Salmon are coming home after a century: Lifeform of the week

The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Makes a great gift. Get yours today!

Salmon are coming home after a century

The Associated Press reported November 16, 2024, that hundreds of salmon are already returning to their ancestral spawning grounds on the Klamath River in southern Oregon and northern California. Their return follows what experts have called the world’s largest dam removal effort.

Completion of the demolition of four hydroelectric dams came a month ahead of schedule, AP said, and right in time for salmon mating season!

The National Oceanic and Atmospheric Administration (NOAA) had reported last summer on the dam removal project. They said it restores 420 miles (676 km) of watershed habitat for salmon. NOAA Research Fisheries biologist Tommy Williams called it a boon for the salmon ecosystem, saying:

When you simplify the habitat as we did with the dams, salmon can’t express the full range of their life-history diversity. The Klamath watershed is very prone to disturbance. The environment throughout the historical range of Pacific salmon and steelhead is very dynamic. We have fires, floods, earthquakes, you name it.

These fish not only deal with it well, it’s required for their survival by allowing the expression of the full range of their diversity. It challenges them.

Why destroy the dams?

Built from 1908 to 1962, the purpose of these dams was to provide electricity to cities, farms and mines in the region. The dams’ purpose was not to store water for drinking or irrigation or to prevent flooding.

Indigenous tribes were among those who suffered the effects of the dams. The Yurok tribe, which has always inhabited and managed the forests, rivers and coastal areas throughout Northern California, watched helplessly as salmon, sturgeon, trout and others lost their ancestral home following the construction of the dams.

Map, with a twisty blue river running into the sea, and a gray area representing the river watershed.
Salmon and many more creatures inhabit the Klamath River. It runs along the California-Oregon border. Image via Shannon1/ Wikipedia (CC BY-SA 4.0).

The dams’ disadvantages

Who owns the dams is who controls the water. The Federal Government currently owns and self-regulates only 4% of dams; most are privately owned. PacifiCorp was the current private owner of the Klamath River dams in question. And these dams produced less than 2% of the energy the company supplied to their customers.

In the face of numerous protests and hundreds of millions spent on federally ordered improvements for maintenance and sustainability, it was agreed to demolish four of the eight dams.

Will the past decades of damming forever change the future of this river? It’s too soon to say. However, local tribes have already begun to see hundreds of salmon arrive in the newly released tributaries.

Among forested hills, a concrete wall across a stream stands above some water gushing out of a gate in it.
This is the John C. Boyle Dam. It is one of the 4 dams removed in 2024. Image via Bobjgalindo/ Wikipedia (CC BY-SA 3.0).

What are the benefits of the dams’ demolition?

When the dams were operational, the water behind them was a hot soup filled with bacteria and algae. In fact, in 2002, the Klamath River suffered severely from an unprecedented lethal event: a branchiomycosis (gill rot) epidemic that killed approximately 34,000 fish. This was caused by rising water temperatures and low river flows.

All four dams have already been demolished, and it is estimated that by early next year, every remaining piece of concrete will be removed. The project reopens hundreds of miles of habitat for threatened fish that had been isolated for more than a century.

These migratory fish, which encountered insurmountable barriers along their ancestral routes, will finally be able to return to their historic habitat.

Blue river in a steep forested valley, with some white wildflowers in the foreground.
Demolishing the dams will allow water to flow again and run fresh. Salmon will be able to return to healthy waters. Image via Bureau of Land Management Oregon and Washington/ Wikipedia (public domain).

Salmon are migratory fish

Having open, clean and fresh waterways is important because adult salmon return from the sea to the rivers where they were born to spawn or lay their eggs. In fact, they are anadromous fish, which means that they live both in fresh water, which is where they hatch, and in salt water, which is where they live most of their lives.

They also have a strong, flexible tail fin that helps them swim against the current to return to the rivers where they were born. They can even swim at 31 miles per hour (50 kph). Impressive!

A sinuous blue river in a forested landscape flows past sandbars into the ocean.
Aerial view of the mouth of the Klamath River. Salmon spend most of their time in salt water in the sea or ocean. When they’re adults, they return to the rivers where they were spawned, that is, freshwater. Image via U.S. Army Corps of Engineers/ Wikipedia (public domain).

Salmon reproduction is amazing

Did you know salmon change color? Young salmon are silvery but, as adults, they develop a darker color with spots. And that’s not the only thing that changes. When breeding season comes, males modify their jaws. The lower jaw curves upward, giving rise to a hook.

This change in the salmon’s mouth allows it to have the best weapon to fight with other males for females. In fact, the size of this weapon is enough to deter less-developed competitors.

Males defend the areas of the river that are best suited for laying eggs and attack other males that come close. Females, which have hardly undergone any physical changes, dig into the gravel to deposit their eggs, which they cover up later. Then, they leave the area while their partner stays for several days or even weeks.

But the most surprising thing is that after breeding, males develop teeth again and lose their hook. Those who manage to survive and return to the river the following year transform once again. But then their jaws will be even larger.

A gray salmon jumping upstream over a shallow waterfall.
Salmon have a strong and flexible tail fin that helps them swim against the current to return to the rivers where they were hatched. Males also develop a hook-shaped jaw just before the mating season. Image via Drew Farwell/ Unsplash.

Are all salmon orange?

Some salmon are orange inside, which is a rare color in nature. These fish are carnivorous, feeding on smaller fish, crustaceans such as shrimp, and insects. Thus, the color of their flesh depends on the number of crustaceans they consume. The more crustaceans they eat, the more pink or red their flesh will be. This is also true of flamingos. What curious animals surround us!

