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Were Neptune’s inner moons born from an ancient cataclysm?

Neptune's inner moons: Hazy-looking planet with rings and several small moons near it.
View larger. | This infrared image from the James Webb Space Telescope, taken on July 12, 2022, shows Neptune, its rings and some of its inner moons. A new study shows that Neptune’s inner moons might have formed through the destruction of a previous family of moons. Image via NASA/ ESA/ CSA/ STScI; Image Processing: Joseph DePasquale (STScI)/ Naomi Rowe-Gurney (NASA-GSFC).
  • How did Neptune’s inner moons form? Scientists have considered various possibilities.
  • A new hypothesis suggests that they formed from the remnants of a previous family of moons. Those moons would have been mostly obliterated when Neptune’s gravity captured Triton, the planet’s largest moon.
  • Two of the studied moons, surprisingly, have rich clay deposits. But the third moon has none. Why?

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Neptune’s inner moons

Neptune has 16 known moons. NASA’s James Webb Space Telescope recently took a closer look at three of the innermost small moons – Larissa, Galatea and Proteus – and found something interesting; they have a unique composition among all the bodies in the solar system.

Having looked into this surprising finding, a team of researchers said on July 29, 2026, that these moons likely formed from the remnants of a former system of moons around Neptune. They believe these moons were destroyed when the planet’s current largest moon, Triton, was captured by Neptune billions of years ago.

Ryleigh Davis, a former Caltech graduate student, now at UC San Diego, is the lead author of a new paper about these moons. She said:

If Neptune once had a system of moons that looked something like what we see at Uranus today [a stable family of multiple moons of different sizes orbiting the planet], we expect it would’ve been completely destroyed by the process of Triton getting captured. This is exciting new evidence that something catastrophic happened at Neptune that completely destroyed its original satellites, and we’re getting to see the fingerprints left behind by that process.

Those former icy moons are all gone now, except maybe for Nereid. Scientists think it might be the sole survivor of that catastrophe.

Davis and her colleagues published their peer-reviewed findings in Science Advances on July 29, 2026.

Diagram showing a planet with rings in black and white, with 2 colored squares, 1 on either side, with text labels.
View larger. | Infrared view from the James Webb Space Telescope of the moon Larissa, and Neptune and its rings. Image via Davis et al. 2026; NASA/ ESA/ CSA JWST data/ Caltech.

Clays on Larissa, Galatea and in the rings

The researchers wanted to study Neptune’s inner moons more, to learn more about the planet’s history. There is still much that scientists don’t know about these small, distant worlds.

Astronomers had only recently obtained spectroscopy data for the moons, which tells scientists what kinds of molecules are present.

Surprisingly, they found phyllosilicates, or clays, on the moons, and in Neptune’s rings. It was an unexpected discovery, as Davis noted:

Phyllosilicates had never been detected anywhere in the outer solar system beyond Jupiter, so that was not on our list of things to look for. We were shocked to find the observed clays, which had to come from objects that were much, much bigger than Neptune’s small inner ring moons.

Webb found the signatures of magnesium-rich phyllosilicates (clays). Why was this surprising?

Diagram in 4 parts showing a blue planet with rings and moons, as the moons formed and changed.
View larger. | This diagram depicts how the current inner moons of Neptune formed. The capture of Triton by Neptune destroyed the previous family of moons. The current small moon then formed from their debris. Image via R. Davis/ Caltech (License: original content).

Where did the clays come from?

Clays require water to form. But no water ice was found on any of the moons or in the rings. And it’s way too cold for liquid water. So the moons and rings must have originated from some body or bodies that did have ice. Davis explained:

That’s really surprising because everything out in this part of the solar system is really icy. So, we’re fairly confident that they had to come from deep inside something that was big enough to generate enough heat that it melted its water ice. We think the most likely place would be an original system of icy moons, although it’s a bit of a mystery where the ice may have gone.

Scientist Mike Brown at Caltech added:

It took diligent detective work from Ryleigh before we understood what we were seeing. Sometimes in science you are trying to find evidence to evaluate a specific hypothesis, and, sometimes, something that you had not been thinking about just hits you in the face.

Fuzzy, oblong gray object on black background.
Nereid is the 3rd-largest moon of Neptune. It might be the only original inner moon left that survived the cataclysm caused by Triton. This is still the best image of the moon, captured by Voyager 2 on August 24, 1989. Image via NASA/ Wikimedia Commons.

No clays for Proteus and an unknown mineral

There’s another twist, though. Proteus is the largest of the three small moons. And it doesn’t have the clays on it. Why? It might simply have originated from a part of the former debris where clays were absent. Or, perhaps there were clays originally, but heat destroyed them.

Plus, Webb identified a hydrated mineral that is on all three moons. But scientists don’t know what it is yet. It hasn’t even been seen elsewhere in the solar system. Davis said:

We see something that doesn’t really look like anything else we’ve identified in the solar system; it doesn’t match anything we have in our spectral libraries. We assume it’s some form of hydrated rock from the moons as well, but there’s still a lot of mystery.

This is reminiscent of another recent discovery. Scientists found a mineral that is present on the surfaces of both Pluto and Saturn’s moon Titan. But again, it’s never been seen before anywhere else, until now.

Smiling woman wearing a dark blue blazer and white shirt.
Ryleigh Davis at UC San Diego is the lead author of the new paper about Neptune’s inner moons. Image via GitHub.

A destroyed Kuiper Belt object?

The researchers consider the system of ancient moons to be the most likely scenario to explain the current inner moons of Neptune. But there is another possibility. A larger single object from the Kuiper Belt beyond Neptune, about the size of Pluto, might have passed too close to Neptune. Neptune’s immense gravity would then have shredded the object. Davis said:

Either way, what we’re seeing on these moons had to come from deep inside something much larger. That material is normally permanently buried—we can only infer what’s there. Here, a catastrophic event essentially turned these ancient moons inside out, and we get to see what was hidden inside.

But if Triton did play a role, then it would have had a big effect on how the current moons formed and their behavior. Davis noted:

If you bring Triton in, and you smash up your large moons, we think only 1 percent or so of that material stayed around in the system. But the actual behavior of that material might be really different if Triton is still there shaking things up for a long time. So, looking forward, understanding how that process actually proceeds would be interesting. From there, the question is: ‘Can we learn anything about how big the initial moons had to be to have formed and provided this material?’

Bottom line: A new study suggests that Neptune’s inner moons formed when Neptune captured its largest moon Triton, and a family of original small icy moons was destroyed.

Source: Neptune’s inner moons and rings are exposed icy body interiors

Via Caltech

Read more: Are Uranus and Neptune rock giants and not ice giants?

Read more: New moons! Uranus now has 28 and Neptune 16

The post Were Neptune’s inner moons born from an ancient cataclysm? first appeared on EarthSky.



from EarthSky https://ift.tt/0qQCXIe
Neptune's inner moons: Hazy-looking planet with rings and several small moons near it.
View larger. | This infrared image from the James Webb Space Telescope, taken on July 12, 2022, shows Neptune, its rings and some of its inner moons. A new study shows that Neptune’s inner moons might have formed through the destruction of a previous family of moons. Image via NASA/ ESA/ CSA/ STScI; Image Processing: Joseph DePasquale (STScI)/ Naomi Rowe-Gurney (NASA-GSFC).
  • How did Neptune’s inner moons form? Scientists have considered various possibilities.
  • A new hypothesis suggests that they formed from the remnants of a previous family of moons. Those moons would have been mostly obliterated when Neptune’s gravity captured Triton, the planet’s largest moon.
  • Two of the studied moons, surprisingly, have rich clay deposits. But the third moon has none. Why?

You deserve a daily dose of good news. For the latest in science and the night sky, subscribe to EarthSky’s free daily newsletter.

Neptune’s inner moons

Neptune has 16 known moons. NASA’s James Webb Space Telescope recently took a closer look at three of the innermost small moons – Larissa, Galatea and Proteus – and found something interesting; they have a unique composition among all the bodies in the solar system.

Having looked into this surprising finding, a team of researchers said on July 29, 2026, that these moons likely formed from the remnants of a former system of moons around Neptune. They believe these moons were destroyed when the planet’s current largest moon, Triton, was captured by Neptune billions of years ago.

Ryleigh Davis, a former Caltech graduate student, now at UC San Diego, is the lead author of a new paper about these moons. She said:

If Neptune once had a system of moons that looked something like what we see at Uranus today [a stable family of multiple moons of different sizes orbiting the planet], we expect it would’ve been completely destroyed by the process of Triton getting captured. This is exciting new evidence that something catastrophic happened at Neptune that completely destroyed its original satellites, and we’re getting to see the fingerprints left behind by that process.

Those former icy moons are all gone now, except maybe for Nereid. Scientists think it might be the sole survivor of that catastrophe.

Davis and her colleagues published their peer-reviewed findings in Science Advances on July 29, 2026.

Diagram showing a planet with rings in black and white, with 2 colored squares, 1 on either side, with text labels.
View larger. | Infrared view from the James Webb Space Telescope of the moon Larissa, and Neptune and its rings. Image via Davis et al. 2026; NASA/ ESA/ CSA JWST data/ Caltech.

Clays on Larissa, Galatea and in the rings

The researchers wanted to study Neptune’s inner moons more, to learn more about the planet’s history. There is still much that scientists don’t know about these small, distant worlds.

Astronomers had only recently obtained spectroscopy data for the moons, which tells scientists what kinds of molecules are present.

Surprisingly, they found phyllosilicates, or clays, on the moons, and in Neptune’s rings. It was an unexpected discovery, as Davis noted:

Phyllosilicates had never been detected anywhere in the outer solar system beyond Jupiter, so that was not on our list of things to look for. We were shocked to find the observed clays, which had to come from objects that were much, much bigger than Neptune’s small inner ring moons.

Webb found the signatures of magnesium-rich phyllosilicates (clays). Why was this surprising?

Diagram in 4 parts showing a blue planet with rings and moons, as the moons formed and changed.
View larger. | This diagram depicts how the current inner moons of Neptune formed. The capture of Triton by Neptune destroyed the previous family of moons. The current small moon then formed from their debris. Image via R. Davis/ Caltech (License: original content).

Where did the clays come from?

Clays require water to form. But no water ice was found on any of the moons or in the rings. And it’s way too cold for liquid water. So the moons and rings must have originated from some body or bodies that did have ice. Davis explained:

That’s really surprising because everything out in this part of the solar system is really icy. So, we’re fairly confident that they had to come from deep inside something that was big enough to generate enough heat that it melted its water ice. We think the most likely place would be an original system of icy moons, although it’s a bit of a mystery where the ice may have gone.

Scientist Mike Brown at Caltech added:

It took diligent detective work from Ryleigh before we understood what we were seeing. Sometimes in science you are trying to find evidence to evaluate a specific hypothesis, and, sometimes, something that you had not been thinking about just hits you in the face.

