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The night sky in the time of the dinosaurs

Silhouette of two dinos at night with the stars and Milky Way behind them.
What did the night sky look like in the time of the dinosaurs? Image via Stephen Leonardi/ Pexels.

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

The night sky in the time of the dinosaurs

Step outside on a moonless night and gaze at the night sky. Your eyes will likely first seek out familiar patterns of stars, such as the constellations Orion the Hunter or Sagittarius the Archer. There are just certain sights that make a stargazer feel at home. But if you could travel back to the age of the dinosaurs, most of the familiar stars would be nowhere to be seen.

During the long reign of dinosaurs – from roughly 230 to 66 million years ago – the constellations we recognize today didn’t exist, at least not in their current forms. Stars are not only constantly being born and dying, they’re also always on the move. Just like our sun and its solar system, stars follow their own path through the Milky Way galaxy. And over millions of years, these differences can create a whole new starscape overhead.

The stars have changed in location over time

The stars the dinosaurs saw would not have been the same as the ones we see today. For starters, 100 million years ago, we would have been on the other side of the Milky Way galaxy. And all the other stars would have been following their own individual paths through our Milky Way. So while you might picture our galaxy as a spinning disk like a Frisbee, in reality, the stars aren’t anchored in the same exact locations. The stars drift closer and farther from each other. And the constellations morph into new configurations.

But some of the stars we currently know would at least have existed in the time of the dinosaurs. That includes stars such as Sirius and Vega. Sirius is about 200 to 300 million years old. And Vega is about 500 million years old. Where precisely they were that long ago in relation to us, however, is unclear.

Meanwhile, other stars such as Orion the Hunter’s Rigel and Betelgeuse are considerably younger. They didn’t come into existence until after the age of the dinosaurs. Rigel is a mere 8 million years old, and Betelgeuse is perhaps 10 million years old.


This video shows you how chaotic the motion of individual stars can be in the galaxy. This data is from the Gaia spacecraft and it shows the proper motions of 40,000 stars, all located within 326 light-years of the solar system. It follows stars from the present day out to 400,000 years into the future.

Focusing on Canis Major

When we talk about the skies the dinosaurs saw, that’s some 100 million years ago. And Sirius has existed for 200 to 300 million years. So let’s look at it and some other stars in Canis Major the Greater Dog as an example.

Sirius (Alpha Canis Majoris) is currently the brightest star in Earth’s nighttime sky. But, in fact, a couple other stars in Canis Major once shone much brighter than Sirius.

While stars appear bright to us partly because of their size, it’s also largely because of how close they are to us. Sirius is not a particularly massive star. It just happens to be nearby. And our distance to stars changes over time due to the motions of our solar system and the other stars.

Just 4.7 million years ago, a star that is now unremarkable in our sky – Epsilon Canis Majoris – was once as bright as Venus! At its brightest, Epsilon Canis Majoris was magnitude -3.99, when it was 34 light-years away from us. So, for a time, it was the brightest star in Earth’s night sky. Today, it shines at a decent magnitude 1.5 from a distance of 430 light-years.

Another star in Canis Major, Beta Canis Majoris, also got a turn at being the brightest star in our sky. Beta Canis Majoris was at its brightest 4.4 million years ago. At that time, it shone at magnitude -3.65 from a distance of 37 light-years.

Sirius, our current brightest star, shines at magnitude -1.46 from a distance of 8.6 light-years. It will continue to get a bit closer and brighter, maxxing out at magnitude -1.68 in 60,000 years, when it comes within 7.8 light-years of us.

Constellations and clusters in the time of the dinosaurs

So, it makes sense that if today’s stars were in different locations or not even in existence yet 100 million years ago, the constellations we see now would not have been the same constellations the dinosaurs saw. But what about other hallmarks of the sky, such as star clusters?

Well, for example, the Pleiades star cluster is a group of young, bright blue stars around 100 million years old. They would have still been forming during the age of the dinosaurs.

On the other hand, the Hyades star cluster – that V-shaped formation that makes up Taurus the Bull’s head – has been around for some 750 million years. But it would have been in a different configuration as the stars drifted into their current locations relative to each other. And, as for all stars and star clusters, they are not moving along with us through the galaxy. They chart their own course.

Something familiar! The Milky Way

The glowing band of the Milky Way would still have stretched across the sky. This hazy river of light formed by billions of distant stars has been around much longer than the dinosaurs. And its overall appearance to the unaided eye wouldn’t have changed dramatically over 100 million years. It’s just the brightest and nearest stars themselves that would have been different. But the background glow of our galaxy in the age of the dinosaurs would at least be a familiar sight to us.

See the best Milky Way photos of 2025 here

Colorful core of the Milky Way standing tall over the dark landscape.
View at EarthSky Community Photos. | Steve Price in The Knolls, Utah, captured this image on August 26, 2022. Thank you, Steve!

Our solar system in the age of the dinosaurs

The planets themselves, as little dots of light in the night sky, would have looked relatively the same. But if dinosaurs had been clever and “handy” enough to invent the telescope, a closeup look at Saturn would have been quite different. Astronomers think Saturn’s ring system is only about 10 to 100 million years old. So the dinosaurs most likely wouldn’t have seen rings around Saturn, had they been able to see the planet that closely.

The moon would have been slightly different in the age of the dinosaurs as well. It would have been just a bit closer to Earth 100 million years ago, so it would have appeared a bit larger in our sky. And, therefore, total solar eclipses would have lasted a little longer.

Another cool feature dinosaurs would have seen on the moon: erupting volcanoes! This information comes from China’s Chang’e 5 mission over the past couple years. Researchers discovered tiny glass beads in lunar samples brought back to Earth. And analysis of the beads indicates volcanoes were erupting on the moon as recently as 120 million years ago, while dinosaurs were still roaming Earth. What a sight that must have been.

No artificial light pollution and no satellites

Dinosaurs would have been looking at an exquisitely pure and dark night sky. There were no artificial lights or satellites or even airplanes marring the majestic night. The skies at night, especially during new moon, would have been dramatically dark. Meteor showers and auroras would have been some great options for nighttime entertainment after the skies grew dark.

The Milky Way could have cast shadows of the dinos as they lumbered across the landscape. Compare that to today, where, as recently as 2016, scientists in the journal Science Advances said that nearly 80% of U.S. citizens can’t even see the Milky Way due to light pollution.

If you’re ever offered a chance to ride in a time machine back to the age of the dinosaurs, don’t forget to stop and admire the stars.

A T-rex dino with the Milky Way behind him.
The night sky in the time of the dinosaurs would have looked somewhat different than we see today. Image via Jake Fagan/ Unsplash.

Bottom line: The night sky in the time of the dinosaurs would have looked much different than today’s. Some famous stars had not yet been born, while familiar features, such as the moon, would have been closer and still volcanically active.

Read more: Our sun might be a migrant from the inner Milky Way

Read more: Which Milky Way spiral arm contains our sun?

The post The night sky in the time of the dinosaurs first appeared on EarthSky.



from EarthSky https://ift.tt/nDzMHFs
Silhouette of two dinos at night with the stars and Milky Way behind them.
What did the night sky look like in the time of the dinosaurs? Image via Stephen Leonardi/ Pexels.

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

The night sky in the time of the dinosaurs

Step outside on a moonless night and gaze at the night sky. Your eyes will likely first seek out familiar patterns of stars, such as the constellations Orion the Hunter or Sagittarius the Archer. There are just certain sights that make a stargazer feel at home. But if you could travel back to the age of the dinosaurs, most of the familiar stars would be nowhere to be seen.

During the long reign of dinosaurs – from roughly 230 to 66 million years ago – the constellations we recognize today didn’t exist, at least not in their current forms. Stars are not only constantly being born and dying, they’re also always on the move. Just like our sun and its solar system, stars follow their own path through the Milky Way galaxy. And over millions of years, these differences can create a whole new starscape overhead.

The stars have changed in location over time

The stars the dinosaurs saw would not have been the same as the ones we see today. For starters, 100 million years ago, we would have been on the other side of the Milky Way galaxy. And all the other stars would have been following their own individual paths through our Milky Way. So while you might picture our galaxy as a spinning disk like a Frisbee, in reality, the stars aren’t anchored in the same exact locations. The stars drift closer and farther from each other. And the constellations morph into new configurations.

But some of the stars we currently know would at least have existed in the time of the dinosaurs. That includes stars such as Sirius and Vega. Sirius is about 200 to 300 million years old. And Vega is about 500 million years old. Where precisely they were that long ago in relation to us, however, is unclear.

Meanwhile, other stars such as Orion the Hunter’s Rigel and Betelgeuse are considerably younger. They didn’t come into existence until after the age of the dinosaurs. Rigel is a mere 8 million years old, and Betelgeuse is perhaps 10 million years old.


This video shows you how chaotic the motion of individual stars can be in the galaxy. This data is from the Gaia spacecraft and it shows the proper motions of 40,000 stars, all located within 326 light-years of the solar system. It follows stars from the present day out to 400,000 years into the future.

Focusing on Canis Major

When we talk about the skies the dinosaurs saw, that’s some 100 million years ago. And Sirius has existed for 200 to 300 million years. So let’s look at it and some other stars in Canis Major the Greater Dog as an example.

Sirius (Alpha Canis Majoris) is currently the brightest star in Earth’s nighttime sky. But, in fact, a couple other stars in Canis Major once shone much brighter than Sirius.

While stars appear bright to us partly because of their size, it’s also largely because of how close they are to us. Sirius is not a particularly massive star. It just happens to be nearby. And our distance to stars changes over time due to the motions of our solar system and the other stars.

Just 4.7 million years ago, a star that is now unremarkable in our sky – Epsilon Canis Majoris – was once as bright as Venus! At its brightest, Epsilon Canis Majoris was magnitude -3.99, when it was 34 light-years away from us. So, for a time, it was the brightest star in Earth’s night sky. Today, it shines at a decent magnitude 1.5 from a distance of 430 light-years.

Another star in Canis Major, Beta Canis Majoris, also got a turn at being the brightest star in our sky. Beta Canis Majoris was at its brightest 4.4 million years ago. At that time, it shone at magnitude -3.65 from a distance of 37 light-years.

Sirius, our current brightest star, shines at magnitude -1.46 from a distance of 8.6 light-years. It will continue to get a bit closer and brighter, maxxing out at magnitude -1.68 in 60,000 years, when it comes within 7.8 light-years of us.

Constellations and clusters in the time of the dinosaurs

So, it makes sense that if today’s stars were in different locations or not even in existence yet 100 million years ago, the constellations we see now would not have been the same constellations the dinosaurs saw. But what about other hallmarks of the sky, such as star clusters?

Well, for example, the Pleiades star cluster is a group of young, bright blue stars around 100 million years old. They would have still been forming during the age of the dinosaurs.

On the other hand, the Hyades star cluster – that V-shaped formation that makes up Taurus the Bull’s head – has been around for some 750 million years. But it would have been in a different configuration as the stars drifted into their current locations relative to each other. And, as for all stars and star clusters, they are not moving along with us through the galaxy. They chart their own course.