Two fish, darker on top with silver bellies, jumping upstream over a small, turbulent waterfall.
Young salmon are silvery and, as adults, they develop a darker color with spots. Image via Brandon/ Unsplash.
Fish, underwater, with many small dark dots, silver above and red on its side and belly.
Salmon feed on crustaceans such as shrimp. That’s what gives them their orange color inside. Image via NOAA Fisheries (public domain).

Bottom line: Salmon are coming back to their ancestral homes after the demolition of four dams on the Klamath River, which flows along the California-Oregon border.

Via NOAA

Via Associated Press

Flamingos are beautiful and peculiar: Lifeform of the week

Ocean sunfish are odd, gentle giants: Lifeform of the week

The post Salmon are coming home after a century: Lifeform of the week first appeared on EarthSky.



from EarthSky https://ift.tt/QfDEGSn

The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Makes a great gift. Get yours today!

Salmon are coming home after a century

The Associated Press reported November 16, 2024, that hundreds of salmon are already returning to their ancestral spawning grounds on the Klamath River in southern Oregon and northern California. Their return follows what experts have called the world’s largest dam removal effort.

Completion of the demolition of four hydroelectric dams came a month ahead of schedule, AP said, and right in time for salmon mating season!

The National Oceanic and Atmospheric Administration (NOAA) had reported last summer on the dam removal project. They said it restores 420 miles (676 km) of watershed habitat for salmon. NOAA Research Fisheries biologist Tommy Williams called it a boon for the salmon ecosystem, saying:

When you simplify the habitat as we did with the dams, salmon can’t express the full range of their life-history diversity. The Klamath watershed is very prone to disturbance. The environment throughout the historical range of Pacific salmon and steelhead is very dynamic. We have fires, floods, earthquakes, you name it.

These fish not only deal with it well, it’s required for their survival by allowing the expression of the full range of their diversity. It challenges them.

Why destroy the dams?

Built from 1908 to 1962, the purpose of these dams was to provide electricity to cities, farms and mines in the region. The dams’ purpose was not to store water for drinking or irrigation or to prevent flooding.

Indigenous tribes were among those who suffered the effects of the dams. The Yurok tribe, which has always inhabited and managed the forests, rivers and coastal areas throughout Northern California, watched helplessly as salmon, sturgeon, trout and others lost their ancestral home following the construction of the dams.

Map, with a twisty blue river running into the sea, and a gray area representing the river watershed.
Salmon and many more creatures inhabit the Klamath River. It runs along the California-Oregon border. Image via Shannon1/ Wikipedia (CC BY-SA 4.0).

The dams’ disadvantages

Who owns the dams is who controls the water. The Federal Government currently owns and self-regulates only 4% of dams; most are privately owned. PacifiCorp was the current private owner of the Klamath River dams in question. And these dams produced less than 2% of the energy the company supplied to their customers.

In the face of numerous protests and hundreds of millions spent on federally ordered improvements for maintenance and sustainability, it was agreed to demolish four of the eight dams.

Will the past decades of damming forever change the future of this river? It’s too soon to say. However, local tribes have already begun to see hundreds of salmon arrive in the newly released tributaries.

Among forested hills, a concrete wall across a stream stands above some water gushing out of a gate in it.
This is the John C. Boyle Dam. It is one of the 4 dams removed in 2024. Image via Bobjgalindo/ Wikipedia (CC BY-SA 3.0).

What are the benefits of the dams’ demolition?

When the dams were operational, the water behind them was a hot soup filled with bacteria and algae. In fact, in 2002, the Klamath River suffered severely from an unprecedented lethal event: a branchiomycosis (gill rot) epidemic that killed approximately 34,000 fish. This was caused by rising water temperatures and low river flows.

All four dams have already been demolished, and it is estimated that by early next year, every remaining piece of concrete will be removed. The project reopens hundreds of miles of habitat for threatened fish that had been isolated for more than a century.

These migratory fish, which encountered insurmountable barriers along their ancestral routes, will finally be able to return to their historic habitat.

Blue river in a steep forested valley, with some white wildflowers in the foreground.
Demolishing the dams will allow water to flow again and run fresh. Salmon will be able to return to healthy waters. Image via Bureau of Land Management Oregon and Washington/ Wikipedia (public domain).

Salmon are migratory fish

Having open, clean and fresh waterways is important because adult salmon return from the sea to the rivers where they were born to spawn or lay their eggs. In fact, they are anadromous fish, which means that they live both in fresh water, which is where they hatch, and in salt water, which is where they live most of their lives.

They also have a strong, flexible tail fin that helps them swim against the current to return to the rivers where they were born. They can even swim at 31 miles per hour (50 kph). Impressive!

A sinuous blue river in a forested landscape flows past sandbars into the ocean.
Aerial view of the mouth of the Klamath River. Salmon spend most of their time in salt water in the sea or ocean. When they’re adults, they return to the rivers where they were spawned, that is, freshwater. Image via U.S. Army Corps of Engineers/ Wikipedia (public domain).

Salmon reproduction is amazing

Did you know salmon change color? Young salmon are silvery but, as adults, they develop a darker color with spots. And that’s not the only thing that changes. When breeding season comes, males modify their jaws. The lower jaw curves upward, giving rise to a hook.

This change in the salmon’s mouth allows it to have the best weapon to fight with other males for females. In fact, the size of this weapon is enough to deter less-developed competitors.

Males defend the areas of the river that are best suited for laying eggs and attack other males that come close. Females, which have hardly undergone any physical changes, dig into the gravel to deposit their eggs, which they cover up later. Then, they leave the area while their partner stays for several days or even weeks.

But the most surprising thing is that after breeding, males develop teeth again and lose their hook. Those who manage to survive and return to the river the following year transform once again. But then their jaws will be even larger.