Fuzzy, oblong gray object on black background.
Nereid is the 3rd-largest moon of Neptune. It might be the only original inner moon left that survived the cataclysm caused by Triton. This is still the best image of the moon, captured by Voyager 2 on August 24, 1989. Image via NASA/ Wikimedia Commons.

No clays for Proteus and an unknown mineral

There’s another twist, though. Proteus is the largest of the three small moons. And it doesn’t have the clays on it. Why? It might simply have originated from a part of the former debris where clays were absent. Or, perhaps there were clays originally, but heat destroyed them.

Plus, Webb identified a hydrated mineral that is on all three moons. But scientists don’t know what it is yet. It hasn’t even been seen elsewhere in the solar system. Davis said:

We see something that doesn’t really look like anything else we’ve identified in the solar system; it doesn’t match anything we have in our spectral libraries. We assume it’s some form of hydrated rock from the moons as well, but there’s still a lot of mystery.

This is reminiscent of another recent discovery. Scientists found a mineral that is present on the surfaces of both Pluto and Saturn’s moon Titan. But again, it’s never been seen before anywhere else, until now.

Smiling woman wearing a dark blue blazer and white shirt.
Ryleigh Davis at UC San Diego is the lead author of the new paper about Neptune’s inner moons. Image via GitHub.

A destroyed Kuiper Belt object?

The researchers consider the system of ancient moons to be the most likely scenario to explain the current inner moons of Neptune. But there is another possibility. A larger single object from the Kuiper Belt beyond Neptune, about the size of Pluto, might have passed too close to Neptune. Neptune’s immense gravity would then have shredded the object. Davis said:

Either way, what we’re seeing on these moons had to come from deep inside something much larger. That material is normally permanently buried—we can only infer what’s there. Here, a catastrophic event essentially turned these ancient moons inside out, and we get to see what was hidden inside.

But if Triton did play a role, then it would have had a big effect on how the current moons formed and their behavior. Davis noted:

If you bring Triton in, and you smash up your large moons, we think only 1 percent or so of that material stayed around in the system. But the actual behavior of that material might be really different if Triton is still there shaking things up for a long time. So, looking forward, understanding how that process actually proceeds would be interesting. From there, the question is: ‘Can we learn anything about how big the initial moons had to be to have formed and provided this material?’

Bottom line: A new study suggests that Neptune’s inner moons formed when Neptune captured its largest moon Triton, and a family of original small icy moons was destroyed.

Source: Neptune’s inner moons and rings are exposed icy body interiors

Via Caltech

Read more: Are Uranus and Neptune rock giants and not ice giants?

Read more: New moons! Uranus now has 28 and Neptune 16

The post Were Neptune’s inner moons born from an ancient cataclysm? first appeared on EarthSky.



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Mars Curiosity rover’s 7 minutes of terror 14 years ago

Science news, night sky events and beautiful photos, all in one place. Click here to subscribe to EarthSky’s free daily newsletter.

14 years ago on August 5: A nail-biter of a Mars landing

On August 5, 2012, NASA achieved one of the most challenging feats in planetary exploration: landing the Curiosity rover safely on Mars. The rover was not just another spacecraft reaching the red planet — it was a 1-ton (900 kg) mobile laboratory that needed a completely new landing system to reach the surface.

After entering Mars’ atmosphere at around 13,000 miles per hour (about 21,000 kph), Curiosity had only seven minutes to slow down, navigate through the thin Mars atmosphere, deploy a parachute and be lowered gently to the ground by a rocket-powered “sky crane.” Engineers couldn’t control the landing in real time; they could only wait for the signals to arrive from Mars.

Those seven minutes became known as the “seven minutes of terror” — a dramatic name for a sequence in which years of engineering had to work perfectly on another planet.

Getting there is easy, but landing there is not

Years before the landing of Curiosity, in 2003, veteran NASA official Firouz Naderi summed up Mars’ historical significance for space exploration:

Mars is a favorite target.

We – the United States and former USSR – have been going to Mars for 40 years. The first time we flew by a planet, it was Mars. The first time we orbited a planet, it was Mars. And the first time we landed on a planet it was Mars. The first time we roved around the surface of a planet, it was Mars. We go there often.

At that time – around the turn of this century – the world was averaging about two failures for every three spacecraft launched toward Mars, according to NASA. In fact, there were a total of 39 Mars missions launched and 25 failures, or partial failures, by the year 2000, according to Wikipedia.

But then we got better at it. And as the video above shows, Curiosity’s landing used a combination of complicated new technologies, including a new guided entry system and a rocket-powered sky crane that used cables to lower the 1-ton (900 kg) robot rover to the Martian surface.

Mars Curiosity rover is still going strong

Since 2012, Curiosity has been crawling across Mars’ surface and exploring Gale crater. The rover has traveled more than 20 miles (32 km) across Mars. It has learned, among many other things, that Gale crater might once have held a great salty lake.

Read more: Mars rover Curiosity heads for intriguing ‘spiderwebs’

Read more: Martian rock crushed by Curiosity hides a surprise!

Mars Curiosity: Spacecraft hovering above the surface, firing retrorockets, with cables from the craft lowering the rover.
Artist’s concept of Curiosity rover’s landing on Mars via a “sky crane” and cables. The new rover that arrived at Mars in March 2021 – Perseverance – also landed on Mars via sky crane. Image via NASA.
Dusty 6-wheeled rover looking our way with a camera on a pole, in reddish Martian desert.
Curiosity took this self-portrait on May 11, 2016, at the “Okoruso” drilling site in the foothills of Mount Sharp, the central peak of Gale crater. If Gale crater once held a lake, Mount Sharp might have been an island in the middle of that lake. This self-portrait combines multiple images taken with the rover’s Mars Hand Lens Imager (MAHLI), during the 1,338th Martian day, or sol, of the rover’s work on Mars. Image via NASA.

Perseverance was the next to land

Curiosity was followed to Mars by another robot rover, Perseverance, which launched from Earth on July 30, 2020. Finally, Perseverance touched down on Mars landing in Jezero crater on February 18, 2021. Perseverance is largely the same design as Curiosity. When the $2.4 billion spacecraft carrying it reached Mars, it also hit the atmosphere at high speed (more than 12,000 miles per hour or 19,000 kph) and then came to a complete stop on Mars’ surface seven minutes later. Like Curiosity, it landed via “sky crane,” but with one big difference: the sky crane technology was now tried-and-true.

Still, as with Curiosity, space engineers surely experienced a nail-biting seven minutes, waiting to hear that the Perseverance rover had set down successfully, as gently as it could, on Mars’ surface.

There, it joined the other rovers in the search for life on Mars and an exploration of the planet’s surface, atmosphere and history. Perseverance brought with it a special helicopter named Ingenuity, that explored the Martian surface as well until its mission ended in January 2024.

Why focus so many spacecraft on Mars?

Read more from the NY Times: Too much Mars? This is an interesting discussion between two veteran space journalists about why Mars seems to absorb so much of the oxygen – and budgetary resources – in the rooms where explorations of our solar system are decided.

Animated view of a parachute opening, seen from below.
Parachute test for Mars Perseverance rover. The images for this animation were taken on September 7, 2018, during the 3rd and final flight of the Advanced Supersonic Parachute Inflation Research Experiment (ASPIRE) project. Read more about this GIF via NASA/ JPL-Caltech.

Why is landing on Mars so hard? This 2017 video from MinutePhysics does a great job of explaining it:

Bottom line: Watch a NASA video describing the final seven minutes of the Curiosity rover’s chilling descent to the surface of Mars 14 years ago on August 5, 2012.

Read more: Curiosity rover on Mars snags highest-resolution panorama yet

Read more: Mars rover measures key life ingredient

The post Mars Curiosity rover’s 7 minutes of terror 14 years ago first appeared on EarthSky.



from EarthSky https://ift.tt/dWpJ6vY

Science news, night sky events and beautiful photos, all in one place. Click here to subscribe to EarthSky’s free daily newsletter.

14 years ago on August 5: A nail-biter of a Mars landing

On August 5, 2012, NASA achieved one of the most challenging feats in planetary exploration: landing the Curiosity rover safely on Mars. The rover was not just another spacecraft reaching the red planet — it was a 1-ton (900 kg) mobile laboratory that needed a completely new landing system to reach the surface.

After entering Mars’ atmosphere at around 13,000 miles per hour (about 21,000 kph), Curiosity had only seven minutes to slow down, navigate through the thin Mars atmosphere, deploy a parachute and be lowered gently to the ground by a rocket-powered “sky crane.” Engineers couldn’t control the landing in real time; they could only wait for the signals to arrive from Mars.

Those seven minutes became known as the “seven minutes of terror” — a dramatic name for a sequence in which years of engineering had to work perfectly on another planet.

Getting there is easy, but landing there is not

Years before the landing of Curiosity, in 2003, veteran NASA official Firouz Naderi summed up Mars’ historical significance for space exploration:

Mars is a favorite target.

We – the United States and former USSR – have been going to Mars for 40 years. The first time we flew by a planet, it was Mars. The first time we orbited a planet, it was Mars. And the first time we landed on a planet it was Mars. The first time we roved around the surface of a planet, it was Mars. We go there often.

At that time – around the turn of this century – the world was averaging about two failures for every three spacecraft launched toward Mars, according to NASA. In fact, there were a total of 39 Mars missions launched and 25 failures, or partial failures, by the year 2000, according to Wikipedia.

But then we got better at it. And as the video above shows, Curiosity’s landing used a combination of complicated new technologies, including a new guided entry system and a rocket-powered sky crane that used cables to lower the 1-ton (900 kg) robot rover to the Martian surface.

Mars Curiosity rover is still going strong

Since 2012, Curiosity has been crawling across Mars’ surface and exploring Gale crater. The rover has traveled more than 20 miles (32 km) across Mars. It has learned, among many other things, that Gale crater might once have held a great salty lake.

Read more: Mars rover Curiosity heads for intriguing ‘spiderwebs’

Read more: Martian rock crushed by Curiosity hides a surprise!

Mars Curiosity: Spacecraft hovering above the surface, firing retrorockets, with cables from the craft lowering the rover.
Artist’s concept of Curiosity rover’s landing on Mars via a “sky crane” and cables. The new rover that arrived at Mars in March 2021 – Perseverance – also landed on Mars via sky crane. Image via NASA.
Dusty 6-wheeled rover looking our way with a camera on a pole, in reddish Martian desert.
Curiosity took this self-portrait on May 11, 2016, at the “Okoruso” drilling site in the foothills of Mount Sharp, the central peak of Gale crater. If Gale crater once held a lake, Mount Sharp might have been an island in the middle of that lake. This self-portrait combines multiple images taken with the rover’s Mars Hand Lens Imager (MAHLI), during the 1,338th Martian day, or sol, of the rover’s work on Mars. Image via NASA.

