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Spica, the bright beacon of Virgo, is 2 stars

Brilliant blue-white star Spica with 4 rays against star field.
Even though our eyes see the star Spica as 1 star, it’s really at least 2. And we see it as distinctly blue-white. Photo by Fred Espenak at AstroPixels. Used with permission.

Spica is a close double star

The star Spica – aka Alpha Virginis – is the brightest star in the constellation Virgo the Maiden. From a distance of about 250 light-years, Spica appears to us on Earth as a lone bluish-white star in a quiet region of the sky. But Spica consists of two stars and maybe more. Both stars are larger and hotter than our sun. And they’re separated by only 11 million miles (less than 18 million km), in contrast to Earth’s distance from our sun of 93 million miles (150 million km). They orbit their common center of gravity in only four days.

We say that Earth is 1 astronomical unit (aka 1 AU) from our sun. Spica’s two stars are only .12 AU from each other, a small fraction of the Earth-sun distance.

And the two stars in the Spica system are individually indistinguishable from a single point of light, even with a telescope. Only the analysis of its light with a spectroscope – an instrument that splits light into its component colors – revealed the dual nature of this star.

Hot, hot, hot

Spica’s two stars are so close, and they orbit so quickly around each other, that their mutual gravity distorts each star into an egg shape. It’s thought that the pointed ends of these egg-shaped stars face each other as they whirl around.

The pair of stars are both dwarfs, brightening near the end of their lifetimes.

Spica is one of the hottest 1st-magnitude stars. The hottest of the pair is 22,400 Kelvin (about 40,000 F or 22,000 C). That’s blistering in contrast to the sun’s 5,800 Kelvin (about 10,000 F or 5,500 C). This star might someday explode as a supernova.

The light from Spica’s two stars, taken together, is on average more than 12,100 times brighter than our sun’s light. Their estimated diameters are 7.8 and 4 times our sun’s diameter.

Spica is one of several bright stars that the moon can occult (eclipse). Furthermore, based on observations of how the star’s light is extinguished when the moon passes in front, some astronomers think that it may not just be a spectroscopic binary star. Instead, they feel that there may be as many as three other stars in the system. In that case, Spica would not be a single or even a double star, but a quintuple star!

How to find Spica

The best evening views of Spica come from northern spring to late northern summer, when this star arcs across the southern sky in the evening. So in the month of May, as seen from the Northern Hemisphere, you’ll find Spica in the southeast in early evening. Then, from the Southern Hemisphere, Spica is closer to due east. From all of Earth in May, as night passes, Spica appears to move westward. Spica rises earlier each evening so that – by the end of August – Spica can be viewed only briefly in the west to west-southwest sky as darkness falls.

At least there’s a foolproof way to find Spica, using the Big Dipper as a guide. Scouts and stargazers remember this trick with the saying: Follow the arc to Arcturus, and speed on (or drive a spike) to Spica.

Look for the Big Dipper

First, look for the Big Dipper in the northern sky. It’s highest in the evening sky in the northern spring and summer. Notice that the Big Dipper has a bowl and a long, curved handle. Follow the arc of the Dipper’s handle outward, away from the Dipper’s bowl. The first bright star you come to is orange Arcturus. Then drive a spike (or speed on) along this curving path. And the next bright star you come to is Spica.

Spica shines at magnitude 1.04, making it the brightest light in Virgo. In fact, it’s the 15th-brightest star visible from anywhere on Earth. It’s virtually the same brightness as Antares in the constellation Scorpius, so sometimes Antares is listed as the 15th and Spica as the 16th brightest.

Kite shaped constellation with a tail pointing to a dot labeled Arcturus and then to another dot labeled Spica.
In northern spring, look northeast to southeast in the evening. You’ll find the Big Dipper in the northeast evening sky. Then, follow the arc to Arcturus, and drive a spike (speed on) to Spica.
Star chart showing Big Dipper with line to Arcturus continuing to Spica.
In northern summer, look northwest to southwest. You’ll find the Big Dipper in the northwest evening sky. But you can still follow the arc to Arcturus, and drive a spike (speed on) to Spica.

History and mythology of Spica

The name Spica is from the Latin word for “ear” (of grain). The general connotation is that Spica refers to an “ear of wheat.” Indeed, the star and the constellation Virgo itself were sometimes associated with the Greek goddess of the harvest, Demeter.

There are many names and stories for Spica’s constellation – Virgo – in mythology, and by association with Spica as well. Fewer stories refer to Spica independently. Many classical references refer to Virgo’s stars as a goddess or with some association with wheat or the harvest, since the sun passes through Virgo in the fall. In Greece and Rome she typically was Astraea, the very personification of Justice; or Persephone, daughter of Demeter. In Egypt, Virgo was identified with Isis, and Spica was considered her lute bearer. In ancient China, Spica was a special star of spring known as the Horn.

One Arabic name was Azimech, derived from words meaning Defenseless One or Solitary One. This title may be in reference to Spica’s solitary status with no other bright stars nearby. But Spica is not the most solitary star. That honor goes to Fomalhaut, sometimes called the Autumn Star.

Spica’s position is RA: 13h 25m 12s, dec: -11° 09′ 41″

Antique colored etching of winged young woman in long dress holding a wheat ear, with labeled scattered stars.
Here’s a classical illustration of the constellation Virgo the Maiden, with Spica embedded in the wheat in her left hand. Image via Urania’s Mirror/ Wikipedia.

Bottom line: Spica is the brightest star in Virgo. Spica is at least two stars orbiting extremely close together, distorting each other into egg shapes.

Virgo the Maiden represents a harvest goddess

The post Spica, the bright beacon of Virgo, is 2 stars first appeared on EarthSky.



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Brilliant blue-white star Spica with 4 rays against star field.
Even though our eyes see the star Spica as 1 star, it’s really at least 2. And we see it as distinctly blue-white. Photo by Fred Espenak at AstroPixels. Used with permission.

Spica is a close double star

The star Spica – aka Alpha Virginis – is the brightest star in the constellation Virgo the Maiden. From a distance of about 250 light-years, Spica appears to us on Earth as a lone bluish-white star in a quiet region of the sky. But Spica consists of two stars and maybe more. Both stars are larger and hotter than our sun. And they’re separated by only 11 million miles (less than 18 million km), in contrast to Earth’s distance from our sun of 93 million miles (150 million km). They orbit their common center of gravity in only four days.

We say that Earth is 1 astronomical unit (aka 1 AU) from our sun. Spica’s two stars are only .12 AU from each other, a small fraction of the Earth-sun distance.

And the two stars in the Spica system are individually indistinguishable from a single point of light, even with a telescope. Only the analysis of its light with a spectroscope – an instrument that splits light into its component colors – revealed the dual nature of this star.

Hot, hot, hot

Spica’s two stars are so close, and they orbit so quickly around each other, that their mutual gravity distorts each star into an egg shape. It’s thought that the pointed ends of these egg-shaped stars face each other as they whirl around.

The pair of stars are both dwarfs, brightening near the end of their lifetimes.

Spica is one of the hottest 1st-magnitude stars. The hottest of the pair is 22,400 Kelvin (about 40,000 F or 22,000 C). That’s blistering in contrast to the sun’s 5,800 Kelvin (about 10,000 F or 5,500 C). This star might someday explode as a supernova.

The light from Spica’s two stars, taken together, is on average more than 12,100 times brighter than our sun’s light. Their estimated diameters are 7.8 and 4 times our sun’s diameter.

Spica is one of several bright stars that the moon can occult (eclipse). Furthermore, based on observations of how the star’s light is extinguished when the moon passes in front, some astronomers think that it may not just be a spectroscopic binary star. Instead, they feel that there may be as many as three other stars in the system. In that case, Spica would not be a single or even a double star, but a quintuple star!

How to find Spica

The best evening views of Spica come from northern spring to late northern summer, when this star arcs across the southern sky in the evening. So in the month of May, as seen from the Northern Hemisphere, you’ll find Spica in the southeast in early evening. Then, from the Southern Hemisphere, Spica is closer to due east. From all of Earth in May, as night passes, Spica appears to move westward. Spica rises earlier each evening so that – by the end of August – Spica can be viewed only briefly in the west to west-southwest sky as darkness falls.

At least there’s a foolproof way to find Spica, using the Big Dipper as a guide. Scouts and stargazers remember this trick with the saying: Follow the arc to Arcturus, and speed on (or drive a spike) to Spica.

Look for the Big Dipper

First, look for the Big Dipper in the northern sky. It’s highest in the evening sky in the northern spring and summer. Notice that the Big Dipper has a bowl and a long, curved handle. Follow the arc of the Dipper’s handle outward, away from the Dipper’s bowl. The first bright star you come to is orange Arcturus. Then drive a spike (or speed on) along this curving path. And the next bright star you come to is Spica.

Spica shines at magnitude 1.04, making it the brightest light in Virgo. In fact, it’s the 15th-brightest star visible from anywhere on Earth. It’s virtually the same brightness as Antares in the constellation Scorpius, so sometimes Antares is listed as the 15th and Spica as the 16th brightest.

Kite shaped constellation with a tail pointing to a dot labeled Arcturus and then to another dot labeled Spica.
In northern spring, look northeast to southeast in the evening. You’ll find the Big Dipper in the northeast evening sky. Then, follow the arc to Arcturus, and drive a spike (speed on) to Spica.
Star chart showing Big Dipper with line to Arcturus continuing to Spica.
In northern summer, look northwest to southwest. You’ll find the Big Dipper in the northwest evening sky. But you can still follow the arc to Arcturus, and drive a spike (speed on) to Spica.

History and mythology of Spica

The name Spica is from the Latin word for “ear” (of grain). The general connotation is that Spica refers to an “ear of wheat.” Indeed, the star and the constellation Virgo itself were sometimes associated with the Greek goddess of the harvest, Demeter.

There are many names and stories for Spica’s constellation – Virgo – in mythology, and by association with Spica as well. Fewer stories refer to Spica independently. Many classical references refer to Virgo’s stars as a goddess or with some association with wheat or the harvest, since the sun passes through Virgo in the fall. In Greece and Rome she typically was Astraea, the very personification of Justice; or Persephone, daughter of Demeter. In Egypt, Virgo was identified with Isis, and Spica was considered her lute bearer. In ancient China, Spica was a special star of spring known as the Horn.

One Arabic name was Azimech, derived from words meaning Defenseless One or Solitary One. This title may be in reference to Spica’s solitary status with no other bright stars nearby. But Spica is not the most solitary star. That honor goes to Fomalhaut, sometimes called the Autumn Star.

Spica’s position is RA: 13h 25m 12s, dec: -11° 09′ 41″

Antique colored etching of winged young woman in long dress holding a wheat ear, with labeled scattered stars.
Here’s a classical illustration of the constellation Virgo the Maiden, with Spica embedded in the wheat in her left hand. Image via Urania’s Mirror/ Wikipedia.

Bottom line: Spica is the brightest star in Virgo. Spica is at least two stars orbiting extremely close together, distorting each other into egg shapes.