A gray salmon jumping upstream over a shallow waterfall.
Salmon have a strong and flexible tail fin that helps them swim against the current to return to the rivers where they were hatched. Males also develop a hook-shaped jaw just before the mating season. Image via Drew Farwell/ Unsplash.

Are all salmon orange?

Some salmon are orange inside, which is a rare color in nature. These fish are carnivorous, feeding on smaller fish, crustaceans such as shrimp, and insects. Thus, the color of their flesh depends on the number of crustaceans they consume. The more crustaceans they eat, the more pink or red their flesh will be. This is also true of flamingos. What curious animals surround us!

Two fish, darker on top with silver bellies, jumping upstream over a small, turbulent waterfall.
Young salmon are silvery and, as adults, they develop a darker color with spots. Image via Brandon/ Unsplash.
Fish, underwater, with many small dark dots, silver above and red on its side and belly.
Salmon feed on crustaceans such as shrimp. That’s what gives them their orange color inside. Image via NOAA Fisheries (public domain).

Bottom line: Salmon are coming back to their ancestral homes after the demolition of four dams on the Klamath River, which flows along the California-Oregon border.

Via NOAA

Via Associated Press

Flamingos are beautiful and peculiar: Lifeform of the week

Ocean sunfish are odd, gentle giants: Lifeform of the week

The post Salmon are coming home after a century: Lifeform of the week first appeared on EarthSky.



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Is this a volcanic exoplanet? Hints are in its atmosphere

Volcanic exoplanet: Planet with wispy white clouds. A bright sun is at the edge in the distance, with many more stars in the background.
Artist’s concept of L 98-59 d, a super-Earth world 35 light-years away. Now, new results from NASA’s Webb Space Telescope suggest it might be an active volcanic exoplanet with a sulfur-rich atmosphere. Image via NASA.
  • L 98-59 d is a super-Earth exoplanet, discovered in 2019. It’s 35 light-years away and about 1.5 times the size of Earth.
  • The Webb space telescope observed the planet again recently, looking for evidence of an atmosphere.
  • It found the planet has a sulfur-rich atmosphere, the new results suggest. Astronomers said it might be an active volcanic world, with volcanoes reminiscent of those on Jupiter’s volcanic moon Io.

The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Makes a great gift. Get yours today!

Is this a volcanic exoplanet?

Volcanoes are common in our solar system. Earth, Mars and Venus all have them. Even some moons do, for example, Jupiter’s moon Io. But what about distant exoplanets around other stars? On November 11, 2024, researchers at The Open University in the U.K. said they’ve found possible evidence for a sulfur-rich atmosphere on a planet 35 light-years away. The planet is labeled L 98-59 d. It’s about 1.5 times the size of Earth. The researchers tentatively detected the gases sulfur dioxide (SO2) and hydrogen sulfide (H2S) in its atmosphere. If confirmed, it would indicate the surface is likely molten or volcanic. Exoplanet L 98-59 d would also be the smallest of the distant planets known so far that have confirmed atmospheres.

The researchers used NASA’s Webb Space Telescope to make the discovery.

Researcher Agnibha Banerjee at The Open University wrote about the new findings in The Conversation on November 11, 2024.

The researchers published their peer-reviewed findings in The Astrophysical Letters on October 30, 2024.

Meet L 98-59 d

L 98-59 d is a rocky planet, like Earth, and about 1.5 times the size of Earth. This puts it in the category of super-Earth. It orbits an M-type star – or red dwarf – 35 light-years from Earth. NASA’s Transiting Exoplanet Survey Satellite (TESS) space telescope discovered it in 2019.

TESS used the transit method to detect the planet. That’s when a planet transits – passes in front of – its star, as seen from Earth. L 98-59 d orbits close to its star, completing an orbit in only 7.5 days.

A volcanic exoplanet with a sulfur-rich atmosphere?

Banerjee and colleagues used NASA’s Webb Space Telescope to observe one transit of the planet. As the planet passed in front of the star, Webb tried to detect an atmosphere. It did so by analyzing the transmission spectrum of the planet. That is where some light is absorbed by the atmosphere and some is transmitted through it. In the spectrum, the dark lines and dim bands of light correspond to atoms and molecules in the planet’s atmosphere. And, indeed, the analysis showed evidence of a possible atmosphere, more specifically an atmosphere filled with sulfur dioxide and hydrogen sulfide. The paper stated:

The atmospheric spectrum indicates the possible presence of the sulfur-bearing species H2S and SO2, which could hint at active volcanism on this planet if verified by future observations.

What does that mean?

Planet-like body with mottled surface of various bright colors, on black background. A small bluish plume shape is at the top.
View larger. | L 98-59 d’s volcanoes are likely more similar to those on Jupiter’s moon Io than those on Earth. NASA’s Galileo spacecraft obtained this image on June 28, 1997. Here, an active volcano erupts on the moon’s limb at the top. Image via NASA/JPL/ University of Arizona.

A volcanic world, but not like Earth

The discovery of those two gases suggests L 98-59 d is likely a volcanic or molten world. However, it would be unlike any of the planets in our solar system that have volcanoes. Earth, of course, has many active volcanoes. In addition, there is growing evidence that Venus’ volcanoes are still active as well. And there are huge volcanoes on Mars, although they have been dead or dormant for millions to billions of years. But Earth’s atmosphere is dominated by nitrogen, while the atmospheres of Venus and Mars are mostly carbon dioxide.

An Io-like world?

So, this means the volcanic processes on L 98-59 d are likely quite different. In fact, they might be more similar to Jupiter’s moon Io, which is the most volcanically active body in our solar system. On Io, tidal heating drives volcanism. Jupiter’s immense gravity pulls and squeezes Io, heating it on the inside.

