as it closed in on the black hole.
  • It’s the first evidence of a supernova created in close interactions between a star and black hole.

The Center for Astrophysics | Harvard & Smithsonian published this original story on August 13, 2025. Edits by EarthSky.

New type of supernova from a star trying to eat a black hole

Astronomers said this week they’ve discovered a new type of supernova. It appears to be a massive star that exploded while trying to envelop a black hole companion in its outer layers.

If it’s true, it’s one of the strangest stellar explosions we’ve yet seen. The Zwicky Transient Facility discovered the blast, named SN 2023zkd, in July 2023.

A new artificial intelligence (AI) algorithm – designed to scan for unusual explosions in real time – first detected the explosion. That early alert allowed astronomers to begin follow-up observations immediately, an essential step in creating a model that explains the explosion. By the time the explosion was over, a large set of telescopes, both on the ground and from space, had observed it.

The scientists think the most likely interpretation of the data is that a star of perhaps 10 solar masses was locked in a deadly orbit with a black hole of about the same mass. The star and black hole drew closer to each other, with the star trying to envelop the hole in its outer layers, and the hole pulling material from the star until … boom! The star exploded as a supernova.

A team led by the Center for Astrophysics | Harvard & Smithsonian and the Massachusetts Institute of Technology (MIT) made the discovery as part of the Young Supernova Experiment. The peer-reviewed Astrophysical Journal published the study on August 13, 2025.

What triggered the supernova?

Alexander Gagliano is the lead author of the study and a fellow at the NSF Institute for Artificial Intelligence and Fundamental Interactions. Gagliano said:

Our analysis shows that the blast was sparked by a catastrophic encounter with a black hole companion, and is the strongest evidence to date that such close interactions can actually detonate a star. Our machine learning system flagged SN 2023zkd months before its most unusual behavior, which gave us ample time to secure the critical observations needed to unravel this extraordinary explosion.

An alternative interpretation the team considered is that the black hole completely tore the star apart before it could explode on its own. In that case, the black hole quickly pulled in the star’s debris, and supernova emission was generated when the debris crashed into the gas surrounding it. Both cases leave a single, heavier black hole behind.

Witnessing the new type of supernova

Located about 730 million light-years from Earth, SN 2023zkd initially looked like a typical supernova. It had a single burst of light. But as the scientists tracked its decline over several months, it did something unexpected: it brightened again. To understand this unusual behavior, the scientists analyzed archival data, which showed something even more unusual. The system had been slowly brightening for more than four years before the explosion. Scientists rarely see that kind of long-term activity before the explosion in supernovas.

Detailed analysis revealed the explosion’s light was shaped by material the star had shed in the years before it died. The early brightening came from the supernova’s blast wave hitting low-density gas. The second, delayed peak was caused by a slower but sustained collision with a thick, disk-like cloud. This structure – and the star’s erratic pre-explosion behavior – suggest the dying star was under extreme gravitational stress. And that stress was likely from a nearby, compact companion such as a black hole.

V. Ashley Villar is a CfA assistant professor of astronomy in the Harvard Faculty of Arts and Sciences and a co-author on the study. Villar said:

2023zkd shows some of the clearest signs we’ve seen of a massive star interacting with a companion in the years before explosion. We think this might be part of a whole class of hidden explosions that AI will help us discover.

More chances to catch supernovas in the act

Gagliano said:

This discovery shows how important it is to study how massive stars interact with companions as they approach the end of their lives. We’ve known for some time that most massive stars are in binaries, but catching one in the act of exchanging mass shortly before it explodes is incredibly rare.

With the Vera C. Rubin Observatory recently unveiling its first images and preparing to survey the entire sky every few nights, this discovery marks a glimpse of what’s to come. Powerful new observatories, combined with real-time AI systems, will soon allow astronomers to uncover many more rare and complex explosions and begin to map how massive stars live and die in binary systems.

The Young Supernova Experiment will continue to complement Rubin by using the Pan-STARRS1 and Pan-STARRS2 telescopes to identify supernovas shortly after explosion. This approach offers a cost-effective way to study the dynamic nearby universe. Gagliano said:

We’re now entering an era where we can automatically catch these rare events as they happen, not just after the fact. That means we can finally start connecting the dots between how a star lives and how it dies, and that’s incredibly exciting.

Bottom line: Astronomers believe they’ve found a new type of supernova. They say it exploded as a star tried to envelop its black hole companion.

Source: Evidence for an Instability-induced Binary Merger in the Double-peaked, Helium-rich Type IIn Supernova 2023zkd

Via the Center for Astrophysics | Harvard & Smithsonian

The post New type of supernova, as a black hole triggers a star explosion first appeared on EarthSky.



from EarthSky https://ift.tt/uLdhE7C
New type of supernova: A smaller, black sphere at center surrounded by a large, bright disk with a big blue sphere in it.
View larger. | Artist’s concept of a new type of supernova, showing the explosive interaction between a black hole and a massive nearby star (blue). As the separation between the star and the black hole decreased, the black hole’s intense gravity pulled gas and dust off the star into a disk. Meanwhile, the star’s outer layers were expanding, trying to swallow the hole. Ultimately, gravitational stress from the black hole triggered the star’s explosion. Collisions between the stellar explosion and shells of material from earlier interactions – located above and below the disk – powered a dramatic re-brightening event. Image via Melissa Weiss/ CfA.
  • A massive star and its black hole companion circled each other – closer and closer – as the star’s outer layers were expanding, trying to swallow the hole, while the hole was siphoning material off the star.
  • The star became unstable and exploded as it closed in on the black hole.
  • It’s the first evidence of a supernova created in close interactions between a star and black hole.

The Center for Astrophysics | Harvard & Smithsonian published this original story on August 13, 2025. Edits by EarthSky.

New type of supernova from a star trying to eat a black hole

Astronomers said this week they’ve discovered a new type of supernova. It appears to be a massive star that exploded while trying to envelop a black hole companion in its outer layers.

If it’s true, it’s one of the strangest stellar explosions we’ve yet seen. The Zwicky Transient Facility discovered the blast, named SN 2023zkd, in July 2023.

A new artificial intelligence (AI) algorithm – designed to scan for unusual explosions in real time – first detected the explosion. That early alert allowed astronomers to begin follow-up observations immediately, an essential step in creating a model that explains the explosion. By the time the explosion was over, a large set of telescopes, both on the ground and from space, had observed it.

The scientists think the most likely interpretation of the data is that a star of perhaps 10 solar masses was locked in a deadly orbit with a black hole of about the same mass. The star and black hole drew closer to each other, with the star trying to envelop the hole in its outer layers, and the hole pulling material from the star until … boom! The star exploded as a supernova.

A team led by the Center for Astrophysics | Harvard & Smithsonian and the Massachusetts Institute of Technology (MIT) made the discovery as part of the Young Supernova Experiment. The peer-reviewed Astrophysical Journal published the study on August 13, 2025.

What triggered the supernova?

Alexander Gagliano is the lead author of the study and a fellow at the NSF Institute for Artificial Intelligence and Fundamental Interactions. Gagliano said:

Our analysis shows that the blast was sparked by a catastrophic encounter with a black hole companion, and is the strongest evidence to date that such close interactions can actually detonate a star. Our machine learning system flagged SN 2023zkd months before its most unusual behavior, which gave us ample time to secure the critical observations needed to unravel this extraordinary explosion.

An alternative interpretation the team considered is that the black hole completely tore the star apart before it could explode on its own. In that case, the black hole quickly pulled in the star’s debris, and supernova emission was generated when the debris crashed into the gas surrounding it. Both cases leave a single, heavier black hole behind.

Witnessing the new type of supernova

Located about 730 million light-years from Earth, SN 2023zkd initially looked like a typical supernova. It had a single burst of light. But as the scientists tracked its decline over several months, it did something unexpected: it brightened again. To understand this unusual behavior, the scientists analyzed archival data, which showed something even more unusual. The system had been slowly brightening for more than four years before the explosion. Scientists rarely see that kind of long-term activity before the explosion in supernovas.

Detailed analysis revealed the explosion’s light was shaped by material the star had shed in the years before it died. The early brightening came from the supernova’s blast wave hitting low-density gas. The second, delayed peak was caused by a slower but sustained collision with a thick, disk-like cloud. This structure – and the star’s erratic pre-explosion behavior – suggest the dying star was under extreme gravitational stress. And that stress was likely from a nearby, compact companion such as a black hole.

V. Ashley Villar is a CfA assistant professor of astronomy in the Harvard Faculty of Arts and Sciences and a co-author on the study. Villar said:

2023zkd shows some of the clearest signs we’ve seen of a massive star interacting with a companion in the years before explosion. We think this might be part of a whole class of hidden explosions that AI will help us discover.

More chances to catch supernovas in the act

Gagliano said:

This discovery shows how important it is to study how massive stars interact with companions as they approach the end of their lives. We’ve known for some time that most massive stars are in binaries, but catching one in the act of exchanging mass shortly before it explodes is incredibly rare.

With the Vera C. Rubin Observatory recently unveiling its first images and preparing to survey the entire sky every few nights, this discovery marks a glimpse of what’s to come. Powerful new observatories, combined with real-time AI systems, will soon allow astronomers to uncover many more rare and complex explosions and begin to map how massive stars live and die in binary systems.

The Young Supernova Experiment will continue to complement Rubin by using the Pan-STARRS1 and Pan-STARRS2 telescopes to identify supernovas shortly after explosion. This approach offers a cost-effective way to study the dynamic nearby universe. Gagliano said:

We’re now entering an era where we can automatically catch these rare events as they happen, not just after the fact. That means we can finally start connecting the dots between how a star lives and how it dies, and that’s incredibly exciting.

Bottom line: Astronomers believe they’ve found a new type of supernova. They say it exploded as a star tried to envelop its black hole companion.

Source: Evidence for an Instability-induced Binary Merger in the Double-peaked, Helium-rich Type IIn Supernova 2023zkd

Via the Center for Astrophysics | Harvard & Smithsonian

The post New type of supernova, as a black hole triggers a star explosion first appeared on EarthSky.