Perseverance was the next to land

Curiosity was followed to Mars by another robot rover, Perseverance, which launched from Earth on July 30, 2020. Finally, Perseverance touched down on Mars landing in Jezero crater on February 18, 2021. Perseverance is largely the same design as Curiosity. When the $2.4 billion spacecraft carrying it reached Mars, it also hit the atmosphere at high speed (more than 12,000 miles per hour or 19,000 kph) and then came to a complete stop on Mars’ surface seven minutes later. Like Curiosity, it landed via “sky crane,” but with one big difference: the sky crane technology was now tried-and-true.

Still, as with Curiosity, space engineers surely experienced a nail-biting seven minutes, waiting to hear that the Perseverance rover had set down successfully, as gently as it could, on Mars’ surface.

There, it joined the other rovers in the search for life on Mars and an exploration of the planet’s surface, atmosphere and history. Perseverance brought with it a special helicopter named Ingenuity, that explored the Martian surface as well until its mission ended in January 2024.

Why focus so many spacecraft on Mars?

Read more from the NY Times: Too much Mars? This is an interesting discussion between two veteran space journalists about why Mars seems to absorb so much of the oxygen – and budgetary resources – in the rooms where explorations of our solar system are decided.

Animated view of a parachute opening, seen from below.
Parachute test for Mars Perseverance rover. The images for this animation were taken on September 7, 2018, during the 3rd and final flight of the Advanced Supersonic Parachute Inflation Research Experiment (ASPIRE) project. Read more about this GIF via NASA/ JPL-Caltech.

Why is landing on Mars so hard? This 2017 video from MinutePhysics does a great job of explaining it:

Bottom line: Watch a NASA video describing the final seven minutes of the Curiosity rover’s chilling descent to the surface of Mars 14 years ago on August 5, 2012.

Read more: Curiosity rover on Mars snags highest-resolution panorama yet

Read more: Mars rover measures key life ingredient

The post Mars Curiosity rover’s 7 minutes of terror 14 years ago first appeared on EarthSky.



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Double star 61 Cygni: Why is it known as the Flying Star?

Star chart: Many white stars, several labeled including 61 Cygni, and 2 reddish nebulae.
In this finder chart, 61 Cygni is marked in the crosshairs. If you could imagine Deneb, Sadr and Aljanah as part of a rough rectangle, 61 Cygni would be in the 4th corner. Alternately, you can find Zeta Cygni and draw an imaginary line to Deneb. Then, you would find 61 Cygni about halfway between the 2 stars. But what’s so special about this star? Image via Stellarium. Used with permission.

You deserve a daily dose of good news. For the latest in science and the night sky, subscribe to EarthSky’s free daily newsletter.

They call it the Flying Star

61 Cygni is a double star in the constellation Cygnus the Swan. It’s not a standout star in brightness … so what’s so special about it?

61 Cygni is particularly cool because it has one of the highest proper motions of any visible star. That’s its movement across the dome of our sky.

So if you took photos of 61 Cygni over the course of several years, you’d see it shift position in the sky with respect to the more distant stars around it.

This unusual motion across our sky has earned 61 Cygni the nickname the Flying Star.

61 Cygni has a high proper motion

So why does this star have such a high proper motion? Imagine two people running across your field of view, one closer to you and the other farther away. In relation to the more distant landscape, the person closer to you would appear to cover more ground – more objects would pass behind them – than the person farther away.

In a similar way, very distant stars appear “fixed” in relationship to each other. However, they’re actually moving through space in their various journeys around the center of our Milky Way galaxy. But most are so far away that we can’t easily detect their proper motions. On the other hand, 61 Cygni is different. It moves relatively rapidly in front of the fixed stars because it is relatively near Earth.

While not the closest star to the sun (that honor goes to the Alpha Centauri system), 61 Cygni is just 11.4 light-years distant. That makes it the 4th-closest star that’s visible to the unaided eye, after Alpha Centauri, Sirius and Epsilon Eridani.

Animation showing two close stars very visibly moving against background stars.
In this sequence of images taken from 2012 to 2020, 61 Cygni’s motion can be seen against the backdrop of more distant stars. Image via IndividusObservantis/ Wikimedia Commons.
Complex diagram: Sun, with lines forming an angle toward an object with arrows showing its motion.
The motion of a star in space, from our Earth-bound perspective, can be broken into 2 components. The transverse velocity is its motion across the dome of the sky. That annual motion, measured as an angle, is called proper motion. Radial velocity is the star’s movement either toward or away from us. It’s measured spectroscopically. Image via Brews ohare/ Wikimedia Commons.

Science of 61 Cygni

61 Cygni isn’t just one star. It’s a binary system, with two stars that take about 659 years to orbit one another. To the unaided eye and through most binoculars, it appears as one star. However, if you look at it through a modestly-sized telescope, you’ll see it resolved as two stars. They have apparent magnitudes of 5.21 and 6.03.

The 61 Cygni binary system is the 15th-nearest known star system to us. Both are K-type dwarf stars in the main sequence, thought to have formed 6 billion years ago (the sun, in comparison, is 4.6 billion years old).

The more massive star of the pair has 70% of our sun’s mass and puts out 15% of our sun’s total electromagnetic energy. Its companion has 63% of our sun’s mass and shines at just 8.5% of our sun’s luminosity. Both are a bit over half the size of our sun. They’re also variable stars, exhibiting small changes in brightness over time.

Three spheres: one larger yellow one, two smaller orange ones close together.
Size comparison of our sun (left), 61 Cygni A (lower) and 61 Cygni B (upper right). Image via RJHall/ Wikimedia Commons.

The history of 61 Cygni

61 Cygni has no role in classical mythology. Of course, since it’s barely visible to the eye, it’s not surprising that the ancients apparently left no written reference to it at all. But its role in the history of astronomy is assured.

The motion of 61 Cygni across our sky, while large compared to other stars, can’t be easily detected with the eye alone over the span of a human lifetime. It was with the arrival of telescopes and through meticulous observations that astronomers discovered high proper motions of stars.

Astronomer Giuseppe Piazzi, in 1792, first noticed that 61 Cygni had a high proper motion when he compared his observations to those taken by another astronomer 40 years earlier. By 1804, he had gathered enough information to be the first to publish about this extraordinary star that he nicknamed the Flying Star.

Piazzi correctly noted that this high proper motion indicated that 61 Cygni was a nearby star, and that parallax measurements could be used to figure out its distance. German astronomer F.W. Bessel was the first to get reliable measurements of the 61 Cygni stars’ parallaxes that gave a distance of 10.4 light-years, which is pretty close to the distance we know today, 11.4 light-years. It’s also the first time a star’s distance was reliably measured.

How to see it

61 Cygni is roughly halfway between two other stars that you can probably identify. First is Deneb, the brightest star in the constellation Cygnus the Swan. And the other star is Zeta Cygni, at one end of the Swan’s wing. You’ll find 61 Cygni between these two. Several other similarly dim stars are located nearby, so you’ll need a detailed finder star chart to properly identify 61 Cygni. Take a look at our chart at the top of this post.

61 Cygni’s position is RA: 21h 06m 55s, Dec: +38° 44′ 57″
Proper motion: 4″ in Right Ascension, 3″ in Declination
Parallax: 0.286″

A sparse faint star field with two beautiful yellowish-orange stars, almost equally bright, in the center.
The 61 Cygni binary stars, photographed using a camera attached to a 12-inch telescope. Image via Tom and Jane Wildoner/ Dark Side Observatory. Used with permission.

Bottom line: 61 Cygni, while faint to the unaided eye, is one of the closest stars to Earth. It exhibits a high proper motion – or motion across the sky – compared to other stars.

Read more: Double stars: How to find, observe and enjoy them

The post Double star 61 Cygni: Why is it known as the Flying Star? first appeared on EarthSky.



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Star chart: Many white stars, several labeled including 61 Cygni, and 2 reddish nebulae.
In this finder chart, 61 Cygni is marked in the crosshairs. If you could imagine Deneb, Sadr and Aljanah as part of a rough rectangle, 61 Cygni would be in the 4th corner. Alternately, you can find Zeta Cygni and draw an imaginary line to Deneb. Then, you would find 61 Cygni about halfway between the 2 stars. But what’s so special about this star? Image via Stellarium. Used with permission.

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They call it the Flying Star

61 Cygni is a double star in the constellation Cygnus the Swan. It’s not a standout star in brightness … so what’s so special about it?

61 Cygni is particularly cool because it has one of the highest proper motions of any visible star. That’s its movement across the dome of our sky.

So if you took photos of 61 Cygni over the course of several years, you’d see it shift position in the sky with respect to the more distant stars around it.

This unusual motion across our sky has earned 61 Cygni the nickname the Flying Star.

61 Cygni has a high proper motion

So why does this star have such a high proper motion? Imagine two people running across your field of view, one closer to you and the other farther away. In relation to the more distant landscape, the person closer to you would appear to cover more ground – more objects would pass behind them – than the person farther away.

In a similar way, very distant stars appear “fixed” in relationship to each other. However, they’re actually moving through space in their various journeys around the center of our Milky Way galaxy. But most are so far away that we can’t easily detect their proper motions. On the other hand, 61 Cygni is different. It moves relatively rapidly in front of the fixed stars because it is relatively near Earth.

While not the closest star to the sun (that honor goes to the Alpha Centauri system), 61 Cygni is just 11.4 light-years distant. That makes it the 4th-closest star that’s visible to the unaided eye, after Alpha Centauri, Sirius and Epsilon Eridani.

Animation showing two close stars very visibly moving against background stars.
In this sequence of images taken from 2012 to 2020, 61 Cygni’s motion can be seen against the backdrop of more distant stars. Image via IndividusObservantis/ Wikimedia Commons.
Complex diagram: Sun, with lines forming an angle toward an object with arrows showing its motion.
The motion of a star in space, from our Earth-bound perspective, can be broken into 2 components. The transverse velocity is its motion across the dome of the sky. That annual motion, measured as an angle, is called proper motion. Radial velocity is the star’s movement either toward or away from us. It’s measured spectroscopically. Image via Brews ohare/ Wikimedia Commons.

Science of 61 Cygni

61 Cygni isn’t just one star. It’s a binary system, with two stars that take about 659 years to orbit one another. To the unaided eye and through most binoculars, it appears as one star. However, if you look at it through a modestly-sized telescope, you’ll see it resolved as two stars. They have apparent magnitudes of 5.21 and 6.03.

The 61 Cygni binary system is the 15th-nearest known star system to us. Both are K-type dwarf stars in the main sequence, thought to have formed 6 billion years ago (the sun, in comparison, is 4.6 billion years old).

The more massive star of the pair has 70% of our sun’s mass and puts out 15% of our sun’s total electromagnetic energy. Its companion has 63% of our sun’s mass and shines at just 8.5% of our sun’s luminosity. Both are a bit over half the size of our sun. They’re also variable stars, exhibiting small changes in brightness over time.