As a result, Io’s insides are constantly melting and spewing out through volcanoes. This may be similar to L 98-59 d, because it orbits so close to its star.

If L 98-59 d is truly volcanically active, and in a way not seen on rocky planets in our own solar system, that would be exciting for planetary scientists. It would be a chance to get a glimpse of volcanic processes not seen on planets before. As the paper noted:

The rocky planets in the solar system all have different atmospheric compositions, and the study of such atmospheres in exoplanetary systems could unlock a rich diversity of unexplored chemistries.

Bottom line: L 98-59 d, a super-Earth 35 light-years away, may be a volcanic exoplanet. NASA’s Webb space telescope has detected a possible sulfur-rich atmosphere.

Source: Atmospheric Retrievals Suggest the Presence of a Secondary Atmosphere and Possible Sulfur Species on L98-59 d from JWST Nirspec G395H Transmission Spectroscopy

Via The Conversation

Read more:

Is there a volcanic exomoon orbiting this giant exoplanet?

Wow! New volcano on Jupiter’s moon Io

Active Venus volcanoes revealed again in Magellan data

The post Is this a volcanic exoplanet? Hints are in its atmosphere first appeared on EarthSky.



from EarthSky https://ift.tt/1MsU7AV
Volcanic exoplanet: Planet with wispy white clouds. A bright sun is at the edge in the distance, with many more stars in the background.
Artist’s concept of L 98-59 d, a super-Earth world 35 light-years away. Now, new results from NASA’s Webb Space Telescope suggest it might be an active volcanic exoplanet with a sulfur-rich atmosphere. Image via NASA.
  • L 98-59 d is a super-Earth exoplanet, discovered in 2019. It’s 35 light-years away and about 1.5 times the size of Earth.
  • The Webb space telescope observed the planet again recently, looking for evidence of an atmosphere.
  • It found the planet has a sulfur-rich atmosphere, the new results suggest. Astronomers said it might be an active volcanic world, with volcanoes reminiscent of those on Jupiter’s volcanic moon Io.

The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Makes a great gift. Get yours today!

Is this a volcanic exoplanet?

Volcanoes are common in our solar system. Earth, Mars and Venus all have them. Even some moons do, for example, Jupiter’s moon Io. But what about distant exoplanets around other stars? On November 11, 2024, researchers at The Open University in the U.K. said they’ve found possible evidence for a sulfur-rich atmosphere on a planet 35 light-years away. The planet is labeled L 98-59 d. It’s about 1.5 times the size of Earth. The researchers tentatively detected the gases sulfur dioxide (SO2) and hydrogen sulfide (H2S) in its atmosphere. If confirmed, it would indicate the surface is likely molten or volcanic. Exoplanet L 98-59 d would also be the smallest of the distant planets known so far that have confirmed atmospheres.

The researchers used NASA’s Webb Space Telescope to make the discovery.

Researcher Agnibha Banerjee at The Open University wrote about the new findings in The Conversation on November 11, 2024.

The researchers published their peer-reviewed findings in The Astrophysical Letters on October 30, 2024.

Meet L 98-59 d

L 98-59 d is a rocky planet, like Earth, and about 1.5 times the size of Earth. This puts it in the category of super-Earth. It orbits an M-type star – or red dwarf – 35 light-years from Earth. NASA’s Transiting Exoplanet Survey Satellite (TESS) space telescope discovered it in 2019.

TESS used the transit method to detect the planet. That’s when a planet transits – passes in front of – its star, as seen from Earth. L 98-59 d orbits close to its star, completing an orbit in only 7.5 days.

A volcanic exoplanet with a sulfur-rich atmosphere?

Banerjee and colleagues used NASA’s Webb Space Telescope to observe one transit of the planet. As the planet passed in front of the star, Webb tried to detect an atmosphere. It did so by analyzing the transmission spectrum of the planet. That is where some light is absorbed by the atmosphere and some is transmitted through it. In the spectrum, the dark lines and dim bands of light correspond to atoms and molecules in the planet’s atmosphere. And, indeed, the analysis showed evidence of a possible atmosphere, more specifically an atmosphere filled with sulfur dioxide and hydrogen sulfide. The paper stated:

The atmospheric spectrum indicates the possible presence of the sulfur-bearing species H2S and SO2, which could hint at active volcanism on this planet if verified by future observations.

What does that mean?

Planet-like body with mottled surface of various bright colors, on black background. A small bluish plume shape is at the top.
View larger. | L 98-59 d’s volcanoes are likely more similar to those on Jupiter’s moon Io than those on Earth. NASA’s Galileo spacecraft obtained this image on June 28, 1997. Here, an active volcano erupts on the moon’s limb at the top. Image via NASA/JPL/ University of Arizona.

A volcanic world, but not like Earth

The discovery of those two gases suggests L 98-59 d is likely a volcanic or molten world. However, it would be unlike any of the planets in our solar system that have volcanoes. Earth, of course, has many active volcanoes. In addition, there is growing evidence that Venus’ volcanoes are still active as well. And there are huge volcanoes on Mars, although they have been dead or dormant for millions to billions of years. But Earth’s atmosphere is dominated by nitrogen, while the atmospheres of Venus and Mars are mostly carbon dioxide.

An Io-like world?

So, this means the volcanic processes on L 98-59 d are likely quite different. In fact, they might be more similar to Jupiter’s moon Io, which is the most volcanically active body in our solar system. On Io, tidal heating drives volcanism. Jupiter’s immense gravity pulls and squeezes Io, heating it on the inside.

As a result, Io’s insides are constantly melting and spewing out through volcanoes. This may be similar to L 98-59 d, because it orbits so close to its star.