Something familiar! The Milky Way

The glowing band of the Milky Way would still have stretched across the sky. This hazy river of light formed by billions of distant stars has been around much longer than the dinosaurs. And its overall appearance to the unaided eye wouldn’t have changed dramatically over 100 million years. It’s just the brightest and nearest stars themselves that would have been different. But the background glow of our galaxy in the age of the dinosaurs would at least be a familiar sight to us.

See the best Milky Way photos of 2025 here

Colorful core of the Milky Way standing tall over the dark landscape.
View at EarthSky Community Photos. | Steve Price in The Knolls, Utah, captured this image on August 26, 2022. Thank you, Steve!

Our solar system in the age of the dinosaurs

The planets themselves, as little dots of light in the night sky, would have looked relatively the same. But if dinosaurs had been clever and “handy” enough to invent the telescope, a closeup look at Saturn would have been quite different. Astronomers think Saturn’s ring system is only about 10 to 100 million years old. So the dinosaurs most likely wouldn’t have seen rings around Saturn, had they been able to see the planet that closely.

The moon would have been slightly different in the age of the dinosaurs as well. It would have been just a bit closer to Earth 100 million years ago, so it would have appeared a bit larger in our sky. And, therefore, total solar eclipses would have lasted a little longer.

Another cool feature dinosaurs would have seen on the moon: erupting volcanoes! This information comes from China’s Chang’e 5 mission over the past couple years. Researchers discovered tiny glass beads in lunar samples brought back to Earth. And analysis of the beads indicates volcanoes were erupting on the moon as recently as 120 million years ago, while dinosaurs were still roaming Earth. What a sight that must have been.

No artificial light pollution and no satellites

Dinosaurs would have been looking at an exquisitely pure and dark night sky. There were no artificial lights or satellites or even airplanes marring the majestic night. The skies at night, especially during new moon, would have been dramatically dark. Meteor showers and auroras would have been some great options for nighttime entertainment after the skies grew dark.

The Milky Way could have cast shadows of the dinos as they lumbered across the landscape. Compare that to today, where, as recently as 2016, scientists in the journal Science Advances said that nearly 80% of U.S. citizens can’t even see the Milky Way due to light pollution.

If you’re ever offered a chance to ride in a time machine back to the age of the dinosaurs, don’t forget to stop and admire the stars.

A T-rex dino with the Milky Way behind him.
The night sky in the time of the dinosaurs would have looked somewhat different than we see today. Image via Jake Fagan/ Unsplash.

Bottom line: The night sky in the time of the dinosaurs would have looked much different than today’s. Some famous stars had not yet been born, while familiar features, such as the moon, would have been closer and still volcanically active.

Read more: Our sun might be a migrant from the inner Milky Way

Read more: Which Milky Way spiral arm contains our sun?

The post The night sky in the time of the dinosaurs first appeared on EarthSky.



from EarthSky https://ift.tt/nDzMHFs

Ancestors of mammals laid eggs, says new fossil evidence

A grey drawing of an embryo in a shell. This fossil is evidence that the ancestors of mammals laid eggs.
Artist’s concept of the embryonic Lystrosaurus in its shell. The reconstruction is based on a fossil found in South Africa. It’s evidence that the ancestors of mammals laid eggs. Image via Sophie Vrard and Julien Benoit/ University of the Witwatersrand.
  • A 250-million-year-old fossil of an embryonic Lystrosaurus — an extinct animal that’s an ancestor of mammals — shows these creatures laid eggs.
  • Lystrosaurus, a piglike herbivore with a turtlelike beak and tusks, survived Earth’s worst mass extinction at the end of the Permian Epoch.
  • Advanced CT scanning revealed the tiny skeleton inside a rock nodule. And it had characteristics that confirmed the animal died before hatching.

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

CT scans of a rock nodule reveal a tiny skeleton

When researchers found a 250-million-year-old rock nodule with bits of fossil bone on its surface, they were curious to know what was inside. So they used advanced x-ray CT scans to study the rock’s interior. What they discovered was a tiny curled-up skeleton, tightly packed as if inside an egg. It was an embryonic Lystrosaurus, an animal that’s an evolutionary ancestor of mammals. The team said on April 9, 2026, that this fossil is strong evidence that the precursors to mammals laid eggs, instead of giving birth to live offspring.

Co-author Jennifer Botha of the University of the Witwatersrand said:

This fossil was discovered during a field excursion I led in 2008, nearly 17 years ago. My preparator and exceptional fossil finder, John Nyaphuli, identified a small nodule that at first revealed only tiny flecks of bone. As he carefully prepared the specimen, it became clear that it was a perfectly curled-up Lystrosaurus hatchling. I suspected even then that it had died within the egg, but at the time, we simply didn’t have the technology to confirm it.

The scientists published their study in the peer-reviewed journal PLOS One on April 9, 2026.

Lystrosaurus was a precursor to mammals

Lystrosaurus was a strange-looking beast. It had a sprawling piglike body, with a horny turtlelike beak on its head, as well as two tusklike teeth. These herbivorous creatures lived during the Late Permian and Early Triassic, approximately 259 to 247 million years ago.

At least four species of Lystrosaurus once roamed Pangea, an ancient supercontinent. Scientists have found fossils of these creatures in Antarctica, India, China, Mongolia, Russia and South Africa.

At the end of the Permian Epoch, about 252 million years ago, Earth underwent its most severe mass extinction. Major volcanic eruptions were the main triggers of this extinction. As a result, many animal species vanished forever. But Lystrosaurus survived and went on to thrive despite the unstable environment with hot conditions and long dry spells.

Scientists interested in mammalian reproduction have wondered if mammal ancestors gave birth to live young or laid eggs. They also wondered how they cared for their young. Most mammals today give birth to live young. But there’s a type of mammal called monotremes that lay eggs. They also nurse their young with milk. Monotremes – the platypus and four species of echidnas – are only found in Australia and New Guinea.

A grey-brown animal with a beak and two tusks.
This is an artist’s depiction of Lystrosaurus georgi. It’s 1 of at least 4 known species of Lystrosaurus. Image via Dmitry Bogdanov/ Wikimedia Commons (GNU FDL).

Using the latest tech to see inside the rock

The scientists could not fully extract the fragile fossil from the rock without risking damage to it. So, they turned to advanced synchrotron x-ray computed tomography (CT). Here, x-ray pulses probed the interior of the rock nodule to reveal its internal structure, in this case, the fossilized bones of Lystrosaurus. The result was a three-dimensional image reconstruction of the bones.

The team carried out this work at The European Synchrotron in France. Vincent Fernandez, who works at this facility, commented:

Understanding reproduction in mammal ancestors has been a long-lasting enigma and this fossil provides a key piece to this puzzle. It was essential that we scanned the fossil just right to capture the level of detail needed to resolve such tiny, delicate bones.

A colorful diagram of the fossil parts inside the rock.
The Lystrosaurus embryo skeleton parts are color-coded in this three-dimensional image derived from the CT scan. The ribs are blue, backbones are shades of green, forelimbs are red, the femur is yellow, the skull is light red and the mandible is light orange. Image via Julien Benoit/ University of the Witwatersrand.

How scientists established this fossil was in an egg

How did the scientists know that this fossil was an embryonic Lystrosaurus? Lead author Julien Benoit of the University of the Witwatersrand said:

When I saw the incomplete mandibular symphysis [process of growing together], I was genuinely excited. The mandible, the lower jaw, is made up of two halves that must fuse before the animal can feed. The fact that this fusion had not yet occurred shows that the individual would have been incapable of feeding itself.

There were additional signs as well. For instance, other skeletal features – its shape, size, curled posture, weak limbs and the condition of its pelvis — indicated that this was an animal that was not capable of surviving on its own. In fact, it was still in its final stages of development. And the way it was curled up, in such a compact way, indicated it was in an egg.

So why haven’t scientists found Lystrosaurus eggs before? The researchers suggest that these eggs could have been soft-shelled, and therefore not preserved during the fossilization process.

A dark grey rock with bits of dark bone on the surface, held in a person's hand.
This is the rock nodule containing the embryonic Lystrosaurus fossil. The researchers used an advanced x-ray CT scanner to see the skeleton inside the rock. Image via Julien Benoit/ University of the Witwatersrand.

What the egg tells us about the ancestors of mammals

Lystrosaurus was a medium-sized animal, ranging in length from 2 to 8 feet (0.6 to 2.4 meters), depending on the species. On average, they were about 3 feet (0.9 meters) long.

Based on the size of the fossil, the researchers think the egg was about 3 inches long (7.6 cm) and 2 inches (5 cm) wide. It may have weighed about 4 ounces (113 grams). In addition, the animal’s skull was about 1.4 inches in length (35.5 mm).

This suggested that Lystrosaurus laid relatively large eggs for its body size. In modern-day animals, a large egg means there is more yolk in it, providing food for the embryo to develop into a fairly mature juvenile form. In other words, Lystrosaurus could move around shortly after birth and feed itself.

So the researchers think Lystrosaurus did not produce milk for its young, like mammals do today.

The team also said large eggs are better able to survive drought conditions because they are more resistant to drying out. This could be the reason why Lystrosaurus was able to survive the Permian extinction.

Bottom line: Scientists discovered a 250-million-year-old Lystrosaurus fossil that was still in its egg. Its shows these ancestors of mammals laid eggs.

Source: The first non-mammalian synapsid embryo from the Triassic of South Africa

Via The European Synchrotron

Read more: Some tropical mammals shy away from the full moon

Read more: What caused the Great Dying?

The post Ancestors of mammals laid eggs, says new fossil evidence first appeared on EarthSky.



from EarthSky https://ift.tt/8nze1py
A grey drawing of an embryo in a shell. This fossil is evidence that the ancestors of mammals laid eggs.
Artist’s concept of the embryonic Lystrosaurus in its shell. The reconstruction is based on a fossil found in South Africa. It’s evidence that the ancestors of mammals laid eggs. Image via Sophie Vrard and Julien Benoit/ University of the Witwatersrand.
  • A 250-million-year-old fossil of an embryonic Lystrosaurus — an extinct animal that’s an ancestor of mammals — shows these creatures laid eggs.
  • Lystrosaurus, a piglike herbivore with a turtlelike beak and tusks, survived Earth’s worst mass extinction at the end of the Permian Epoch.
  • Advanced CT scanning revealed the tiny skeleton inside a rock nodule. And it had characteristics that confirmed the animal died before hatching.

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

CT scans of a rock nodule reveal a tiny skeleton

When researchers found a 250-million-year-old rock nodule with bits of fossil bone on its surface, they were curious to know what was inside. So they used advanced x-ray CT scans to study the rock’s interior. What they discovered was a tiny curled-up skeleton, tightly packed as if inside an egg. It was an embryonic Lystrosaurus, an animal that’s an evolutionary ancestor of mammals. The team said on April 9, 2026, that this fossil is strong evidence that the precursors to mammals laid eggs, instead of giving birth to live offspring.