Three spheres: one larger yellow one, two smaller orange ones close together.
Size comparison of our sun (left), 61 Cygni A (lower) and 61 Cygni B (upper right). Image via RJHall/ Wikimedia Commons.

The history of 61 Cygni

61 Cygni has no role in classical mythology. Of course, since it’s barely visible to the eye, it’s not surprising that the ancients apparently left no written reference to it at all. But its role in the history of astronomy is assured.

The motion of 61 Cygni across our sky, while large compared to other stars, can’t be easily detected with the eye alone over the span of a human lifetime. It was with the arrival of telescopes and through meticulous observations that astronomers discovered high proper motions of stars.

Astronomer Giuseppe Piazzi, in 1792, first noticed that 61 Cygni had a high proper motion when he compared his observations to those taken by another astronomer 40 years earlier. By 1804, he had gathered enough information to be the first to publish about this extraordinary star that he nicknamed the Flying Star.

Piazzi correctly noted that this high proper motion indicated that 61 Cygni was a nearby star, and that parallax measurements could be used to figure out its distance. German astronomer F.W. Bessel was the first to get reliable measurements of the 61 Cygni stars’ parallaxes that gave a distance of 10.4 light-years, which is pretty close to the distance we know today, 11.4 light-years. It’s also the first time a star’s distance was reliably measured.

How to see it

61 Cygni is roughly halfway between two other stars that you can probably identify. First is Deneb, the brightest star in the constellation Cygnus the Swan. And the other star is Zeta Cygni, at one end of the Swan’s wing. You’ll find 61 Cygni between these two. Several other similarly dim stars are located nearby, so you’ll need a detailed finder star chart to properly identify 61 Cygni. Take a look at our chart at the top of this post.

61 Cygni’s position is RA: 21h 06m 55s, Dec: +38° 44′ 57″
Proper motion: 4″ in Right Ascension, 3″ in Declination
Parallax: 0.286″

A sparse faint star field with two beautiful yellowish-orange stars, almost equally bright, in the center.
The 61 Cygni binary stars, photographed using a camera attached to a 12-inch telescope. Image via Tom and Jane Wildoner/ Dark Side Observatory. Used with permission.

Bottom line: 61 Cygni, while faint to the unaided eye, is one of the closest stars to Earth. It exhibits a high proper motion – or motion across the sky – compared to other stars.

Read more: Double stars: How to find, observe and enjoy them

The post Double star 61 Cygni: Why is it known as the Flying Star? first appeared on EarthSky.



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Venus rings found high above planet’s thick clouds

Venus rings. Two black-and-white images of Venus set side by side. One reveals rings in the atmosphere.
Venus rings! On the right, an unpolarized view of the cloud tops of Venus on the left (a) shows a smooth, regular brightness. On the left, a view in polarized light (b) reveals a set of planet-circling concentric rings – really, atmospheric ripples – in the dense, high atmosphere. Image via Gourav Mahapatra/The Planetary Science Journal

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A group of Dutch astrophysicists has stumbled across a set of giant “rings” on Venus. They’re not solid planetary rings (like Saturn’s), but planet-circling concentric banding, hidden high in the atmosphere of Venus. And they’re not visible to the eye, but can be seen in polarized light, which blocks some scattered light and enhances subtle patterns. They are waves/ ripples in Venus’ atmosphere, but very ring-like! The group discovered them while taking a 2nd look at images of Venus captured in 2010 by the William Herschel Telescope.

The rings appear to be the result of differences in gas density above the cloud tops. A simulation of Venus’ atmosphere created for the study shows gravity waves could be driving the phenomenon. The same kind of gravity waves create the broad, expanding rings that spread across a pond after you toss in a stone. And gravity waves help shape weather and climate patterns on Earth.

A paper detailing the discovery published on July 9, 2026 in the Planetary Science Journal of the American Astronomical Society.

Venus rings found high in its atmosphere

The announcement of rings in Venus’ atmosphere is recent, but the data was collected in 2010. The authors said they captured the images while waiting for the sky to darken enough to continue their hunt for exoplanets:

The Venus images we present here are truly serendipitous. They were captured [using] the 4.2-meter William Herschel Telescope … during a period of about 36 minutes in which we were waiting for the end of the astronomical evening twilight on May 24, 2010. [We were waiting] to start observations of circumstellar disks [around exoplanets].

The Extreme Polarimeter (ExPo) was an instrument designed to detect circumstellar disks of gas and debris around distant stars. Signs of exoplanets are often hidden within these disks. ExPo has since been decommissioned and disassembled.

The giant rings on Venus are centered on a region downwind of the planet’s subsolar point, the continuously moving spot on Venus’ surface from which the sun appears directly overhead (at the zenith). The subsolar point on Venus moves slowly, as the planet takes 117 Earth days to complete one rotation.

Giant Rings on Venus. Six black-and-white images of Venus stacked three rows deep and two columns wide. Three of the images show rings. The others do not.
Images captured through 6 different polarization filters by the William Herschel Telescope on the Canary Islands revealed a previously unknown set of rings in the planet’s atmosphere. Image via Gourav Mahapatra/The Planetary Science Journal

Images of Venus rings are one-of-a-kind

At first, because they’re almost centered on the brightest point on the planet’s disk, the researchers thought the giant rings on Venus might be an artifact of the ExPo detector. But the tool for measuring the polarization of light waves was designed to avoid such errors. Six different kinds of filters were used to create six sets of images, and the rings only showed up in three of them.

The science team had no other explanation: the rings are really there. And these are the only pictures of them ever taken.

The images from ExPo were captured under the extremely dark skies above the Canary Islands off the coast of Africa during a night of exceptionally clear skies. Unfortunately, the paper explains why that’s not the only reason other images of the rings can’t be taken with ExPo on the Magellan Telescope:

We have no other images of Venus with rings, as we did not have other opportunities to observe Venus under such advantageous seeing conditions and, due to the experimental nature of ExPo, the instrument has been taken apart and its optical components reused for other experiments. To the best of our knowledge, there are no other polarimeters available that combine imaging with ExPo’s high polarimetric sensitivity.

Upcoming mission to Venus to help explain ring mystery

The researchers, of course, want more observations to deepen our understanding of how and why these Venus rings form. They want both ground-based imagery, as well as measurements taken by space-based telescopes.

They might get an extremely close look from ESA’s EnVision mission. It includes plans to carry a high-resolution polarimeter into orbit around Venus. Launch is scheduled for 2032.

But who knows? The rings might not be there when the orbiter arrives. No one knows how often this atmospheric ring feature forms or how long it lasts.

And, despite not finding an error in the way ExPo collected the data, it’s still possible the rings are a false signal. While it looks like a newly discovered weather pattern, there isn’t enough information to be sure. The researchers said:

Moreover, ExPo was an experimental instrument that was not later reinstalled in an identical configuration and has since been dismantled. For these reasons, the present observations cannot by themselves establish a definitive detection of a new Venusian atmospheric phenomenon and should instead be viewed as a candidate signal that requires independent confirmation.

Still, what we see in the first ring images is enough to let the team speculate about how the rings came to be:

If the observed pattern is astrophysical rather than instrumental, one plausible explanation is spatial variation in the gas density above the hazes and clouds. Such planet-wide density variations could result from atmospheric waves emanating from the region close to the subsolar point. …

Bottom line: New analysis of images taken in 2010 reveal giant Venus rings. The rings are high in the Venus atmosphere. They are ripples in the atmosphere, not solid particles.

Source: Planet-wide, Concentric Density Waves in Venus’s Upper Atmosphere Revealed through Polarimetry? (DOI 10.3847/PSJ/ae7e6f)

Read more: New evidence of lava tube on Venus found in old radar data

The post Venus rings found high above planet’s thick clouds first appeared on EarthSky.



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Venus rings. Two black-and-white images of Venus set side by side. One reveals rings in the atmosphere.
Venus rings! On the right, an unpolarized view of the cloud tops of Venus on the left (a) shows a smooth, regular brightness. On the left, a view in polarized light (b) reveals a set of planet-circling concentric rings – really, atmospheric ripples – in the dense, high atmosphere. Image via Gourav Mahapatra/The Planetary Science Journal

Science matters. Wonder matters. You matter. Join our 2026 Donation Campaign today.

A group of Dutch astrophysicists has stumbled across a set of giant “rings” on Venus. They’re not solid planetary rings (like Saturn’s), but planet-circling concentric banding, hidden high in the atmosphere of Venus. And they’re not visible to the eye, but can be seen in polarized light, which blocks some scattered light and enhances subtle patterns. They are waves/ ripples in Venus’ atmosphere, but very ring-like! The group discovered them while taking a 2nd look at images of Venus captured in 2010 by the William Herschel Telescope.

The rings appear to be the result of differences in gas density above the cloud tops. A simulation of Venus’ atmosphere created for the study shows gravity waves could be driving the phenomenon. The same kind of gravity waves create the broad, expanding rings that spread across a pond after you toss in a stone. And gravity waves help shape weather and climate patterns on Earth.

A paper detailing the discovery published on July 9, 2026 in the Planetary Science Journal of the American Astronomical Society.

Venus rings found high in its atmosphere

The announcement of rings in Venus’ atmosphere is recent, but the data was collected in 2010. The authors said they captured the images while waiting for the sky to darken enough to continue their hunt for exoplanets:

The Venus images we present here are truly serendipitous. They were captured [using] the 4.2-meter William Herschel Telescope … during a period of about 36 minutes in which we were waiting for the end of the astronomical evening twilight on May 24, 2010. [We were waiting] to start observations of circumstellar disks [around exoplanets].

The Extreme Polarimeter (ExPo) was an instrument designed to detect circumstellar disks of gas and debris around distant stars. Signs of exoplanets are often hidden within these disks. ExPo has since been decommissioned and disassembled.

The giant rings on Venus are centered on a region downwind of the planet’s subsolar point, the continuously moving spot on Venus’ surface from which the sun appears directly overhead (at the zenith). The subsolar point on Venus moves slowly, as the planet takes 117 Earth days to complete one rotation.

Giant Rings on Venus. Six black-and-white images of Venus stacked three rows deep and two columns wide. Three of the images show rings. The others do not.
Images captured through 6 different polarization filters by the William Herschel Telescope on the Canary Islands revealed a previously unknown set of rings in the planet’s atmosphere. Image via Gourav Mahapatra/The Planetary Science Journal

Images of Venus rings are one-of-a-kind

At first, because they’re almost centered on the brightest point on the planet’s disk, the researchers thought the giant rings on Venus might be an artifact of the ExPo detector. But the tool for measuring the polarization of light waves was designed to avoid such errors. Six different kinds of filters were used to create six sets of images, and the rings only showed up in three of them.

The science team had no other explanation: the rings are really there. And these are the only pictures of them ever taken.