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Delphinus the Dolphin has a graceful kite shape

Star chart: Summer Triangle outlined with its apex stars labeled and 3 small constellations near it.
Once you’re familiar with the Summer Triangle, you can use it to star-hop to several nearby small constellations: Delphinus the Dolphin, Sagitta the Arrow and Vulpecula the Fox. Just be sure you’re looking in a dark sky! Chart via EarthSky.

How to see Delphinus

Delphinus the Dolphin is the 69th-largest of the 88 constellations. It comes into view each year on northern summer evenings. And by northern fall, it’s well placed for viewing, arcing high across the sky each night. However, its stars are faint. So to see it, you’ll want a dark sky.

Delphinus lies just outside of the line connecting the stars Deneb in Cygnus the Swan and Altair in Aquila the Eagle. These bright stars form two corners of the famous asterism called the Summer Triangle. Scan along that line with your eye or binoculars. If your sky is dark enough, Delphinus will pop into view.

One could argue that Delphinus looks very much like the animal it’s supposed to represent (this is not always the case with constellations, as you might have noticed). Its faint stars form a kite shape with a tail. Then the little dolphin appears to leap out of the dark waters of the night sky.

Star chart of constellation Delphinus with 5 stars, 3 labeled.
A closeup on the constellation Delphinus the Dolphin and 3 of its named stars. Chart via EarthSky.

The stars of the Dolphin

The brightest star in the Dolphin is Beta Delphini, which shines at magnitude 3.6. The star also goes by the name Rotanev. Lying 101 light-years from Earth, it marks the point in the constellation where the Dolphin’s body connects with its tail.

The second brightest star is Alpha Delphini, at magnitude 3.7. This star’s nickname is Sualocin. Lying 254 light-years away, it marks the back of the Dolphin.

By the way, these two stars’ common names, Rotanev and Sualocin, are part of a puzzle. Italian astronomer Nicolaus Venator named these two stars. Can you solve the puzzle? Hint: try reading the stars’ names backward.

The nose of Delphinus is Gamma Delphini, a double star. The pair of stars shine at magnitude 4.2 and 5.1. They lie approximately 101 light-years away.

The belly of the dolphin is Delta Delphini, a magnitude 4.4 star lying 223 light-years away.

Although Delphinus is a small constellation, it contains an asterism: Job’s Coffin. The four stars that mark the body of the Dolphin are the same stars that form Job’s Coffin.

The tail of the dolphin contains one star, Epsilon Delphini or Aldulfin. The magnitude-4.0 star lies 330 light-years away.

In 2013, a bright nova exploded in Delphinus not far from Sualocin. The nova, V339 Delphini, was temporarily visible to the unaided eye.

Star field with labeled objects, and small bright dot circled in blue and labeled Nova.
This image of the night sky shows the region of Delphinus and the Summer Triangle where nova V339 briefly lit up in 2013. Image via NASA/ Wikimedia Commons.

Deep-sky objects

Most of the deep-sky objects in Delphinus are quite dim. The brightest of these is NGC 6934, a globular cluster found about 4 degrees out from the tail. NGC 6934 shines at magnitude 8.9. Another globular cluster, NGC 7006, lies off the nose of the Dolphin. If you draw a line from Sualocin through the nose star Gamma and extend it for about twice that distance, you’ll reach NGC 7006. NGC 7006 shines at magnitude 10.6.

Two planetary nebulae lie within the northwestern boundary of the constellation. Both shine with a magnitude of 12. NGC 6905 – the Blue Flash Nebula – lies directly above the Dolphin’s back. The other planetary nebula – NGC 6891 – is above Delphinus’ tail. A number of galaxies are scattered about Delphinus; however, most of them are 12th magnitude and dimmer, making them very hard to spot without a large telescope.

Small, hazy light blue blob with barely perceptible features, in starfield.
The Blue Flash Nebula, NGC 6905, lies above the back of Delphinus the Dolphin. Image via Digital Sky Survey 2/ In-the-Sky.org/ Dominic Ford. Used with permission.

Delphinus and a neutrino

In 2021, scientists announced they’d pinpointed the origin of a neutrino, or high-energy particle. And it came from the direction of Delphinus the Dolphin.

They believe that, in a cataclysmic event, a supermassive black hole and a star drew too close together. The black hole shredded the star, which released the cosmic ray neutrino. Scientists detected the neutrino using the IceCube Neutrino Observatory at the Amundsen-Scott South Pole Station in Antarctica. So much info from such a tiny particle! Read more about the discovery.

Star chart with black stars on white of constellation Delphinus showing the outline and labels on the stars.
Star chart of the constellation Delphinus. Image by IAU/ Wikipedia (CC BY 3.0).

Delphinus in history and mythology

The name Delphinus means dolphin in Latin. But it was a Greek astronomer – Ptolemy of Alexandria in the second century CE – who first cataloged these stars. In Greek mythology, Delphinus represents the dolphin sent by the sea god Poseidon to fetch Amphitrite, a goddess of the sea and one of the fabled Nereids. It’s said Poseidon chose Amphitrite from among her sisters as they performed a dance on the isle of Naxos. The dolphin carried Amphitrite to Poseidon, and she became his wife. He rewarded the dolphin by making it a constellation.

In another story, Delphinus saves the Greek poet Arion when he is attacked by robbers on a ship. They were about to kill Arion, but he begged permission to sing a final song. His captors agreed, and the poet stood on the deck of the ship and sang a dirge accompanied by his lyre. He then threw himself overboard. A dolphin who’d heard his song and been charmed by the music saved him.

Antique colored etching of an ugly fish next to a flying eagle, all scattered with stars.
In this drawing from Urania’s Mirror, Delphinus the Dolphin is the green sea creature at left. Image via Wikipedia.

Bottom line: Delphinus the Dolphin is a petite constellation that looks like the animal it’s supposed to represent. Look for the dolphin leaping under the Summer Triangle.

The post Delphinus the Dolphin has a graceful kite shape first appeared on EarthSky.



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Star chart: Summer Triangle outlined with its apex stars labeled and 3 small constellations near it.
Once you’re familiar with the Summer Triangle, you can use it to star-hop to several nearby small constellations: Delphinus the Dolphin, Sagitta the Arrow and Vulpecula the Fox. Just be sure you’re looking in a dark sky! Chart via EarthSky.

How to see Delphinus

Delphinus the Dolphin is the 69th-largest of the 88 constellations. It comes into view each year on northern summer evenings. And by northern fall, it’s well placed for viewing, arcing high across the sky each night. However, its stars are faint. So to see it, you’ll want a dark sky.

Delphinus lies just outside of the line connecting the stars Deneb in Cygnus the Swan and Altair in Aquila the Eagle. These bright stars form two corners of the famous asterism called the Summer Triangle. Scan along that line with your eye or binoculars. If your sky is dark enough, Delphinus will pop into view.

One could argue that Delphinus looks very much like the animal it’s supposed to represent (this is not always the case with constellations, as you might have noticed). Its faint stars form a kite shape with a tail. Then the little dolphin appears to leap out of the dark waters of the night sky.

Star chart of constellation Delphinus with 5 stars, 3 labeled.
A closeup on the constellation Delphinus the Dolphin and 3 of its named stars. Chart via EarthSky.

The stars of the Dolphin

The brightest star in the Dolphin is Beta Delphini, which shines at magnitude 3.6. The star also goes by the name Rotanev. Lying 101 light-years from Earth, it marks the point in the constellation where the Dolphin’s body connects with its tail.

The second brightest star is Alpha Delphini, at magnitude 3.7. This star’s nickname is Sualocin. Lying 254 light-years away, it marks the back of the Dolphin.

By the way, these two stars’ common names, Rotanev and Sualocin, are part of a puzzle. Italian astronomer Nicolaus Venator named these two stars. Can you solve the puzzle? Hint: try reading the stars’ names backward.

The nose of Delphinus is Gamma Delphini, a double star. The pair of stars shine at magnitude 4.2 and 5.1. They lie approximately 101 light-years away.

The belly of the dolphin is Delta Delphini, a magnitude 4.4 star lying 223 light-years away.

Although Delphinus is a small constellation, it contains an asterism: Job’s Coffin. The four stars that mark the body of the Dolphin are the same stars that form Job’s Coffin.

The tail of the dolphin contains one star, Epsilon Delphini or Aldulfin. The magnitude-4.0 star lies 330 light-years away.

In 2013, a bright nova exploded in Delphinus not far from Sualocin. The nova, V339 Delphini, was temporarily visible to the unaided eye.

Star field with labeled objects, and small bright dot circled in blue and labeled Nova.
This image of the night sky shows the region of Delphinus and the Summer Triangle where nova V339 briefly lit up in 2013. Image via NASA/ Wikimedia Commons.

Deep-sky objects

Most of the deep-sky objects in Delphinus are quite dim. The brightest of these is NGC 6934, a globular cluster found about 4 degrees out from the tail. NGC 6934 shines at magnitude 8.9. Another globular cluster, NGC 7006, lies off the nose of the Dolphin. If you draw a line from Sualocin through the nose star Gamma and extend it for about twice that distance, you’ll reach NGC 7006. NGC 7006 shines at magnitude 10.6.

Two planetary nebulae lie within the northwestern boundary of the constellation. Both shine with a magnitude of 12. NGC 6905 – the Blue Flash Nebula – lies directly above the Dolphin’s back. The other planetary nebula – NGC 6891 – is above Delphinus’ tail. A number of galaxies are scattered about Delphinus; however, most of them are 12th magnitude and dimmer, making them very hard to spot without a large telescope.

Small, hazy light blue blob with barely perceptible features, in starfield.
The Blue Flash Nebula, NGC 6905, lies above the back of Delphinus the Dolphin. Image via Digital Sky Survey 2/ In-the-Sky.org/ Dominic Ford. Used with permission.

Delphinus and a neutrino

In 2021, scientists announced they’d pinpointed the origin of a neutrino, or high-energy particle. And it came from the direction of Delphinus the Dolphin.

They believe that, in a cataclysmic event, a supermassive black hole and a star drew too close together. The black hole shredded the star, which released the cosmic ray neutrino. Scientists detected the neutrino using the IceCube Neutrino Observatory at the Amundsen-Scott South Pole Station in Antarctica. So much info from such a tiny particle! Read more about the discovery.