Co-author Jennifer Botha of the University of the Witwatersrand said:

This fossil was discovered during a field excursion I led in 2008, nearly 17 years ago. My preparator and exceptional fossil finder, John Nyaphuli, identified a small nodule that at first revealed only tiny flecks of bone. As he carefully prepared the specimen, it became clear that it was a perfectly curled-up Lystrosaurus hatchling. I suspected even then that it had died within the egg, but at the time, we simply didn’t have the technology to confirm it.

The scientists published their study in the peer-reviewed journal PLOS One on April 9, 2026.

Lystrosaurus was a precursor to mammals

Lystrosaurus was a strange-looking beast. It had a sprawling piglike body, with a horny turtlelike beak on its head, as well as two tusklike teeth. These herbivorous creatures lived during the Late Permian and Early Triassic, approximately 259 to 247 million years ago.

At least four species of Lystrosaurus once roamed Pangea, an ancient supercontinent. Scientists have found fossils of these creatures in Antarctica, India, China, Mongolia, Russia and South Africa.

At the end of the Permian Epoch, about 252 million years ago, Earth underwent its most severe mass extinction. Major volcanic eruptions were the main triggers of this extinction. As a result, many animal species vanished forever. But Lystrosaurus survived and went on to thrive despite the unstable environment with hot conditions and long dry spells.

Scientists interested in mammalian reproduction have wondered if mammal ancestors gave birth to live young or laid eggs. They also wondered how they cared for their young. Most mammals today give birth to live young. But there’s a type of mammal called monotremes that lay eggs. They also nurse their young with milk. Monotremes – the platypus and four species of echidnas – are only found in Australia and New Guinea.

A grey-brown animal with a beak and two tusks.
This is an artist’s depiction of Lystrosaurus georgi. It’s 1 of at least 4 known species of Lystrosaurus. Image via Dmitry Bogdanov/ Wikimedia Commons (GNU FDL).

Using the latest tech to see inside the rock

The scientists could not fully extract the fragile fossil from the rock without risking damage to it. So, they turned to advanced synchrotron x-ray computed tomography (CT). Here, x-ray pulses probed the interior of the rock nodule to reveal its internal structure, in this case, the fossilized bones of Lystrosaurus. The result was a three-dimensional image reconstruction of the bones.

The team carried out this work at The European Synchrotron in France. Vincent Fernandez, who works at this facility, commented:

Understanding reproduction in mammal ancestors has been a long-lasting enigma and this fossil provides a key piece to this puzzle. It was essential that we scanned the fossil just right to capture the level of detail needed to resolve such tiny, delicate bones.

A colorful diagram of the fossil parts inside the rock.
The Lystrosaurus embryo skeleton parts are color-coded in this three-dimensional image derived from the CT scan. The ribs are blue, backbones are shades of green, forelimbs are red, the femur is yellow, the skull is light red and the mandible is light orange. Image via Julien Benoit/ University of the Witwatersrand.

How scientists established this fossil was in an egg

How did the scientists know that this fossil was an embryonic Lystrosaurus? Lead author Julien Benoit of the University of the Witwatersrand said:

When I saw the incomplete mandibular symphysis [process of growing together], I was genuinely excited. The mandible, the lower jaw, is made up of two halves that must fuse before the animal can feed. The fact that this fusion had not yet occurred shows that the individual would have been incapable of feeding itself.

There were additional signs as well. For instance, other skeletal features – its shape, size, curled posture, weak limbs and the condition of its pelvis — indicated that this was an animal that was not capable of surviving on its own. In fact, it was still in its final stages of development. And the way it was curled up, in such a compact way, indicated it was in an egg.

So why haven’t scientists found Lystrosaurus eggs before? The researchers suggest that these eggs could have been soft-shelled, and therefore not preserved during the fossilization process.

A dark grey rock with bits of dark bone on the surface, held in a person's hand.
This is the rock nodule containing the embryonic Lystrosaurus fossil. The researchers used an advanced x-ray CT scanner to see the skeleton inside the rock. Image via Julien Benoit/ University of the Witwatersrand.

What the egg tells us about the ancestors of mammals

Lystrosaurus was a medium-sized animal, ranging in length from 2 to 8 feet (0.6 to 2.4 meters), depending on the species. On average, they were about 3 feet (0.9 meters) long.

Based on the size of the fossil, the researchers think the egg was about 3 inches long (7.6 cm) and 2 inches (5 cm) wide. It may have weighed about 4 ounces (113 grams). In addition, the animal’s skull was about 1.4 inches in length (35.5 mm).

This suggested that Lystrosaurus laid relatively large eggs for its body size. In modern-day animals, a large egg means there is more yolk in it, providing food for the embryo to develop into a fairly mature juvenile form. In other words, Lystrosaurus could move around shortly after birth and feed itself.

So the researchers think Lystrosaurus did not produce milk for its young, like mammals do today.

The team also said large eggs are better able to survive drought conditions because they are more resistant to drying out. This could be the reason why Lystrosaurus was able to survive the Permian extinction.

Bottom line: Scientists discovered a 250-million-year-old Lystrosaurus fossil that was still in its egg. Its shows these ancestors of mammals laid eggs.

Source: The first non-mammalian synapsid embryo from the Triassic of South Africa

Via The European Synchrotron

Read more: Some tropical mammals shy away from the full moon

Read more: What caused the Great Dying?

The post Ancestors of mammals laid eggs, says new fossil evidence first appeared on EarthSky.



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Coma Berenices galaxy cluster, best in April and May

Coma Berenices Galaxy Cluster: Black background with large ovals of light and very many smaller points and smudges.
View larger. | This mosaic shows part of the immense Coma Berenices galaxy cluster. Be sure to view larger! Image via Hubble Space Telescope/ NASA/ ESA/ J. Mack (STScI)/ J. Madrid (Australian Telescope National Facility).

The Coma Berenices galaxy cluster

Galaxies with their billions of stars are the building blocks of our universe. But galaxies aren’t spread homogeneously throughout space. Instead, they collect in clusters. From Earth, one of the densest and most famous of the galaxy clusters is the Coma Berenices cluster. It’s located in the direction to the constellation Coma Berenices (Berenice’s Hair). And it’s best viewed in the evening in April and May.

It’s hard to get an exact count of the number of galaxies in this cluster. Counts vary based on how small or faint the galaxies are, and how big the telescopes are that are doing the counting. But scientists estimate the cluster contains as many as 10,000 or more member galaxies.

Indeed, there are more individual galaxies in this cluster than there are stars visible to the unaided human eye on a clear, dark night.

The center of the Coma cluster lies about 320 million light-years away. And the cluster itself spans about 20 million light-years of space. That’s in contrast to our home galaxy, the Milky Way, which is about 100,000 light-years wide. And it’s in contrast to our own Local Group of galaxies, our local cluster of galaxies, which is about 10 million light-years wide and contains about 50 galaxies.

An old – but beautiful – name for this region of sky is the Realm of the Galaxies. Writing an article by that name for Frosty Drew Observatory in the year 2000, the late Leslie Coleman, a previous director of Frosty Drew, explained:

Even in the eyepiece of the 16″ [telescope], many of the galaxies in this area overlap each other! There simply isn’t room enough in this region of the sky to fit them.

It occupies a small area of sky

The central part of the Coma Berenices cluster covers a roughly circular area about 1 1/2 degrees across. That’s nine times the area of a full moon, which is about 1/2 a degree across.

But the full cluster might extend farther across our sky. And numerous other galaxy clusters – some closer or farther away – are also in this same area of the sky.

This part of the sky is the site of the famous open star cluster known as the Coma Berenices star cluster, as well as the most distant galaxy cluster visible through telescopes. To see the star cluster and the galaxy cluster you need a dark sky.

It contains thousands of galaxies

So the constellation Coma Berenices appears to the eye as a cluster of stars. But a telescope reveals a vast region of distant galaxies in this part of the sky. The chart below gives you an idea of the number of galaxies in that region of the sky.

How to find the Coma Berenices galaxy cluster

The constellation Coma Berenices lies between the constellations Leo the Lion and Boötes the Herdsman.

The galaxy cluster is near the northern border of the constellation Coma Berenices.

Star chart with black dots on white for stars and a blue star showing location of a galaxy cluster.
A chart of the constellation Coma Berenices. Here, the blue star indicates the approximate location of the center of the Coma Berenices galaxy cluster. Image via IAU.

A myriad of galaxies

So the center of the Coma Berenices galaxy cluster is about 320 million light-years away. And it’s not getting any closer! In fact, the entire cluster is flying away from us at the rate of about more than 15 million mph (24 million kph)!

The galaxies in the Coma Berenices cluster is filled with galaxies in all shapes and sizes, from giant ellipticals to spirals to irregular dwarf galaxies.

Fuzzy-looking galaxies on a black background.
This image shows the elliptical galaxy NGC 4889 in front of hundreds of background galaxies. These giant ellipticals lie at the center of the Coma cluster. Image via Hubble Space Telescope.
Black background with many small scattered light ovals and spirals.
View larger. | This section of the Coma Berenices galaxy cluster is about 1/3 of the way from the cluster’s center. The bright spiral galaxy in the upper left is distinctly brighter and bluer than surrounding galaxies and has dusty spiral arms that appear reddish brown against the whiter disk of the galaxy. These are all clues that this galaxy underwent a disturbance at some point in the past. Image via NASA/ Wikimedia Commons (public domain).
Bluish galaxies on a black background.
Most galaxies in the Coma Cluster are dwarfs, not unlike our Milky Way galaxy’s Small and Large Magellanic Clouds. These little galaxies are tough to see in visible light. But infrared views have increased the Coma Cluster’s galaxy count. This composite combines infrared Spitzer Space Telescope image data (red and green) with visible light Sloan Sky Survey data (blue) for the central part of the Coma Galaxy Cluster. The field of view here is over 1 degree wide. It’s dominated by 2 giant ellipticals, in blue. Many of the small green smudges are identified as dwarf galaxies, Image via NASA, JPL-Caltech, SDSS, Leigh Jenkins, Ann Hornschemeier (Goddard Space Flight Center) et al.

Coma Berenices galaxy cluster in science

Most galaxies in the central part of the cluster are giant elliptical, the result of galaxy mergers. The two brightest members – both giant ellipticals – are NGC 4889 and NGC 4874. Each one is at least two to three times larger than our own Milky Way galaxy. Farther out from the center are several spiral galaxies.

But most galaxies in the Coma Berenices galaxy cluster are dwarf galaxies. Maybe they resemble the Milky Way’s companions, the Large and Small Magellanic Clouds.

Large detailed spiral galaxy with lots of smaller fuzzy oblong galaxies behind it.
Closeup on the majestic face-on spiral galaxy NGC 4911 located deep within the Coma Berenices galaxy cluster. Image via NASA.