Virgo the Maiden represents a harvest goddess

The post Spica, the bright beacon of Virgo, is 2 stars first appeared on EarthSky.



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Crepuscular rays are sunbeams in twilight skies

Sunset view with dark rays cut into the orange glow and over a lake.
View at EarthSky Community Photos. | Juliana Karoway at Lake Quinsigamond, Shrewsbury, Massachusetts, captured this image on May 14, 2024. Juliana wrote: “Can you please tell me something about these clouds? I’ve never seen a sunset like this before!” Gladly, Juliana, and thanks for sharing! These are crepuscular rays, sunbeams you can see in twilight skies thanks to small particles in the air. Read on to find out more about them.

What are crepuscular rays?

Crepuscular means resembling twilight or dim. This phenomenon occurs around sunrise or sunset, when the sun is below the horizon. And you can also see crepuscular rays when the sun is hiding behind clouds. They’re more noticeable when the sky is a bit darker and there is greater contrast between dark and light. We can see the rays of light thanks to dust, smoke or water droplets that scatter the light toward our eyes.

The darker streaks beside the sunbeams are due to shadows, where the terrain or clouds block the sunlight from coming through. Sometimes those obstructions are below the horizon from your point of view, so it may not seem immediately clear what’s causing the darker rays.

When crepuscular rays extend from behind a cloud toward the ground, they also go by the nickname Jacob’s Ladder. The term comes from a story in the Bible where Jacob has a dream in which he sees a ladder leading up to the golden light of heaven with angels ascending and descending.

Parallel lines that seem to converge

Crepuscular rays appear to fan across the sky. But these sunbeams are really parallel to each other. In fact, sometimes you can trace them all the way across the sky to the point on the horizon opposite the sunset. So, the next time you see them, remember to turn around. You might spot the fainter and less noticeable anticrepuscular rays. The illusion is similar to standing on train tracks and seeing how they appear to converge in the far distance in front of and behind you.

Left: orange sunrise, blue streaks coming out from a point on the horizon. Right: similar streaks in darker sky.
View at EarthSky Community Photos. | Ron Haggett in Yuma, Arizona, captured crepuscular rays (left) and anticrepuscular rays (right) on the morning of September 1, 2021. He wrote: “These photos were taken 9 minutes apart (6:00 and 6:09 a.m., local time). The image on the left is looking east before sunrise. Sunbeams can also extend across the sky and appear to converge at the antisolar point, the point on the celestial sphere opposite the sun’s direction. In this case, they’re called antisolar rays. The image on the right is at the antisolar point (due west).” Thank you, Ron!
Crepuscular rays: Arc of pink clouds and dark rays reaching from east to west horizon in long, flat picture.
View at EarthSky Community Photos. | Brendan Barnes captured crepuscular rays running all the way across the sky in this panoramic photo taken in Guam on October 28, 2020. He wrote: “I woke up this morning to bright pink clouds outside my window, so I ran upstairs to the roof and found crepuscular rays going the entire way from the rising sun toward the horizon to the west!” Thank you, Brendan!

Photo gallery of crepuscular rays

All of these photos were contributed by EarthSky friends. Thanks for sharing your awesome photos with us! Would you like to contribute? Submit your image here.

Clouds over water with 4 dark radial rays from horizon to zenith. All reflected in the water.
View at Earthsky Community Photos. | Guy Newlan in Orlando, Florida, captured this image on August 19, 2023. He wrote: “A cirrocumulus layer was an excellent screen for pre-sunrise crepuscular rays.” Thanks, Guy!
Lights of a small village at bottom, a distant mountain, and blue and pink radial streaks of light above.
View at EarthSky Community Photos. | Jenney Disimon captured these crepuscular rays in Sabah, North Borneo, Malaysia, on April 19, 2023. Jenney wrote: “On waking up, this was what I first saw. Crepuscular rays as the background of the iconic Mt. Kinabalu at dawn. And somewhere hidden was the old crescent moon. What an awesome sight!” Thank you!
Blue-grey sky with vast orange light rays coming from the bottom left. Two tiny dots white dots in the sky.
View at EarthSky Community Photos. | Helio C. Vital in Rio de Janeiro, Brazil, took this photo on March 1, 2023. Helio wrote: “The photo shows Jupiter and Venus only 35 arcminutes apart in the midst of bright crepuscular rays. Thank you!

Moon rays or moonbeams

Bright, small moon under clouds, reflected in a lake. Dark rays show across the moonlit clouds.
James Younger frequently camps at Vancouver Island and catches many wonderful sky sights from its shores. He captured these moon rays (in the clouds above) in August 2017.

Bottom line: Crepuscular rays are shadows in the sky of distant terrain or clouds. They form around twilight when particles in the atmosphere reflect the sun’s light beams toward our eyes. Sometimes you can see anticrepuscular rays on the horizon opposite the sun.

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

The post Crepuscular rays are sunbeams in twilight skies first appeared on EarthSky.



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Sunset view with dark rays cut into the orange glow and over a lake.
View at EarthSky Community Photos. | Juliana Karoway at Lake Quinsigamond, Shrewsbury, Massachusetts, captured this image on May 14, 2024. Juliana wrote: “Can you please tell me something about these clouds? I’ve never seen a sunset like this before!” Gladly, Juliana, and thanks for sharing! These are crepuscular rays, sunbeams you can see in twilight skies thanks to small particles in the air. Read on to find out more about them.

What are crepuscular rays?

Crepuscular means resembling twilight or dim. This phenomenon occurs around sunrise or sunset, when the sun is below the horizon. And you can also see crepuscular rays when the sun is hiding behind clouds. They’re more noticeable when the sky is a bit darker and there is greater contrast between dark and light. We can see the rays of light thanks to dust, smoke or water droplets that scatter the light toward our eyes.

The darker streaks beside the sunbeams are due to shadows, where the terrain or clouds block the sunlight from coming through. Sometimes those obstructions are below the horizon from your point of view, so it may not seem immediately clear what’s causing the darker rays.

When crepuscular rays extend from behind a cloud toward the ground, they also go by the nickname Jacob’s Ladder. The term comes from a story in the Bible where Jacob has a dream in which he sees a ladder leading up to the golden light of heaven with angels ascending and descending.

Parallel lines that seem to converge

Crepuscular rays appear to fan across the sky. But these sunbeams are really parallel to each other. In fact, sometimes you can trace them all the way across the sky to the point on the horizon opposite the sunset. So, the next time you see them, remember to turn around. You might spot the fainter and less noticeable anticrepuscular rays. The illusion is similar to standing on train tracks and seeing how they appear to converge in the far distance in front of and behind you.

Left: orange sunrise, blue streaks coming out from a point on the horizon. Right: similar streaks in darker sky.
View at EarthSky Community Photos. | Ron Haggett in Yuma, Arizona, captured crepuscular rays (left) and anticrepuscular rays (right) on the morning of September 1, 2021. He wrote: “These photos were taken 9 minutes apart (6:00 and 6:09 a.m., local time). The image on the left is looking east before sunrise. Sunbeams can also extend across the sky and appear to converge at the antisolar point, the point on the celestial sphere opposite the sun’s direction. In this case, they’re called antisolar rays. The image on the right is at the antisolar point (due west).” Thank you, Ron!
Crepuscular rays: Arc of pink clouds and dark rays reaching from east to west horizon in long, flat picture.
View at EarthSky Community Photos. | Brendan Barnes captured crepuscular rays running all the way across the sky in this panoramic photo taken in Guam on October 28, 2020. He wrote: “I woke up this morning to bright pink clouds outside my window, so I ran upstairs to the roof and found crepuscular rays going the entire way from the rising sun toward the horizon to the west!” Thank you, Brendan!

Photo gallery of crepuscular rays

All of these photos were contributed by EarthSky friends. Thanks for sharing your awesome photos with us! Would you like to contribute? Submit your image here.

Clouds over water with 4 dark radial rays from horizon to zenith. All reflected in the water.
View at Earthsky Community Photos. | Guy Newlan in Orlando, Florida, captured this image on August 19, 2023. He wrote: “A cirrocumulus layer was an excellent screen for pre-sunrise crepuscular rays.” Thanks, Guy!
Lights of a small village at bottom, a distant mountain, and blue and pink radial streaks of light above.
View at EarthSky Community Photos. | Jenney Disimon captured these crepuscular rays in Sabah, North Borneo, Malaysia, on April 19, 2023. Jenney wrote: “On waking up, this was what I first saw. Crepuscular rays as the background of the iconic Mt. Kinabalu at dawn. And somewhere hidden was the old crescent moon. What an awesome sight!” Thank you!
Blue-grey sky with vast orange light rays coming from the bottom left. Two tiny dots white dots in the sky.
View at EarthSky Community Photos. | Helio C. Vital in Rio de Janeiro, Brazil, took this photo on March 1, 2023. Helio wrote: “The photo shows Jupiter and Venus only 35 arcminutes apart in the midst of bright crepuscular rays. Thank you!

Moon rays or moonbeams

Bright, small moon under clouds, reflected in a lake. Dark rays show across the moonlit clouds.
James Younger frequently camps at Vancouver Island and catches many wonderful sky sights from its shores. He captured these moon rays (in the clouds above) in August 2017.

Bottom line: Crepuscular rays are shadows in the sky of distant terrain or clouds. They form around twilight when particles in the atmosphere reflect the sun’s light beams toward our eyes. Sometimes you can see anticrepuscular rays on the horizon opposite the sun.

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

The post Crepuscular rays are sunbeams in twilight skies first appeared on EarthSky.



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Giant hummingbirds with backpacks help discover a species

Researchers from UNM’s Museum of Southwestern Biology (MSB) in Albuquerque, New Mexico, wanted to know what happens with giant hummingbirds during winter. These birds breed along the Pacific Coast of central Chile, but after that, they just disappear.

Thanks to a tiny backpack adapted for these birds, the team was able to follow them until they were super high in the Andes! And not only that, this study led them to the discovery of a new species of hummingbird that inhabits the Andes. You can read the full study, published on May 13, 2024, at the National Library of Medicine.

Giant hummingbirds, tiny backpacks

Giant hummingbirds: 2 hands holding a green bird with a long and thin beak. It has a little, blue backpack on its back.
Here’s a giant hummingbird with a geo-locator backpack, in the Valparaíso region of Chile. These giant hummingbirds helped discover a new species. Image via Chris Witt/ University of New Mexico/ Museum of Southwestern Biology.

The group of researchers found some great assistants for their eight-year-long study. These assistants have feathers, are colorful, move really fast and are tougher than some might think. They are giant hummingbirds!

The team, led by ornithologist Jessie Williamson, wanted to study the migratory habits of giant hummingbirds, as they breed along the Pacific coasts of central Chile and seemingly vanish after breeding. The last clue they had came from Charles Darwin, who in the 19th century speculated they migrated to the Atacama Desert region of northern Chile.