If L 98-59 d is truly volcanically active, and in a way not seen on rocky planets in our own solar system, that would be exciting for planetary scientists. It would be a chance to get a glimpse of volcanic processes not seen on planets before. As the paper noted:

The rocky planets in the solar system all have different atmospheric compositions, and the study of such atmospheres in exoplanetary systems could unlock a rich diversity of unexplored chemistries.

Bottom line: L 98-59 d, a super-Earth 35 light-years away, may be a volcanic exoplanet. NASA’s Webb space telescope has detected a possible sulfur-rich atmosphere.

Source: Atmospheric Retrievals Suggest the Presence of a Secondary Atmosphere and Possible Sulfur Species on L98-59 d from JWST Nirspec G395H Transmission Spectroscopy

Via The Conversation

Read more:

Is there a volcanic exomoon orbiting this giant exoplanet?

Wow! New volcano on Jupiter’s moon Io

Active Venus volcanoes revealed again in Magellan data

The post Is this a volcanic exoplanet? Hints are in its atmosphere first appeared on EarthSky.



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Orion the Hunter is back in the evening sky

Star chart of constellation Orion with stars, Belt, and a nebula labeled.
Orion the Hunter – a very noticeable constellation – rises in the east on November evenings. You can’t miss it! Chart via EarthSky.

Orion the Hunter’s season in the sky

November evenings are a great time to say hello to everyone’s favorite constellation: Orion the Hunter. Find Orion now and enjoy it for months to come! Without a doubt, Orion is the easiest-to-identify of all constellations. Look for it in the eastern sky this month, say, between the hours of 10 p.m. and midnight (that’s your local time, the time on your clock no matter where you are). You’ll notice Orion’s Belt first. The Belt is made of three stars in a short, straight row. The Belt stars aren’t the brightest in the sky. But they’re the reason Orion will catch your eye.

And you’ll also notice Orion’s two brightest stars – Betelgeuse and Rigel – shining on opposite sides of the Belt.

You can find this constellation easily. Then you can point it out to your friends!

So look for Orion. It’s at this time of the year – around mid-November and into early December – that casual skywatchers start to notice Orion and comment on it.

The 2025 EarthSky Lunar Calendar makes a great gift. Get yours today!

Bright but slightly fuzzy stars in wide array high above dark landscape, and one single one near horizon.
View at EarthSky Community Photos. | Sergei Timofeevski shared this image from November 13, 2023. Sergei wrote: “The constellation Orion the Hunter and the star Sirius rising just above the eastern horizon in the Anza-Borrego Desert State Park, California.” Thank you, Sergei! Note bright Sirius is on the bottom, and Orion’s Belt pointing to it.

As the weeks pass …

In mid-November, Orion doesn’t reach its highest point until an hour or two after midnight your local time. Northern Hemisphere skywatchers will find it high in the south at its highest point. Southern Hemisphere skywatchers will find it northward.

Like all stars seen from Earth, Orion’s stars rise some four minutes earlier with each passing day, or about two hours earlier with each passing month. If you see Orion shining in the east at 10 p.m. tonight, look for this constellation to be in the same place in the sky at about 8 p.m. a month from now. Or if Orion is due south at 2 a.m. tomorrow, look for Orion to be due south at midnight one month later.

This shift in Orion’s location is due to Earth’s movement in orbit around the sun. As we move around the sun, our perspective on the stars surrounding us shifts. At the same hour daily, all the stars in the eastern half of the sky climb up a bit higher. And at the same time on your clock each day, all the stars in the western half of the sky sink a bit closer to the western horizon.

Star map of Orion

A star map of Orion (in green lines) with its stars and many others, in black on white.
A map of Orion the Hunter, showing the locations of Betelgeuse and Rigel. Image via IAU/ Sky & Telescope magazine/ Wikimedia Commons (CC BY 3.0).

Bottom line: By mid-to-late November, the famous constellation Orion the Hunter is back in the evening sky! Its most recognizable feature is called Orion’s Belt: a short, straight line of three medium-bright stars.

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

The post Orion the Hunter is back in the evening sky first appeared on EarthSky.



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Star chart of constellation Orion with stars, Belt, and a nebula labeled.
Orion the Hunter – a very noticeable constellation – rises in the east on November evenings. You can’t miss it! Chart via EarthSky.

Orion the Hunter’s season in the sky

November evenings are a great time to say hello to everyone’s favorite constellation: Orion the Hunter. Find Orion now and enjoy it for months to come! Without a doubt, Orion is the easiest-to-identify of all constellations. Look for it in the eastern sky this month, say, between the hours of 10 p.m. and midnight (that’s your local time, the time on your clock no matter where you are). You’ll notice Orion’s Belt first. The Belt is made of three stars in a short, straight row. The Belt stars aren’t the brightest in the sky. But they’re the reason Orion will catch your eye.

And you’ll also notice Orion’s two brightest stars – Betelgeuse and Rigel – shining on opposite sides of the Belt.

You can find this constellation easily. Then you can point it out to your friends!

So look for Orion. It’s at this time of the year – around mid-November and into early December – that casual skywatchers start to notice Orion and comment on it.

The 2025 EarthSky Lunar Calendar makes a great gift. Get yours today!

Bright but slightly fuzzy stars in wide array high above dark landscape, and one single one near horizon.
View at EarthSky Community Photos. | Sergei Timofeevski shared this image from November 13, 2023. Sergei wrote: “The constellation Orion the Hunter and the star Sirius rising just above the eastern horizon in the Anza-Borrego Desert State Park, California.” Thank you, Sergei! Note bright Sirius is on the bottom, and Orion’s Belt pointing to it.