The images from ExPo were captured under the extremely dark skies above the Canary Islands off the coast of Africa during a night of exceptionally clear skies. Unfortunately, the paper explains why that’s not the only reason other images of the rings can’t be taken with ExPo on the Magellan Telescope:

We have no other images of Venus with rings, as we did not have other opportunities to observe Venus under such advantageous seeing conditions and, due to the experimental nature of ExPo, the instrument has been taken apart and its optical components reused for other experiments. To the best of our knowledge, there are no other polarimeters available that combine imaging with ExPo’s high polarimetric sensitivity.

Upcoming mission to Venus to help explain ring mystery

The researchers, of course, want more observations to deepen our understanding of how and why these Venus rings form. They want both ground-based imagery, as well as measurements taken by space-based telescopes.

They might get an extremely close look from ESA’s EnVision mission. It includes plans to carry a high-resolution polarimeter into orbit around Venus. Launch is scheduled for 2032.

But who knows? The rings might not be there when the orbiter arrives. No one knows how often this atmospheric ring feature forms or how long it lasts.

And, despite not finding an error in the way ExPo collected the data, it’s still possible the rings are a false signal. While it looks like a newly discovered weather pattern, there isn’t enough information to be sure. The researchers said:

Moreover, ExPo was an experimental instrument that was not later reinstalled in an identical configuration and has since been dismantled. For these reasons, the present observations cannot by themselves establish a definitive detection of a new Venusian atmospheric phenomenon and should instead be viewed as a candidate signal that requires independent confirmation.

Still, what we see in the first ring images is enough to let the team speculate about how the rings came to be:

If the observed pattern is astrophysical rather than instrumental, one plausible explanation is spatial variation in the gas density above the hazes and clouds. Such planet-wide density variations could result from atmospheric waves emanating from the region close to the subsolar point. …

Bottom line: New analysis of images taken in 2010 reveal giant Venus rings. The rings are high in the Venus atmosphere. They are ripples in the atmosphere, not solid particles.

Source: Planet-wide, Concentric Density Waves in Venus’s Upper Atmosphere Revealed through Polarimetry? (DOI 10.3847/PSJ/ae7e6f)

Read more: New evidence of lava tube on Venus found in old radar data

The post Venus rings found high above planet’s thick clouds first appeared on EarthSky.



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9 mind-blowing space facts that will shock you

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

EarthSky isn’t powered by billionaires. We’re powered by you. Support EarthSky’s 2026 Donation Campaign and help keep science accessible.

9 mind-blowing space facts that will shock you

Almost everything about outer space is amazing, from what we might find on Earth’s moon to the visible boundary of our universe … it can all leave you scratching your head. Here are nine truly mind-blowing facts about our Earth, sun, solar system and universe. Enjoy … and share (you’ll be a hit at your next dinner party).

1. There might be dinosaur fossils on the moon

Some 65 million years ago, an asteroid hurtled toward Earth. When it hit, it triggered a mass extinction, ending the rein of the dinosaurs. At that time, dinosaurs had already been around for some 200 million years. So, many generations had already died and their bones had become fossilized in earthly rocks.

And, when the dinosaur-killing asteroid hit Earth, it impacted so violently that some of the rocks jettisoned from the impact flew into space. And it’s possible some of those rocks with fossilized dinosaurs might have ultimately ended up on the moon, colliding with it in much the same way a SpaceX rocket is colliding with the moon tonight, August 5, 2026.

So there could be rocks with dinosaur fossils on the moon!

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

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

The distance between objects in space is vast. As an example of this, if you took all the other planets in the solar system, you could pack them tightly between Earth and the moon.

There are a couple of caveats here. First, we are stacking the planets pole to pole so we don’t have to worry about Saturn’s rings.

Second, we’re performing this feat during apogee, or when the moon is farthest away from Earth in its elliptical orbit.

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

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

Sound waves can’t travel through the vacuum of space. They need a medium (like air or water) to travel because they are vibrations of particles. Space is a vacuum with almost no particles, so sound cannot travel through it.

And while it might seem charming to not only see – but also hear the universe around us – mostly what we’d hear is the sound of the sun screaming.

If sound waves could travel through space, we’d hear the sun roaring. That roar would pound our ears at about 100 decibels. It’d be like standing next to Niagara Falls all day long. It’d only be as night fell, and we turned away from the sun, that we’d get some peace and quiet.

Animation of a solar flare.
A view of the sun producing an X (strong) flare on June 30, 2026. Read our daily sun news here. Image via NOAA.

4. That roar would linger

But what if you could hear the sun, and it suddenly disappeared? In that case, the light from it would be gone in eight minutes. But the sound from the sun would continue for 13 years.

Light traveling from the sun to Earth takes 8 minutes to reach us. But light is more than 850,000 times faster than sound. So if sound could similarly travel through space, what we hear at this moment is really closer to 13 years old.

So it’d take eight minutes to see the sun wink out. But its roar would continue for 13 years.

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

Stars are born, evolve and die, just like humans. Some of the stars we see now didn’t exist during the Age of Dinosaurs, from about 252 million to 66 million years ago.

So when the dinosaurs looked up at the night sky, they saw different stars and constellations than we see now.

Consider the constellation Orion the Hunter. Its famous bright blue star Rigel is just 8 million years old. And its famous red star Betelgeuse – marking Orion’s shoulder – is only 10 million years old.

If they ever looked up, the dinosaurs couldn’t have seen the figure of Orion. Likewise, they never saw the Big Dipper, or the Teapot of Sagittarius.

And, also, remember, our solar system is orbiting the center of our Milky Way galaxy. So during the height of the dinosaurs’ rein, Earth was on the opposite side of the galaxy from now.

6. Galaxies collide, but stars don’t (usually)

You might have already guessed it from mind-blowing fact number two, but there is a lot of space in space.

In fact, there’s so much space between things in our universe that even though the Milky Way and Andromeda galaxies might collide and merge one day, it’s unlikely that any of stars (or planets) will collide.

Instead, when Andromeda and the Milky Way collide, they’ll pass through one another like ghosts.

The galaxies themselves won’t be unaffected, though. The collision will distort their shapes. Plus, collisions between clouds of gas and dust in the two galaxies are expected to ignite bursts of new star formation!

Source: EarthSky

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

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

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

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

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

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

So what is the observable universe? It’s all the light we can see in the universe.

And although light is speedy, it still has its limits. We can only see light that has had time to reach Earth since it was emitted.

So while the universe might be infinite, our view of it is not. Our view of the universe stretches in every direction around us for about 46.5 billion light-years. That means the total width of the observable universe from one side of us to the other is 93 billion light-years wide. But we measure the observable universe at nearly 14 billion years old, starting with the Big Bang.

So how can the observable universe be wider than the universe is old? It’s because the universe has been expanding throughout the time the light has been traveling.

Light from the most distant objects has been on its way for about 13.8 billion years. But, during that time, the space between those objects and us has stretched. As a result, those objects are now about 46.5 billion light-years away, even though their light has been traveling for only 13.8 billion years.

9. Most of the universe will move beyond our sight

If we look far, far into the future, our view from the Milky Way galaxy will become increasingly limited by the expanding universe. Astronomers call the ultimate boundary of what we can ever observe the cosmic event horizon. Because light travels at a finite speed and the expansion of the universe is accelerating, there are regions of space whose light will never reach us.

Over time, galaxies that are not gravitationally bound to our own will recede ever farther away. Eventually, the light from those galaxies will become so stretched and faint that we will no longer be able to see them. In fact, the universe’s expansion has been accelerating for about the last 5 billion years. As Katie Mack explains in her book The End of Everything:

As the expansion of the universe accelerates, galaxies that are currently inside our Hubble radius will be outside it. Eventually, no galaxies outside our Local Group will be visible.

Someday, every galaxy beyond our Local Group will disappear from view, leaving future astronomers with no direct evidence that the vast universe we see today ever existed.

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

Read our daily sun news

New map of Andromeda galaxy and its colossal ecosystem

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



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

EarthSky isn’t powered by billionaires. We’re powered by you. Support EarthSky’s 2026 Donation Campaign and help keep science accessible.

9 mind-blowing space facts that will shock you

Almost everything about outer space is amazing, from what we might find on Earth’s moon to the visible boundary of our universe … it can all leave you scratching your head. Here are nine truly mind-blowing facts about our Earth, sun, solar system and universe. Enjoy … and share (you’ll be a hit at your next dinner party).

1. There might be dinosaur fossils on the moon

Some 65 million years ago, an asteroid hurtled toward Earth. When it hit, it triggered a mass extinction, ending the rein of the dinosaurs. At that time, dinosaurs had already been around for some 200 million years. So, many generations had already died and their bones had become fossilized in earthly rocks.

And, when the dinosaur-killing asteroid hit Earth, it impacted so violently that some of the rocks jettisoned from the impact flew into space. And it’s possible some of those rocks with fossilized dinosaurs might have ultimately ended up on the moon, colliding with it in much the same way a SpaceX rocket is colliding with the moon tonight, August 5, 2026.

So there could be rocks with dinosaur fossils on the moon!

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

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

The distance between objects in space is vast. As an example of this, if you took all the other planets in the solar system, you could pack them tightly between Earth and the moon.

There are a couple of caveats here. First, we are stacking the planets pole to pole so we don’t have to worry about Saturn’s rings.

Second, we’re performing this feat during apogee, or when the moon is farthest away from Earth in its elliptical orbit.

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

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

Sound waves can’t travel through the vacuum of space. They need a medium (like air or water) to travel because they are vibrations of particles. Space is a vacuum with almost no particles, so sound cannot travel through it.

And while it might seem charming to not only see – but also hear the universe around us – mostly what we’d hear is the sound of the sun screaming.

If sound waves could travel through space, we’d hear the sun roaring. That roar would pound our ears at about 100 decibels. It’d be like standing next to Niagara Falls all day long. It’d only be as night fell, and we turned away from the sun, that we’d get some peace and quiet.

Animation of a solar flare.
A view of the sun producing an X (strong) flare on June 30, 2026. Read our daily sun news here. Image via NOAA.

4. That roar would linger

But what if you could hear the sun, and it suddenly disappeared? In that case, the light from it would be gone in eight minutes. But the sound from the sun would continue for 13 years.

Light traveling from the sun to Earth takes 8 minutes to reach us. But light is more than 850,000 times faster than sound. So if sound could similarly travel through space, what we hear at this moment is really closer to 13 years old.

So it’d take eight minutes to see the sun wink out. But its roar would continue for 13 years.

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

Stars are born, evolve and die, just like humans. Some of the stars we see now didn’t exist during the Age of Dinosaurs, from about 252 million to 66 million years ago.

So when the dinosaurs looked up at the night sky, they saw different stars and constellations than we see now.

Consider the constellation Orion the Hunter. Its famous bright blue star Rigel is just 8 million years old. And its famous red star Betelgeuse – marking Orion’s shoulder – is only 10 million years old.