But, how to track them? The team decided to create tiny backpacks that would fit them. Even though giant hummingbirds are the largest kind of hummingbird, they are still only up to 10 inches (25 cm) long. So, their backpacks had to be small and light enough that they wouldn’t interfere with the birds’ hovering style of flight. Williamson wrote:

It took a lot of trial and error to come up with a suitable harness design. Hummingbirds are challenging to work with because they are lightweight with long wings and short legs. They’re nature’s tiny acrobats.

A long flight to the Andes

The team discovered that migratory giant hummingbirds can ascend over 13,000 feet (4 km) in elevation to the high Andes. If you know about the Andes flight disaster that occurred at the Andes in 1972, you know that this environment is extremely rough. This is why hummingbirds employ the same acclimatization strategy used by professional mountaineers. They don’t fly straight up to high altitudes; they pause their upward climb for periods of days to allow their blood and lungs to acclimatize.

These birds can fly as far north as the mountains of Peru. The roundtrip journey covers more than 5,200 miles (8,370 km). As comparison, that’s the distance between New York City and Buenos Aires in Argentina. It’s one of the longest, if not the longest hummingbird migration in the world.

Map of South America. Most of the map looks green, but there is a brown, long, thin line along the left side.
Map of the Andes, the longest continental mountain range in the world. The Andes extend from north to south through 7 South American countries: Venezuela, Colombia, Ecuador, Peru, Bolivia, Chile and Argentina. Image via Carlos A Arango / Wikipedia (public domain).

Finding of a new species

At first, the research goal was simply to learn where the migratory population went. But it also led to a fascinating discovery:

It turns out that in the Andes there are not one, but two groups of giant hummingbirds. The northern population stays in the high Andes year-round, while the southern population migrates from sea level up to 13,000 feet (4,000 m) during the non-breeding months. The two species overlap their stays at the high elevation wintering grounds.

Christopher Witt, Professor and Director of the Museum of Southwestern Biology, wrote:

Nobody had figured out where migratory giant hummingbirds go because they were hiding among the non-migratory giant hummingbirds. The two forms of giant hummingbird look almost identical. For centuries, ornithologists and birders never noticed that they were different. We couldn’t have figured this out without the miniaturized trackers.

2 species of giant hummingbird

After the discovery, the team did further research to learn more about how different these species are, and to understand how they evolved until they became two different species. Co-author Ethan Gyllenhaal wrote:

Natural history collections were absolutely essential to this work. Including DNA from 154-year-old type specimens was key to solving this evolutionary puzzle.

The authors say the shift in migratory behavior is what drove speciation. It seems that the migratory and high-elevation resident giant hummingbirds had been evolving separately for about 3 million years! The hummingbirds that live in the high Andes year-round are larger and have notably different blood and lungs.

Now, the researchers are proposing names to differentiate these two species … Any cool names come to your mind?

Bottom line: Giant hummingbirds with tiny backpacks helped discover a new species of hummingbird, as they were tracked up high in the Andes.

Sources: How miniature backpacks led to the discovery of the world’s largest hummingbird species

Via National Library of Medicine: Extreme elevational migration spurred cryptic speciation in giant hummingbirds

Read more: Hummingbirds, tiny and colorful: Lifeform of the week

The post Giant hummingbirds with backpacks help discover a species first appeared on EarthSky.



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Researchers from UNM’s Museum of Southwestern Biology (MSB) in Albuquerque, New Mexico, wanted to know what happens with giant hummingbirds during winter. These birds breed along the Pacific Coast of central Chile, but after that, they just disappear.

Thanks to a tiny backpack adapted for these birds, the team was able to follow them until they were super high in the Andes! And not only that, this study led them to the discovery of a new species of hummingbird that inhabits the Andes. You can read the full study, published on May 13, 2024, at the National Library of Medicine.

Giant hummingbirds, tiny backpacks

Giant hummingbirds: 2 hands holding a green bird with a long and thin beak. It has a little, blue backpack on its back.
Here’s a giant hummingbird with a geo-locator backpack, in the Valparaíso region of Chile. These giant hummingbirds helped discover a new species. Image via Chris Witt/ University of New Mexico/ Museum of Southwestern Biology.

The group of researchers found some great assistants for their eight-year-long study. These assistants have feathers, are colorful, move really fast and are tougher than some might think. They are giant hummingbirds!

The team, led by ornithologist Jessie Williamson, wanted to study the migratory habits of giant hummingbirds, as they breed along the Pacific coasts of central Chile and seemingly vanish after breeding. The last clue they had came from Charles Darwin, who in the 19th century speculated they migrated to the Atacama Desert region of northern Chile.

But, how to track them? The team decided to create tiny backpacks that would fit them. Even though giant hummingbirds are the largest kind of hummingbird, they are still only up to 10 inches (25 cm) long. So, their backpacks had to be small and light enough that they wouldn’t interfere with the birds’ hovering style of flight. Williamson wrote:

It took a lot of trial and error to come up with a suitable harness design. Hummingbirds are challenging to work with because they are lightweight with long wings and short legs. They’re nature’s tiny acrobats.

A long flight to the Andes

The team discovered that migratory giant hummingbirds can ascend over 13,000 feet (4 km) in elevation to the high Andes. If you know about the Andes flight disaster that occurred at the Andes in 1972, you know that this environment is extremely rough. This is why hummingbirds employ the same acclimatization strategy used by professional mountaineers. They don’t fly straight up to high altitudes; they pause their upward climb for periods of days to allow their blood and lungs to acclimatize.

These birds can fly as far north as the mountains of Peru. The roundtrip journey covers more than 5,200 miles (8,370 km). As comparison, that’s the distance between New York City and Buenos Aires in Argentina. It’s one of the longest, if not the longest hummingbird migration in the world.

Map of South America. Most of the map looks green, but there is a brown, long, thin line along the left side.
Map of the Andes, the longest continental mountain range in the world. The Andes extend from north to south through 7 South American countries: Venezuela, Colombia, Ecuador, Peru, Bolivia, Chile and Argentina. Image via Carlos A Arango / Wikipedia (public domain).

Finding of a new species

At first, the research goal was simply to learn where the migratory population went. But it also led to a fascinating discovery:

It turns out that in the Andes there are not one, but two groups of giant hummingbirds. The northern population stays in the high Andes year-round, while the southern population migrates from sea level up to 13,000 feet (4,000 m) during the non-breeding months. The two species overlap their stays at the high elevation wintering grounds.

Christopher Witt, Professor and Director of the Museum of Southwestern Biology, wrote:

Nobody had figured out where migratory giant hummingbirds go because they were hiding among the non-migratory giant hummingbirds. The two forms of giant hummingbird look almost identical. For centuries, ornithologists and birders never noticed that they were different. We couldn’t have figured this out without the miniaturized trackers.

2 species of giant hummingbird

After the discovery, the team did further research to learn more about how different these species are, and to understand how they evolved until they became two different species. Co-author Ethan Gyllenhaal wrote:

Natural history collections were absolutely essential to this work. Including DNA from 154-year-old type specimens was key to solving this evolutionary puzzle.

The authors say the shift in migratory behavior is what drove speciation. It seems that the migratory and high-elevation resident giant hummingbirds had been evolving separately for about 3 million years! The hummingbirds that live in the high Andes year-round are larger and have notably different blood and lungs.

Now, the researchers are proposing names to differentiate these two species … Any cool names come to your mind?

Bottom line: Giant hummingbirds with tiny backpacks helped discover a new species of hummingbird, as they were tracked up high in the Andes.

Sources: How miniature backpacks led to the discovery of the world’s largest hummingbird species

Via National Library of Medicine: Extreme elevational migration spurred cryptic speciation in giant hummingbirds

Read more: Hummingbirds, tiny and colorful: Lifeform of the week

The post Giant hummingbirds with backpacks help discover a species first appeared on EarthSky.



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The Northern Crown is a beautiful star pattern in May

Northern Crown: Six bright stars in bowl shape against a starry sky, Alphecca noticeably brighter.
Corona Borealis, the Northern Crown, with its brightest star Alphecca. In fact, this time of the year is perfect to see this semicircle of stars in the evening sky. Image via Fred Espenak/ AstroPixels. Used with permission.

The Northern Crown graces the summer skies

Tonight, look for a constellation that’s easy to see on the sky’s dome, if your sky is dark enough. Corona Borealis – aka the Northern Crown – is exciting to find. In fact, it’s easy to pick out as an almost-perfect semicircle of stars. You’ll find this beautiful star pattern in the evening sky from now until October.

Plus, the constellation Corona Borealis is easy to find since it’s located more or less along a line between two bright stars. The first is Arcturus in the constellation Boötes the Herdsman and the second is Vega in the constellation Lyra the Harp.

Star chart showing stars Vega and Arcturus in corners and small semicircle of stars between them, all labeled.
After nightfall and in the early evening, you’ll see Arcturus fairly high in the east, noticeable for its brightness and yellow-orange color. Next, look for Vega rather low in the northeast. It’s a bright blue-white star. Then look for the Northern Crown between these 2 bright stars. It’s a bit closer to Arcturus.

However, you’ll need a fairly dark sky to clearly see Corona Borealis between Vega and Arcturus. Then, once you find the semicircle of stars, it’s very noticeable.

The brightest star of the Northern Crown

The brightest star in Corona Borealis is Alphecca, also known as Gemma, sometimes called the Pearl of the Crown. The name Alphecca originated with a description of Corona Borealis as the “broken one.” This was in reference to the fact that these stars appear in a semicircle, rather than a full circle. Alphecca is a blue-white star, with an intrinsic luminosity some 60 times that of our sun. It’s located about 75 light-years from Earth.

Grid with dots and lines showing star patterns.
The C-shaped – or semicircle – constellation Corona Borealis shines between the constellations Boötes and Hercules. Image via IAU. Used with permission.

Watch for a ‘new star’ in the Northern Crown

T Coronae Borealis, or T CrB, is located 3,000 light-years away from Earth. It is a recurring nova with outbursts about every 80 years. Its last outburst was in 1946, and astronomers believe another will occur between February and September 2024.

The star system, normally of magnitude +10, is far too dim to see with the unaided eye. When the nova occurs, it will jump to around magnitude +2. That is roughly the same brightness to the North Star, Polaris.

Once its brightness peaks, it should be visible to the unaided eye for several days and just over a week with binoculars before it dims again, possibly for another 80 years.

Star chart of Corona Borealis, stars in black on white, with red circle indicating location of star TCrB.
Star chart of Corona Borealis with red circle indicating location of star T CrB. Image via IAU/ Wikipedia/ (CC BY-SA 4.0).
Man on rooftop of city looking at outlines of several labeled constellations drawn onto night sky.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, Madhya Pradesh, India, captured this photo of Boötes, Virgo and Corona Borealis on March 5, 2021. He wrote: “Spring constellations twinkling in the eastern horizon.” Thank you, Prateek!

Bottom line: Look for Corona Borealis – the Northern Crown – between the brilliant stars Arcturus and Vega tonight! In fact, this constellation is very noticeable, if you have a dark sky.