Star chart with black stars on white of constellation Delphinus showing the outline and labels on the stars.
Star chart of the constellation Delphinus. Image by IAU/ Wikipedia (CC BY 3.0).

Delphinus in history and mythology

The name Delphinus means dolphin in Latin. But it was a Greek astronomer – Ptolemy of Alexandria in the second century CE – who first cataloged these stars. In Greek mythology, Delphinus represents the dolphin sent by the sea god Poseidon to fetch Amphitrite, a goddess of the sea and one of the fabled Nereids. It’s said Poseidon chose Amphitrite from among her sisters as they performed a dance on the isle of Naxos. The dolphin carried Amphitrite to Poseidon, and she became his wife. He rewarded the dolphin by making it a constellation.

In another story, Delphinus saves the Greek poet Arion when he is attacked by robbers on a ship. They were about to kill Arion, but he begged permission to sing a final song. His captors agreed, and the poet stood on the deck of the ship and sang a dirge accompanied by his lyre. He then threw himself overboard. A dolphin who’d heard his song and been charmed by the music saved him.

Antique colored etching of an ugly fish next to a flying eagle, all scattered with stars.
In this drawing from Urania’s Mirror, Delphinus the Dolphin is the green sea creature at left. Image via Wikipedia.

Bottom line: Delphinus the Dolphin is a petite constellation that looks like the animal it’s supposed to represent. Look for the dolphin leaping under the Summer Triangle.

The post Delphinus the Dolphin has a graceful kite shape first appeared on EarthSky.



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Can you see a full circle rainbow? All you need to know

View of a big city and green hillside with an almost full rainbow showing.
View at EarthSky Community Photos. | Meiying Lee captured this image in Taiwan on July 23, 2025, and wrote: “I was overjoyed! This evening, rain drifted in from the east, and with it, the rainbow slowly moved closer and closer, until it reached right in front of me. I saw a nearly full circle rainbow, so close it felt within arm’s reach! Of course, the rain kept moving too, soon it was right above me, and I ended up completely soaked.” Thank you, Meiying.

What makes a rainbow?

When sunlight and raindrops combine to make a rainbow, they can make a whole circle of light in the sky. But it’s a very rare sight. Sky conditions must be just right for this, and even if they are, the bottom part of a full-circle rainbow is usually blocked by your horizon. That’s why we see rainbows not as circles, but as arcs across our sky.

When you see a rainbow, notice the height of the sun. It helps determine how much of an arc you’ll see. The lower the sun, the higher the top of the rainbow. If you could get up high enough, you’d see that some rainbows continue below the horizon seen from closer to sea-level. Mountain climbers sometimes see more of a full-circle rainbow. However, even a high mountain isn’t high enough to show you the whole circle.

Pilots do sometimes report seeing genuine full circle rainbows. They’d be tough to see out the small windows we passengers look through, but pilots have a much better view from up front.

Similar sky optics

By the way, we searched for images of full circle rainbows. But most of the ones we found weren’t really rainbows. They were either halos around the sun or airplane glories.


What’s NOT a rainbow? Hear from a master of sky optics.

Do you have a great picture of a rainbow? Submit it to our EarthSky Community Photos page.

Enjoying EarthSky? Sign up for our free daily newsletter today!

Bottom line: Can you ever see a full circle rainbow in the sky? Yes, but they’re most often seen by pilots, who have a good view of the sky from the wide front windows of a plane.

The post Can you see a full circle rainbow? All you need to know first appeared on EarthSky.



from EarthSky https://ift.tt/acM809d
View of a big city and green hillside with an almost full rainbow showing.
View at EarthSky Community Photos. | Meiying Lee captured this image in Taiwan on July 23, 2025, and wrote: “I was overjoyed! This evening, rain drifted in from the east, and with it, the rainbow slowly moved closer and closer, until it reached right in front of me. I saw a nearly full circle rainbow, so close it felt within arm’s reach! Of course, the rain kept moving too, soon it was right above me, and I ended up completely soaked.” Thank you, Meiying.

What makes a rainbow?

When sunlight and raindrops combine to make a rainbow, they can make a whole circle of light in the sky. But it’s a very rare sight. Sky conditions must be just right for this, and even if they are, the bottom part of a full-circle rainbow is usually blocked by your horizon. That’s why we see rainbows not as circles, but as arcs across our sky.

When you see a rainbow, notice the height of the sun. It helps determine how much of an arc you’ll see. The lower the sun, the higher the top of the rainbow. If you could get up high enough, you’d see that some rainbows continue below the horizon seen from closer to sea-level. Mountain climbers sometimes see more of a full-circle rainbow. However, even a high mountain isn’t high enough to show you the whole circle.

Pilots do sometimes report seeing genuine full circle rainbows. They’d be tough to see out the small windows we passengers look through, but pilots have a much better view from up front.

Similar sky optics

By the way, we searched for images of full circle rainbows. But most of the ones we found weren’t really rainbows. They were either halos around the sun or airplane glories.


What’s NOT a rainbow? Hear from a master of sky optics.

Do you have a great picture of a rainbow? Submit it to our EarthSky Community Photos page.

Enjoying EarthSky? Sign up for our free daily newsletter today!

Bottom line: Can you ever see a full circle rainbow in the sky? Yes, but they’re most often seen by pilots, who have a good view of the sky from the wide front windows of a plane.

The post Can you see a full circle rainbow? All you need to know first appeared on EarthSky.



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Surprisingly chaotic early universe had supersonic turbulence

Chaotic early universe: Bright looping filaments in yellows, blues, reds and greens on black background.
This is a 3D view of clumps of gas in the center of a dark matter mini-halo. A new study in Taiwan said the chaotic early universe experienced supersonic turbulence in its star-forming clouds. Image via Chen et al./ The Astrophysical Journal Letters (CC BY-SA 4.0).
  • What was the early universe like? Astronomers thought the first stars were gigantic and drifted in isolation in relatively calm clouds of gas.
  • But the first star-forming clouds were turbulent and clumpy, a new study from researchers in Taiwan suggests. The turbulence reached supersonic speeds. This was only a few hundred million years after the Big Bang.
  • The first stars in the universe were less massive but more numerous than previously thought, the study says.

The early universe

What did the early universe look like, before there were any stars? Researchers at the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan have a new answer. On August 5, 2025, the researchers said their cutting-edge simulations show the universe was turbulent, clumpy and supersonic. These were the first star-forming clouds, or early forms of galaxies. The researchers studied a mini-halo of dark matter – 10 million times more massive than our sun – to track the movements of gas within a star-forming cloud.

A dark matter mini-halo is a small, gravitationally bound clump of dark matter that can exist within a larger dark matter halo. A single dark matter halo contains multiple smaller clumps of dark matter, held together by gravity.

Astrophysicist Ke-Jung Chen at ASIAA led the research team. The researchers used the GIZMO simulation code and high-resolution cosmological data from the IllustrisTNG project for their study. GIZMO is a flexible, massively parallel, multi-physics simulation code. The IllustrisTNG project, likewise, is an ongoing series of large, cosmological magnetohydrodynamical simulations of galaxy formation. Magnetohydrodynamics (MHD) is a field of study that examines the behavior of electrically conducting fluids, like plasmas and liquid metals, in the presence of magnetic fields.

The new findings reveal how chaotic the universe was only a few hundred million years after the Big Bang. You might think it was a generally tranquil place, but it was anything but!

The researchers published their peer-reviewed findings in The Astrophysical Journal Letters on July 30, 2025.

4 squares with blue wispy cloud-like formations in them. Each square is a zoomed-in image of part of the square before it, in sequence.
View larger. | Successive zoom-ins of the dark matter mini-halo the researchers observed in the study. Image via Chen et al./ The Astrophysical Journal Letters (CC BY-SA 4.0).

A turbulent and chaotic early universe

It seems natural to think that before the first stars and galaxies formed, the universe was a rather quiet place. But the new findings from Chen and his team suggest just the opposite.

The first star-forming clouds – not the fully-formed galaxies we see now – were clumpy and surprisingly turbulent. In fact, that turbulence was supersonic, reaching speeds of up to five times faster than the speed of sound. (The speed of sound is about 761 miles per hour or 1,225 kph).

Gas falling into the dark matter mini-halos generated the turbulence. The turbulence was powerful enough to shred the cloud into multiple dense clumps. For the dark matter mini-halo that the researchers studied, one of the resulting clumps was ready to form a new star eight times as massive as the sun.

Chen said:

This is the first time we’ve been able to resolve the full development of turbulence during the earliest phases of the first star formation. It shows that violent, chaotic motions were not only present, they were crucial in shaping the first stars.

Short man wearing a dark jacket and blue jeans standing in front of a very large tree.
Astrophysicist Ke-Jung Chen at the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan is the lead author of the new study about the early universe. Image via Ke-Jung Chen.

1st stars less massive but more numerous

Interestingly, the results also suggest that the first stars born in the universe were less massive but more numerous than previously thought. This contradicts earlier star formation models. In that scenario, the first stars were gigantic and solitary. They drifted through much smoother and less chaotic clouds of gas.

The results could also help explain another mystery. That mystery is the lack of chemical fingerprints from the massive first stars – which exploded – in the oldest stars we see today. But astronomers have never confirmed those fingerprints. If such massive stars were rare, as the study suggests, that could explain the lack of leftover chemical signatures.

The findings might also help astronomers better understand other cosmic phenomena as well. This includes early-universe magnetic fields, the formation of black holes and the origin of the chemical elements in the universe. As Chen noted:

This simulation represents a leap forward in connecting large-scale cosmic structure formation with the microscopic processes that govern star birth. By uncovering the role of turbulence, we’re one step closer to understanding how the cosmic dawn began.

Bottom line: In a surprisingly chaotic early universe, the first star-forming clouds experienced supersonic turbulence only a few hundred million years after the Big Bang.