Coma Berenices galaxy cluster in history

The earliest stargazers couldn’t have seen the Coma galaxy cluster. It’s too faint for viewing by the human eye (or binoculars and even small telescopes). So it has no associated mythology. But the Coma cluster still has an interesting history.

In fact, it helped lead to our discovery of dark matter in the universe. Dark matter was unknown and unsuspected until a Swiss-American astronomer, Fritz Zwicky, announced he had discovered it in the Coma Berenices galaxy cluster in the 1930s.

Zwicky tallied up the visible galaxies in the cluster and estimated their masses. Then, he observed the motions of galaxies near the edge of the cluster, which are determined by the total gravity (and hence mass) of the cluster. He found the mass derived from the latter method greatly exceeded that from visual inspection.

Zwicky knew that if the law of gravity is correct – and there’s no reason to doubt it – the only answer could be an additional source of mass, which he called dunkle Materie in German.

Today, scientists believe they see the imprint of dark matter throughout the universe. They think it’s at least five times more prevalent than the more familiar visible matter, such as the stars and galaxies we can see. Unseen and mysterious, this matter greatly increases the total mass and gravitational strength of the universe, affecting its evolution and fate.

Black and white photo of a middle-aged man sitting behind a desk in suit and tie, with papers in front of him.
Astronomer Fritz Zwicky 1st predicted the existence of dark matter in the 1930s, following his observations of the Coma Berenices galaxy cluster. Image via Wikimedia Commons (public domain).

Coordinates of the Coma Berenices galaxy cluster

The center of the Coma Berenices galaxy cluster is located at approximately RA: 12h 59m, dec: +27° 59′.

Bottom line: Myriads of galaxies – in all shapes and sizes and visible only in telescopes – shine in the Coma Berenices galaxy cluster.

The post Coma Berenices galaxy cluster, best in April and May first appeared on EarthSky.



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Coma Berenices Galaxy Cluster: Black background with large ovals of light and very many smaller points and smudges.
View larger. | This mosaic shows part of the immense Coma Berenices galaxy cluster. Be sure to view larger! Image via Hubble Space Telescope/ NASA/ ESA/ J. Mack (STScI)/ J. Madrid (Australian Telescope National Facility).

The Coma Berenices galaxy cluster

Galaxies with their billions of stars are the building blocks of our universe. But galaxies aren’t spread homogeneously throughout space. Instead, they collect in clusters. From Earth, one of the densest and most famous of the galaxy clusters is the Coma Berenices cluster. It’s located in the direction to the constellation Coma Berenices (Berenice’s Hair). And it’s best viewed in the evening in April and May.

It’s hard to get an exact count of the number of galaxies in this cluster. Counts vary based on how small or faint the galaxies are, and how big the telescopes are that are doing the counting. But scientists estimate the cluster contains as many as 10,000 or more member galaxies.

Indeed, there are more individual galaxies in this cluster than there are stars visible to the unaided human eye on a clear, dark night.

The center of the Coma cluster lies about 320 million light-years away. And the cluster itself spans about 20 million light-years of space. That’s in contrast to our home galaxy, the Milky Way, which is about 100,000 light-years wide. And it’s in contrast to our own Local Group of galaxies, our local cluster of galaxies, which is about 10 million light-years wide and contains about 50 galaxies.

An old – but beautiful – name for this region of sky is the Realm of the Galaxies. Writing an article by that name for Frosty Drew Observatory in the year 2000, the late Leslie Coleman, a previous director of Frosty Drew, explained:

Even in the eyepiece of the 16″ [telescope], many of the galaxies in this area overlap each other! There simply isn’t room enough in this region of the sky to fit them.

It occupies a small area of sky

The central part of the Coma Berenices cluster covers a roughly circular area about 1 1/2 degrees across. That’s nine times the area of a full moon, which is about 1/2 a degree across.

But the full cluster might extend farther across our sky. And numerous other galaxy clusters – some closer or farther away – are also in this same area of the sky.

This part of the sky is the site of the famous open star cluster known as the Coma Berenices star cluster, as well as the most distant galaxy cluster visible through telescopes. To see the star cluster and the galaxy cluster you need a dark sky.

It contains thousands of galaxies

So the constellation Coma Berenices appears to the eye as a cluster of stars. But a telescope reveals a vast region of distant galaxies in this part of the sky. The chart below gives you an idea of the number of galaxies in that region of the sky.

How to find the Coma Berenices galaxy cluster

The constellation Coma Berenices lies between the constellations Leo the Lion and Boötes the Herdsman.

The galaxy cluster is near the northern border of the constellation Coma Berenices.

Star chart with black dots on white for stars and a blue star showing location of a galaxy cluster.
A chart of the constellation Coma Berenices. Here, the blue star indicates the approximate location of the center of the Coma Berenices galaxy cluster. Image via IAU.

A myriad of galaxies

So the center of the Coma Berenices galaxy cluster is about 320 million light-years away. And it’s not getting any closer! In fact, the entire cluster is flying away from us at the rate of about more than 15 million mph (24 million kph)!

The galaxies in the Coma Berenices cluster is filled with galaxies in all shapes and sizes, from giant ellipticals to spirals to irregular dwarf galaxies.

Fuzzy-looking galaxies on a black background.
This image shows the elliptical galaxy NGC 4889 in front of hundreds of background galaxies. These giant ellipticals lie at the center of the Coma cluster. Image via Hubble Space Telescope.
Black background with many small scattered light ovals and spirals.
View larger. | This section of the Coma Berenices galaxy cluster is about 1/3 of the way from the cluster’s center. The bright spiral galaxy in the upper left is distinctly brighter and bluer than surrounding galaxies and has dusty spiral arms that appear reddish brown against the whiter disk of the galaxy. These are all clues that this galaxy underwent a disturbance at some point in the past. Image via NASA/ Wikimedia Commons (public domain).
Bluish galaxies on a black background.
Most galaxies in the Coma Cluster are dwarfs, not unlike our Milky Way galaxy’s Small and Large Magellanic Clouds. These little galaxies are tough to see in visible light. But infrared views have increased the Coma Cluster’s galaxy count. This composite combines infrared Spitzer Space Telescope image data (red and green) with visible light Sloan Sky Survey data (blue) for the central part of the Coma Galaxy Cluster. The field of view here is over 1 degree wide. It’s dominated by 2 giant ellipticals, in blue. Many of the small green smudges are identified as dwarf galaxies, Image via NASA, JPL-Caltech, SDSS, Leigh Jenkins, Ann Hornschemeier (Goddard Space Flight Center) et al.

Coma Berenices galaxy cluster in science

Most galaxies in the central part of the cluster are giant elliptical, the result of galaxy mergers. The two brightest members – both giant ellipticals – are NGC 4889 and NGC 4874. Each one is at least two to three times larger than our own Milky Way galaxy. Farther out from the center are several spiral galaxies.

But most galaxies in the Coma Berenices galaxy cluster are dwarf galaxies. Maybe they resemble the Milky Way’s companions, the Large and Small Magellanic Clouds.

Large detailed spiral galaxy with lots of smaller fuzzy oblong galaxies behind it.
Closeup on the majestic face-on spiral galaxy NGC 4911 located deep within the Coma Berenices galaxy cluster. Image via NASA.

Coma Berenices galaxy cluster in history

The earliest stargazers couldn’t have seen the Coma galaxy cluster. It’s too faint for viewing by the human eye (or binoculars and even small telescopes). So it has no associated mythology. But the Coma cluster still has an interesting history.

In fact, it helped lead to our discovery of dark matter in the universe. Dark matter was unknown and unsuspected until a Swiss-American astronomer, Fritz Zwicky, announced he had discovered it in the Coma Berenices galaxy cluster in the 1930s.

Zwicky tallied up the visible galaxies in the cluster and estimated their masses. Then, he observed the motions of galaxies near the edge of the cluster, which are determined by the total gravity (and hence mass) of the cluster. He found the mass derived from the latter method greatly exceeded that from visual inspection.

Zwicky knew that if the law of gravity is correct – and there’s no reason to doubt it – the only answer could be an additional source of mass, which he called dunkle Materie in German.

Today, scientists believe they see the imprint of dark matter throughout the universe. They think it’s at least five times more prevalent than the more familiar visible matter, such as the stars and galaxies we can see. Unseen and mysterious, this matter greatly increases the total mass and gravitational strength of the universe, affecting its evolution and fate.

Black and white photo of a middle-aged man sitting behind a desk in suit and tie, with papers in front of him.
Astronomer Fritz Zwicky 1st predicted the existence of dark matter in the 1930s, following his observations of the Coma Berenices galaxy cluster. Image via Wikimedia Commons (public domain).

Coordinates of the Coma Berenices galaxy cluster

The center of the Coma Berenices galaxy cluster is located at approximately RA: 12h 59m, dec: +27° 59′.

Bottom line: Myriads of galaxies – in all shapes and sizes and visible only in telescopes – shine in the Coma Berenices galaxy cluster.

The post Coma Berenices galaxy cluster, best in April and May first appeared on EarthSky.



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2026 Lyrid meteor shower: All you need to know

Milky Way with a bright Lyrid meteor. Some trees and a hill are in the foreground.
View at EarthSky Community Photos. | Jeremy Evans of California captured a Lyrid meteor zipping along the Milky way on April 22, 2025. Jeremy wrote: “Lyrids meteor shower, April 22nd at peak activity. It was a quiet shower this year. I had my camera going all night and only caught one meteor. This single frame is from an all night 1200 frame time lapse on my front deck, I’m very fortunate to live under dark Bortle 2 skies. The glow on the horizon is from the last quarter moon just before rising. This meteor also left smoke trails.” Thank you, Jeremy.

April 2026 meteors … the Lyrids

When to watch in 2026: After midnight and through dawn on the morning of April 22. The predicted** peak is 19:15 UTC on April 22. The peak of the Lyrids is narrow (no weeks-long stretches of meteor-watching, as with some showers). In 2026, the first quarter moon falls at 2:32 UTC on April 24. So meteor watching after midnight and before dawn on April 22 will be under a dark and moonless sky.
Radiant: Rises before midnight, highest in the sky at dawn.
Nearest moon phase: First quarter moon falls at 2:32 UTC on April 24. So a fat waxing crescent moon – that sets after midnight – won’t interfere with the peak morning of the 2026’s Lyrid meteor shower. The best time to watch is after midnight and before dawn on the morning of April 22.
Duration of shower: April 15 to April 29. This time period is when we’re passing through the meteor stream in space!
Expected meteors at peak, under ideal conditions: In a dark sky with no moon, you might see 10 to 15 Lyrids per hour. The Lyrids are known for uncommon surges that can sometimes bring rates of up to 100 per hour! Read more about Lyrid outbursts. Lyrids are known for their bright and colorful meteors, sometimes even producing fireballs. Fireballs are exceptionally bright meteors that outshine the planet Venus.
Note for Southern Hemisphere: This shower’s radiant point is far to the north on the sky’s dome. So the Southern Hemisphere will see fewer Lyrid meteors. Still, you might see some!
Meteor train possibilities? In a moonless sky, a few Lyrid meteors can leave persistent trains. That is, they leave a trail of ionized gases that glow for a few seconds after the meteor has passed. Lyrids are known to produce fireballs.