Read more: A ‘new star’ from a nova outburst is expected soon

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

The post The Northern Crown is a beautiful star pattern in May first appeared on EarthSky.



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Northern Crown: Six bright stars in bowl shape against a starry sky, Alphecca noticeably brighter.
Corona Borealis, the Northern Crown, with its brightest star Alphecca. In fact, this time of the year is perfect to see this semicircle of stars in the evening sky. Image via Fred Espenak/ AstroPixels. Used with permission.

The Northern Crown graces the summer skies

Tonight, look for a constellation that’s easy to see on the sky’s dome, if your sky is dark enough. Corona Borealis – aka the Northern Crown – is exciting to find. In fact, it’s easy to pick out as an almost-perfect semicircle of stars. You’ll find this beautiful star pattern in the evening sky from now until October.

Plus, the constellation Corona Borealis is easy to find since it’s located more or less along a line between two bright stars. The first is Arcturus in the constellation Boötes the Herdsman and the second is Vega in the constellation Lyra the Harp.

Star chart showing stars Vega and Arcturus in corners and small semicircle of stars between them, all labeled.
After nightfall and in the early evening, you’ll see Arcturus fairly high in the east, noticeable for its brightness and yellow-orange color. Next, look for Vega rather low in the northeast. It’s a bright blue-white star. Then look for the Northern Crown between these 2 bright stars. It’s a bit closer to Arcturus.

However, you’ll need a fairly dark sky to clearly see Corona Borealis between Vega and Arcturus. Then, once you find the semicircle of stars, it’s very noticeable.

The brightest star of the Northern Crown

The brightest star in Corona Borealis is Alphecca, also known as Gemma, sometimes called the Pearl of the Crown. The name Alphecca originated with a description of Corona Borealis as the “broken one.” This was in reference to the fact that these stars appear in a semicircle, rather than a full circle. Alphecca is a blue-white star, with an intrinsic luminosity some 60 times that of our sun. It’s located about 75 light-years from Earth.

Grid with dots and lines showing star patterns.
The C-shaped – or semicircle – constellation Corona Borealis shines between the constellations Boötes and Hercules. Image via IAU. Used with permission.

Watch for a ‘new star’ in the Northern Crown

T Coronae Borealis, or T CrB, is located 3,000 light-years away from Earth. It is a recurring nova with outbursts about every 80 years. Its last outburst was in 1946, and astronomers believe another will occur between February and September 2024.

The star system, normally of magnitude +10, is far too dim to see with the unaided eye. When the nova occurs, it will jump to around magnitude +2. That is roughly the same brightness to the North Star, Polaris.

Once its brightness peaks, it should be visible to the unaided eye for several days and just over a week with binoculars before it dims again, possibly for another 80 years.

Star chart of Corona Borealis, stars in black on white, with red circle indicating location of star TCrB.
Star chart of Corona Borealis with red circle indicating location of star T CrB. Image via IAU/ Wikipedia/ (CC BY-SA 4.0).
Man on rooftop of city looking at outlines of several labeled constellations drawn onto night sky.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, Madhya Pradesh, India, captured this photo of Boötes, Virgo and Corona Borealis on March 5, 2021. He wrote: “Spring constellations twinkling in the eastern horizon.” Thank you, Prateek!

Bottom line: Look for Corona Borealis – the Northern Crown – between the brilliant stars Arcturus and Vega tonight! In fact, this constellation is very noticeable, if you have a dark sky.

Read more: A ‘new star’ from a nova outburst is expected soon

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

The post The Northern Crown is a beautiful star pattern in May first appeared on EarthSky.



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Is AI to blame for our failure to find alien civilizations?

AI: A radio dish under a partly pink, starry and cloudy sky.
View at EarthSky Community Photos. | Ross Stone captured the May 10, 2024, aurora from Owens Valley Radio Observatory in Big Pine, California. Thank you, Ross! Read on to find out if AI could be the reason we’ve never detected an alien civilization.

By Michael Garrett, University of Manchester

Is AI to blame for a lack of alien civilizations?

Artificial intelligence (AI) has progressed at an astounding pace over the last few years. Some scientists are now looking toward the development of artificial superintelligence (ASI). ASI is a form of AI that would not only surpass human intelligence but would not be bound by the learning speeds of humans.

But what if this milestone isn’t just a remarkable achievement? What if it also represents a formidable bottleneck in the development of all civilizations? One so challenging that it thwarts their long-term survival?

This idea is at the heart of a research paper I recently published in Acta Astronautica. Could AI be the universe’s great filter? A threshold so hard to overcome that it prevents most life from evolving into space-faring civilizations?

This concept might explain why the search for extraterrestrial intelligence (SETI) has yet to detect the signatures of advanced technical civilizations elsewhere in the galaxy.

Attention astronomy enthusiasts! Are you looking for a way to show your support for astronomy education? Donate to EarthSky.org here and help us bring knowledge of the night sky and our universe to people worldwide.

The great filter

The great filter hypothesis is ultimately a proposed solution to the Fermi Paradox. This questions why, in a universe vast and ancient enough to host billions of potentially habitable planets, we have not detected any signs of alien civilizations. The hypothesis suggests there are insurmountable hurdles in the evolutionary timeline of civilizations. Those hurdles prevent them from developing into space-faring entities.

I believe the emergence of ASI could be such a filter. AI’s rapid advancement, potentially leading to ASI, may intersect with a critical phase in a civilization’s development: the transition from a single-planet species to a multiplanetary one.

This is where many civilizations could falter. AI could make much more rapid progress than our ability either to control it or sustainably explore and populate our solar system.

Artificial superintelligence pitfalls

The challenge with AI, and specifically ASI, lies in its autonomous, self-amplifying and improving nature. It possesses the potential to enhance its own capabilities at a speed that outpaces our own evolutionary timelines without AI.

The potential for something to go badly wrong is enormous. It could lead to the downfall of both biological and AI civilizations before they ever get the chance to become multiplanetary. For example, if nations increasingly rely on and cede power to autonomous AI systems that compete against each other. They could use those military capabilities to kill and destroy on an unprecedented scale. This could potentially lead to the destruction of our entire civilization, including the AI systems themselves.

In this scenario, I estimate the typical longevity of a technological civilization might be less than 100 years. That’s roughly the time between being able to receive and broadcast signals between the stars (1960), and the estimated emergence of ASI (2040) on Earth. This is alarmingly short when set against the cosmic timescale of billions of years.

This estimate, when plugged into optimistic versions of the Drake equation – which attempts to estimate the number of active, communicative extraterrestrial civilizations in the Milky Way – suggests that, at any given time, there are only a handful of intelligent civilizations out there. Moreover, like us, their relatively modest technological activities could make them quite challenging to detect.

Image of the star-studded cluster NGC 6440.
There’s a mindboggling number of planets out there. Image via NASA/ ESA/ CSA/ James Webb telescope.

AI wake-up call

This research is not simply a cautionary tale of potential doom. It serves as a wake-up call for humanity to establish robust regulatory frameworks to guide the development of AI, including military systems.

This is not just about preventing the malevolent use of AI on Earth. It’s also about ensuring the evolution of AI aligns with the long-term survival of our species. It suggests we need to put more resources into becoming a multiplanetary society as soon as possible. And that’s a goal that has lain dormant since the heady days of the Apollo project. But lately it’s been reignited by advances made by private companies.

As the historian Yuval Noah Harari noted, nothing in history has prepared us for the impact of introducing non-conscious, super-intelligent entities to our planet. Recently, the implications of autonomous AI decision-making have led to calls from prominent leaders in the field for a moratorium on the development of AI. That is, until a responsible form of control and regulation can be introduced.

But even if every country agreed to abide by strict rules and regulation, rogue organizations will be difficult to rein in.

AI in the military

The integration of autonomous AI in military defense systems has to be an area of particular concern. There is already evidence that humans will voluntarily relinquish significant power to increasingly capable systems. That’s because they can carry out useful tasks much more rapidly and effectively without human intervention. Governments are therefore reluctant to regulate in this area given the strategic advantages AI offers. And some of these examples have been recently and devastatingly demonstrated in Gaza.

This means we already edge dangerously close to a precipice where autonomous weapons operate beyond ethical boundaries and sidestep international law. In such a world, surrendering power to AI systems in order to gain a tactical advantage could inadvertently set off a chain of rapidly escalating, highly destructive events. In the blink of an eye, the collective intelligence of our planet could be obliterated.

Humanity is at a crucial point in its technological trajectory. Our actions now could determine whether we become an enduring interstellar civilization, or succumb to the challenges posed by our own creations.

Looking at AI through a SETI lens

Using SETI as a lens through which we can examine our future development adds a new dimension to the discussion on the future of AI. It is up to all of us to ensure that when we reach for the stars, we do so not as a cautionary tale for other civilizations. Instead, it should be as a beacon of hope: a species that learned to thrive alongside AI.The Conversation

Michael Garrett, Sir Bernard Lovell chair of Astrophysics and Director of Jodrell Bank Centre for Astrophysics, University of Manchester

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

Bottom line: Is AI – artificial intelligence – the great filter that alien civilizations are unable to evolve beyond? The threat of AI and our own self-destruction, here.

The post Is AI to blame for our failure to find alien civilizations? first appeared on EarthSky.



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AI: A radio dish under a partly pink, starry and cloudy sky.
View at EarthSky Community Photos. | Ross Stone captured the May 10, 2024, aurora from Owens Valley Radio Observatory in Big Pine, California. Thank you, Ross! Read on to find out if AI could be the reason we’ve never detected an alien civilization.

By Michael Garrett, University of Manchester

Is AI to blame for a lack of alien civilizations?

Artificial intelligence (AI) has progressed at an astounding pace over the last few years. Some scientists are now looking toward the development of artificial superintelligence (ASI). ASI is a form of AI that would not only surpass human intelligence but would not be bound by the learning speeds of humans.

But what if this milestone isn’t just a remarkable achievement? What if it also represents a formidable bottleneck in the development of all civilizations? One so challenging that it thwarts their long-term survival?

This idea is at the heart of a research paper I recently published in Acta Astronautica. Could AI be the universe’s great filter? A threshold so hard to overcome that it prevents most life from evolving into space-faring civilizations?

This concept might explain why the search for extraterrestrial intelligence (SETI) has yet to detect the signatures of advanced technical civilizations elsewhere in the galaxy.

Attention astronomy enthusiasts! Are you looking for a way to show your support for astronomy education? Donate to EarthSky.org here and help us bring knowledge of the night sky and our universe to people worldwide.

The great filter

The great filter hypothesis is ultimately a proposed solution to the Fermi Paradox. This questions why, in a universe vast and ancient enough to host billions of potentially habitable planets, we have not detected any signs of alien civilizations. The hypothesis suggests there are insurmountable hurdles in the evolutionary timeline of civilizations. Those hurdles prevent them from developing into space-faring entities.