If they ever looked up, the dinosaurs couldn’t have seen the figure of Orion. Likewise, they never saw the Big Dipper, or the Teapot of Sagittarius.

And, also, remember, our solar system is orbiting the center of our Milky Way galaxy. So during the height of the dinosaurs’ rein, Earth was on the opposite side of the galaxy from now.

6. Galaxies collide, but stars don’t (usually)

You might have already guessed it from mind-blowing fact number two, but there is a lot of space in space.

In fact, there’s so much space between things in our universe that even though the Milky Way and Andromeda galaxies might collide and merge one day, it’s unlikely that any of stars (or planets) will collide.

Instead, when Andromeda and the Milky Way collide, they’ll pass through one another like ghosts.

The galaxies themselves won’t be unaffected, though. The collision will distort their shapes. Plus, collisions between clouds of gas and dust in the two galaxies are expected to ignite bursts of new star formation!

Source: EarthSky

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

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

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

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

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

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

So what is the observable universe? It’s all the light we can see in the universe.

And although light is speedy, it still has its limits. We can only see light that has had time to reach Earth since it was emitted.

So while the universe might be infinite, our view of it is not. Our view of the universe stretches in every direction around us for about 46.5 billion light-years. That means the total width of the observable universe from one side of us to the other is 93 billion light-years wide. But we measure the observable universe at nearly 14 billion years old, starting with the Big Bang.

So how can the observable universe be wider than the universe is old? It’s because the universe has been expanding throughout the time the light has been traveling.

Light from the most distant objects has been on its way for about 13.8 billion years. But, during that time, the space between those objects and us has stretched. As a result, those objects are now about 46.5 billion light-years away, even though their light has been traveling for only 13.8 billion years.

9. Most of the universe will move beyond our sight

If we look far, far into the future, our view from the Milky Way galaxy will become increasingly limited by the expanding universe. Astronomers call the ultimate boundary of what we can ever observe the cosmic event horizon. Because light travels at a finite speed and the expansion of the universe is accelerating, there are regions of space whose light will never reach us.

Over time, galaxies that are not gravitationally bound to our own will recede ever farther away. Eventually, the light from those galaxies will become so stretched and faint that we will no longer be able to see them. In fact, the universe’s expansion has been accelerating for about the last 5 billion years. As Katie Mack explains in her book The End of Everything:

As the expansion of the universe accelerates, galaxies that are currently inside our Hubble radius will be outside it. Eventually, no galaxies outside our Local Group will be visible.

Someday, every galaxy beyond our Local Group will disappear from view, leaving future astronomers with no direct evidence that the vast universe we see today ever existed.

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

Read our daily sun news

New map of Andromeda galaxy and its colossal ecosystem

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Perseid meteor shower 2026: All you need to know

Star chart with constellations Cassiopeia and Perseus with radial arrows between them.
The annual Perseid meteors radiate from a point in the constellation Perseus the Hero. In August, the radiant of the Perseid meteor shower rises in late evening and is highest at dawn.

Perseids peak mornings August 12 and 13

Predicted peak: The peak is predicted** for 14:53 UTC on August 13, 2026. So the mornings of August 12 and 13 are probably your best bets. August 14 might be good as well, but be aware that the Perseids tend to fall off rapidly after their peak.
When to watch: The moon will be a new moon during 2026’s peak of the Perseid meteor shower. So you’ll have dark skies for meteor viewing. This shower rises to a peak gradually, then falls off rapidly. And Perseid meteors tend to strengthen in number as late night deepens into the wee hours before dawn. The shower is often best just before dawn.
Radiant: The radiant rises late in the evening and is highest at dawn. See the chart above.
Nearest moon phase: The new moon falls at 17:37 UTC on August 12. In fact, those lucky enough to be observing the August 12 total solar eclipse, might see some Perseids during totality.
Duration of shower: July 14 to September 1. This time period is when we’re passing through the meteor stream in space!
Expected meteors at peak, under ideal conditions: Under a dark sky with no moon, skywatchers frequently report 90 meteors per hour, or more. In 2026, you’ll have a moonless sky to watch for Perseids. The August Perseid meteor shower is rich and steady, from early August through the peak. The meteors are colorful and many of them are bright. And they frequently leave persistent trains. All of these factors make the Perseid shower perhaps the most beloved meteor shower for the Northern Hemisphere.

Report a fireball (very bright meteor) to the American Meteor Society: it’s fun and easy!

Diagram: Perseus, Andromeda and Pegasus above the horizon with a meteors streaking away from Perseus with explanatory text.
The view looking toward the east-northeast horizon during the Perseid meteor shower. In 2026, the best time to watch is the after midnight through dawn on the mornings of August 12 and 13. You’ll have dark skies for meteor viewing. Image via Guy Ottewell’s Astronomical Calendar 2026. Used with permission.

Perseid meteor shower radiant point

Around the peak mornings, if you trace all the Perseid meteors backward, they seem to come from the constellation Perseus near the famous Double Cluster. Hence, the meteor shower is named in honor of the constellation Perseus the Hero.

Diagram of Earth globe with lines toward location of moon, sun, and direction the meteors are coming in.
Diagram of the 2026 Perseid meteor shower as seen from above the Earth’s surface, looking down. Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.

Of course, there’s no real connection between the meteor shower radiant and the constellation Perseus. The stars in Perseus are many light-years distant, while these meteors burn up about 60 miles (100 km) above the Earth’s surface.

The Perseids’ parent comet

From the late, great Don Machholz (1952-2022), who discovered 12 comets …

The parent comet responsible for the Perseid meteor shower is a rather large comet called 109P/Swift-Tuttle. The comet orbits the sun approximately every 133 years. Lewis Swift of Marathon, New York, visually discovered it on July 16, 1862, using an 11-centimeter (4.3-inch) refractor lens telescope. He did not report it immediately, believing that he was observing Comet Schmidt, which was found two weeks prior. Then, three days later, Horace Tuttle picked it up from Harvard Observatory. Scientists calculated that the comet would return in 120 years. That is, that we would see it again in 1982.

So, 1982 came and went. And the comet didn’t show up. Oops! It was back to the drawing board, and this time, the appearance of a comet observed in 1737 was considered a possible early appearance of the comet. Now, the orbital period was more like 130 years. Brian Marsden published new orbital elements and an ephemeris as to where to find it for its 1992 return.

In the 1980s, many of us visual comet hunters would, from time to time, cover the part of the sky where the incoming comet was supposed to appear. The 1991 outburst of Perseid meteors indicated that the comet was probably on its way back. Another meteor outburst in 1992 seemed to confirm that.

On September 26, 1992, Tsuruhiko Kiuchi, an amateur astronomer and comet hunter, picked up the comet in the evening sky just north of the bowl of the Big Dipper. Knowing where to look, I observed this comet 16 hours later and made a brightness estimate 5 times brighter than the original report. Others then confirmed this. Later, Gary Kronk suggested that the comets observed in 69 BCE and 188 CE were also appearances of this comet, a theory later confirmed.

Do Perseid meteors ever hit the ground?

Meteors that hit the ground intact are called meteorites. But few – if any – meteors in annual showers become meteorites. That’s primarily because of the flimsy nature of cometary debris. Comets are made of ices. Most meteorites, on the other hand, are the remains of rocky or metallic asteroids.

In ancient Greek star lore, Perseus is the son of the god Zeus and the mortal Danaë. It was said that the Perseid shower commemorates the time when Zeus visited Danaë, the mother of Perseus, in a shower of gold.

So think of the ephemeral nature of meteors in meteor showers, as you stand outside watching for Perseids in 2025. Most meteors strike Earth’s atmosphere unseen. You can consider any Perseid meteor you do see in 2025 as there for your viewing pleasure!

By the way, 2023 was a fantastic year for the Perseids: Enjoy this gallery of Perseid meteor photos from around the world, 2023.

A few Perseid meteor shower photos from EarthSky’s community

Long, thin, bright streak of light behind broken clouds, lighting them up.
View at EarthSky Community Photos. | Joel Coombs in Pahranagat National Wildlife Refuge, Nevada, captured this photo of a fireball on August 12, 2021. He wrote: “2 Perseids in 1 shot and 1 is a fireball. Went up to Upper Pahranagat Lake in hopes of getting a couple shots of the Perseids. With thunderstorms building all day, I wasn’t very hopeful. Clouds were rolling through all night, but there were clearings here and there. Just as the clouds were coming back I got to see this.” Thank you, Joel!
Night sky with the cloudy, dim Way and a very long, thin glowing white streak parallel to it.
View at EarthSky Community Photos. | Peter Ryan in Point Judith, Rhode Island, captured this photo of a Perseid with the Milky Way on August 13, 2021, and wrote: “A single Perseid meteor alongside the Milky Way.” Thank you, Peter!

More Perseid meteor shower photos from EarthSky’s community

Blue sky with many stars and a long streak in the middle. There is a tree without leaves at the bottom.
View at EarthSky Community Photos. | Riste Spiroski shared this shot from Ohrid, Macedonia, and wrote: “We spent about 2 hours planning this shot and were lucky to catch it while enjoying the Perseid meteor shower, seeing over 10 bright meteors in less than an hour.” Awesome! Thank you.
A few clouds and a thin, long, very bright meteor trail streaking across center of starry sky.
View at EarthSky Community Photos. | Joel Weatherly in Edmonton, Alberta, Canada, captured this photo of a meteor on August 12, 2021. He wrote: “Here’s a photo of a bright Perseid meteor I caught streaking across the sky last night. This meteor sported a brilliant green hue and even left a faint persistent train.” Thank you, Joel!
Bright streak of light with two glowing bulges in night sky above mountains.
View at EarthSky Community Photos. | Garth Battista of Halcottsville, New York, took this photo of a Perseid meteor over the Catskill Mountains on August 13, 2020. Thank you, Garth!

Bottom line: The Perseid meteor shower will peak around the mornings of August 13 in 2026. And you’ll have dark skies to watch this year’s Perseid meteors.

**Predicted peak times and dates for meteor showers are from the American Meteor Society. Note that meteor shower peak times can vary.

EarthSky’s meteor shower guide

Meteor showers: Tips for watching the show

Learn how to shoot photos of meteors

The post Perseid meteor shower 2026: All you need to know first appeared on EarthSky.



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Star chart with constellations Cassiopeia and Perseus with radial arrows between them.
The annual Perseid meteors radiate from a point in the constellation Perseus the Hero. In August, the radiant of the Perseid meteor shower rises in late evening and is highest at dawn.