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

Animation of blazing meteor expanding to fireball as it flies from right to left.
Meteors and comets are 2 different things. This image shows a “fireball” – a very bright meteor – falling earthward. During a meteor shower, meteor watchers most often see earthgrazer fireballs like this one in the early part of the night. Image via NASA/ George Varros/ Wikipedia (public domain).

The Lyrid meteor shower parent comet

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

Most meteor showers are caused by debris from a passing comet. For the Lyrids, the comet is named Comet Thatcher. Maybe you’re wondering: Have I ever observed Comet Thatcher? The answer is no. And your children won’t see it either. 

Astronomers first noticed this comet in 1861, around the time of its last perihelion, or closest point to the sun. It takes roughly 415 years to go around the sun once. Its path brings it within the Earth’s orbit, then it goes really far away, a distance of about 110 astronomical units (AU). That’s 110 times farther from the sun than we are. 

So Comet Thatcher is now far away, still traveling outward, away from our sun. It’ll reach its farthest point from the sun around the year 2070, and then begin its return trip to reach its next perihelion around year 2283.

The Lyrid meteor shower – spawned by this comet – seems to outburst, or produce an unexpectedly large number of meteors, every 60 years. The next Lyrid outburst is due in 2042. The outbursts happen because of the planets’ reshaping the long trail of comet debris left behind by Comet Thatcher in its long orbit. This debris is what intercepts Earth’s orbit yearly to create the meteor shower.

It was Alfred E. Thatcher from New York City who discovered this comet – now officially C/1861 G1 (Thatcher) – on April 5, 1861. At that time the comet was in the direction of our sky’s north polar region, toward what we see as the constellation Draco. Alfred Thatcher was using a 4.5-inch-diameter (11cm) refracting telescope, magnifying 30 times. The comet was shining at magnitude 7.5, fainter than the unaided eye can see.

But over the next few weeks, as the comet approached both the sun and the Earth, it brightened considerably. It became visible to the eye and remained so until it disappeared into the evening twilight in early June 1861. Observers in the Southern Hemisphere picked it up in late July and followed the comet for the next five weeks, until it became too faint to see from anywhere on Earth.

Comet Thatcher will be back in the year 2278. But its debris trail, the Lyrid meteor shower, will be here every April.

A long oval orbit of a comet above concentric colored rings.
This illustration shows the parent comet of the Lyrid shower, Comet Thatcher. This comet has a long orbit around the sun, longer than any of the major planets. At the bottom of this image, you see our sun and the relatively tiny orbits of the terrestrial planets, Mercury, Venus, Earth and Mars. The longer lines, bisecting the image, represent the orbits of some of the outer, gaseous planets. And check out this comet’s orbit, in white! Comet Thatcher – the parent comet of the Lyrids – orbits the sun roughly every 415 years. It hasn’t been seen since the year 1861. Its orbit is littered with icy debris. It’s when that icy cometary debris enters Earth’s atmosphere that we see Lyrid meteors! Special thanks to our friend Bob King, aka AstroBob, for this wonderful illustration.

How to find the Lyrid meteor shower radiant point

Chart showing constellation Lyra and radial arrows from meteor shower radiant point near it.
Lyrid meteors radiate from near the bright star Vega in the constellation Lyra the Harp. You don’t need to identify Vega or Lyra in order to watch the Lyrid meteor shower. But you do need to know when the radiant rises, in this case in the northeast before midnight. That’s why the Lyrids are typically best between midnight and dawn. You’ll see the most meteors after the radiant has come over the horizon. The meteors radiate from there, but will appear unexpectedly, in any and all parts of the sky. Image via EarthSky.

From the Northern Hemisphere. The bright star Vega in the constellation Lyra – near the radiant point for the Lyrid shower – rises above your local horizon, in the northeast, around 9 to 10 p.m. your local time in April. That’s the time on your clock, from mid-latitudes, from the northern part of the globe. Vega climbs upward through the rest of the night. By midnight, Vega is high enough in the sky that meteors radiating from that direction streak across your sky. Just before dawn, Vega and the radiant point shine high overhead, and the meteors will be raining down from the top of the Northern Hemisphere sky.

From the Southern Hemisphere. Vega – and the Lyrid meteors’ radiant point – don’t rise until the hours before dawn from the southern mid-latitudes. From there, the radiant point never gets very high in the sky. Many of the meteors that come from this point head northward, below your horizon if you’re in the Southern Hemisphere. Thus, you have a narrower window for watching this particular, far-northern shower. Still, you might see some meteors!

The higher Vega appears in your sky, the more meteors you’re likely to see.

Lyrids radiant point and surrounding constellations

Round chart with labeled constellations and stars, and radial lines marked 'Lyrids' near Lyra.
The radiant point of the Lyrid meteor shower, seen here in sky mode (from the the earth’s surface, looking up). Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.
Diagram: Cygnus, Lyra, Hercules, Corona Borealis and Bootes above the horizon with a meteors streaking away from Lyra, with explanatory text.
The view looking toward the east-northeast horizon during the Lyrid meteor shower. In 2026, the best time to watch is after midnight and before dawn on April 22. Image via Guy Ottewell’s Astronomical Calendar 2026. Used with permission.
Diagram of Earth globe with lines toward location of moon, sun, and direction the meteors are coming in.
Diagram of the 2026 Lyrid meteor shower as seen from above the Earth’s surface, looking down. Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.

Lyrid meteors and Earth, from space

On the night of April 21, 2012, the Lyrid meteor shower peaked in the skies over Earth. Astronaut Don Pettit aboard the International Space Station trained his camera on Earth. Video footage from that night can be seen in the video below. The bright points of light are the meteors ablating – or burning up – in Earth’s atmosphere.

Video via NASA.

Lyrid meteor shower in history

The Lyrid meteor shower has the distinction of being among the oldest of known meteor showers. Records of this shower go back for some 2,700 years. In fact, the ancient Chinese seem to have observed the Lyrid meteors falling like rain in the year 687 BCE. That time period in ancient China, by the way, corresponds with what is called the Spring and Autumn Period (about 771 to 476 BCE), which tradition associates with the Chinese teacher and philosopher Confucius, one of the first to espouse the principle:

Do not do to others what you do not want done to yourself.

Ancient Chinese drawing of Confucius, old bearded man in Chinese costume.
Portrait of Confucius. Was he a meteor-watcher? Image via Wikipedia (public domain).

Lyrid meteor photos from the EarthSky community

Submit your night sky photos to EarthSky here

Dark blue sky with two parallel streaks of Lyrid meteors in the sky.
View at EarthSky Community Photos. | Kathie O’Donnell of South Dakota captured this image on April 20, 2024, and wrote: “Had one night of very clear skies. Surprised to see twin Lyrids upon reviewing my all-night GoPro images. Found several others but they were very faint.” Thank you, Kathie!
Starry sky with Milky Way, a Lyrid meteor and some satellite trails.
View at EarthSky Community Photos. | Steve Price captured this image in Utah on April 20, 2023, and wrote: “One Lyrid meteor streaking past the Eagle Nebula and a couple of early morning satellites. The foreground is blurred from the star tracker following the stars. A little bit of green and red airglow is showing on the left”. Thank you, Steve.
Lyrid meteor in starry, Milky Way sky and rocks in foreground.
View at EarthSky Community Photos. | Nils Ribi captured this image in Utah on April 17, 2023, and wrote: “I was setting up to photograph the Milky Way over the Windows section of Arches National Park in the very early morning hours of April 17, 2023. As I was, I noticed a couple Lyrid meteors in the northeast sky. I set the camera up in that direction and was able to capture a couple of photos. This is the best one. I then proceeded to get a nice pano photo of the Milky Way over the North Window. Life is good!” Thank you, Nils!

Bottom line: The best time to watch the Lyrid meteor shower is after midnight and before dawn on the morning of April 22. You’ll have a dark and moonless sky then. We hope you see some meteors!

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

Visit EarthSky’s meteor shower guide

Meteor showers: Tips for watching the show

Learn how to shoot photos of meteors

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Milky Way with a bright Lyrid meteor. Some trees and a hill are in the foreground.
View at EarthSky Community Photos. | Jeremy Evans of California captured a Lyrid meteor zipping along the Milky way on April 22, 2025. Jeremy wrote: “Lyrids meteor shower, April 22nd at peak activity. It was a quiet shower this year. I had my camera going all night and only caught one meteor. This single frame is from an all night 1200 frame time lapse on my front deck, I’m very fortunate to live under dark Bortle 2 skies. The glow on the horizon is from the last quarter moon just before rising. This meteor also left smoke trails.” Thank you, Jeremy.

April 2026 meteors … the Lyrids

When to watch in 2026: After midnight and through dawn on the morning of April 22. The predicted** peak is 19:15 UTC on April 22. The peak of the Lyrids is narrow (no weeks-long stretches of meteor-watching, as with some showers). In 2026, the first quarter moon falls at 2:32 UTC on April 24. So meteor watching after midnight and before dawn on April 22 will be under a dark and moonless sky.
Radiant: Rises before midnight, highest in the sky at dawn.
Nearest moon phase: First quarter moon falls at 2:32 UTC on April 24. So a fat waxing crescent moon – that sets after midnight – won’t interfere with the peak morning of the 2026’s Lyrid meteor shower. The best time to watch is after midnight and before dawn on the morning of April 22.
Duration of shower: April 15 to April 29. This time period is when we’re passing through the meteor stream in space!
Expected meteors at peak, under ideal conditions: In a dark sky with no moon, you might see 10 to 15 Lyrids per hour. The Lyrids are known for uncommon surges that can sometimes bring rates of up to 100 per hour! Read more about Lyrid outbursts. Lyrids are known for their bright and colorful meteors, sometimes even producing fireballs. Fireballs are exceptionally bright meteors that outshine the planet Venus.
Note for Southern Hemisphere: This shower’s radiant point is far to the north on the sky’s dome. So the Southern Hemisphere will see fewer Lyrid meteors. Still, you might see some!
Meteor train possibilities? In a moonless sky, a few Lyrid meteors can leave persistent trains. That is, they leave a trail of ionized gases that glow for a few seconds after the meteor has passed. Lyrids are known to produce fireballs.

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

Animation of blazing meteor expanding to fireball as it flies from right to left.
Meteors and comets are 2 different things. This image shows a “fireball” – a very bright meteor – falling earthward. During a meteor shower, meteor watchers most often see earthgrazer fireballs like this one in the early part of the night. Image via NASA/ George Varros/ Wikipedia (public domain).

The Lyrid meteor shower parent comet

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

Most meteor showers are caused by debris from a passing comet. For the Lyrids, the comet is named Comet Thatcher. Maybe you’re wondering: Have I ever observed Comet Thatcher? The answer is no. And your children won’t see it either. 