As the weeks pass …

In mid-November, Orion doesn’t reach its highest point until an hour or two after midnight your local time. Northern Hemisphere skywatchers will find it high in the south at its highest point. Southern Hemisphere skywatchers will find it northward.

Like all stars seen from Earth, Orion’s stars rise some four minutes earlier with each passing day, or about two hours earlier with each passing month. If you see Orion shining in the east at 10 p.m. tonight, look for this constellation to be in the same place in the sky at about 8 p.m. a month from now. Or if Orion is due south at 2 a.m. tomorrow, look for Orion to be due south at midnight one month later.

This shift in Orion’s location is due to Earth’s movement in orbit around the sun. As we move around the sun, our perspective on the stars surrounding us shifts. At the same hour daily, all the stars in the eastern half of the sky climb up a bit higher. And at the same time on your clock each day, all the stars in the western half of the sky sink a bit closer to the western horizon.

Star map of Orion

A star map of Orion (in green lines) with its stars and many others, in black on white.
A map of Orion the Hunter, showing the locations of Betelgeuse and Rigel. Image via IAU/ Sky & Telescope magazine/ Wikimedia Commons (CC BY 3.0).

Bottom line: By mid-to-late November, the famous constellation Orion the Hunter is back in the evening sky! Its most recognizable feature is called Orion’s Belt: a short, straight line of three medium-bright stars.

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First close-up image of a star outside the Milky Way

Star outside the Milky Way: Bright orange oval blob with a sketchy ring around it and some other lines on a black background.
This is the first close-up picture of a star outside the Milky Way galaxy, WOH G64. The star lies in a neighboring galaxy known as the Large Magellanic Cloud, which is more than 160,000 light-years away. The GRAVITY instrument on the European Southern Observatory’s Very Large Telescope Interferometer captured this image. The bright oval is a dusty envelope around the star, which is in the last stages before a supernova. Image via ESO/ K. Ohnaka et al. 

First close-up image of a star outside the Milky Way

On November 21, 2024, astronomers at the European Southern Observatory said that they’ve captured a close-up image of a star in another galaxy for the first time. The star is WOH G64, lying 160,000 light-years away in the Large Magellanic Cloud, a neighboring dwarf galaxy of the Milky Way. Astronomers believe the large oval shape is the dusty cocoon of a star in the last stages of life before it goes supernova.

The astronomers published their findings in the peer-reviewed journal Astronomy and Astrophysics on November 21, 2024.

Lead author Keiichi Ohnaka of the Andrés Bello National University in Chile said:

We discovered an egg-shaped cocoon closely surrounding the star. We are excited because this may be related to the drastic ejection of material from the dying star before a supernova explosion.

The behemoth star

Astronomers have known about this star for decades and nicknamed it the behemoth star. It’s a red supergiant about 2,000 times the size of our sun.

To get this image, the team used the GRAVITY instrument on the European Southern Observatory’s Very Large Telescope Interferometer in Chile’s Atacama Desert. This second-generation instruments captures the light of four telescopes and makes the resolution of the star possible.

Comparing the new, close-up image of the star to previous observations, astronomers could see that the star has dimmed. Co-author Gerd Weigelt of the Max Planck Institute for Radio Astronomy in Germany said:

We have found that the star has been experiencing a significant change in the last 10 years, providing us with a rare opportunity to witness a star’s life in real time.

The star is likely making its last exhalations, expelling the dusty ring and cocoon we see in the image. Co-author Jacco van Loon of Keele University in the UK said:

This star is one of the most extreme of its kind, and any drastic change may bring it closer to an explosive end.

More observations

After this the team will make more observations to better understand what is happening with the star. They found the stretched-out cocoon shape surprising, and said it:

… could be explained by either the star’s shedding or by the influence of a yet-undiscovered companion star.

Additionally, the fainter elliptical ring could be the inner rim of a dusty torus, but more observations are needed to confirm that theory.

Bright orange blob at center with darker orange tendrils across the face and in a ring.
Artist’s concept of WOH G64. The main features of this star are its dusty, oval cocoon and dusty ring. Scientists will need more observations to nail down the nature of its egg and ring shapes. Image via ESO/ L. Calçada.

Bottom line: Astronomers have taken the first close-up image of a star in a galaxy outside of our own Milky Way. And this star – WOH G64 in the Large Magellanic Cloud – appears to be getting ready to go supernova.

Source: Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic Cloud

Via ESO

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Star outside the Milky Way: Bright orange oval blob with a sketchy ring around it and some other lines on a black background.
This is the first close-up picture of a star outside the Milky Way galaxy, WOH G64. The star lies in a neighboring galaxy known as the Large Magellanic Cloud, which is more than 160,000 light-years away. The GRAVITY instrument on the European Southern Observatory’s Very Large Telescope Interferometer captured this image. The bright oval is a dusty envelope around the star, which is in the last stages before a supernova. Image via ESO/ K. Ohnaka et al. 

First close-up image of a star outside the Milky Way

On November 21, 2024, astronomers at the European Southern Observatory said that they’ve captured a close-up image of a star in another galaxy for the first time. The star is WOH G64, lying 160,000 light-years away in the Large Magellanic Cloud, a neighboring dwarf galaxy of the Milky Way. Astronomers believe the large oval shape is the dusty cocoon of a star in the last stages of life before it goes supernova.

The astronomers published their findings in the peer-reviewed journal Astronomy and Astrophysics on November 21, 2024.

Lead author Keiichi Ohnaka of the Andrés Bello National University in Chile said:

We discovered an egg-shaped cocoon closely surrounding the star. We are excited because this may be related to the drastic ejection of material from the dying star before a supernova explosion.

The behemoth star

Astronomers have known about this star for decades and nicknamed it the behemoth star. It’s a red supergiant about 2,000 times the size of our sun.