I believe the emergence of ASI could be such a filter. AI’s rapid advancement, potentially leading to ASI, may intersect with a critical phase in a civilization’s development: the transition from a single-planet species to a multiplanetary one.

This is where many civilizations could falter. AI could make much more rapid progress than our ability either to control it or sustainably explore and populate our solar system.

Artificial superintelligence pitfalls

The challenge with AI, and specifically ASI, lies in its autonomous, self-amplifying and improving nature. It possesses the potential to enhance its own capabilities at a speed that outpaces our own evolutionary timelines without AI.

The potential for something to go badly wrong is enormous. It could lead to the downfall of both biological and AI civilizations before they ever get the chance to become multiplanetary. For example, if nations increasingly rely on and cede power to autonomous AI systems that compete against each other. They could use those military capabilities to kill and destroy on an unprecedented scale. This could potentially lead to the destruction of our entire civilization, including the AI systems themselves.

In this scenario, I estimate the typical longevity of a technological civilization might be less than 100 years. That’s roughly the time between being able to receive and broadcast signals between the stars (1960), and the estimated emergence of ASI (2040) on Earth. This is alarmingly short when set against the cosmic timescale of billions of years.

This estimate, when plugged into optimistic versions of the Drake equation – which attempts to estimate the number of active, communicative extraterrestrial civilizations in the Milky Way – suggests that, at any given time, there are only a handful of intelligent civilizations out there. Moreover, like us, their relatively modest technological activities could make them quite challenging to detect.

Image of the star-studded cluster NGC 6440.
There’s a mindboggling number of planets out there. Image via NASA/ ESA/ CSA/ James Webb telescope.

AI wake-up call

This research is not simply a cautionary tale of potential doom. It serves as a wake-up call for humanity to establish robust regulatory frameworks to guide the development of AI, including military systems.

This is not just about preventing the malevolent use of AI on Earth. It’s also about ensuring the evolution of AI aligns with the long-term survival of our species. It suggests we need to put more resources into becoming a multiplanetary society as soon as possible. And that’s a goal that has lain dormant since the heady days of the Apollo project. But lately it’s been reignited by advances made by private companies.

As the historian Yuval Noah Harari noted, nothing in history has prepared us for the impact of introducing non-conscious, super-intelligent entities to our planet. Recently, the implications of autonomous AI decision-making have led to calls from prominent leaders in the field for a moratorium on the development of AI. That is, until a responsible form of control and regulation can be introduced.

But even if every country agreed to abide by strict rules and regulation, rogue organizations will be difficult to rein in.

AI in the military

The integration of autonomous AI in military defense systems has to be an area of particular concern. There is already evidence that humans will voluntarily relinquish significant power to increasingly capable systems. That’s because they can carry out useful tasks much more rapidly and effectively without human intervention. Governments are therefore reluctant to regulate in this area given the strategic advantages AI offers. And some of these examples have been recently and devastatingly demonstrated in Gaza.

This means we already edge dangerously close to a precipice where autonomous weapons operate beyond ethical boundaries and sidestep international law. In such a world, surrendering power to AI systems in order to gain a tactical advantage could inadvertently set off a chain of rapidly escalating, highly destructive events. In the blink of an eye, the collective intelligence of our planet could be obliterated.

Humanity is at a crucial point in its technological trajectory. Our actions now could determine whether we become an enduring interstellar civilization, or succumb to the challenges posed by our own creations.

Looking at AI through a SETI lens

Using SETI as a lens through which we can examine our future development adds a new dimension to the discussion on the future of AI. It is up to all of us to ensure that when we reach for the stars, we do so not as a cautionary tale for other civilizations. Instead, it should be as a beacon of hope: a species that learned to thrive alongside AI.The Conversation

Michael Garrett, Sir Bernard Lovell chair of Astrophysics and Director of Jodrell Bank Centre for Astrophysics, University of Manchester

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

Bottom line: Is AI – artificial intelligence – the great filter that alien civilizations are unable to evolve beyond? The threat of AI and our own self-destruction, here.

The post Is AI to blame for our failure to find alien civilizations? first appeared on EarthSky.



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Astronomers find 60 Dyson sphere candidates, among millions of searched stars

Dyson sphere: Bright star surrounded by multiple solid, thin rings, with millions of other stars in background.
View larger. | Illustration of a hypothetical Dyson sphere, a partial sphere composed of giant rings around the host star. Image via Kevin Gill/ Wikimedia Commons (CC BY 2.0).


EarthSky’s Will Triggs created this 1-minute video summary for you, of the recent discovery of 60 Dyson sphere candidates.
  • If any truly exist, Dyson spheres, or Dyson swarms, are artificial megastructures, built by extraterrestrial civilization to harness their stars’ energy.
  • Astronomers have found 60 possible candidates stars, after searching through millions of stars for signs of Dyson spheres.
  • The 60 candidate stars range from red dwarfs to larger stars including sun-like stars, up to 6,500 light-years away. All show excesses of infrared heat that, so far, scientists haven’t explained.

60 new Dyson sphere candidates

If they exist, Dyson spheres are gargantuan artificial structures, built by extraterrestrial civilizations around around their stars, with the goal of capturing energy. First proposed in 1960 by physicist Freeman Dyson, they are an incredible thought experiment. But do such objects really exist? Two teams of astronomers in Sweden and Italy recently conducted a new search for possible evidence of Dyson spheres. The astronomers examined 5 million stars, up to 6,500 light-years away. And they found 60 possible candidate stars. The stars, both red dwarfs (or M dwarfs) and larger ones including sun-like stars, are emitting up to 60 times more infrared heat than scientists expected.

However, the results fit with what astronomers would expect to see from Dyson spheres. The teams found the candidates in the latest Gaia DR3 data from the European Gaia satellite as well as the Two Micron All Sky Survey (2MASS) and Wide-field Infrared Survey Explorer (WISE).

The researchers said it is difficult to explain the observations with currently known natural processes. And even if the process is most likely a previously unknown natural phenomenon, it’s still a fascinating discovery.

Jonathan O’Callaghan, a science journalist based in London, wrote about the head-scratching results in New Scientist on May 10, 2024.

Two new papers are currently available in the Monthly Notices of the Royal Astronomical Society and arXiv. The first one (May 6, 2024) focuses on seven red dwarf stars, and the second one (March 27, 2024) covers the other 53 stars.

A technosignature hiding in public data

The first paper stated:

Dyson spheres, megastructures that could be constructed by advanced civilizations to harness the radiation energy of their host stars, represent a potential technosignature, that in principle may be hiding in public data already collected as part of large astronomical surveys.

7 Dyson sphere candidates around red dwarfs

The stars studied range from red dwarfs to sun-like stars to ones larger than our sun. Additionally, most of the stars are also older, although a few appear to be young.

Matías Suazo at Uppsala University in Sweden led the team that discovered the seven candidates around red dwarf stars. All these candidates are within 900 light-years of Earth.

Like the second team, they found an excess of infrared radiation around those stars. According to the researchers, the stars appeared up to 60 times brighter in infrared than they expected. This excess infrared radiation is one of the signatures of possible Dyson spheres. The paper said:

Finally, the pipeline identifies seven candidates deserving of further analysis. All of these objects are M dwarfs, for which astrophysical phenomena cannot easily account for the observed infrared excess emission.

There are several natural explanations for the infrared excess in literature, but none of them clearly explains such a phenomenon in the candidates, especially given that all are M dwarfs.

And, as of now, at least, difficult to explain with known natural causes. So, could there be a non-natural explanation? It’s possible, and as Suazo said in New Scientist:

The most fascinating explanation could be actual Dyson spheres.

Unexplained spikes in infrared radiation

As the researchers explained, the spikes in infrared radiation with these seven red dwarfs are consistent with a temperature up to 400 degrees Celsius (750 degrees Fahrenheit). They would, theoretically, be consistent with a partial Dyson sphere, where multiple giant segments or satellites orbit the star instead of one closed sphere. That’s a variation of a Dyson sphere that scientists have also theorized. The New Scientist article said:

This excess infrared heat would have been caused by temperatures of up to 400 degrees Celsius, consistent with what we might expect from a Dyson sphere. Up to 16% of each star would have to be obscured to account for the excess, meaning it would more likely be a variant of the idea called a Dyson swarm – a collection of large satellites orbiting the star to collect energy – if truly of artificial origin.

Co-author Jason Wright at Pennsylvania State University said:

This isn’t like a single solid shell around the star.

12 squares, 2 with graph charts and 10 with fuzzy black circles, with text labels.
View larger. | Photometric images – which measure the light in terms of its perceived brightness to the human eye – of 2 red dwarf Dyson sphere candidates. All images are centered in the position of the candidates, according to Gaia DR3. All sources are clear mid-infrared emitters with no clear contaminators or signatures that indicate an obvious mid-infrared origin. The red circle marks the location of the star according to Gaia DR3. Image via Suazo et al./ Monthly Notices of the Royal Astronomical Society (CC BY 4.0).

53 more candidates

The seven candidates around red dwarf stars are intriguing, but there’s more. Specifically, 53 more candidates, all larger stars, some like our own sun. These were the focus of the second paper. Gabriella Contardo at the International School for Advanced Studies (SISSA) in Italy led this search. These stars are up to 6,500 light-years away. The paper said:

Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) technosignatures along the lines of Dyson spheres. In this paper, we conduct a large search for such excesses, designed as a data-driven contextual anomaly detection pipeline. We focus our search on FGK stars close to the main sequence to favor non-young host stars. We look for excess in the mid-infrared, unlocking a large sample to search in while favoring extreme infrared excess akin to the ones produced by extreme debris disks.

While most of the stars are older, a few appear to be younger, as the paper noted:

We obtained a set of 53 candidates that display interesting mid-infrared excess. A few of those objects appear to be young stars (showing high hydrogen alpha emission). A significant fraction of our candidates seems to have variability in the optical, and some in the mid-infrared. This can also indicate youth, but a proper age estimation using gyrochronology and a variability analysis is required.

Possible explanations

Scientists don’t know the cause of the excess infrared heat on all these stars. The observations fit with what astronomers have said they would expect to see from Dyson spheres or swarms, based on theoretical studies. Of course, that doesn’t prove these really are alien megastructures … at least not yet. Hot, planet-forming debris disks – protoplanetary disks – are one possibility. The problem is most of the 60 stars are old. Any planet-forming debris disks should have cooled and disappeared by now. That is, of course, apart from possible asteroid belts or Oort clouds, like in our own solar system. But even those are extremely cold environments.

Likewise, another idea is each star just happens to be in front of a more distant galaxy, as seen from Earth. But how likely is that? We don’t know yet.

More observations needed

To be sure, while the observations are difficult to explain with known natural processes, there could still be some other natural mechanism, unknown until now, that would explain them. Only further observations, perhaps by the James Webb Space Telescope, will help scientists figure out what’s really going on. As Contardo noted:

Both sets of candidates are interesting. You need follow-up observations to confirm anything.

Wright added:

Either we’ll rule them all out and say Dyson spheres are quite rare and very hard to find, or they’ll hang around as candidates and we’ll study the heck out of them.