Astronomers first noticed this comet in 1861, around the time of its last perihelion, or closest point to the sun. It takes roughly 415 years to go around the sun once. Its path brings it within the Earth’s orbit, then it goes really far away, a distance of about 110 astronomical units (AU). That’s 110 times farther from the sun than we are. 

So Comet Thatcher is now far away, still traveling outward, away from our sun. It’ll reach its farthest point from the sun around the year 2070, and then begin its return trip to reach its next perihelion around year 2283.

The Lyrid meteor shower – spawned by this comet – seems to outburst, or produce an unexpectedly large number of meteors, every 60 years. The next Lyrid outburst is due in 2042. The outbursts happen because of the planets’ reshaping the long trail of comet debris left behind by Comet Thatcher in its long orbit. This debris is what intercepts Earth’s orbit yearly to create the meteor shower.

It was Alfred E. Thatcher from New York City who discovered this comet – now officially C/1861 G1 (Thatcher) – on April 5, 1861. At that time the comet was in the direction of our sky’s north polar region, toward what we see as the constellation Draco. Alfred Thatcher was using a 4.5-inch-diameter (11cm) refracting telescope, magnifying 30 times. The comet was shining at magnitude 7.5, fainter than the unaided eye can see.

But over the next few weeks, as the comet approached both the sun and the Earth, it brightened considerably. It became visible to the eye and remained so until it disappeared into the evening twilight in early June 1861. Observers in the Southern Hemisphere picked it up in late July and followed the comet for the next five weeks, until it became too faint to see from anywhere on Earth.

Comet Thatcher will be back in the year 2278. But its debris trail, the Lyrid meteor shower, will be here every April.

A long oval orbit of a comet above concentric colored rings.
This illustration shows the parent comet of the Lyrid shower, Comet Thatcher. This comet has a long orbit around the sun, longer than any of the major planets. At the bottom of this image, you see our sun and the relatively tiny orbits of the terrestrial planets, Mercury, Venus, Earth and Mars. The longer lines, bisecting the image, represent the orbits of some of the outer, gaseous planets. And check out this comet’s orbit, in white! Comet Thatcher – the parent comet of the Lyrids – orbits the sun roughly every 415 years. It hasn’t been seen since the year 1861. Its orbit is littered with icy debris. It’s when that icy cometary debris enters Earth’s atmosphere that we see Lyrid meteors! Special thanks to our friend Bob King, aka AstroBob, for this wonderful illustration.

How to find the Lyrid meteor shower radiant point

Chart showing constellation Lyra and radial arrows from meteor shower radiant point near it.
Lyrid meteors radiate from near the bright star Vega in the constellation Lyra the Harp. You don’t need to identify Vega or Lyra in order to watch the Lyrid meteor shower. But you do need to know when the radiant rises, in this case in the northeast before midnight. That’s why the Lyrids are typically best between midnight and dawn. You’ll see the most meteors after the radiant has come over the horizon. The meteors radiate from there, but will appear unexpectedly, in any and all parts of the sky. Image via EarthSky.

From the Northern Hemisphere. The bright star Vega in the constellation Lyra – near the radiant point for the Lyrid shower – rises above your local horizon, in the northeast, around 9 to 10 p.m. your local time in April. That’s the time on your clock, from mid-latitudes, from the northern part of the globe. Vega climbs upward through the rest of the night. By midnight, Vega is high enough in the sky that meteors radiating from that direction streak across your sky. Just before dawn, Vega and the radiant point shine high overhead, and the meteors will be raining down from the top of the Northern Hemisphere sky.

From the Southern Hemisphere. Vega – and the Lyrid meteors’ radiant point – don’t rise until the hours before dawn from the southern mid-latitudes. From there, the radiant point never gets very high in the sky. Many of the meteors that come from this point head northward, below your horizon if you’re in the Southern Hemisphere. Thus, you have a narrower window for watching this particular, far-northern shower. Still, you might see some meteors!

The higher Vega appears in your sky, the more meteors you’re likely to see.

Lyrids radiant point and surrounding constellations

Round chart with labeled constellations and stars, and radial lines marked 'Lyrids' near Lyra.
The radiant point of the Lyrid meteor shower, seen here in sky mode (from the the earth’s surface, looking up). Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.
Diagram: Cygnus, Lyra, Hercules, Corona Borealis and Bootes above the horizon with a meteors streaking away from Lyra, with explanatory text.
The view looking toward the east-northeast horizon during the Lyrid meteor shower. In 2026, the best time to watch is after midnight and before dawn on April 22. Image via Guy Ottewell’s Astronomical Calendar 2026. Used with permission.
Diagram of Earth globe with lines toward location of moon, sun, and direction the meteors are coming in.
Diagram of the 2026 Lyrid meteor shower as seen from above the Earth’s surface, looking down. Chart via Guy Ottewell’s 2026 Astronomical Calendar. Used with permission.

Lyrid meteors and Earth, from space

On the night of April 21, 2012, the Lyrid meteor shower peaked in the skies over Earth. Astronaut Don Pettit aboard the International Space Station trained his camera on Earth. Video footage from that night can be seen in the video below. The bright points of light are the meteors ablating – or burning up – in Earth’s atmosphere.

Video via NASA.

Lyrid meteor shower in history

The Lyrid meteor shower has the distinction of being among the oldest of known meteor showers. Records of this shower go back for some 2,700 years. In fact, the ancient Chinese seem to have observed the Lyrid meteors falling like rain in the year 687 BCE. That time period in ancient China, by the way, corresponds with what is called the Spring and Autumn Period (about 771 to 476 BCE), which tradition associates with the Chinese teacher and philosopher Confucius, one of the first to espouse the principle:

Do not do to others what you do not want done to yourself.

Ancient Chinese drawing of Confucius, old bearded man in Chinese costume.
Portrait of Confucius. Was he a meteor-watcher? Image via Wikipedia (public domain).

Lyrid meteor photos from the EarthSky community

Submit your night sky photos to EarthSky here

Dark blue sky with two parallel streaks of Lyrid meteors in the sky.
View at EarthSky Community Photos. | Kathie O’Donnell of South Dakota captured this image on April 20, 2024, and wrote: “Had one night of very clear skies. Surprised to see twin Lyrids upon reviewing my all-night GoPro images. Found several others but they were very faint.” Thank you, Kathie!
Starry sky with Milky Way, a Lyrid meteor and some satellite trails.
View at EarthSky Community Photos. | Steve Price captured this image in Utah on April 20, 2023, and wrote: “One Lyrid meteor streaking past the Eagle Nebula and a couple of early morning satellites. The foreground is blurred from the star tracker following the stars. A little bit of green and red airglow is showing on the left”. Thank you, Steve.
Lyrid meteor in starry, Milky Way sky and rocks in foreground.
View at EarthSky Community Photos. | Nils Ribi captured this image in Utah on April 17, 2023, and wrote: “I was setting up to photograph the Milky Way over the Windows section of Arches National Park in the very early morning hours of April 17, 2023. As I was, I noticed a couple Lyrid meteors in the northeast sky. I set the camera up in that direction and was able to capture a couple of photos. This is the best one. I then proceeded to get a nice pano photo of the Milky Way over the North Window. Life is good!” Thank you, Nils!

Bottom line: The best time to watch the Lyrid meteor shower is after midnight and before dawn on the morning of April 22. You’ll have a dark and moonless sky then. We hope you see some meteors!

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

Visit EarthSky’s meteor shower guide

Meteor showers: Tips for watching the show

Learn how to shoot photos of meteors

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



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The tree-kangaroo lives in the hidden world of the treetops


Meet the tree-kangaroo! Image via Alex Gisby/ Unsplash.

Meet the tree-kangaroo

Deep in the lush rainforests of Papua New Guinea, Indonesia and northern Australia lives a unique mammal: the tree-kangaroo. Unlike the iconic kangaroos that bound across open plains, these animals have taken a completely different evolutionary path. And it leads upward, into the trees. Mysterious, agile and rarely seen, tree-kangaroos reveal a fascinating side of marsupial life that many people don’t even know exists.

Tree-kangaroos are part of the macropod family of marsupials. Macropods includes includes kangaroos, wallabies and quokkas, among others. The ancestors of modern macropods likely lived in the trees. But millions of years ago, the animals descended to life on the ground. Tree-kangaroos, however, eventually returned to life in the trees. And now they are well-adapted to an arboreal lifestyle.

Odd appearance, genius design for the canopy

While tree-kangaroos share ancestry with ground kangaroos, their bodies are much more conducive to life in the trees. Tree-kangaroos’ limbs are shorter and more muscular, making climbing easier than hopping long distances. The front legs are nearly as strong as the back ones, which helps them grip branches and pull themselves upward.

Their long, thick tails act as a counterbalance when navigating through the trees. This gives them stability as they move along narrow branches. Their fur is dense and often soft, ranging in color from reddish-brown to grey or even golden tones, depending on the species. With rounded ears and a compact body, they often resemble a small bear more than a typical kangaroo.

Golden/orangish animal walking on 4 long legs. It has short ears.
Tree-kangaroos have dense fur that varies from red and brown to gray in color. Their legs differ from ground kangaroos. They also have short ears that make them look like little bears! Image via Kunal Kalra/ Unsplash.

Dining in the rainforest canopy

Tree-kangaroos are primarily found in the tropical rainforests and mountainous regions of Papua New Guinea and Indonesia. Plus, a few species live in northeastern Australia. These environments are dense, humid and layered with vegetation, providing the perfect setting for an animal that spends most of its life above the ground.

A brownish/gray animal on a tree, holding its long tail with its right hand.
These animals live among trees, branches and leaves. They have strong legs and long tails that help them move in that habitat with great agility. Image via Russnamitz/ iNaturalist (CC0 1.0)

They are mostly herbivorous, feeding on leaves, fruits, flowers and sometimes bark. Because their diet is rich in fibrous plant material, their digestive systems are specially adapted to break it down efficiently. They rarely come down to the forest floor, because staying in the trees offers both food and protection.

Tree-kangaroos have a complex, multi-chambered stomach that allows them to ferment tough plant material with the help of microorganisms. This process breaks down cellulose, which would otherwise be difficult to digest. And it extracts as many nutrients as possible from their leafy diet. Interestingly, the fermentation can last up to 24 hours, which helps explain why they spend long periods resting between feeding sessions to conserve energy.

A brownish/golden animal feeding on a long, green leaf.
Look at this tree-kangaroo feeding. They are herbivorous. Image via Robin Teng/ Unsplash.

The tree-kangaroo is a surprising master of movement

They may have a slow metabolism, but when they move, they make it count. In fact, one of the most striking things about tree-kangaroos is how agile they are in an environment that seems difficult to navigate. They can leap distances of up to around 30 feet (about 9 meters) between branches. And they are capable of dropping from heights of up to 60 feet (nearly 18 meters) to the ground without serious injury.