To get this image, the team used the GRAVITY instrument on the European Southern Observatory’s Very Large Telescope Interferometer in Chile’s Atacama Desert. This second-generation instruments captures the light of four telescopes and makes the resolution of the star possible.

Comparing the new, close-up image of the star to previous observations, astronomers could see that the star has dimmed. Co-author Gerd Weigelt of the Max Planck Institute for Radio Astronomy in Germany said:

We have found that the star has been experiencing a significant change in the last 10 years, providing us with a rare opportunity to witness a star’s life in real time.

The star is likely making its last exhalations, expelling the dusty ring and cocoon we see in the image. Co-author Jacco van Loon of Keele University in the UK said:

This star is one of the most extreme of its kind, and any drastic change may bring it closer to an explosive end.

More observations

After this the team will make more observations to better understand what is happening with the star. They found the stretched-out cocoon shape surprising, and said it:

… could be explained by either the star’s shedding or by the influence of a yet-undiscovered companion star.

Additionally, the fainter elliptical ring could be the inner rim of a dusty torus, but more observations are needed to confirm that theory.

Bright orange blob at center with darker orange tendrils across the face and in a ring.
Artist’s concept of WOH G64. The main features of this star are its dusty, oval cocoon and dusty ring. Scientists will need more observations to nail down the nature of its egg and ring shapes. Image via ESO/ L. Calçada.

Bottom line: Astronomers have taken the first close-up image of a star in a galaxy outside of our own Milky Way. And this star – WOH G64 in the Large Magellanic Cloud – appears to be getting ready to go supernova.

Source: Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic Cloud

Via ESO

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Could the space station leak lead to ‘catastrophic failure’?

Space station leak: The space station with modules and solar panels all hooked together above a cloudy Earth.
The Crew Dragon captured this view of the International Space Station (ISS) on November 8, 2021. Earlier, in 2019, the space station sprang a leak in one of its modules. Then, on November 13, 2024, NASA said in a meeting that the space station leak presents the possibility of a “catastrophic failure”. Image via NASA Flickr.

Space station leak could be ‘catastrophic’

In 2019, one of the modules on the International Space Station (ISS) sprang a leak. The leak is on a Russian portion of the space station – a transfer tunnel – called PrK. It separates a docking port from the rest of the module. Overall, the leak loses about 3.7 pounds (1.7 kilograms) of air per day. As a stopgap solution, astronauts have been sealing off the PrK when not in use. But how severe is the problem? According to Roscosmos, it’s safe, but according to NASA, it could lead to “the possibility of a catastrophic failure.”

On November 13, 2024, NASA held a meeting on the safety and operational readiness of the space station. In that meeting, former astronaut Bob Cabana, chair of the NASA International Space Station Advisory Committee, reported on a September 2024 discussion between NASA and Russia’s space agency, Roscosmos, concerning the leak.

Jeff Foust, reporting for SpaceNews, wrote:

Cabana said at the committee meeting that there is no agreement between NASA and Roscosmos on the severity of the issue. ‘While the Russian team continues to search for and seal the leaks, it does not believe catastrophic disintegration of the PrK is realistic,’ he said. ‘NASA has expressed concerns about the structural integrity of the PrK and the possibility of a catastrophic failure.’

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Managing risks on the space station

Previously, NASA released a report on September 26, 2024, of its management of risks on the space station. As of now, the current plan is to keep the space station in good working order through 2030, with a deorbit in 2031.

The report said:

NASA and Roscosmos continue to work together to address structural issues with the Russian Service Module Transfer Tunnel. Cracks and air leaks in the tunnel are a top safety risk … both agencies are collaborating to investigate and mitigate the cracks and leaks; determine the root cause, which includes sharing sample metals, welds and Roscosmos investigation reports; and monitor the station for new leaks.

In February 2024 NASA identified an increase in the leak rate … Later, in May and June 2024, ISS Program and Roscosmos officials met to discuss heightened concerns with the increased leak rate. Subsequently, the ISS Program elevated the Service Module Transfer Tunnel leak risk to the highest level of risk in its risk management system. According to NASA, Roscosmos is confident they will be able to monitor and close the hatch to the Service Module prior to the leak rate reaching an untenable level. However, NASA and Roscosmos have not reached an agreement on the point at which the leak rate is untenable.

Although the root cause of the leak remains unknown, both agencies have narrowed their focus to internal and external welds. As of June 2024, there was no indication of other leaks on the station.

Graphic showing breakdown of the parts of the space station by country and the problem area in red.
View larger. | Here’s a breakdown of the space station segments by space agency. The location of the PrK is in red. Image via NASA.

A disagreement over the leak

Currently, neither space agency is sure what caused the leak. Indeed, as Foust reported:

Russian engineers believe the cracks are likely caused by ‘high cyclic fatigue’ from micro-vibrations. NASA, by contrast, believes several factors are at play, including pressure and mechanical stress, residual stress, material properties of the module and environmental exposure.

In addition, Foust quoted Cabana as saying:

The Russians believe that continued operations are safe but they can’t prove to our satisfaction that they are, and the U.S. believes that it’s not safe but we can’t prove to the Russians’ satisfaction that that’s the case.

So, the space agencies are going to look to outside experts to identify the root cause of the problem and thus the best solution.

Bottom line: In 2019, the space station acquired a leak in a transfer tunnel. NASA said the space station leak could lead to a “catastrophic failure.”

Via SpaceNews

Via NASA’s Management to Risks to Sustaining ISS Operations through 2030

The post Could the space station leak lead to ‘catastrophic failure’? first appeared on EarthSky.