Via ASIAA

Source: Formation of Supersonic Turbulence in the Primordial Star-forming Cloud

Read more: Surprising galaxy shines through fog of the early universe

Read more: Red monsters were massive galaxies in the early universe

The post Surprisingly chaotic early universe had supersonic turbulence first appeared on EarthSky.



from EarthSky https://ift.tt/AjOXrL2
Chaotic early universe: Bright looping filaments in yellows, blues, reds and greens on black background.
This is a 3D view of clumps of gas in the center of a dark matter mini-halo. A new study in Taiwan said the chaotic early universe experienced supersonic turbulence in its star-forming clouds. Image via Chen et al./ The Astrophysical Journal Letters (CC BY-SA 4.0).
  • What was the early universe like? Astronomers thought the first stars were gigantic and drifted in isolation in relatively calm clouds of gas.
  • But the first star-forming clouds were turbulent and clumpy, a new study from researchers in Taiwan suggests. The turbulence reached supersonic speeds. This was only a few hundred million years after the Big Bang.
  • The first stars in the universe were less massive but more numerous than previously thought, the study says.

The early universe

What did the early universe look like, before there were any stars? Researchers at the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan have a new answer. On August 5, 2025, the researchers said their cutting-edge simulations show the universe was turbulent, clumpy and supersonic. These were the first star-forming clouds, or early forms of galaxies. The researchers studied a mini-halo of dark matter – 10 million times more massive than our sun – to track the movements of gas within a star-forming cloud.

A dark matter mini-halo is a small, gravitationally bound clump of dark matter that can exist within a larger dark matter halo. A single dark matter halo contains multiple smaller clumps of dark matter, held together by gravity.

Astrophysicist Ke-Jung Chen at ASIAA led the research team. The researchers used the GIZMO simulation code and high-resolution cosmological data from the IllustrisTNG project for their study. GIZMO is a flexible, massively parallel, multi-physics simulation code. The IllustrisTNG project, likewise, is an ongoing series of large, cosmological magnetohydrodynamical simulations of galaxy formation. Magnetohydrodynamics (MHD) is a field of study that examines the behavior of electrically conducting fluids, like plasmas and liquid metals, in the presence of magnetic fields.

The new findings reveal how chaotic the universe was only a few hundred million years after the Big Bang. You might think it was a generally tranquil place, but it was anything but!

The researchers published their peer-reviewed findings in The Astrophysical Journal Letters on July 30, 2025.

4 squares with blue wispy cloud-like formations in them. Each square is a zoomed-in image of part of the square before it, in sequence.
View larger. | Successive zoom-ins of the dark matter mini-halo the researchers observed in the study. Image via Chen et al./ The Astrophysical Journal Letters (CC BY-SA 4.0).

A turbulent and chaotic early universe

It seems natural to think that before the first stars and galaxies formed, the universe was a rather quiet place. But the new findings from Chen and his team suggest just the opposite.

The first star-forming clouds – not the fully-formed galaxies we see now – were clumpy and surprisingly turbulent. In fact, that turbulence was supersonic, reaching speeds of up to five times faster than the speed of sound. (The speed of sound is about 761 miles per hour or 1,225 kph).

Gas falling into the dark matter mini-halos generated the turbulence. The turbulence was powerful enough to shred the cloud into multiple dense clumps. For the dark matter mini-halo that the researchers studied, one of the resulting clumps was ready to form a new star eight times as massive as the sun.

Chen said:

This is the first time we’ve been able to resolve the full development of turbulence during the earliest phases of the first star formation. It shows that violent, chaotic motions were not only present, they were crucial in shaping the first stars.

Short man wearing a dark jacket and blue jeans standing in front of a very large tree.
Astrophysicist Ke-Jung Chen at the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan is the lead author of the new study about the early universe. Image via Ke-Jung Chen.

1st stars less massive but more numerous

Interestingly, the results also suggest that the first stars born in the universe were less massive but more numerous than previously thought. This contradicts earlier star formation models. In that scenario, the first stars were gigantic and solitary. They drifted through much smoother and less chaotic clouds of gas.

The results could also help explain another mystery. That mystery is the lack of chemical fingerprints from the massive first stars – which exploded – in the oldest stars we see today. But astronomers have never confirmed those fingerprints. If such massive stars were rare, as the study suggests, that could explain the lack of leftover chemical signatures.

The findings might also help astronomers better understand other cosmic phenomena as well. This includes early-universe magnetic fields, the formation of black holes and the origin of the chemical elements in the universe. As Chen noted:

This simulation represents a leap forward in connecting large-scale cosmic structure formation with the microscopic processes that govern star birth. By uncovering the role of turbulence, we’re one step closer to understanding how the cosmic dawn began.

Bottom line: In a surprisingly chaotic early universe, the first star-forming clouds experienced supersonic turbulence only a few hundred million years after the Big Bang.

Via ASIAA

Source: Formation of Supersonic Turbulence in the Primordial Star-forming Cloud

Read more: Surprising galaxy shines through fog of the early universe

Read more: Red monsters were massive galaxies in the early universe

The post Surprisingly chaotic early universe had supersonic turbulence first appeared on EarthSky.



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Female gorillas favor moving to groups that have gal pals

Two adult gorillas with two infants.
Here are 3 generations of mountain gorillas. Gutangara is holding her infant daughter (right). Next to her is her adult daughter Shishikara and grandson Kira (not facing the camera). Image via Dian Fossey Gorilla Fund/ University of Zurich.
  • Female mountain gorillas prefer joining groups with familiar females they lived with before.
  • They avoid groups that include males they grew up with.
  • Strong female social bonds influence group choice more than group size or composition.

What influences an animal to join a new social group?

In many animal societies, an individual often leaves its birth group to join another group. Scientists who study social animals have long wondered: How do they decide which group to join? On August 5, 2025, a new study revealed some answers for mountain gorillas. Researchers from the University of Zurich ran statistical analyses on 20 years of gorilla observations. Their results revealed female gorillas preferred to join groups with females they had lived with in the past. And they avoided groups that had males they had grown up with.

Co-author Robin Morrison of the University of Zurich said:

Going into a new group could feel pretty scary, with individuals usually entering at the bottom of the social hierarchy. A familiar female might help reduce this, providing a social ally.

It could also act like a recommendation from a friend – if a female they know has chosen to stay in this group, it could indicate positive things about the group as a whole or the dominant male leading that group.

The researchers published their findings in the peer-reviewed journal Proceedings of the Royal Society B on August 6, 2025.

New insights from two decades of gorilla observations

The movement of animals to different social groups is called dispersal. It’s a behavior that’s crucial for the overall health of a population. For instance, it avoids inbreeding within a group. It also increases genetic diversity, cultivates relationships between groups and, in some instances, spreads knowledge and culture.

For this study, the scientists analyzed observations of mountain gorillas in the Volcanoes National Park in Rwanda. Trained field teams gathered these observations between 2003 and 2023.

The scientists wanted to know: When a female moves to a new group, why did she pick that group?

The researchers decided to focus on females. That’s because males are harder to track; when they leave a group, they typically live a solitary life before creating their own social group. Females, on the other hand, transfer from one group to another or join a solitary male.

The scientists scrutinized 152 dispersals, made by 56 female mountain gorillas ranging in age from 6 to 43 years. Most moves to another group were undertaken alone, by adults and subadults over 6 years in age. The female gorillas, the researchers found, dispersed on average about 2.8 times to different groups during that 20-year period, with dispersions ranging from 1 to 11.

Female gorillas invest in relationships with other females

Female gorillas were generally not influenced by the size of a group or its demographics. They picked new groups based on the presence of females they had already lived with. Moreover, they were more strongly influenced to join a group if they had previously lived with those females for at least five years and seen them in the last two years.

Morrison added:

Investing in these relationships clearly matters. Spatial separation can be ephemeral with individuals being reunited in the future, easing the difficult process of starting over in a new social group.

Two female gorillas with an infant.
Two adult female mountain gorillas resting in close physical contact, with an infant. Image via Dian Fossey Gorilla Fund.

Female gorillas avoid groups with males they grew up with

In addition, females avoided going to groups that had males they grew up with.

The paper’s lead author, Victoire Martignac of the University of Zurich, said:

Because female mountain gorillas do not know with certainty who their fathers are, they might rely on a simple rule like ‘avoid any group with males I grew up with’ as the likelihood of them being related will be higher than with males they did not grow up with.

Because females can disperse multiple times, they will become familiar with many males from different groups. Yet, when choosing their next group, they only avoid males they grew up with. This really tells us that it’s not just who they know that matters but how they know them.

Deep social ties

This study shows how deep wide-ranging social ties affect the dispersal of female gorillas, allowing the formation of new relationships and sustaining current ones. And groups often interact and share overlapping ranges, indicating that relationships spread beyond group boundaries.

Martignac observed:

This mirrors a key aspect of human societies: the existence of strong ties between different social groups. As humans, we’re constantly moving across jobs, cities and social groups. We do it so effortlessly that we forget how unusual this flexibility actually is within the animal kingdom.

This is a reminder of the meaningfulness of social relationships kept across boundaries and how this extended network of relationships might have played a key role in the evolution of larger and more cooperative societies.

A group of about 30 mountain gorillas in green vegetation.
An encounter between 2 gorilla groups. This provides an opportunity for females to learn about their neighbors to decide if they want to join them. Image via Dian Fossey Gorilla Fund/ Eurekalert.

Continuing the legacy of Dian Fossey

Since 1967, mountain gorillas (Gorilla beringei beringei) have been monitored at Volcanoes National Park in Rwanda by the Dian Fossey Gorilla Fund. Dian Fossey was a pioneering primatologist who did groundbreaking studies on gorillas and championed their conservation. Tragically, she was murdered in 1985, in her cabin in Rwanda.

Tara Stoinski, a paper co-author and CEO of the Dian Fossey Gorilla Fund, commented on the value of long-term studies:

Being able to study dispersal, to track not only where individuals are from but also where they go, and to construct their whole social history in such detail, is only possible because of decades of data collection. With just a few years and a few groups, all of these inter-group ties and extended networks would be invisible to us. This really highlights the value of long-term observations on multiple groups in better understanding the evolution of sociality.

Bottom line: Female gorillas prefer to join groups with females they had lived with in the past. They also avoided groups with males they grew up with.

Source: Dispersed female networks: female gorillas’ inter-group relationships influence dispersal decisions

Via:
University of Zurich
Dian Fossey Gorilla Fund
Eurekalert

Read more: Chimpanzees wear blades of grass in their ears and rears

The post Female gorillas favor moving to groups that have gal pals first appeared on EarthSky.