Perseids peak mornings August 12 and 13

Predicted peak: The peak is predicted** for 14:53 UTC on August 13, 2026. So the mornings of August 12 and 13 are probably your best bets. August 14 might be good as well, but be aware that the Perseids tend to fall off rapidly after their peak.
When to watch: The moon will be a new moon during 2026’s peak of the Perseid meteor shower. So you’ll have dark skies for meteor viewing. This shower rises to a peak gradually, then falls off rapidly. And Perseid meteors tend to strengthen in number as late night deepens into the wee hours before dawn. The shower is often best just before dawn.
Radiant: The radiant rises late in the evening and is highest at dawn. See the chart above.
Nearest moon phase: The new moon falls at 17:37 UTC on August 12. In fact, those lucky enough to be observing the August 12 total solar eclipse, might see some Perseids during totality.
Duration of shower: July 14 to September 1. This time period is when we’re passing through the meteor stream in space!
Expected meteors at peak, under ideal conditions: Under a dark sky with no moon, skywatchers frequently report 90 meteors per hour, or more. In 2026, you’ll have a moonless sky to watch for Perseids. The August Perseid meteor shower is rich and steady, from early August through the peak. The meteors are colorful and many of them are bright. And they frequently leave persistent trains. All of these factors make the Perseid shower perhaps the most beloved meteor shower for the Northern Hemisphere.

Report a fireball (very bright meteor) to the American Meteor Society: it’s fun and easy!

Diagram: Perseus, Andromeda and Pegasus above the horizon with a meteors streaking away from Perseus with explanatory text.
The view looking toward the east-northeast horizon during the Perseid meteor shower. In 2026, the best time to watch is the after midnight through dawn on the mornings of August 12 and 13. You’ll have dark skies for meteor viewing. Image via Guy Ottewell’s Astronomical Calendar 2026. Used with permission.

Perseid meteor shower radiant point

Around the peak mornings, if you trace all the Perseid meteors backward, they seem to come from the constellation Perseus near the famous Double Cluster. Hence, the meteor shower is named in honor of the constellation Perseus the Hero.

Diagram of Earth globe with lines toward location of moon, sun, and direction the meteors are coming in.
Diagram of the 2026 Perseid meteor shower as seen from above the Earth’s surface, looking down. Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.

Of course, there’s no real connection between the meteor shower radiant and the constellation Perseus. The stars in Perseus are many light-years distant, while these meteors burn up about 60 miles (100 km) above the Earth’s surface.

The Perseids’ parent comet

From the late, great Don Machholz (1952-2022), who discovered 12 comets …

The parent comet responsible for the Perseid meteor shower is a rather large comet called 109P/Swift-Tuttle. The comet orbits the sun approximately every 133 years. Lewis Swift of Marathon, New York, visually discovered it on July 16, 1862, using an 11-centimeter (4.3-inch) refractor lens telescope. He did not report it immediately, believing that he was observing Comet Schmidt, which was found two weeks prior. Then, three days later, Horace Tuttle picked it up from Harvard Observatory. Scientists calculated that the comet would return in 120 years. That is, that we would see it again in 1982.

So, 1982 came and went. And the comet didn’t show up. Oops! It was back to the drawing board, and this time, the appearance of a comet observed in 1737 was considered a possible early appearance of the comet. Now, the orbital period was more like 130 years. Brian Marsden published new orbital elements and an ephemeris as to where to find it for its 1992 return.

In the 1980s, many of us visual comet hunters would, from time to time, cover the part of the sky where the incoming comet was supposed to appear. The 1991 outburst of Perseid meteors indicated that the comet was probably on its way back. Another meteor outburst in 1992 seemed to confirm that.

On September 26, 1992, Tsuruhiko Kiuchi, an amateur astronomer and comet hunter, picked up the comet in the evening sky just north of the bowl of the Big Dipper. Knowing where to look, I observed this comet 16 hours later and made a brightness estimate 5 times brighter than the original report. Others then confirmed this. Later, Gary Kronk suggested that the comets observed in 69 BCE and 188 CE were also appearances of this comet, a theory later confirmed.

Do Perseid meteors ever hit the ground?

Meteors that hit the ground intact are called meteorites. But few – if any – meteors in annual showers become meteorites. That’s primarily because of the flimsy nature of cometary debris. Comets are made of ices. Most meteorites, on the other hand, are the remains of rocky or metallic asteroids.

In ancient Greek star lore, Perseus is the son of the god Zeus and the mortal Danaë. It was said that the Perseid shower commemorates the time when Zeus visited Danaë, the mother of Perseus, in a shower of gold.

So think of the ephemeral nature of meteors in meteor showers, as you stand outside watching for Perseids in 2025. Most meteors strike Earth’s atmosphere unseen. You can consider any Perseid meteor you do see in 2025 as there for your viewing pleasure!

By the way, 2023 was a fantastic year for the Perseids: Enjoy this gallery of Perseid meteor photos from around the world, 2023.

A few Perseid meteor shower photos from EarthSky’s community

Long, thin, bright streak of light behind broken clouds, lighting them up.
View at EarthSky Community Photos. | Joel Coombs in Pahranagat National Wildlife Refuge, Nevada, captured this photo of a fireball on August 12, 2021. He wrote: “2 Perseids in 1 shot and 1 is a fireball. Went up to Upper Pahranagat Lake in hopes of getting a couple shots of the Perseids. With thunderstorms building all day, I wasn’t very hopeful. Clouds were rolling through all night, but there were clearings here and there. Just as the clouds were coming back I got to see this.” Thank you, Joel!
Night sky with the cloudy, dim Way and a very long, thin glowing white streak parallel to it.
View at EarthSky Community Photos. | Peter Ryan in Point Judith, Rhode Island, captured this photo of a Perseid with the Milky Way on August 13, 2021, and wrote: “A single Perseid meteor alongside the Milky Way.” Thank you, Peter!

More Perseid meteor shower photos from EarthSky’s community

Blue sky with many stars and a long streak in the middle. There is a tree without leaves at the bottom.
View at EarthSky Community Photos. | Riste Spiroski shared this shot from Ohrid, Macedonia, and wrote: “We spent about 2 hours planning this shot and were lucky to catch it while enjoying the Perseid meteor shower, seeing over 10 bright meteors in less than an hour.” Awesome! Thank you.
A few clouds and a thin, long, very bright meteor trail streaking across center of starry sky.
View at EarthSky Community Photos. | Joel Weatherly in Edmonton, Alberta, Canada, captured this photo of a meteor on August 12, 2021. He wrote: “Here’s a photo of a bright Perseid meteor I caught streaking across the sky last night. This meteor sported a brilliant green hue and even left a faint persistent train.” Thank you, Joel!
Bright streak of light with two glowing bulges in night sky above mountains.
View at EarthSky Community Photos. | Garth Battista of Halcottsville, New York, took this photo of a Perseid meteor over the Catskill Mountains on August 13, 2020. Thank you, Garth!

Bottom line: The Perseid meteor shower will peak around the mornings of August 13 in 2026. And you’ll have dark skies to watch this year’s Perseid meteors.

**Predicted peak times and dates for meteor showers are from the American Meteor Society. Note that meteor shower peak times can vary.

EarthSky’s meteor shower guide

Meteor showers: Tips for watching the show

Learn how to shoot photos of meteors

The post Perseid meteor shower 2026: All you need to know first appeared on EarthSky.



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Weaponizing Fraud: Trump Withholds Over $1B in Medicaid From California and Minnesota

Weaponizing Fraud: Trump Withholds Over $1B in Medicaid From California and Minnesota

The Trump administration announced on July 21, 2026, that it’s withholding US$867 million in federal healthcare funding for California and $200 million for Minnesota – a total of more than $1 billion.

Federal officials said the two states had failed to provide sufficient evidence that a number of disputed medical claims were legitimate. These include bills for in-home care and other services covered by the two states’ Medicaid programs for low-income residents.

Medicaid administrators say the funds can be recovered if the states supply the requested documentation. But the action is highly unusual: Typically, Medicaid officials partner with states to conduct an audit when they suspect fraud, a careful process that often takes years.

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Federal agents execute a search in December 2025 tied to potential Medicaid fraud in Bloomington, Minn. Christopher Juhn/Anadolu via Getty Images via The Conversation

It’s the second time in 2026 that the Trump administration has withheld or deferred federal Medicaid funds for several states, including California and Minnesota, because of alleged fraud and abuse. The Democratic governors of those states have called the decision a politically motivated attack on their constituents.

I’m a historian of social policy who led the first comprehensive historical overview of Medi-Cal, California’s statewide Medicaid system. I’ve found that U.S. leaders have long used the language of fraud and abuse to blur the line between correcting very real failures within Medicaid and – as I believe the Trump administration is currently doing – discrediting and defunding the program itself.

Who pays when Medicaid is cut? It affects children’s health care, nursing home care, disability services and health insurance.

Slashing the safety net

The Medicaid restrictions are part of the Trump administration’s overall efforts to slash federal funding for the safety net.

The large tax-and-spending bill that Trump signed into law in July 2025 as the cornerstone of his second-term agenda pared eligibility for Medicaid by introducing work requirements for some adults. It is cutting close to $1 trillion in federal spending on the program over the next decade.

Researchers estimate that almost 12 million people, on top of the estimated 28 million without health insurance in 2025, could become uninsured by 2034 due to these changes. By mid-2026, more than 3 million people had already lost their insurance coverage due to Republican changes to the Affordable Care Act.

‘Padlocking’ the ‘cookie jar’

In February 2026, Vice President JD Vance, Health Secretary Robert F. Kennedy Jr. and Dr. Mehmet Oz, the administrator of the Centers for Medicare & Medicaid Services, or CMS, announced a new anti-fraud initiative called Comprehensive Regulations to Uncover Suspicious Healthcare.

Also known by its rather unsubtle acronym, CRUSH, this initiative is taking unprecedented steps to withhold and defer funds in response to suspected fraud. “CMS is done trying to catch fraudsters with their hands in the cookie jar,” Oz said in announcing CRUSH’s formation. “Instead, we’re padlocking the jar and letting them starve.”

To be sure, Medicaid fraud, waste and abuse – such as providers billing Medicaid for services that are unnecessary or never rendered – are very real problems that cost taxpayers billions of dollars annually. They do divert funds from the low-income and disabled Americans enrolled in the program.

But the Trump administration’s latest moves are part of a much broader history of weaponizing Medicaid fraud and abuse – both real and imagined. I see them as a politicized attempt to prove that Medicaid itself is wasteful, that state governments cannot be trusted to administer federal money, and that public benefits inevitably invite dishonesty.

RFK Jr

Secretary of Health and Human Services Robert F. Kennedy Jr. speaks about alleged Medicaid fraud and charges in Minneapolis in May 2026. Christopher Juhn/Anadolu via Getty Images via The Conversation

Providing little oversight at the start

Medicaid was established, along with Medicare for older adults, in 1965 as part of President Lyndon B. Johnson’s “Great Society” reforms. Despite providing millions of Americans with health insurance coverage for the first time, these programs had few centralized mechanisms for the kind of federal oversight that could prevent and catch fraud and abuse.