The first paper concluded:

We would like to stress that although our candidates display properties consistent with partial Dyson spheres, it is definitely premature to presume that the mid-infrared presented in these sources originated from them. The mid-infrared data quality for these objects is typically quite low, and we require additional data to determine their nature.

Spherical shape composed of many tiny white dots arranged in rings, on black background.
View larger. | Another concept, this one of a Dyson swarm, with many individual smaller panels or satellites surrounding the host star. Image via Vedexent at English Wikipedia/ Wikimedia Commons (CC BY-SA 3.0).

The invention of the Dyson sphere

In the 1960s, physicist and astronomer Freeman J. Dyson proposed the idea of artificial megastructures built by an alien civilization more advanced than our own. Their objective is to capture as much heat from the host star as possible, for energy purposes. Various concepts range from complete spheres around the stars to partial spheres or rings. An alternative to a complete sphere enclosing the star would be a partial sphere. These solar panels would orbit and surround the host star as a Dyson swarm.

Bottom line: Two teams of astronomers in Europe say they have found 60 Dyson sphere candidates. Are they alien megastructures or a previously unknown natural phenomenon?

Source: Project Hephaistos – II. Dyson sphere candidates from Gaia DR3, 2MASS and WISE

Source: A Data-Driven Search For Mid-Infrared Excesses Among Five Million Main-Sequence FGK Stars

Via New Scientist

Read more: A Dyson sphere harvests the energy of stars

Read more: How Gaia could help find Dyson spheres

The post Astronomers find 60 Dyson sphere candidates, among millions of searched stars first appeared on EarthSky.



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Dyson sphere: Bright star surrounded by multiple solid, thin rings, with millions of other stars in background.
View larger. | Illustration of a hypothetical Dyson sphere, a partial sphere composed of giant rings around the host star. Image via Kevin Gill/ Wikimedia Commons (CC BY 2.0).


EarthSky’s Will Triggs created this 1-minute video summary for you, of the recent discovery of 60 Dyson sphere candidates.
  • If any truly exist, Dyson spheres, or Dyson swarms, are artificial megastructures, built by extraterrestrial civilization to harness their stars’ energy.
  • Astronomers have found 60 possible candidates stars, after searching through millions of stars for signs of Dyson spheres.
  • The 60 candidate stars range from red dwarfs to larger stars including sun-like stars, up to 6,500 light-years away. All show excesses of infrared heat that, so far, scientists haven’t explained.

60 new Dyson sphere candidates

If they exist, Dyson spheres are gargantuan artificial structures, built by extraterrestrial civilizations around around their stars, with the goal of capturing energy. First proposed in 1960 by physicist Freeman Dyson, they are an incredible thought experiment. But do such objects really exist? Two teams of astronomers in Sweden and Italy recently conducted a new search for possible evidence of Dyson spheres. The astronomers examined 5 million stars, up to 6,500 light-years away. And they found 60 possible candidate stars. The stars, both red dwarfs (or M dwarfs) and larger ones including sun-like stars, are emitting up to 60 times more infrared heat than scientists expected.

However, the results fit with what astronomers would expect to see from Dyson spheres. The teams found the candidates in the latest Gaia DR3 data from the European Gaia satellite as well as the Two Micron All Sky Survey (2MASS) and Wide-field Infrared Survey Explorer (WISE).

The researchers said it is difficult to explain the observations with currently known natural processes. And even if the process is most likely a previously unknown natural phenomenon, it’s still a fascinating discovery.

Jonathan O’Callaghan, a science journalist based in London, wrote about the head-scratching results in New Scientist on May 10, 2024.

Two new papers are currently available in the Monthly Notices of the Royal Astronomical Society and arXiv. The first one (May 6, 2024) focuses on seven red dwarf stars, and the second one (March 27, 2024) covers the other 53 stars.

A technosignature hiding in public data

The first paper stated:

Dyson spheres, megastructures that could be constructed by advanced civilizations to harness the radiation energy of their host stars, represent a potential technosignature, that in principle may be hiding in public data already collected as part of large astronomical surveys.

7 Dyson sphere candidates around red dwarfs

The stars studied range from red dwarfs to sun-like stars to ones larger than our sun. Additionally, most of the stars are also older, although a few appear to be young.

Matías Suazo at Uppsala University in Sweden led the team that discovered the seven candidates around red dwarf stars. All these candidates are within 900 light-years of Earth.

Like the second team, they found an excess of infrared radiation around those stars. According to the researchers, the stars appeared up to 60 times brighter in infrared than they expected. This excess infrared radiation is one of the signatures of possible Dyson spheres. The paper said:

Finally, the pipeline identifies seven candidates deserving of further analysis. All of these objects are M dwarfs, for which astrophysical phenomena cannot easily account for the observed infrared excess emission.

There are several natural explanations for the infrared excess in literature, but none of them clearly explains such a phenomenon in the candidates, especially given that all are M dwarfs.

And, as of now, at least, difficult to explain with known natural causes. So, could there be a non-natural explanation? It’s possible, and as Suazo said in New Scientist:

The most fascinating explanation could be actual Dyson spheres.

Unexplained spikes in infrared radiation

As the researchers explained, the spikes in infrared radiation with these seven red dwarfs are consistent with a temperature up to 400 degrees Celsius (750 degrees Fahrenheit). They would, theoretically, be consistent with a partial Dyson sphere, where multiple giant segments or satellites orbit the star instead of one closed sphere. That’s a variation of a Dyson sphere that scientists have also theorized. The New Scientist article said:

This excess infrared heat would have been caused by temperatures of up to 400 degrees Celsius, consistent with what we might expect from a Dyson sphere. Up to 16% of each star would have to be obscured to account for the excess, meaning it would more likely be a variant of the idea called a Dyson swarm – a collection of large satellites orbiting the star to collect energy – if truly of artificial origin.

Co-author Jason Wright at Pennsylvania State University said:

This isn’t like a single solid shell around the star.

12 squares, 2 with graph charts and 10 with fuzzy black circles, with text labels.
View larger. | Photometric images – which measure the light in terms of its perceived brightness to the human eye – of 2 red dwarf Dyson sphere candidates. All images are centered in the position of the candidates, according to Gaia DR3. All sources are clear mid-infrared emitters with no clear contaminators or signatures that indicate an obvious mid-infrared origin. The red circle marks the location of the star according to Gaia DR3. Image via Suazo et al./ Monthly Notices of the Royal Astronomical Society (CC BY 4.0).

53 more candidates

The seven candidates around red dwarf stars are intriguing, but there’s more. Specifically, 53 more candidates, all larger stars, some like our own sun. These were the focus of the second paper. Gabriella Contardo at the International School for Advanced Studies (SISSA) in Italy led this search. These stars are up to 6,500 light-years away. The paper said:

Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) technosignatures along the lines of Dyson spheres. In this paper, we conduct a large search for such excesses, designed as a data-driven contextual anomaly detection pipeline. We focus our search on FGK stars close to the main sequence to favor non-young host stars. We look for excess in the mid-infrared, unlocking a large sample to search in while favoring extreme infrared excess akin to the ones produced by extreme debris disks.

While most of the stars are older, a few appear to be younger, as the paper noted:

We obtained a set of 53 candidates that display interesting mid-infrared excess. A few of those objects appear to be young stars (showing high hydrogen alpha emission). A significant fraction of our candidates seems to have variability in the optical, and some in the mid-infrared. This can also indicate youth, but a proper age estimation using gyrochronology and a variability analysis is required.

Possible explanations

Scientists don’t know the cause of the excess infrared heat on all these stars. The observations fit with what astronomers have said they would expect to see from Dyson spheres or swarms, based on theoretical studies. Of course, that doesn’t prove these really are alien megastructures … at least not yet. Hot, planet-forming debris disks – protoplanetary disks – are one possibility. The problem is most of the 60 stars are old. Any planet-forming debris disks should have cooled and disappeared by now. That is, of course, apart from possible asteroid belts or Oort clouds, like in our own solar system. But even those are extremely cold environments.

Likewise, another idea is each star just happens to be in front of a more distant galaxy, as seen from Earth. But how likely is that? We don’t know yet.

More observations needed

To be sure, while the observations are difficult to explain with known natural processes, there could still be some other natural mechanism, unknown until now, that would explain them. Only further observations, perhaps by the James Webb Space Telescope, will help scientists figure out what’s really going on. As Contardo noted:

Both sets of candidates are interesting. You need follow-up observations to confirm anything.

Wright added:

Either we’ll rule them all out and say Dyson spheres are quite rare and very hard to find, or they’ll hang around as candidates and we’ll study the heck out of them.

The first paper concluded:

We would like to stress that although our candidates display properties consistent with partial Dyson spheres, it is definitely premature to presume that the mid-infrared presented in these sources originated from them. The mid-infrared data quality for these objects is typically quite low, and we require additional data to determine their nature.

Spherical shape composed of many tiny white dots arranged in rings, on black background.
View larger. | Another concept, this one of a Dyson swarm, with many individual smaller panels or satellites surrounding the host star. Image via Vedexent at English Wikipedia/ Wikimedia Commons (CC BY-SA 3.0).

The invention of the Dyson sphere

In the 1960s, physicist and astronomer Freeman J. Dyson proposed the idea of artificial megastructures built by an alien civilization more advanced than our own. Their objective is to capture as much heat from the host star as possible, for energy purposes. Various concepts range from complete spheres around the stars to partial spheres or rings. An alternative to a complete sphere enclosing the star would be a partial sphere. These solar panels would orbit and surround the host star as a Dyson swarm.

Bottom line: Two teams of astronomers in Europe say they have found 60 Dyson sphere candidates. Are they alien megastructures or a previously unknown natural phenomenon?

Source: Project Hephaistos – II. Dyson sphere candidates from Gaia DR3, 2MASS and WISE

Source: A Data-Driven Search For Mid-Infrared Excesses Among Five Million Main-Sequence FGK Stars

Via New Scientist

Read more: A Dyson sphere harvests the energy of stars

Read more: How Gaia could help find Dyson spheres

The post Astronomers find 60 Dyson sphere candidates, among millions of searched stars first appeared on EarthSky.



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Meet Regulus, Leo the Lion’s Heart

Star chart: animal-shaped constellation with head at right side and bright star, Regulus, in chest area.
Leo the Lion’s brightest star is Regulus, the Lion’s Heart. Regulus is the dot at the bottom of a backward question mark pattern of stars, called the Sickle. An easily identifiable triangle depicts the Lion’s hindquarters and tail. The star Denebola marks the tail of the Lion. Chart via EarthSky.

Regulus, the brightest star in the constellation Leo the Lion, is a harbinger of spring in the Northern Hemisphere. It crept higher in the sky with each passing day in March and April, as winter favorites like Orion descended westward. And now, in May, this blue-white star is brilliant in the eastern evening sky as soon as the sun goes down.