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Two adult gorillas with two infants.
Here are 3 generations of mountain gorillas. Gutangara is holding her infant daughter (right). Next to her is her adult daughter Shishikara and grandson Kira (not facing the camera). Image via Dian Fossey Gorilla Fund/ University of Zurich.
  • Female mountain gorillas prefer joining groups with familiar females they lived with before.
  • They avoid groups that include males they grew up with.
  • Strong female social bonds influence group choice more than group size or composition.

What influences an animal to join a new social group?

In many animal societies, an individual often leaves its birth group to join another group. Scientists who study social animals have long wondered: How do they decide which group to join? On August 5, 2025, a new study revealed some answers for mountain gorillas. Researchers from the University of Zurich ran statistical analyses on 20 years of gorilla observations. Their results revealed female gorillas preferred to join groups with females they had lived with in the past. And they avoided groups that had males they had grown up with.

Co-author Robin Morrison of the University of Zurich said:

Going into a new group could feel pretty scary, with individuals usually entering at the bottom of the social hierarchy. A familiar female might help reduce this, providing a social ally.

It could also act like a recommendation from a friend – if a female they know has chosen to stay in this group, it could indicate positive things about the group as a whole or the dominant male leading that group.

The researchers published their findings in the peer-reviewed journal Proceedings of the Royal Society B on August 6, 2025.

New insights from two decades of gorilla observations

The movement of animals to different social groups is called dispersal. It’s a behavior that’s crucial for the overall health of a population. For instance, it avoids inbreeding within a group. It also increases genetic diversity, cultivates relationships between groups and, in some instances, spreads knowledge and culture.

For this study, the scientists analyzed observations of mountain gorillas in the Volcanoes National Park in Rwanda. Trained field teams gathered these observations between 2003 and 2023.

The scientists wanted to know: When a female moves to a new group, why did she pick that group?

The researchers decided to focus on females. That’s because males are harder to track; when they leave a group, they typically live a solitary life before creating their own social group. Females, on the other hand, transfer from one group to another or join a solitary male.

The scientists scrutinized 152 dispersals, made by 56 female mountain gorillas ranging in age from 6 to 43 years. Most moves to another group were undertaken alone, by adults and subadults over 6 years in age. The female gorillas, the researchers found, dispersed on average about 2.8 times to different groups during that 20-year period, with dispersions ranging from 1 to 11.

Female gorillas invest in relationships with other females

Female gorillas were generally not influenced by the size of a group or its demographics. They picked new groups based on the presence of females they had already lived with. Moreover, they were more strongly influenced to join a group if they had previously lived with those females for at least five years and seen them in the last two years.

Morrison added:

Investing in these relationships clearly matters. Spatial separation can be ephemeral with individuals being reunited in the future, easing the difficult process of starting over in a new social group.

Two female gorillas with an infant.
Two adult female mountain gorillas resting in close physical contact, with an infant. Image via Dian Fossey Gorilla Fund.

Female gorillas avoid groups with males they grew up with

In addition, females avoided going to groups that had males they grew up with.

The paper’s lead author, Victoire Martignac of the University of Zurich, said:

Because female mountain gorillas do not know with certainty who their fathers are, they might rely on a simple rule like ‘avoid any group with males I grew up with’ as the likelihood of them being related will be higher than with males they did not grow up with.

Because females can disperse multiple times, they will become familiar with many males from different groups. Yet, when choosing their next group, they only avoid males they grew up with. This really tells us that it’s not just who they know that matters but how they know them.

Deep social ties

This study shows how deep wide-ranging social ties affect the dispersal of female gorillas, allowing the formation of new relationships and sustaining current ones. And groups often interact and share overlapping ranges, indicating that relationships spread beyond group boundaries.

Martignac observed:

This mirrors a key aspect of human societies: the existence of strong ties between different social groups. As humans, we’re constantly moving across jobs, cities and social groups. We do it so effortlessly that we forget how unusual this flexibility actually is within the animal kingdom.

This is a reminder of the meaningfulness of social relationships kept across boundaries and how this extended network of relationships might have played a key role in the evolution of larger and more cooperative societies.

A group of about 30 mountain gorillas in green vegetation.
An encounter between 2 gorilla groups. This provides an opportunity for females to learn about their neighbors to decide if they want to join them. Image via Dian Fossey Gorilla Fund/ Eurekalert.

Continuing the legacy of Dian Fossey

Since 1967, mountain gorillas (Gorilla beringei beringei) have been monitored at Volcanoes National Park in Rwanda by the Dian Fossey Gorilla Fund. Dian Fossey was a pioneering primatologist who did groundbreaking studies on gorillas and championed their conservation. Tragically, she was murdered in 1985, in her cabin in Rwanda.

Tara Stoinski, a paper co-author and CEO of the Dian Fossey Gorilla Fund, commented on the value of long-term studies:

Being able to study dispersal, to track not only where individuals are from but also where they go, and to construct their whole social history in such detail, is only possible because of decades of data collection. With just a few years and a few groups, all of these inter-group ties and extended networks would be invisible to us. This really highlights the value of long-term observations on multiple groups in better understanding the evolution of sociality.

Bottom line: Female gorillas prefer to join groups with females they had lived with in the past. They also avoided groups with males they grew up with.

Source: Dispersed female networks: female gorillas’ inter-group relationships influence dispersal decisions

Via:
University of Zurich
Dian Fossey Gorilla Fund
Eurekalert

Read more: Chimpanzees wear blades of grass in their ears and rears

The post Female gorillas favor moving to groups that have gal pals first appeared on EarthSky.



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Find the Andromeda galaxy using Cassiopeia

Star chart of constellations Cassiopeia and Andromeda with labeled Andromeda galaxy between them.
Here’s the technique most people use to find the Andromeda galaxy. But be sure you’re looking in a dark sky. Look northward for the M – or W – shaped constellation Cassiopeia the Queen. Then locate the star Schedar in Cassiopeia. It’s the constellation’s brightest star, and it points to the Andromeda galaxy. Chart via EarthSky.

The Andromeda galaxy

The Andromeda galaxy is the nearest large spiral galaxy to our Milky Way. It’s about 2.5 million light-years away, teeming with hundreds of billions of stars. In fact, it’s considered the farthest object you can see with the unaided eye.

Read more: The Andromeda galaxy: All you need to know

Use Cassiopeia to find the Andromeda galaxy

Tonight, if you have a dark sky, try star-hopping to the Andromeda galaxy from the constellation Cassiopeia the Queen. If your sky is dark, you might even spot this hazy patch of light with no optical aid, as the ancient stargazers did before the days of city lights.

But what if you aren’t under a dark sky, and you can’t find the Andromeda galaxy with the eyes alone? Well, some stargazers use binoculars and star-hop to the Andromeda galaxy via this W – or M-shaped constellation.

Cassiopeia appears in the northeast sky at nightfall and early evening, then swings upward as evening deepens into late night. Then in the wee hours before dawn, Cassiopeia is found high over Polaris, the North Star. Note that one half of the W is more deeply notched than the other half. This deeper V is your “arrow” in the sky, pointing to the Andromeda galaxy.

Oblique view of a large spiral galaxy with a bright nucleus, dark lanes and thousands of foreground stars.
View at EarthSky Community Photos. | Jan Curtis in Cheyenne, Wyoming, caught Messier 31, the Andromeda galaxy, on September 25, 2024. Jan wrote: “M31 is well-placed this time of year for all-night viewing.” Thank you, Jan!

Finder chart for the Andromeda galaxy

Star chart of constellation Cassiopeia and arrow pointing to Andromeda Galaxy below it.
Draw an imaginary line from the star Kappa Cassiopeiae (abbreviated Kappa) through the star Schedar, then go about 3 times the Kappa-Schedar distance to locate the Andromeda galaxy (Messier 31).Image via Wikimedia. Used with permission.

Binoculars enhance the view

Binoculars are an excellent choice for beginners to observe the Andromeda galaxy, because they are so easy to point. As you stand beneath a dark sky, locate the galaxy with your eye first. Then slowly bring the binoculars up to your eyes so that the galaxy comes into binocular view. If that doesn’t work for you, try sweeping the area with your binoculars. Go slowly, and be sure your eyes are dark-adapted. The galaxy will appear as a fuzzy patch to the eye. Naturally, it’ll appear brighter in binoculars. And can you see its central region is brighter and more concentrated?

But remember, with the eye, binoculars, or with a backyard telescope, the Andromeda galaxy won’t look like the images from famous telescopes and observatories. But it will be beautiful. Plus, it’ll take your breath away. And just think, you’re looking at a galaxy over 2 million light-years away. Wow!

Bottom line: You can find the Andromeda galaxy using the constellation Cassiopeia as a guide. Remember, on a dark night, this galaxy will look like a faint smudge of light. And once you’ve found it with the unaided eye or binoculars, look at it with a telescope if you have one.

Read more: Andromeda galaxy: Find it by star-hopping from Pegasus

Read more: Andromeda galaxy stuns in new images and sounds!

The post Find the Andromeda galaxy using Cassiopeia first appeared on EarthSky.



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Star chart of constellations Cassiopeia and Andromeda with labeled Andromeda galaxy between them.
Here’s the technique most people use to find the Andromeda galaxy. But be sure you’re looking in a dark sky. Look northward for the M – or W – shaped constellation Cassiopeia the Queen. Then locate the star Schedar in Cassiopeia. It’s the constellation’s brightest star, and it points to the Andromeda galaxy. Chart via EarthSky.

The Andromeda galaxy

The Andromeda galaxy is the nearest large spiral galaxy to our Milky Way. It’s about 2.5 million light-years away, teeming with hundreds of billions of stars. In fact, it’s considered the farthest object you can see with the unaided eye.

Read more: The Andromeda galaxy: All you need to know

Use Cassiopeia to find the Andromeda galaxy

Tonight, if you have a dark sky, try star-hopping to the Andromeda galaxy from the constellation Cassiopeia the Queen. If your sky is dark, you might even spot this hazy patch of light with no optical aid, as the ancient stargazers did before the days of city lights.