And the sheer scale and complexity of the Medicaid system – joint federal-state funding, varying eligibility requirements, millions of enrollees and thousands of providers – created opportunities for questionable billing practices among providers.

The 1970s saw a number of highly publicized Medicaid scandals involving nursing homes, laboratories, pharmacies and so-called “Medicaid mills” – healthcare providers that sought to bill the government for large numbers of Medicaid patients for shoddy and often fraudulent care.

A series of high-profile congressional investigations spurred demand for stronger Medicaid oversight and enforcement. That led to the Medicare-Medicaid Anti-Fraud and Abuse Amendments of 1977, which established the national Medicaid Fraud Control Units program.

The state-run Medicaid Fraud Control Units received generous federal matching funds to investigate and prosecute fraud.

The most serious Medicaid fraud was generally committed by healthcare providers and contractors, not patients. Medicaid Fraud Control Units were principally responsible for investigating providers, while also prosecuting the abuse and neglect of patients whose care was billed to Medicaid.

At the same time, however, Medicaid was becoming entangled in a broader political debate over social spending, whether many Americans were becoming too dependent on government benefits, and the alleged use of benefits by people who should not have received them. In the 1980s and 1990s, widely circulated stories about Medicaid exposed fraud and malfeasance by providers.

But disproportionately, they also highlighted the comparatively few instances of fraud by people enrolled in the program, such as cases where they submitted false receipts for covered medically related travel or sold drugs they obtained through Medicaid for free or at low cost.

Using Medicare fraud to justify spending cuts

The distinction between Medicaid and cash assistance programs, such as the Aid to Families with Dependent Children “welfare” program, frequently disappeared in political rhetoric. False or exaggerated stories that portrayed African American single mothers living extravagantly while fraudulently claiming welfare benefits became potent symbols of supposed government failure.

While campaigning as a presidential candidate, Ronald Reagan seized on this trope of the welfare queen” in his attacks on social spending.

People line up at the Baltimore City Welfare Office in 1975

People line up at the Baltimore City Welfare Office in 1975, years before concerns about social spending led to big cuts to safety net programs. O'Halloran/Library of Congress via Getty Images via The Conversation

By the mid-1990s, opposition to welfare programs had become increasingly bipartisan. Politicians in both parties often used tales of Medicaid fraud on the part of providers and recipients to justify tighter eligibility rules and spending cuts.

Federal oversight expanded further with the Deficit Reduction Act of 2005, which created the Medicaid Integrity Program and strengthened federal oversight of state programs. The Affordable Care Act, the landmark healthcare legislation Congress passed in 2010, added new measures to screen providers and verify billing.

Concerns about Medicaid’s “integrity” became highly politicized in the debates surrounding the ACA. Critics of Medicaid expansion argued that increasing the number of people who could get health insurance through the program would increase fraud and improper enrollment. Supporters of expanding Medicaid to help more Americans gain health insurance maintained that anti-fraud rhetoric often disguised ideological opposition to the program’s expansion.

Blurring distinctions then and now

For the six decades that this program has helped millions of low-income Americans get healthcare, politicians have blurred the distinction between protecting Medicaid from abuse and using abuse to discredit Medicaid itself.

In my view, the Trump administration’s campaigns against California and Minnesota continue that pattern. It is using real weaknesses within Medicaid to advance much broader political arguments: that Democratic states cannot be trusted, that public benefits naturally invite abuse, and that withholding funds is itself a form of reform.

The result will no doubt be that fewer low-income Americans will be able to get the healthcare they need.

By Ben Zdencanovic, Assistant Professor of U.S. History, University of Cambridge. This article is republished from The Conversation under a Creative Commons license. Read the original article.

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Weaponizing Fraud: Trump Withholds Over $1B in Medicaid From California and Minnesota

The Trump administration announced on July 21, 2026, that it’s withholding US$867 million in federal healthcare funding for California and $200 million for Minnesota – a total of more than $1 billion.

Federal officials said the two states had failed to provide sufficient evidence that a number of disputed medical claims were legitimate. These include bills for in-home care and other services covered by the two states’ Medicaid programs for low-income residents.

Medicaid administrators say the funds can be recovered if the states supply the requested documentation. But the action is highly unusual: Typically, Medicaid officials partner with states to conduct an audit when they suspect fraud, a careful process that often takes years.

="" p="" height="400">

Federal agents execute a search in December 2025 tied to potential Medicaid fraud in Bloomington, Minn. Christopher Juhn/Anadolu via Getty Images via The Conversation

It’s the second time in 2026 that the Trump administration has withheld or deferred federal Medicaid funds for several states, including California and Minnesota, because of alleged fraud and abuse. The Democratic governors of those states have called the decision a politically motivated attack on their constituents.

I’m a historian of social policy who led the first comprehensive historical overview of Medi-Cal, California’s statewide Medicaid system. I’ve found that U.S. leaders have long used the language of fraud and abuse to blur the line between correcting very real failures within Medicaid and – as I believe the Trump administration is currently doing – discrediting and defunding the program itself.

Who pays when Medicaid is cut? It affects children’s health care, nursing home care, disability services and health insurance.

Slashing the safety net

The Medicaid restrictions are part of the Trump administration’s overall efforts to slash federal funding for the safety net.

The large tax-and-spending bill that Trump signed into law in July 2025 as the cornerstone of his second-term agenda pared eligibility for Medicaid by introducing work requirements for some adults. It is cutting close to $1 trillion in federal spending on the program over the next decade.

Researchers estimate that almost 12 million people, on top of the estimated 28 million without health insurance in 2025, could become uninsured by 2034 due to these changes. By mid-2026, more than 3 million people had already lost their insurance coverage due to Republican changes to the Affordable Care Act.

‘Padlocking’ the ‘cookie jar’

In February 2026, Vice President JD Vance, Health Secretary Robert F. Kennedy Jr. and Dr. Mehmet Oz, the administrator of the Centers for Medicare & Medicaid Services, or CMS, announced a new anti-fraud initiative called Comprehensive Regulations to Uncover Suspicious Healthcare.

Also known by its rather unsubtle acronym, CRUSH, this initiative is taking unprecedented steps to withhold and defer funds in response to suspected fraud. “CMS is done trying to catch fraudsters with their hands in the cookie jar,” Oz said in announcing CRUSH’s formation. “Instead, we’re padlocking the jar and letting them starve.”

To be sure, Medicaid fraud, waste and abuse – such as providers billing Medicaid for services that are unnecessary or never rendered – are very real problems that cost taxpayers billions of dollars annually. They do divert funds from the low-income and disabled Americans enrolled in the program.

But the Trump administration’s latest moves are part of a much broader history of weaponizing Medicaid fraud and abuse – both real and imagined. I see them as a politicized attempt to prove that Medicaid itself is wasteful, that state governments cannot be trusted to administer federal money, and that public benefits inevitably invite dishonesty.

RFK Jr

Secretary of Health and Human Services Robert F. Kennedy Jr. speaks about alleged Medicaid fraud and charges in Minneapolis in May 2026. Christopher Juhn/Anadolu via Getty Images via The Conversation

Providing little oversight at the start

Medicaid was established, along with Medicare for older adults, in 1965 as part of President Lyndon B. Johnson’s “Great Society” reforms. Despite providing millions of Americans with health insurance coverage for the first time, these programs had few centralized mechanisms for the kind of federal oversight that could prevent and catch fraud and abuse.

And the sheer scale and complexity of the Medicaid system – joint federal-state funding, varying eligibility requirements, millions of enrollees and thousands of providers – created opportunities for questionable billing practices among providers.

The 1970s saw a number of highly publicized Medicaid scandals involving nursing homes, laboratories, pharmacies and so-called “Medicaid mills” – healthcare providers that sought to bill the government for large numbers of Medicaid patients for shoddy and often fraudulent care.

A series of high-profile congressional investigations spurred demand for stronger Medicaid oversight and enforcement. That led to the Medicare-Medicaid Anti-Fraud and Abuse Amendments of 1977, which established the national Medicaid Fraud Control Units program.

The state-run Medicaid Fraud Control Units received generous federal matching funds to investigate and prosecute fraud.

The most serious Medicaid fraud was generally committed by healthcare providers and contractors, not patients. Medicaid Fraud Control Units were principally responsible for investigating providers, while also prosecuting the abuse and neglect of patients whose care was billed to Medicaid.

At the same time, however, Medicaid was becoming entangled in a broader political debate over social spending, whether many Americans were becoming too dependent on government benefits, and the alleged use of benefits by people who should not have received them. In the 1980s and 1990s, widely circulated stories about Medicaid exposed fraud and malfeasance by providers.

But disproportionately, they also highlighted the comparatively few instances of fraud by people enrolled in the program, such as cases where they submitted false receipts for covered medically related travel or sold drugs they obtained through Medicaid for free or at low cost.

Using Medicare fraud to justify spending cuts

The distinction between Medicaid and cash assistance programs, such as the Aid to Families with Dependent Children “welfare” program, frequently disappeared in political rhetoric. False or exaggerated stories that portrayed African American single mothers living extravagantly while fraudulently claiming welfare benefits became potent symbols of supposed government failure.

While campaigning as a presidential candidate, Ronald Reagan seized on this trope of the welfare queen” in his attacks on social spending.

People line up at the Baltimore City Welfare Office in 1975

People line up at the Baltimore City Welfare Office in 1975, years before concerns about social spending led to big cuts to safety net programs. O'Halloran/Library of Congress via Getty Images via The Conversation

By the mid-1990s, opposition to welfare programs had become increasingly bipartisan. Politicians in both parties often used tales of Medicaid fraud on the part of providers and recipients to justify tighter eligibility rules and spending cuts.

Federal oversight expanded further with the Deficit Reduction Act of 2005, which created the Medicaid Integrity Program and strengthened federal oversight of state programs. The Affordable Care Act, the landmark healthcare legislation Congress passed in 2010, added new measures to screen providers and verify billing.

Concerns about Medicaid’s “integrity” became highly politicized in the debates surrounding the ACA. Critics of Medicaid expansion argued that increasing the number of people who could get health insurance through the program would increase fraud and improper enrollment. Supporters of expanding Medicaid to help more Americans gain health insurance maintained that anti-fraud rhetoric often disguised ideological opposition to the program’s expansion.

Blurring distinctions then and now

For the six decades that this program has helped millions of low-income Americans get healthcare, politicians have blurred the distinction between protecting Medicaid from abuse and using abuse to discredit Medicaid itself.

In my view, the Trump administration’s campaigns against California and Minnesota continue that pattern. It is using real weaknesses within Medicaid to advance much broader political arguments: that Democratic states cannot be trusted, that public benefits naturally invite abuse, and that withholding funds is itself a form of reform.

The result will no doubt be that fewer low-income Americans will be able to get the healthcare they need.

By Ben Zdencanovic, Assistant Professor of U.S. History, University of Cambridge. This article is republished from The Conversation under a Creative Commons license. Read the original article.

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