Their vertical agility is extraordinary, allowing them to climb up and down trees with impressive control. They scale steep trunks and descend just as skillfully, often headfirst, moving several feet in seconds with powerful, precise movements.

This ability lets them navigate efficiently between trees when necessary, even in fragmented forests. Their movement is not fast in the way we might expect from ground-dwelling kangaroos. But it is remarkably precise and perfectly adapted to their three-dimensional, vertical world.

A medium sized animal with light and dark brown fur sitting on a high, thin tree branch.
Tree-kangaroos have strong forelimbs and curved claws that let them grip bark and branches. They can climb both up and down trees, which is rare among many climbing mammals. Image via Stephen Tafra/ Unsplash.

A life behind the leaves

Tree-kangaroos are generally solitary and elusive, which makes them difficult to study. They tend to be most active at night or during low-light hours, quietly moving through the canopy in search of food. Because they are so well camouflaged and slow-moving, it can be hard to spot them even when they’re nearby.

Another interesting trait is their strong sense of spatial awareness. Living in a three-dimensional environment requires them to remember routes, feeding spots and safe resting areas high above the ground.

Currently, scientists recognize around 14 species of tree-kangaroo, each with its own unique adaptations, appearance and behavior. This diversity highlights just how specialized these animals have become to thrive in the treetops.

Animal with dark brown fur on a branch. Its long, whitish tail is hanging.
With around 14 species, tree-kangaroos are highly specialized animals, uniquely adapted to navigate and survive in the treetops. Image via Joanna Huang/ Unsplash.

Extraordinary species of tree-kangaroo you should know

Not all tree-kangaroos are the same. In fact, there are 14 currently known species. Following are some that stand out for their particularly unusual traits. One of the most striking is the Matschie’s tree-kangaroo, known for its thick, woolly fur and gentle appearance. Native to the Huon Peninsula in Papua New Guinea, it is also one of the most studied species, which has helped scientists better understand how these animals live and behave.

A brown animal with dense fur and a very long tail climbing a trunk.
A young Matschie’s tree-kangaroo at the Bronx Zoo. Image via Fred Hsu/ Wikipedia (CC BY-SA 3.0).

Another fascinating example is the Goodfellow’s tree-kangaroo, easily recognized by its rich chestnut-colored coat and golden stripes. Its vibrant coloration makes it one of the most visually distinctive species, and it has become a symbol of rainforest biodiversity in the regions where it lives, in the tropical forests of Papua New Guinea and Indonesia.

Reddish tree-kangaroo with white belly and tail, next to another with white stripes on its back.
These are Goodfellow’s tree-kangaroos. Image via Tim Williams/ Wikipedia (CC BY 2.0).

The Lumholtz’s tree-kangaroo, which lives in Australia, is quite different from its relatives in the island to the north. It has a more subdued grey-brown coloration and tends to live at lower altitudes. What makes it especially interesting is how relatively accessible it is compared to other species. This gives researchers more opportunities to observe it in the wild.

A dark gray animal high on a branch and eating a leaf. It looks like it is smiling!
A Lumholtz’s tree-kangaroo eating a delicious leaf. Image via bioshots_jm/ iNaturalist (CC0 1.0).

Then there is the elusive Wondiwoi tree-kangaroo. It gained attention due to its rediscovery decades after it was last seen. Its rarity and the mystery surrounding its population make it one of the most intriguing members of the group.

From pouch to branch

Tree-kangaroo mothers carry their young, called joeys, in a pouch, just like other marsupials. At birth, joeys are tiny – usually just 2 inches (about 5 centimeters) long and weighing only a few grams – and completely undeveloped. Amazingly, even at this size, they have the strength to crawl into the pouch by themselves, where they attach to a teat and continue developing safely.

Joeys stay in the pouch for about 8 to 9 months (roughly 240 to 270 days), gradually growing stronger and more coordinated. During this time, they spend most of their days eating and sleeping, but they also begin practicing small jumps inside the pouch, almost like tiny “training sessions” for life in the canopy.

After leaving the pouch, they often remain close to their mothers for several more months, learning vital skills such as climbing, leaping between branches and finding safe resting spots high in the trees. Survival during these early months is challenging, as the dense canopy hides both opportunities and dangers.


Meet little Ori, a Goodfellow’s tree-kangaroo joey, and her mum Mani. Ori lives at the Healesville Sanctuary near Melbourne, Australia.


Read more about Havam, a Matschie’s tree kangaroo joey, here. Havam lives at Woodland Park Zoo in Seattle, Washington.

Rising above: protecting the canopy’s hidden gems

Many species of tree-kangaroo face threats from habitat loss and hunting. This is particularly true in regions where people are clearing forests. Because tree-kangaroos depend so heavily on intact rainforest ecosystems, even small environmental changes can have a big impact on their survival.

However, there is growing awareness about their importance and uniqueness. Conservation programs and protected areas are helping to preserve their habitats. And local communities are increasingly involved in protecting these animals.

Despite the challenges they face, tree-kangaroos continue to thrive in some of the world’s most beautiful and remote forests. Their existence is a reminder that evolution can take surprising paths and that there is still so much to discover and protect in the natural world.

Grayish/brownish animal with black face and hands holding her baby, among tree leaves.
Not your ordinary kangaroos. Endlessly fascinating, tree-kangaroos are marvels of the rainforest we must protect. Here’s a female Lumholt’z tree-kangaroo and her joey in Australia. Image via Mark Gillow/ Wikimedia Commons (CC BY 2.0).

Bottom line: The tree-kangaroo lives high in the rainforest canopy, leaping, climbing and revealing a surprising side of marsupial life few have seen.

Via IFAW

Via World Wildlife Fund

Read more: The gliding possum is a nocturnal acrobat of the forest

Read more: Tasmanian devil population increases with breeding program

The post The tree-kangaroo lives in the hidden world of the treetops first appeared on EarthSky.



from EarthSky https://ift.tt/WzCPA7k


Meet the tree-kangaroo! Image via Alex Gisby/ Unsplash.

Meet the tree-kangaroo

Deep in the lush rainforests of Papua New Guinea, Indonesia and northern Australia lives a unique mammal: the tree-kangaroo. Unlike the iconic kangaroos that bound across open plains, these animals have taken a completely different evolutionary path. And it leads upward, into the trees. Mysterious, agile and rarely seen, tree-kangaroos reveal a fascinating side of marsupial life that many people don’t even know exists.

Tree-kangaroos are part of the macropod family of marsupials. Macropods includes includes kangaroos, wallabies and quokkas, among others. The ancestors of modern macropods likely lived in the trees. But millions of years ago, the animals descended to life on the ground. Tree-kangaroos, however, eventually returned to life in the trees. And now they are well-adapted to an arboreal lifestyle.

Odd appearance, genius design for the canopy

While tree-kangaroos share ancestry with ground kangaroos, their bodies are much more conducive to life in the trees. Tree-kangaroos’ limbs are shorter and more muscular, making climbing easier than hopping long distances. The front legs are nearly as strong as the back ones, which helps them grip branches and pull themselves upward.

Their long, thick tails act as a counterbalance when navigating through the trees. This gives them stability as they move along narrow branches. Their fur is dense and often soft, ranging in color from reddish-brown to grey or even golden tones, depending on the species. With rounded ears and a compact body, they often resemble a small bear more than a typical kangaroo.

Golden/orangish animal walking on 4 long legs. It has short ears.
Tree-kangaroos have dense fur that varies from red and brown to gray in color. Their legs differ from ground kangaroos. They also have short ears that make them look like little bears! Image via Kunal Kalra/ Unsplash.

Dining in the rainforest canopy

Tree-kangaroos are primarily found in the tropical rainforests and mountainous regions of Papua New Guinea and Indonesia. Plus, a few species live in northeastern Australia. These environments are dense, humid and layered with vegetation, providing the perfect setting for an animal that spends most of its life above the ground.

A brownish/gray animal on a tree, holding its long tail with its right hand.
These animals live among trees, branches and leaves. They have strong legs and long tails that help them move in that habitat with great agility. Image via Russnamitz/ iNaturalist (CC0 1.0)

They are mostly herbivorous, feeding on leaves, fruits, flowers and sometimes bark. Because their diet is rich in fibrous plant material, their digestive systems are specially adapted to break it down efficiently. They rarely come down to the forest floor, because staying in the trees offers both food and protection.

Tree-kangaroos have a complex, multi-chambered stomach that allows them to ferment tough plant material with the help of microorganisms. This process breaks down cellulose, which would otherwise be difficult to digest. And it extracts as many nutrients as possible from their leafy diet. Interestingly, the fermentation can last up to 24 hours, which helps explain why they spend long periods resting between feeding sessions to conserve energy.

A brownish/golden animal feeding on a long, green leaf.
Look at this tree-kangaroo feeding. They are herbivorous. Image via Robin Teng/ Unsplash.

The tree-kangaroo is a surprising master of movement

They may have a slow metabolism, but when they move, they make it count. In fact, one of the most striking things about tree-kangaroos is how agile they are in an environment that seems difficult to navigate. They can leap distances of up to around 30 feet (about 9 meters) between branches. And they are capable of dropping from heights of up to 60 feet (nearly 18 meters) to the ground without serious injury.

Their vertical agility is extraordinary, allowing them to climb up and down trees with impressive control. They scale steep trunks and descend just as skillfully, often headfirst, moving several feet in seconds with powerful, precise movements.

This ability lets them navigate efficiently between trees when necessary, even in fragmented forests. Their movement is not fast in the way we might expect from ground-dwelling kangaroos. But it is remarkably precise and perfectly adapted to their three-dimensional, vertical world.

A medium sized animal with light and dark brown fur sitting on a high, thin tree branch.
Tree-kangaroos have strong forelimbs and curved claws that let them grip bark and branches. They can climb both up and down trees, which is rare among many climbing mammals. Image via Stephen Tafra/ Unsplash.

A life behind the leaves

Tree-kangaroos are generally solitary and elusive, which makes them difficult to study. They tend to be most active at night or during low-light hours, quietly moving through the canopy in search of food. Because they are so well camouflaged and slow-moving, it can be hard to spot them even when they’re nearby.

Another interesting trait is their strong sense of spatial awareness. Living in a three-dimensional environment requires them to remember routes, feeding spots and safe resting areas high above the ground.

Currently, scientists recognize around 14 species of tree-kangaroo, each with its own unique adaptations, appearance and behavior. This diversity highlights just how specialized these animals have become to thrive in the treetops.

Animal with dark brown fur on a branch. Its long, whitish tail is hanging.
With around 14 species, tree-kangaroos are highly specialized animals, uniquely adapted to navigate and survive in the treetops. Image via Joanna Huang/ Unsplash.

Extraordinary species of tree-kangaroo you should know

Not all tree-kangaroos are the same. In fact, there are 14 currently known species. Following are some that stand out for their particularly unusual traits. One of the most striking is the Matschie’s tree-kangaroo, known for its thick, woolly fur and gentle appearance. Native to the Huon Peninsula in Papua New Guinea, it is also one of the most studied species, which has helped scientists better understand how these animals live and behave.