But what if you aren’t under a dark sky, and you can’t find the Andromeda galaxy with the eyes alone? Well, some stargazers use binoculars and star-hop to the Andromeda galaxy via this W – or M-shaped constellation.

Cassiopeia appears in the northeast sky at nightfall and early evening, then swings upward as evening deepens into late night. Then in the wee hours before dawn, Cassiopeia is found high over Polaris, the North Star. Note that one half of the W is more deeply notched than the other half. This deeper V is your “arrow” in the sky, pointing to the Andromeda galaxy.

Oblique view of a large spiral galaxy with a bright nucleus, dark lanes and thousands of foreground stars.
View at EarthSky Community Photos. | Jan Curtis in Cheyenne, Wyoming, caught Messier 31, the Andromeda galaxy, on September 25, 2024. Jan wrote: “M31 is well-placed this time of year for all-night viewing.” Thank you, Jan!

Finder chart for the Andromeda galaxy

Star chart of constellation Cassiopeia and arrow pointing to Andromeda Galaxy below it.
Draw an imaginary line from the star Kappa Cassiopeiae (abbreviated Kappa) through the star Schedar, then go about 3 times the Kappa-Schedar distance to locate the Andromeda galaxy (Messier 31).Image via Wikimedia. Used with permission.

Binoculars enhance the view

Binoculars are an excellent choice for beginners to observe the Andromeda galaxy, because they are so easy to point. As you stand beneath a dark sky, locate the galaxy with your eye first. Then slowly bring the binoculars up to your eyes so that the galaxy comes into binocular view. If that doesn’t work for you, try sweeping the area with your binoculars. Go slowly, and be sure your eyes are dark-adapted. The galaxy will appear as a fuzzy patch to the eye. Naturally, it’ll appear brighter in binoculars. And can you see its central region is brighter and more concentrated?

But remember, with the eye, binoculars, or with a backyard telescope, the Andromeda galaxy won’t look like the images from famous telescopes and observatories. But it will be beautiful. Plus, it’ll take your breath away. And just think, you’re looking at a galaxy over 2 million light-years away. Wow!

Bottom line: You can find the Andromeda galaxy using the constellation Cassiopeia as a guide. Remember, on a dark night, this galaxy will look like a faint smudge of light. And once you’ve found it with the unaided eye or binoculars, look at it with a telescope if you have one.

Read more: Andromeda galaxy: Find it by star-hopping from Pegasus

Read more: Andromeda galaxy stuns in new images and sounds!

The post Find the Andromeda galaxy using Cassiopeia first appeared on EarthSky.



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Meet intermediate black holes: Between stellar and massive

Two intermediate black holes in the middle with swirling material around them expanding outward.
Artist concept of 2 intermediate black holes merging that generate gravitational waves. Astronomers can track gravitational waves to help them locate smaller, stellar black holes. Image via Simulating eXtreme Spacetimes (SXS), CC BY-ND 4.0.
  • Intermediate-mass black holes are black holes with masses between stellar black holes and supermassive black holes.
  • Intermediate black holes are hard to detect and much rarer, making them mysterious to astronomers.
  • Understanding these black holes could help scientists learn how supermassive black holes form and grow.

Meet intermediate black holes, the supermassive black hole’s smaller, much more mysterious cousin

By Bill Smith, Vanderbilt University; Karan Jani, Vanderbilt University, and Krystal Ruiz-Rocha, Vanderbilt University

Black holes are massive, strange and incredibly powerful astronomical objects. Scientists know that supermassive black holes reside in the centers of most galaxies.

And they understand how certain stars form the comparatively smaller stellar mass black holes once they reach the end of their life. Understanding how the smaller stellar mass black holes could form the supermassive black holes helps astronomers learn about how the universe grows and evolves.

But there’s an open question in black hole research: What about black holes with masses in between? These are much harder to find than their stellar and supermassive peers, in size range of a few hundred to a few hundred thousand times the mass of the sun.

We’re a team of astronomers who are searching for these in-between black holes, called intermediate black holes. In a new paper, two of us (Krystal and Karan) teamed up with a group of researchers, including postdoctoral researcher Anjali Yelikar, to look at ripples in space-time to spot a few of these elusive black holes merging.

Take me out to the (gravitational wave) ball game

To gain an intuitive idea of how scientists detect stellar mass black holes, imagine you are at a baseball game where you’re sitting directly behind a big concrete column and can’t see the diamond. Even worse, the crowd is deafeningly loud, so it is also nearly impossible to see or hear the game.

But you’re a scientist, so you take out a high-quality microphone and your computer and write a computer algorithm that can take audio data and separate the crowd’s noise from the “thunk” of a bat hitting a ball.

You start recording, and, with enough practice and updates to your hardware and software, you can begin following the game, getting a sense of when a ball is hit, what direction it goes, when it hits a glove, where runners’ feet pound into the dirt and more.

Admittedly, this is a challenging way to watch a baseball game. But unlike baseball, when observing the universe, sometimes the challenging way is all we have.

This principle of recording sound and using computer algorithms to isolate certain sound waves to determine what they are and where they are coming from is similar to how astronomers like us study gravitational waves. Gravitational waves are ripples in space-time that allow us to observe objects such as black holes.

Now imagine implementing a different sound algorithm, testing it over several innings of the game and finding a particular hit that no legal combination of bats and balls could have produced. Imagine the data was suggesting that the ball was bigger and heavier than a legal baseball could be. If our paper was about a baseball game instead of gravitational waves, that’s what we would have found.

Listening for gravitational waves

While the baseball recording setup is designed specifically to hear the sounds of a baseball game, scientists use a specialized observatory called the Laser Interferometer Gravitational-Wave Observatory, or LIGO, to observe the “sound” of two black holes merging out in the universe.

An L-shaped facility with two long arms extending out from a central building.
The LIGO detector in Hanford, Washington, uses lasers to measure the minuscule stretching of space caused by a gravitational wave. Image via LIGO Laboratory.

Scientists look for the gravitational waves that we can measure using LIGO, which has one of the most mind-bogglingly advanced laser and optics systems ever created.

In each event, two “parent” black holes merge into a single, more massive black hole. Using LIGO data, scientists can figure out where and how far away the merger happened, how massive the parents and resultant black holes are, which direction in the sky the merger happened and other key details.

Most of the parent black holes in merger events originally form from stars that have reached the end of their lives – these are stellar mass black holes.

An illustration of a black hole with gas swirling around it, coming from a large cloud around a star on the right.
This artist’s impression shows a binary system containing a stellar mass black hole called IGR J17091-3624. The strong gravity of the black hole, on the left, is pulling gas away from a companion star on the right. Image via NASA/CXC/M.Weiss, CC BY-NC

The black hole mass gap

Not every dying star can create a stellar mass black hole. The ones that do are usually between about 20 to 100 times the mass of the Sun. But due to complicated nuclear physics, really massive stars explode differently and don’t leave behind any remnant, black hole or otherwise.

These physics create what we refer to as the “mass gap” in black holes. A smaller black hole likely formed from a dying star. But we know that a black hole more massive than about 60 times the size of the Sun, while not a supermassive black hole, is still too big to have formed directly from a dying star.

The exact cutoff for the mass gap is still somewhat uncertain, and many astrophysicists are working on more precise measurements. However, we are confident that the mass gaps exist and that we are in the ballpark of the boundary.

We call black holes in this gap lite intermediate mass black holes or lite IMBHs, because they are the least massive black holes that we expect to exist from sources other than stars. They are no longer considered stellar mass black holes.

Calling them “intermediate” also doesn’t quite capture why they are special. They are special because they are much harder to find, astronomers still aren’t sure what astronomical events might create them, and they fill a gap in astronomers’ knowledge of how the universe grows and evolves.

Evidence for IMBHs

In our research, we analyzed 11 black hole merger candidates from LIGO’s third observing run. These candidates were possibly gravitational wave signals that looked promising but still needed more analysis to conclusively confirm.

The data suggested that for those 11 we analyzed, their final post-merger black hole may have been in the lite IMBH range. We found five post-merger black holes that our analysis was 90% confident were lite IMBHs.

Even more critically, we found that one of the events had a parent black hole that was in the mass gap range, and two had parent black holes above the mass gap range. Since we know these black holes can’t come from stars directly, this finding suggests that the universe has some other way of creating black holes this massive.

A parent black hole this massive may already be the product of two other black holes that merged in the past, so observing more IMBHs can help us understand how often black holes are able to “find” each other and merge out in the universe.

LIGO is in the end stages of its fourth observing run. Since this work used data from the third observing run, we are excited to apply our analysis to this new dataset. We expect to continue to search for lite IMBHs, and with this new data we will improve our understanding of how to more confidently “hear” these signals from more massive black holes above all the noise.

Shedding more light on IMBH

We hope this work not only strengthens the case for lite IMBHs in general but helps shed more light on how they are formed.The Conversation

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Bottom line: Intermediate-mass black holes (IMBHs) are black holes with masses between stellar black holes and supermassive black holes. Understanding them could help scientists learn how supermassive black holes form and grow.

Read more: Meet a monster black hole at the dawn of time

The post Meet intermediate black holes: Between stellar and massive first appeared on EarthSky.



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Two intermediate black holes in the middle with swirling material around them expanding outward.
Artist concept of 2 intermediate black holes merging that generate gravitational waves. Astronomers can track gravitational waves to help them locate smaller, stellar black holes. Image via Simulating eXtreme Spacetimes (SXS), CC BY-ND 4.0.
  • Intermediate-mass black holes are black holes with masses between stellar black holes and supermassive black holes.
  • Intermediate black holes are hard to detect and much rarer, making them mysterious to astronomers.
  • Understanding these black holes could help scientists learn how supermassive black holes form and grow.

Meet intermediate black holes, the supermassive black hole’s smaller, much more mysterious cousin

By Bill Smith, Vanderbilt University; Karan Jani, Vanderbilt University, and Krystal Ruiz-Rocha, Vanderbilt University

Black holes are massive, strange and incredibly powerful astronomical objects. Scientists know that supermassive black holes reside in the centers of most galaxies.

And they understand how certain stars form the comparatively smaller stellar mass black holes once they reach the end of their life. Understanding how the smaller stellar mass black holes could form the supermassive black holes helps astronomers learn about how the universe grows and evolves.