You can locate Regulus – also known as Alpha Leonis – at the base of a star pattern that appears like a backward question mark. This pattern, known as the Sickle, makes up the head and forequarters of Leo the Lion.

Regulus is also one of three bright stars to make up the asterism known as the Spring Triangle.

Regulus ranks 21st in the list of brightest stars in our sky. However, although it looks like one star to the eye, it’s actually four stars.

Star chart of Leo. The lines connecting the dots on the head end look like a flipped question mark.
A star chart showing the constellation Leo. On the right is a pattern that looks like a flipped question mark, the Sickle. This is the most recognizable pattern to look for when trying to locate Leo in the sky. Image via Torsten Bronger/ Wikimedia Commons (CC BY-SA 3.0).

Regulus is visible most of the year

Around February 18, Regulus was opposite the sun. It rose above the horizon as the sun set, stayed up all night long, and reached its highest point due south (as seen from the Northern Hemisphere) at local midnight. By early April, Regulus was well up in the southeast an hour after sunset. By early June, it’ll be high in the southwest an hour after sunset. Come early July, Regulus will be low to the west an hour after sunset. And from mid-September through mid-February, Regulus will be in the morning sky.

So, Regulus is visible at some time of night throughout the year, except for about a month on either side of August 22. Look towards Regulus around that date and you’ll see the sun.

Planets and the moon pass near it

Regulus is the only 1st magnitude star to sit almost squarely on the ecliptic, which marks the path of the sun, moon and planets across our sky.

So bright planets sometimes pass near Regulus. For example, in early-July 2024, Venus will visit Regulus in the evening sky. And in early-September, 2024, Mercury will join Regulus in the morning twilight. Also, planets can sometimes occult – or pass in front of – Regulus. The last planet to occult Regulus was Venus on July 7, 1959. Then on October 1, 2044, Venus will occult Regulus again.

And, every month, the moon passes near Regulus. In some years, the moon occults this star as seen from Earth. There will be a series of 20 lunar occultations of Regulus from July 2025 to December 2026. During the December 2026 occultation, Mars and Jupiter will be nearby.

A blue, egg-shaped star

Regulus is located about 79 light-years from Earth. It’s a multiple system with at least four component stars. The main star – Regulus A – is large and blue with a spectral type of B8 IVn. Its surface temperature averages about 12,460 kelvin (21,970 degrees F or 12,190 degrees C), which is much higher than our sun’s surface temperature. Regulus A is 3.8 times the mass of our sun, about 4 times as wide, and almost 300 times as bright.

Regulus spins on its axis once every 16 hours. In contrast, our sun spins on its axis about once every 27 days. This fast rotation causes Regulus A to bulge at its equator, so it appears oblate, or egg-shaped. In fact, if Regulus rotated just a bit faster, it would fly apart! And Regulus is not the only star with a fast spin. The stars Altair and Achernar are also fast spinners with flattened, oblate shapes.

An egg-shaped spheroid with a much smaller sphere at the lower right.
Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) created this computer-generated model of Regulus in 2005. Next to it is a model of the sun for scale. The high rotation rate of Regulus creates pronounced equatorial bulging, such that its diameter across its equator (running nearly vertically in this image) is 1/3 longer than its north-south diameter. Image via Wenjin Huang/ Georgia State University/ NSF.

Regulus is 4 stars

Look through a small telescope using at least 50x magnification, and you can see Regulus as two objects separated by 177 arcseconds. The brighter of the pair is called Regulus A.

The fainter one is Regulus B, a cool “orange” dwarf star with a spectral classification of K2 V. The B star has a mass that is 80% of the sun’s, and it’s half as bright. It has a surface temperature of 4,885 kelvin (8,333 F or 4,612 C), and it shines at magnitude 8.1.

Regulus B, meanwhile, has its own companion: Regulus C. At magnitude 13.5, it’s only visible with powerful telescopes. With just 1/3 the mass of the sun, Regulus C is a red dwarf star with a spectral classification of M4 V. Regulus B and C are gravitationally bound to each other, and together they’re called Regulus BC. The distances between B and C ranged from 4.0 to 2.5 arc seconds between 1867 and 1943. There are no recently available measurements.

The fourth star in the system has never been directly resolved via imaging, but its presence is revealed by spectroscopic analysis of Regulus A. Astronomers think it may be a closely orbiting white dwarf star.

You might have heard of a star called Regulus D. This does not refer to the spectroscopic companion of Regulus A, but to a 12th-magnitude star that sits 212 arcseconds from Regulus. For decades, people believed it to be a companion of Regulus, but recent studies from the Gaia satellite show this to be a background star not related to the Regulus system.

A galaxy photobombs Regulus

Situated 1/3 degree north of Regulus is the galaxy Leo 1, you can see it as a faint patch of light in the photo below. Leo 1 is difficult to see due to its proximity to Regulus. Albert George Wilson found it on photographic plates taken as part of the National Geographic Society-Palomar Observatory Sky Survey in 1950. It would be another 40 years before anyone viewed it visually.

Leo 1 is a dwarf galaxy, and a member of our local group. Amateur astronomers can view it, but this requires dark skies and a large telescope.

In a field of stars, a large, brilliant blue-white star. Above it is a faint horizontal oval smudge of light.
Regulus as photographed using a telescope. The faint smudge above it is the dwarf galaxy Leo I. Image via Fred Espenak. Used with permission.

A rex by any other name

The name Regulus is from the diminutive form of the Latin rex, meaning little king.

Ancient Arab stargazers called Regulus by the name Qalb al-Asad, which means Heart of the Lion. It also bears the nickname Cor Leonis, again meaning Lion’s Heart. Fittingly, King Richard I of England was also famously known as the Lionheart, or more commonly Couer de Lion in French.

There is a great deal of mythology associated with Leo, perhaps the most common tale being that Leo was the Nemean Lion of the Hercules story. Some Peruvians also knew these stars as the Mountain Lion, whereas in China it was sometimes seen as a horse, and at other times as part of a dragon. Christians in the Middle Ages sometimes referred to it as one of Daniel’s lions.

Antique colored etching of two yellow lions, one much larger, with the constellations' stars superimposed.
The larger lion is the constellation Leo, with the star Regulus at its heart, as depicted on a set of constellation cards, Urania’s Mirror, published in London c. 1825. Above it is the faint constellation Leo Minor. Image via Library of Congress/ Wikimedia Commons (public domain).

Bottom line: Regulus, the brightest star in the constellation Leo the Lion, is associated with the arrival of spring and is prominent in May skies. It looks like a single point of light, but is really four stars.

The post Meet Regulus, Leo the Lion’s Heart first appeared on EarthSky.



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Star chart: animal-shaped constellation with head at right side and bright star, Regulus, in chest area.
Leo the Lion’s brightest star is Regulus, the Lion’s Heart. Regulus is the dot at the bottom of a backward question mark pattern of stars, called the Sickle. An easily identifiable triangle depicts the Lion’s hindquarters and tail. The star Denebola marks the tail of the Lion. Chart via EarthSky.

Regulus, the brightest star in the constellation Leo the Lion, is a harbinger of spring in the Northern Hemisphere. It crept higher in the sky with each passing day in March and April, as winter favorites like Orion descended westward. And now, in May, this blue-white star is brilliant in the eastern evening sky as soon as the sun goes down.

You can locate Regulus – also known as Alpha Leonis – at the base of a star pattern that appears like a backward question mark. This pattern, known as the Sickle, makes up the head and forequarters of Leo the Lion.

Regulus is also one of three bright stars to make up the asterism known as the Spring Triangle.

Regulus ranks 21st in the list of brightest stars in our sky. However, although it looks like one star to the eye, it’s actually four stars.

Star chart of Leo. The lines connecting the dots on the head end look like a flipped question mark.
A star chart showing the constellation Leo. On the right is a pattern that looks like a flipped question mark, the Sickle. This is the most recognizable pattern to look for when trying to locate Leo in the sky. Image via Torsten Bronger/ Wikimedia Commons (CC BY-SA 3.0).

Regulus is visible most of the year

Around February 18, Regulus was opposite the sun. It rose above the horizon as the sun set, stayed up all night long, and reached its highest point due south (as seen from the Northern Hemisphere) at local midnight. By early April, Regulus was well up in the southeast an hour after sunset. By early June, it’ll be high in the southwest an hour after sunset. Come early July, Regulus will be low to the west an hour after sunset. And from mid-September through mid-February, Regulus will be in the morning sky.

So, Regulus is visible at some time of night throughout the year, except for about a month on either side of August 22. Look towards Regulus around that date and you’ll see the sun.

Planets and the moon pass near it

Regulus is the only 1st magnitude star to sit almost squarely on the ecliptic, which marks the path of the sun, moon and planets across our sky.

So bright planets sometimes pass near Regulus. For example, in early-July 2024, Venus will visit Regulus in the evening sky. And in early-September, 2024, Mercury will join Regulus in the morning twilight. Also, planets can sometimes occult – or pass in front of – Regulus. The last planet to occult Regulus was Venus on July 7, 1959. Then on October 1, 2044, Venus will occult Regulus again.

And, every month, the moon passes near Regulus. In some years, the moon occults this star as seen from Earth. There will be a series of 20 lunar occultations of Regulus from July 2025 to December 2026. During the December 2026 occultation, Mars and Jupiter will be nearby.

A blue, egg-shaped star

Regulus is located about 79 light-years from Earth. It’s a multiple system with at least four component stars. The main star – Regulus A – is large and blue with a spectral type of B8 IVn. Its surface temperature averages about 12,460 kelvin (21,970 degrees F or 12,190 degrees C), which is much higher than our sun’s surface temperature. Regulus A is 3.8 times the mass of our sun, about 4 times as wide, and almost 300 times as bright.

Regulus spins on its axis once every 16 hours. In contrast, our sun spins on its axis about once every 27 days. This fast rotation causes Regulus A to bulge at its equator, so it appears oblate, or egg-shaped. In fact, if Regulus rotated just a bit faster, it would fly apart! And Regulus is not the only star with a fast spin. The stars Altair and Achernar are also fast spinners with flattened, oblate shapes.

An egg-shaped spheroid with a much smaller sphere at the lower right.
Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) created this computer-generated model of Regulus in 2005. Next to it is a model of the sun for scale. The high rotation rate of Regulus creates pronounced equatorial bulging, such that its diameter across its equator (running nearly vertically in this image) is 1/3 longer than its north-south diameter. Image via Wenjin Huang/ Georgia State University/ NSF.

Regulus is 4 stars

Look through a small telescope using at least 50x magnification, and you can see Regulus as two objects separated by 177 arcseconds. The brighter of the pair is called Regulus A.

The fainter one is Regulus B, a cool “orange” dwarf star with a spectral classification of K2 V. The B star has a mass that is 80% of the sun’s, and it’s half as bright. It has a surface temperature of 4,885 kelvin (8,333 F or 4,612 C), and it shines at magnitude 8.1.