A brown animal with dense fur and a very long tail climbing a trunk.
A young Matschie’s tree-kangaroo at the Bronx Zoo. Image via Fred Hsu/ Wikipedia (CC BY-SA 3.0).

Another fascinating example is the Goodfellow’s tree-kangaroo, easily recognized by its rich chestnut-colored coat and golden stripes. Its vibrant coloration makes it one of the most visually distinctive species, and it has become a symbol of rainforest biodiversity in the regions where it lives, in the tropical forests of Papua New Guinea and Indonesia.

Reddish tree-kangaroo with white belly and tail, next to another with white stripes on its back.
These are Goodfellow’s tree-kangaroos. Image via Tim Williams/ Wikipedia (CC BY 2.0).

The Lumholtz’s tree-kangaroo, which lives in Australia, is quite different from its relatives in the island to the north. It has a more subdued grey-brown coloration and tends to live at lower altitudes. What makes it especially interesting is how relatively accessible it is compared to other species. This gives researchers more opportunities to observe it in the wild.

A dark gray animal high on a branch and eating a leaf. It looks like it is smiling!
A Lumholtz’s tree-kangaroo eating a delicious leaf. Image via bioshots_jm/ iNaturalist (CC0 1.0).

Then there is the elusive Wondiwoi tree-kangaroo. It gained attention due to its rediscovery decades after it was last seen. Its rarity and the mystery surrounding its population make it one of the most intriguing members of the group.

From pouch to branch

Tree-kangaroo mothers carry their young, called joeys, in a pouch, just like other marsupials. At birth, joeys are tiny – usually just 2 inches (about 5 centimeters) long and weighing only a few grams – and completely undeveloped. Amazingly, even at this size, they have the strength to crawl into the pouch by themselves, where they attach to a teat and continue developing safely.

Joeys stay in the pouch for about 8 to 9 months (roughly 240 to 270 days), gradually growing stronger and more coordinated. During this time, they spend most of their days eating and sleeping, but they also begin practicing small jumps inside the pouch, almost like tiny “training sessions” for life in the canopy.

After leaving the pouch, they often remain close to their mothers for several more months, learning vital skills such as climbing, leaping between branches and finding safe resting spots high in the trees. Survival during these early months is challenging, as the dense canopy hides both opportunities and dangers.


Meet little Ori, a Goodfellow’s tree-kangaroo joey, and her mum Mani. Ori lives at the Healesville Sanctuary near Melbourne, Australia.


Read more about Havam, a Matschie’s tree kangaroo joey, here. Havam lives at Woodland Park Zoo in Seattle, Washington.

Rising above: protecting the canopy’s hidden gems

Many species of tree-kangaroo face threats from habitat loss and hunting. This is particularly true in regions where people are clearing forests. Because tree-kangaroos depend so heavily on intact rainforest ecosystems, even small environmental changes can have a big impact on their survival.

However, there is growing awareness about their importance and uniqueness. Conservation programs and protected areas are helping to preserve their habitats. And local communities are increasingly involved in protecting these animals.

Despite the challenges they face, tree-kangaroos continue to thrive in some of the world’s most beautiful and remote forests. Their existence is a reminder that evolution can take surprising paths and that there is still so much to discover and protect in the natural world.

Grayish/brownish animal with black face and hands holding her baby, among tree leaves.
Not your ordinary kangaroos. Endlessly fascinating, tree-kangaroos are marvels of the rainforest we must protect. Here’s a female Lumholt’z tree-kangaroo and her joey in Australia. Image via Mark Gillow/ Wikimedia Commons (CC BY 2.0).

Bottom line: The tree-kangaroo lives high in the rainforest canopy, leaping, climbing and revealing a surprising side of marsupial life few have seen.

Via IFAW

Via World Wildlife Fund

Read more: The gliding possum is a nocturnal acrobat of the forest

Read more: Tasmanian devil population increases with breeding program

The post The tree-kangaroo lives in the hidden world of the treetops first appeared on EarthSky.



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International Dark Sky Week is April 13 to 20

Two people pedaling bikes in the country at night for International Dark Sky week.
International Dark Sky Week is April 13 to 20, 2026. Image via IDA.
  • International Dark Sky Week is a worldwide celebration of the dark and natural night.
  • Light pollution is the human-made alteration of outdoor light levels.
  • Go Dark is the 2026 theme.

According to the International Dark-Sky Association (IDA) – founded in 1988 and based in Tucson, Arizona – light pollution is increasing at a rate twice that of human population growth. And about 80% of people around the world live under a light-polluted sky. That’s why IDA has established an International Dark Sky Week, which in 2026 falls on April 13 to 20. The goal for the week is to Go Dark. According to the IDA:

From the darkness needed for a restful night’s sleep to the activities we enjoy beneath the stars, the night is filled with wonder and importance. Dark nights sustain critical wildlife ecosystems, strengthen the well-being of our communities, enable scientific discovery, and preserve shared cultural knowledge and traditions.

The group also hopes you’ll learn the stars and constellations, and teach them to others.

Also, the IDA hopes you’ll join the global dark sky movement to protect and celebrate our shared heritage of dark night skies. DarkSky International promotes solutions that allow people to appreciate dark, star-filled skies while enjoying the benefits of responsible outdoor lighting.

According to the IDA:

For this International Dark Sky Week we invite you to join us as we discover the night together, exploring its importance and the actions we can take to protect dark skies.

Five labeled panels of sky above a city, suburbs, and country, showing less and less light-polluted view.
Poor lighting in cities leads to larger amounts of light pollution. From a dark country sky, you can see the river of stars that makes up our galaxy, the Milky Way. Image via IDA.

Ways to celebrate International Dark Sky Week

Looking for ways to celebrate International Dark Sky Week? Here’s International Dark Sky Week links for Get out at Night suggestions.

Visit EarthSky’s night sky guide to see what you can view in the sky this week. A highlight that week is the moon near Venus from April 18 to 20. For more information visit EarthSky’s night sky guide.

Visit EarthSky’s Best Places to Stargaze page to find a good dark-sky observing site close to home. Share your night sky photos at EarthSky Community Photos.

Paul Bogard has written extensively on the importance of darkness. His book is titled The End of Night. His TEDx Talk focuses on why we need darkness. You’ll find his TEDx Talk here.

Poster with animals and insects around a bright streetlight.
Curbing light pollution also benefits wildlife. Image via IDA.

Dark-sky photos from the EarthSky Community

Submit your photo to EarthSky here

A starry band in a starry sky above a treeline.
View at EarthSky Community Photos. | Muhammad Bilal in Talagang, Punjab, Pakistan, captured our home galaxy on March 6, 2025. Muhammad wrote: “As the summer is approaching, our very own Milky way Galaxy is back in sky.” Thank you, Muhammad!
An old abandoned house on the prairie with a large, cloudy band of stars above.
View at EarthSky Community Photos. | William Mathe made the 100-mile drive to Last Chance, Colorado, for this scene on March 16, 2024. William wrote: “The ranch house is a bit of a fixer-upper. But it has spectacular views of the core of our little Milky Way galaxy.” Thank you, William!

Bottom line: Celebrate dark night skies and help limit light pollution by raising awareness through the annual International Dark Sky Week, April 13 to 20, 2026. Find links here.

Read more: How can I celebrate International Dark Sky Week?

The post International Dark Sky Week is April 13 to 20 first appeared on EarthSky.



from EarthSky https://ift.tt/vXVxFcb
Two people pedaling bikes in the country at night for International Dark Sky week.
International Dark Sky Week is April 13 to 20, 2026. Image via IDA.
  • International Dark Sky Week is a worldwide celebration of the dark and natural night.
  • Light pollution is the human-made alteration of outdoor light levels.
  • Go Dark is the 2026 theme.

According to the International Dark-Sky Association (IDA) – founded in 1988 and based in Tucson, Arizona – light pollution is increasing at a rate twice that of human population growth. And about 80% of people around the world live under a light-polluted sky. That’s why IDA has established an International Dark Sky Week, which in 2026 falls on April 13 to 20. The goal for the week is to Go Dark. According to the IDA:

From the darkness needed for a restful night’s sleep to the activities we enjoy beneath the stars, the night is filled with wonder and importance. Dark nights sustain critical wildlife ecosystems, strengthen the well-being of our communities, enable scientific discovery, and preserve shared cultural knowledge and traditions.

The group also hopes you’ll learn the stars and constellations, and teach them to others.

Also, the IDA hopes you’ll join the global dark sky movement to protect and celebrate our shared heritage of dark night skies. DarkSky International promotes solutions that allow people to appreciate dark, star-filled skies while enjoying the benefits of responsible outdoor lighting.

According to the IDA:

For this International Dark Sky Week we invite you to join us as we discover the night together, exploring its importance and the actions we can take to protect dark skies.

Five labeled panels of sky above a city, suburbs, and country, showing less and less light-polluted view.
Poor lighting in cities leads to larger amounts of light pollution. From a dark country sky, you can see the river of stars that makes up our galaxy, the Milky Way. Image via IDA.

Ways to celebrate International Dark Sky Week

Looking for ways to celebrate International Dark Sky Week? Here’s International Dark Sky Week links for Get out at Night suggestions.

Visit EarthSky’s night sky guide to see what you can view in the sky this week. A highlight that week is the moon near Venus from April 18 to 20. For more information visit EarthSky’s night sky guide.

Visit EarthSky’s Best Places to Stargaze page to find a good dark-sky observing site close to home. Share your night sky photos at EarthSky Community Photos.

Paul Bogard has written extensively on the importance of darkness. His book is titled The End of Night. His TEDx Talk focuses on why we need darkness. You’ll find his TEDx Talk here.

Poster with animals and insects around a bright streetlight.
Curbing light pollution also benefits wildlife. Image via IDA.

Dark-sky photos from the EarthSky Community

Submit your photo to EarthSky here

A starry band in a starry sky above a treeline.
View at EarthSky Community Photos. | Muhammad Bilal in Talagang, Punjab, Pakistan, captured our home galaxy on March 6, 2025. Muhammad wrote: “As the summer is approaching, our very own Milky way Galaxy is back in sky.” Thank you, Muhammad!
An old abandoned house on the prairie with a large, cloudy band of stars above.
View at EarthSky Community Photos. | William Mathe made the 100-mile drive to Last Chance, Colorado, for this scene on March 16, 2024. William wrote: “The ranch house is a bit of a fixer-upper. But it has spectacular views of the core of our little Milky Way galaxy.” Thank you, William!

Bottom line: Celebrate dark night skies and help limit light pollution by raising awareness through the annual International Dark Sky Week, April 13 to 20, 2026. Find links here.

Read more: How can I celebrate International Dark Sky Week?

The post International Dark Sky Week is April 13 to 20 first appeared on EarthSky.



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