But there’s an open question in black hole research: What about black holes with masses in between? These are much harder to find than their stellar and supermassive peers, in size range of a few hundred to a few hundred thousand times the mass of the sun.

We’re a team of astronomers who are searching for these in-between black holes, called intermediate black holes. In a new paper, two of us (Krystal and Karan) teamed up with a group of researchers, including postdoctoral researcher Anjali Yelikar, to look at ripples in space-time to spot a few of these elusive black holes merging.

Take me out to the (gravitational wave) ball game

To gain an intuitive idea of how scientists detect stellar mass black holes, imagine you are at a baseball game where you’re sitting directly behind a big concrete column and can’t see the diamond. Even worse, the crowd is deafeningly loud, so it is also nearly impossible to see or hear the game.

But you’re a scientist, so you take out a high-quality microphone and your computer and write a computer algorithm that can take audio data and separate the crowd’s noise from the “thunk” of a bat hitting a ball.

You start recording, and, with enough practice and updates to your hardware and software, you can begin following the game, getting a sense of when a ball is hit, what direction it goes, when it hits a glove, where runners’ feet pound into the dirt and more.

Admittedly, this is a challenging way to watch a baseball game. But unlike baseball, when observing the universe, sometimes the challenging way is all we have.

This principle of recording sound and using computer algorithms to isolate certain sound waves to determine what they are and where they are coming from is similar to how astronomers like us study gravitational waves. Gravitational waves are ripples in space-time that allow us to observe objects such as black holes.

Now imagine implementing a different sound algorithm, testing it over several innings of the game and finding a particular hit that no legal combination of bats and balls could have produced. Imagine the data was suggesting that the ball was bigger and heavier than a legal baseball could be. If our paper was about a baseball game instead of gravitational waves, that’s what we would have found.

Listening for gravitational waves

While the baseball recording setup is designed specifically to hear the sounds of a baseball game, scientists use a specialized observatory called the Laser Interferometer Gravitational-Wave Observatory, or LIGO, to observe the “sound” of two black holes merging out in the universe.

An L-shaped facility with two long arms extending out from a central building.
The LIGO detector in Hanford, Washington, uses lasers to measure the minuscule stretching of space caused by a gravitational wave. Image via LIGO Laboratory.

Scientists look for the gravitational waves that we can measure using LIGO, which has one of the most mind-bogglingly advanced laser and optics systems ever created.

In each event, two “parent” black holes merge into a single, more massive black hole. Using LIGO data, scientists can figure out where and how far away the merger happened, how massive the parents and resultant black holes are, which direction in the sky the merger happened and other key details.

Most of the parent black holes in merger events originally form from stars that have reached the end of their lives – these are stellar mass black holes.

An illustration of a black hole with gas swirling around it, coming from a large cloud around a star on the right.
This artist’s impression shows a binary system containing a stellar mass black hole called IGR J17091-3624. The strong gravity of the black hole, on the left, is pulling gas away from a companion star on the right. Image via NASA/CXC/M.Weiss, CC BY-NC

The black hole mass gap

Not every dying star can create a stellar mass black hole. The ones that do are usually between about 20 to 100 times the mass of the Sun. But due to complicated nuclear physics, really massive stars explode differently and don’t leave behind any remnant, black hole or otherwise.

These physics create what we refer to as the “mass gap” in black holes. A smaller black hole likely formed from a dying star. But we know that a black hole more massive than about 60 times the size of the Sun, while not a supermassive black hole, is still too big to have formed directly from a dying star.

The exact cutoff for the mass gap is still somewhat uncertain, and many astrophysicists are working on more precise measurements. However, we are confident that the mass gaps exist and that we are in the ballpark of the boundary.

We call black holes in this gap lite intermediate mass black holes or lite IMBHs, because they are the least massive black holes that we expect to exist from sources other than stars. They are no longer considered stellar mass black holes.

Calling them “intermediate” also doesn’t quite capture why they are special. They are special because they are much harder to find, astronomers still aren’t sure what astronomical events might create them, and they fill a gap in astronomers’ knowledge of how the universe grows and evolves.

Evidence for IMBHs

In our research, we analyzed 11 black hole merger candidates from LIGO’s third observing run. These candidates were possibly gravitational wave signals that looked promising but still needed more analysis to conclusively confirm.

The data suggested that for those 11 we analyzed, their final post-merger black hole may have been in the lite IMBH range. We found five post-merger black holes that our analysis was 90% confident were lite IMBHs.

Even more critically, we found that one of the events had a parent black hole that was in the mass gap range, and two had parent black holes above the mass gap range. Since we know these black holes can’t come from stars directly, this finding suggests that the universe has some other way of creating black holes this massive.

A parent black hole this massive may already be the product of two other black holes that merged in the past, so observing more IMBHs can help us understand how often black holes are able to “find” each other and merge out in the universe.

LIGO is in the end stages of its fourth observing run. Since this work used data from the third observing run, we are excited to apply our analysis to this new dataset. We expect to continue to search for lite IMBHs, and with this new data we will improve our understanding of how to more confidently “hear” these signals from more massive black holes above all the noise.

Shedding more light on IMBH

We hope this work not only strengthens the case for lite IMBHs in general but helps shed more light on how they are formed.The Conversation

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Bottom line: Intermediate-mass black holes (IMBHs) are black holes with masses between stellar black holes and supermassive black holes. Understanding them could help scientists learn how supermassive black holes form and grow.

Read more: Meet a monster black hole at the dawn of time

The post Meet intermediate black holes: Between stellar and massive first appeared on EarthSky.



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9 mind-blowing space facts that will shock you

Space facts: Person standing on a large rock, silhouetted against a starry night sky.
Much about our universe is incredible, but here are 9 mind-blowing space facts you might not have known about the cosmos. Image via Igor Cibulsky/ Pexels.

9 mind-blowing space facts that will shock you

When it comes down to it, almost everything about space is amazing. The billion-year lifespans of some stars, the enormousness of our universe, the bizarre behavior of black holes … they can all leave you scratching your head. Here are 9 truly mind-blowing facts about our Earth, sun, solar system and universe that will make you a hit at your next dinner party.

1. There might be dinosaur fossils on the moon

Some 65 million years ago, an asteroid hurtled toward Earth. When it hit, it helped bring about a mass extinction and the end of the dinosaurs. By this time, dinosaurs had already been around for some 200 million years. So, many generations had already died and their bones had become fossilized in earthly rocks. When the dinosaur-killing asteroid hit Earth, it impacted so violently that some of the rocks jettisoned from the impact flew into space. And it’s possible some of those rocks with fossilized dinosaurs might have landed on the moon. Therefore, there could be rocks with dinosaur fossils on the moon.

Source: Astro Alexandra

Space facts: Gigantic splash around huge, cratered asteroid hitting Earth, with pterodactyls flying in the foreground.
Artist’s concept of an asteroid striking Earth during the age of dinosaurs. The impact might have jettisoned dinosaur fossils to the moon. Image via Britannica.com/ NASA/ Don Davis.

2. All the planets could fit between Earth and the moon

The distance between objects in space is vast. As an example of this, if you took all the other planets in the solar system, you could pack them tightly between Earth and the moon. There are a couple of caveats here. First, we are stacking the planets pole to pole so we don’t have to worry about Saturn’s rings. Second, we’re performing this feat during apogee, or when the moon is farthest away from Earth in its elliptical orbit. Lastly, we’re not including Pluto because it’s not a planet, despite what you may have learned as a kid.

Source: Phil Plait for SyFy

Upper left corner is a small Earth, blackness between and small moon at bottom right.
NASA’s OSIRIS-REx mission caught this view of Earth (left) and the moon (right). Now picture Mercury, Venus, Mars, Jupiter, Saturn, Uranus and Neptune wedged between them. Image via NASA.

3. If we could hear the sun, it would be deafening

Sounds waves can’t travel through the vacuum of space. And while it might seem charming to not only see but be able to hear the universe around us, mostly what we’d hear is the sound of the sun screaming. Because – if sound waves could travel through space – we’d hear the sun roaring. That roar would pound our ears at about 100 decibels. That’s like standing next to Niagara Falls all day long. Fortunately, as night falls and we turn away from the sun, we’d get a little bit of peace and quiet.

Source: Astronomy.com

Brownish sun spinning with active regions bubbling.
A view of our active sun from August 6-8. 2025. Read the daily sun news here. Image via NASA/SDO.

4. That roar would linger

And – if you could hear the sun and it suddenly disappeared – the light from it would be gone in 8 minutes but the sound would continue for 13 years. Light traveling from the sun to Earth takes 8 minutes to reach us. But light is more than 850,000 times faster than sound. So if sound could similarly travel through space, what we hear at this moment is really closer to 13 years old. So if the sun winked out, the last rays of light would end in about 8 minutes, but the roaring would continue for 13 years.

Source: World Atlas

5. The dinosaurs didn’t see the same constellations we do

Stars are born, move through space, evolve and die. Some of the stars we see now didn’t exist during the Age of Dinosaurs, from about 252 million to 66 million years ago. So when the dinosaurs looked up at the night sky, they saw different stars and constellations than we see now. Consider the constellation Orion the Hunter. Its bright blue star denoting one knee is Rigel, which is just 8 million years old. And its famous red star Betelgeuse marking Orion’s shoulder is only 10 million years old. The dinosaurs did not see the figure or Orion, nor the Big Dipper, nor the Teapot of Sagittarius. But also, our solar system is orbiting the center of the Milky Way galaxy. And during the height of the dinosaurs, Earth was on the other side of the galaxy than it is now.

Source: Adler Planetarium

6. Galactic collision doesn’t mean stars crash, too

You might have already guessed from mind-blowing fact number two, but there is a lot of space in space. In fact, there is so much space between things in our universe that even though the Milky Way and Andromeda galaxies might collide and merge one day, it’s unlikely that any of its planets or stars will collide.

Source: EarthSky

Night sky with huge, bright oblique swirl of stars - Andromeda galaxy - next to band of Milky Way
This image represents Earth’s night sky in 3.75 billion years. The Andromeda galaxy (left) will fill our field of view as it heads toward a collision with our Milky Way galaxy. Image via NASA/ ESA/ Z. Levay and R. van der Marel, STScI/ T. Hallas/ A. Mellinger.