Regulus B, meanwhile, has its own companion: Regulus C. At magnitude 13.5, it’s only visible with powerful telescopes. With just 1/3 the mass of the sun, Regulus C is a red dwarf star with a spectral classification of M4 V. Regulus B and C are gravitationally bound to each other, and together they’re called Regulus BC. The distances between B and C ranged from 4.0 to 2.5 arc seconds between 1867 and 1943. There are no recently available measurements.

The fourth star in the system has never been directly resolved via imaging, but its presence is revealed by spectroscopic analysis of Regulus A. Astronomers think it may be a closely orbiting white dwarf star.

You might have heard of a star called Regulus D. This does not refer to the spectroscopic companion of Regulus A, but to a 12th-magnitude star that sits 212 arcseconds from Regulus. For decades, people believed it to be a companion of Regulus, but recent studies from the Gaia satellite show this to be a background star not related to the Regulus system.

A galaxy photobombs Regulus

Situated 1/3 degree north of Regulus is the galaxy Leo 1, you can see it as a faint patch of light in the photo below. Leo 1 is difficult to see due to its proximity to Regulus. Albert George Wilson found it on photographic plates taken as part of the National Geographic Society-Palomar Observatory Sky Survey in 1950. It would be another 40 years before anyone viewed it visually.

Leo 1 is a dwarf galaxy, and a member of our local group. Amateur astronomers can view it, but this requires dark skies and a large telescope.

In a field of stars, a large, brilliant blue-white star. Above it is a faint horizontal oval smudge of light.
Regulus as photographed using a telescope. The faint smudge above it is the dwarf galaxy Leo I. Image via Fred Espenak. Used with permission.

A rex by any other name

The name Regulus is from the diminutive form of the Latin rex, meaning little king.

Ancient Arab stargazers called Regulus by the name Qalb al-Asad, which means Heart of the Lion. It also bears the nickname Cor Leonis, again meaning Lion’s Heart. Fittingly, King Richard I of England was also famously known as the Lionheart, or more commonly Couer de Lion in French.

There is a great deal of mythology associated with Leo, perhaps the most common tale being that Leo was the Nemean Lion of the Hercules story. Some Peruvians also knew these stars as the Mountain Lion, whereas in China it was sometimes seen as a horse, and at other times as part of a dragon. Christians in the Middle Ages sometimes referred to it as one of Daniel’s lions.

Antique colored etching of two yellow lions, one much larger, with the constellations' stars superimposed.
The larger lion is the constellation Leo, with the star Regulus at its heart, as depicted on a set of constellation cards, Urania’s Mirror, published in London c. 1825. Above it is the faint constellation Leo Minor. Image via Library of Congress/ Wikimedia Commons (public domain).

Bottom line: Regulus, the brightest star in the constellation Leo the Lion, is associated with the arrival of spring and is prominent in May skies. It looks like a single point of light, but is really four stars.

The post Meet Regulus, Leo the Lion’s Heart first appeared on EarthSky.



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Which Milky Way spiral arm is ours?


How can we visualize ourselves in our home galaxy, the Milky Way? Join EarthSky’s Deborah Byrd and Marcy Curran as they discuss seeing the Milky Way in our sky, and how to understand your place in it.

Which spiral arm of the Milky Way is ours?

Our Milky Way galaxy is the island of stars we call home. If you imagine it as a disk with spiral arms emanating from the center, our sun is approximately halfway from the center to the visible edge. Our solar system lies between two prominent spiral arms: the Perseus Arm and the Scutum-Centaurus Arm. But we aren’t quite free floating in empty space. We lie on the edge of a relatively minor spiral arm, the Orion-Cygnus Arm, or simply, the Orion Arm or Local Arm.

Join us in making sure everyone has access to the wonders of astronomy. Donate now!

In Michael Carroll’s book Planet Earth, Past and Present: Parallels Between Our World and its Celestial Neighbors, he explains why our position in the galaxy might be important to life on Earth. He writes:

Our location in the galaxy is significant, as it appears that – like planetary systems – galaxies have habitable zones.

An astonishing 95% of the Milky Way’s suns may not be able to sustain habitable planets, because many orbit the galaxy in paths that carry them through the deadly spiral arms. Any star that passes through one of these starry swarms is subject to deadly radiation from the congested stars. Our own solar system orbits far enough from the center to keep it in sync with the rotation of the rest of the galaxy, so that it remains in the quieter space between the spiral arms. The Earth and its planetary siblings are well placed in a quiet, resource-rich niche of a vast and complex galaxy.

The structure of the Milky Way

The Milky Way is a barred spiral galaxy, which means it has a central bar. There’s still a lot we don’t know about the structure of our galaxy. According to the best current knowledge, the Milky Way is about 100,000 light-years across, about 2,000 light-years deep, and has 100 to 400 billion stars. Astronomers once thought that our spiral galaxy had four major arms, but now they say we have just two major arms and many minor arms.

Where, within this vast spiral structure, do our sun and its planets reside? We’re about 26,000 light-years from the center of the galaxy, on the inner edge of the Orion-Cygnus Arm.

Diagram: Milky Way galaxy with 2 main arms and other smaller arms labeled and a golden colored bar in the middle.
View larger. | Artist’s concept of our Milky Way galaxy. Astronomers now believe the Milky Way galaxy has 2 major arms and many minor arms. Our sun is about halfway from the galactic center, on a minor arm that’s sometimes called the Orion Spur. Image via NASA.

The Orion Arm

The Orion Arm of the Milky Way is probably some 3,500 light-years wide. Initially, astronomers thought it was about 10,000 light-years in length. But a study from 2016 suggests it’s more than 20,000 light-years long.

Astronomers continue to piece together the structure of the Milky Way by painstakingly measuring the positions and distances to many stars and gas clouds. Telescopes on the ground and in space determine distances from parallax measurements. For example, the Gaia Space Telescope’s goal is to provide a 3-dimensional map of our Milky Way.

Flat-on view of round spiral galaxy with 2 main arms and short golden bar in the middle.
This Hubble Space Telescope image shows the galaxy UGC 12158. It’s a barred spiral galaxy that scientists think bears a close resemblance to the Milky Way. Image via NASA/ ESA.

How our local spiral arm got its name

The Orion Arm gets its name from the constellation Orion the Hunter, which is one of the most prominent constellations of the Northern Hemisphere winter (Southern Hemisphere summer). Some of the brightest stars and most famous celestial objects of this constellation (Betelgeuse, Rigel, the stars of Orion’s Belt, the Orion nebula) are neighbors to our sun. The reason we see so many bright objects within the constellation Orion is because when we look at it, we’re looking into our own local spiral arm.

Diagram: Labeled astronomical objects in Orion Arm and neighboring regions.
View larger. | Artist’s concept of our galactic neighborhood. Some of the best-known astronomical objects in our sky lie in the Orion Arm, along with our sun. Image via R. Hurt/ Wikimedia Commons (public domain).

Bottom line: Where do we live in the Milky Way galaxy? We lie between the major arms in a smaller spiral arm known as the Orion Arm.

The post Which Milky Way spiral arm is ours? first appeared on EarthSky.



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How can we visualize ourselves in our home galaxy, the Milky Way? Join EarthSky’s Deborah Byrd and Marcy Curran as they discuss seeing the Milky Way in our sky, and how to understand your place in it.

Which spiral arm of the Milky Way is ours?

Our Milky Way galaxy is the island of stars we call home. If you imagine it as a disk with spiral arms emanating from the center, our sun is approximately halfway from the center to the visible edge. Our solar system lies between two prominent spiral arms: the Perseus Arm and the Scutum-Centaurus Arm. But we aren’t quite free floating in empty space. We lie on the edge of a relatively minor spiral arm, the Orion-Cygnus Arm, or simply, the Orion Arm or Local Arm.

Join us in making sure everyone has access to the wonders of astronomy. Donate now!

In Michael Carroll’s book Planet Earth, Past and Present: Parallels Between Our World and its Celestial Neighbors, he explains why our position in the galaxy might be important to life on Earth. He writes:

Our location in the galaxy is significant, as it appears that – like planetary systems – galaxies have habitable zones.

An astonishing 95% of the Milky Way’s suns may not be able to sustain habitable planets, because many orbit the galaxy in paths that carry them through the deadly spiral arms. Any star that passes through one of these starry swarms is subject to deadly radiation from the congested stars. Our own solar system orbits far enough from the center to keep it in sync with the rotation of the rest of the galaxy, so that it remains in the quieter space between the spiral arms. The Earth and its planetary siblings are well placed in a quiet, resource-rich niche of a vast and complex galaxy.

The structure of the Milky Way

The Milky Way is a barred spiral galaxy, which means it has a central bar. There’s still a lot we don’t know about the structure of our galaxy. According to the best current knowledge, the Milky Way is about 100,000 light-years across, about 2,000 light-years deep, and has 100 to 400 billion stars. Astronomers once thought that our spiral galaxy had four major arms, but now they say we have just two major arms and many minor arms.

Where, within this vast spiral structure, do our sun and its planets reside? We’re about 26,000 light-years from the center of the galaxy, on the inner edge of the Orion-Cygnus Arm.

Diagram: Milky Way galaxy with 2 main arms and other smaller arms labeled and a golden colored bar in the middle.
View larger. | Artist’s concept of our Milky Way galaxy. Astronomers now believe the Milky Way galaxy has 2 major arms and many minor arms. Our sun is about halfway from the galactic center, on a minor arm that’s sometimes called the Orion Spur. Image via NASA.

The Orion Arm

The Orion Arm of the Milky Way is probably some 3,500 light-years wide. Initially, astronomers thought it was about 10,000 light-years in length. But a study from 2016 suggests it’s more than 20,000 light-years long.

Astronomers continue to piece together the structure of the Milky Way by painstakingly measuring the positions and distances to many stars and gas clouds. Telescopes on the ground and in space determine distances from parallax measurements. For example, the Gaia Space Telescope’s goal is to provide a 3-dimensional map of our Milky Way.

Flat-on view of round spiral galaxy with 2 main arms and short golden bar in the middle.
This Hubble Space Telescope image shows the galaxy UGC 12158. It’s a barred spiral galaxy that scientists think bears a close resemblance to the Milky Way. Image via NASA/ ESA.

How our local spiral arm got its name

The Orion Arm gets its name from the constellation Orion the Hunter, which is one of the most prominent constellations of the Northern Hemisphere winter (Southern Hemisphere summer). Some of the brightest stars and most famous celestial objects of this constellation (Betelgeuse, Rigel, the stars of Orion’s Belt, the Orion nebula) are neighbors to our sun. The reason we see so many bright objects within the constellation Orion is because when we look at it, we’re looking into our own local spiral arm.

Diagram: Labeled astronomical objects in Orion Arm and neighboring regions.
View larger. | Artist’s concept of our galactic neighborhood. Some of the best-known astronomical objects in our sky lie in the Orion Arm, along with our sun. Image via R. Hurt/ Wikimedia Commons (public domain).

Bottom line: Where do we live in the Milky Way galaxy? We lie between the major arms in a smaller spiral arm known as the Orion Arm.

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