7. There are countless galaxies packed into every patch of sky

If you’ve ever taken time to gaze at some of the deep-field images from our best telescopes, you already know the universe is absolutely packed with galaxies. From the Hubble Ultra Deep Field to the James Webb Space Telescope’s view of distant galaxies to the new Vera C. Rubin Observatory’s look at our distant universe, galaxies are packed in everywhere we look. Brian Greene is a theoretical physicist at Columbia University and author of Until the End of Time. He said:

Hold your thumb at arm’s length against the night sky, and it will cover more than 10 million galaxies in the observable universe.

Source: Brain Greene

Thousands of galaxies of all shapes, with 2 bluish spirals the largest.
Here’s a small section of NSF-DOE Vera C. Rubin Observatory’s total view of the Virgo cluster of galaxies. Visible are 2 prominent spiral galaxies (lower right), 3 merging galaxies (upper right), several groups of distant galaxies, many stars in the Milky Way galaxy and more. Image via NSF-DOE Vera C. Rubin Observatory.

8. The observable universe is wider than light has had time to travel

So what is the observable universe? It’s all the light we can see in the universe. And although light is speedy, it still has its limits. We can only see the light that has had time to travel to Earth since the beginning of the universe. So while the universe might be infinite, our view of it is not. Our view of the universe stretches in every direction around us for about 46.5 billion light-years. Therefore, the total width of the observable universe from one side of us to the other is 93 billion light-years wide. But we measure our universe at nearly 14 billion years old, starting with the Big Bang. So how is the observable universe wider than its age would suggest? It’s because the universe is expanding. So while light from the farthest observed objects has traveled for 13.8 billion years, the space they are in has also expanded, resulting in a much larger observable universe.

Source: Astronomy.com

9. Most of the universe will move beyond our sight

If we look far, far into the future, eventually the view we have from the Milky Way galaxy will become limited by the expanding universe. Astronomers call the boundary of our observable universe the cosmic event horizon. And because of the finite speed of light travel, we can never see beyond it. So, eventually, as the space between objects in the universe expands, everything that is not gravitationally bound to us will be beyond our sight. And, in fact, the expansion of the universe has been speeding up for about the last 5 billion years. As Katie Mack explains in her book The End of Everything:

As the expansion of the universe accelerates, galaxies that are currently inside our Hubble radius [14 billion light-years away] will be outside it. Eventually, no galaxies outside our Local Group will be visible.

Source: Katie Mack

So distant galaxies will eventually become lost to us. That means we better learn to love our neighbors.

Bottom line: Read nine mind-blowing space facts that will surprise and delight you. You’ll be a hit at your next dinner party!

Read our daily sun news

New map of Andromeda galaxy and its colossal ecosystem

The post 9 mind-blowing space facts that will shock you first appeared on EarthSky.



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Space facts: Person standing on a large rock, silhouetted against a starry night sky.
Much about our universe is incredible, but here are 9 mind-blowing space facts you might not have known about the cosmos. Image via Igor Cibulsky/ Pexels.

9 mind-blowing space facts that will shock you

When it comes down to it, almost everything about space is amazing. The billion-year lifespans of some stars, the enormousness of our universe, the bizarre behavior of black holes … they can all leave you scratching your head. Here are 9 truly mind-blowing facts about our Earth, sun, solar system and universe that will make you a hit at your next dinner party.

1. There might be dinosaur fossils on the moon

Some 65 million years ago, an asteroid hurtled toward Earth. When it hit, it helped bring about a mass extinction and the end of the dinosaurs. By this time, dinosaurs had already been around for some 200 million years. So, many generations had already died and their bones had become fossilized in earthly rocks. When the dinosaur-killing asteroid hit Earth, it impacted so violently that some of the rocks jettisoned from the impact flew into space. And it’s possible some of those rocks with fossilized dinosaurs might have landed on the moon. Therefore, there could be rocks with dinosaur fossils on the moon.

Source: Astro Alexandra

Space facts: Gigantic splash around huge, cratered asteroid hitting Earth, with pterodactyls flying in the foreground.
Artist’s concept of an asteroid striking Earth during the age of dinosaurs. The impact might have jettisoned dinosaur fossils to the moon. Image via Britannica.com/ NASA/ Don Davis.

2. All the planets could fit between Earth and the moon

The distance between objects in space is vast. As an example of this, if you took all the other planets in the solar system, you could pack them tightly between Earth and the moon. There are a couple of caveats here. First, we are stacking the planets pole to pole so we don’t have to worry about Saturn’s rings. Second, we’re performing this feat during apogee, or when the moon is farthest away from Earth in its elliptical orbit. Lastly, we’re not including Pluto because it’s not a planet, despite what you may have learned as a kid.

Source: Phil Plait for SyFy

Upper left corner is a small Earth, blackness between and small moon at bottom right.
NASA’s OSIRIS-REx mission caught this view of Earth (left) and the moon (right). Now picture Mercury, Venus, Mars, Jupiter, Saturn, Uranus and Neptune wedged between them. Image via NASA.

3. If we could hear the sun, it would be deafening

Sounds waves can’t travel through the vacuum of space. And while it might seem charming to not only see but be able to hear the universe around us, mostly what we’d hear is the sound of the sun screaming. Because – if sound waves could travel through space – we’d hear the sun roaring. That roar would pound our ears at about 100 decibels. That’s like standing next to Niagara Falls all day long. Fortunately, as night falls and we turn away from the sun, we’d get a little bit of peace and quiet.

Source: Astronomy.com

Brownish sun spinning with active regions bubbling.
A view of our active sun from August 6-8. 2025. Read the daily sun news here. Image via NASA/SDO.

4. That roar would linger

And – if you could hear the sun and it suddenly disappeared – the light from it would be gone in 8 minutes but the sound would continue for 13 years. Light traveling from the sun to Earth takes 8 minutes to reach us. But light is more than 850,000 times faster than sound. So if sound could similarly travel through space, what we hear at this moment is really closer to 13 years old. So if the sun winked out, the last rays of light would end in about 8 minutes, but the roaring would continue for 13 years.

Source: World Atlas

5. The dinosaurs didn’t see the same constellations we do

Stars are born, move through space, evolve and die. Some of the stars we see now didn’t exist during the Age of Dinosaurs, from about 252 million to 66 million years ago. So when the dinosaurs looked up at the night sky, they saw different stars and constellations than we see now. Consider the constellation Orion the Hunter. Its bright blue star denoting one knee is Rigel, which is just 8 million years old. And its famous red star Betelgeuse marking Orion’s shoulder is only 10 million years old. The dinosaurs did not see the figure or Orion, nor the Big Dipper, nor the Teapot of Sagittarius. But also, our solar system is orbiting the center of the Milky Way galaxy. And during the height of the dinosaurs, Earth was on the other side of the galaxy than it is now.

Source: Adler Planetarium

6. Galactic collision doesn’t mean stars crash, too

You might have already guessed from mind-blowing fact number two, but there is a lot of space in space. In fact, there is so much space between things in our universe that even though the Milky Way and Andromeda galaxies might collide and merge one day, it’s unlikely that any of its planets or stars will collide.

Source: EarthSky

Night sky with huge, bright oblique swirl of stars - Andromeda galaxy - next to band of Milky Way
This image represents Earth’s night sky in 3.75 billion years. The Andromeda galaxy (left) will fill our field of view as it heads toward a collision with our Milky Way galaxy. Image via NASA/ ESA/ Z. Levay and R. van der Marel, STScI/ T. Hallas/ A. Mellinger.

7. There are countless galaxies packed into every patch of sky

If you’ve ever taken time to gaze at some of the deep-field images from our best telescopes, you already know the universe is absolutely packed with galaxies. From the Hubble Ultra Deep Field to the James Webb Space Telescope’s view of distant galaxies to the new Vera C. Rubin Observatory’s look at our distant universe, galaxies are packed in everywhere we look. Brian Greene is a theoretical physicist at Columbia University and author of Until the End of Time. He said:

Hold your thumb at arm’s length against the night sky, and it will cover more than 10 million galaxies in the observable universe.

Source: Brain Greene

Thousands of galaxies of all shapes, with 2 bluish spirals the largest.
Here’s a small section of NSF-DOE Vera C. Rubin Observatory’s total view of the Virgo cluster of galaxies. Visible are 2 prominent spiral galaxies (lower right), 3 merging galaxies (upper right), several groups of distant galaxies, many stars in the Milky Way galaxy and more. Image via NSF-DOE Vera C. Rubin Observatory.

8. The observable universe is wider than light has had time to travel

So what is the observable universe? It’s all the light we can see in the universe. And although light is speedy, it still has its limits. We can only see the light that has had time to travel to Earth since the beginning of the universe. So while the universe might be infinite, our view of it is not. Our view of the universe stretches in every direction around us for about 46.5 billion light-years. Therefore, the total width of the observable universe from one side of us to the other is 93 billion light-years wide. But we measure our universe at nearly 14 billion years old, starting with the Big Bang. So how is the observable universe wider than its age would suggest? It’s because the universe is expanding. So while light from the farthest observed objects has traveled for 13.8 billion years, the space they are in has also expanded, resulting in a much larger observable universe.

Source: Astronomy.com

9. Most of the universe will move beyond our sight

If we look far, far into the future, eventually the view we have from the Milky Way galaxy will become limited by the expanding universe. Astronomers call the boundary of our observable universe the cosmic event horizon. And because of the finite speed of light travel, we can never see beyond it. So, eventually, as the space between objects in the universe expands, everything that is not gravitationally bound to us will be beyond our sight. And, in fact, the expansion of the universe has been speeding up for about the last 5 billion years. As Katie Mack explains in her book The End of Everything:

As the expansion of the universe accelerates, galaxies that are currently inside our Hubble radius [14 billion light-years away] will be outside it. Eventually, no galaxies outside our Local Group will be visible.

Source: Katie Mack

So distant galaxies will eventually become lost to us. That means we better learn to love our neighbors.

Bottom line: Read nine mind-blowing space facts that will surprise and delight you. You’ll be a hit at your next dinner party!

Read our daily sun news

New map of Andromeda galaxy and its colossal ecosystem

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