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Space station leak: The space station with modules and solar panels all hooked together above a cloudy Earth.
The Crew Dragon captured this view of the International Space Station (ISS) on November 8, 2021. Earlier, in 2019, the space station sprang a leak in one of its modules. Then, on November 13, 2024, NASA said in a meeting that the space station leak presents the possibility of a “catastrophic failure”. Image via NASA Flickr.

Space station leak could be ‘catastrophic’

In 2019, one of the modules on the International Space Station (ISS) sprang a leak. The leak is on a Russian portion of the space station – a transfer tunnel – called PrK. It separates a docking port from the rest of the module. Overall, the leak loses about 3.7 pounds (1.7 kilograms) of air per day. As a stopgap solution, astronauts have been sealing off the PrK when not in use. But how severe is the problem? According to Roscosmos, it’s safe, but according to NASA, it could lead to “the possibility of a catastrophic failure.”

On November 13, 2024, NASA held a meeting on the safety and operational readiness of the space station. In that meeting, former astronaut Bob Cabana, chair of the NASA International Space Station Advisory Committee, reported on a September 2024 discussion between NASA and Russia’s space agency, Roscosmos, concerning the leak.

Jeff Foust, reporting for SpaceNews, wrote:

Cabana said at the committee meeting that there is no agreement between NASA and Roscosmos on the severity of the issue. ‘While the Russian team continues to search for and seal the leaks, it does not believe catastrophic disintegration of the PrK is realistic,’ he said. ‘NASA has expressed concerns about the structural integrity of the PrK and the possibility of a catastrophic failure.’

The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Keep up with all phases of the moon every night of the year.

Managing risks on the space station

Previously, NASA released a report on September 26, 2024, of its management of risks on the space station. As of now, the current plan is to keep the space station in good working order through 2030, with a deorbit in 2031.

The report said:

NASA and Roscosmos continue to work together to address structural issues with the Russian Service Module Transfer Tunnel. Cracks and air leaks in the tunnel are a top safety risk … both agencies are collaborating to investigate and mitigate the cracks and leaks; determine the root cause, which includes sharing sample metals, welds and Roscosmos investigation reports; and monitor the station for new leaks.

In February 2024 NASA identified an increase in the leak rate … Later, in May and June 2024, ISS Program and Roscosmos officials met to discuss heightened concerns with the increased leak rate. Subsequently, the ISS Program elevated the Service Module Transfer Tunnel leak risk to the highest level of risk in its risk management system. According to NASA, Roscosmos is confident they will be able to monitor and close the hatch to the Service Module prior to the leak rate reaching an untenable level. However, NASA and Roscosmos have not reached an agreement on the point at which the leak rate is untenable.

Although the root cause of the leak remains unknown, both agencies have narrowed their focus to internal and external welds. As of June 2024, there was no indication of other leaks on the station.

Graphic showing breakdown of the parts of the space station by country and the problem area in red.
View larger. | Here’s a breakdown of the space station segments by space agency. The location of the PrK is in red. Image via NASA.

A disagreement over the leak

Currently, neither space agency is sure what caused the leak. Indeed, as Foust reported:

Russian engineers believe the cracks are likely caused by ‘high cyclic fatigue’ from micro-vibrations. NASA, by contrast, believes several factors are at play, including pressure and mechanical stress, residual stress, material properties of the module and environmental exposure.

In addition, Foust quoted Cabana as saying:

The Russians believe that continued operations are safe but they can’t prove to our satisfaction that they are, and the U.S. believes that it’s not safe but we can’t prove to the Russians’ satisfaction that that’s the case.

So, the space agencies are going to look to outside experts to identify the root cause of the problem and thus the best solution.

Bottom line: In 2019, the space station acquired a leak in a transfer tunnel. NASA said the space station leak could lead to a “catastrophic failure.”

Via SpaceNews

Via NASA’s Management to Risks to Sustaining ISS Operations through 2030

The post Could the space station leak lead to ‘catastrophic failure’? first appeared on EarthSky.



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A runaway star moves fast in an unusual direction

Runaway star: Colorful nebula sprinkled with stars, and inset with one labeled star and arrows.
This Hubble Space Telescope image shows a cloud in space where new stars are forming – called 30 Doradus – aka the Tarantula Nebula. The enlarged inset shows a star that appears to have been kicked out of the nebula. In the inset, an arrow points to the runaway star and a dashed arrow to its presumed direction of motion. Image via NASA.

A runaway star moves faster and in a different direction

The sun and all of the Milky Way’s stars are moving in orbit around the center of our galaxy. In fact, it’s more or less orderly, but there are local movements within this general stream of stars, too. Astronomers have identified some Milky Way stars that are moving faster than expected, or in a direction that seems unusual. In view of this unusual motion, they use the term runaway star to describe these renegades.

Stars form in clouds of gas and dust. Multiple stars form from a single cloud. Therefore, many Milky Way stars move through space in loose associations, or more tightly bound open star clusters. By tracking the motions of a runaway star, astronomers can sometimes determine its original stellar association. However, something must have happened to kick the star into fast motion, on a path through space different from its original cluster or association.

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Astronomers point to 2 possible reasons for a runaway star

The first scenario involves two binary star systems – two systems, each containing two stars – that pass close to each other. The encounter can disrupt both systems and eject one or more stars at relatively high speeds.

The second idea involves a supernova explosion in a multiple star system. These powerful explosions can propel associated stars that didn’t explode along new paths, at much-higher speeds.

GD 50 might be from the Pleiades

One runaway star is GD 50, a white dwarf star with a bit more mass than our sun, but smaller than the Earth. A dime as dense as GD 50 would weigh 2,600 pounds (~1,200 kilos) on Earth. GD 50 is in the direction of the constellation Eridanus the River. But, around 2009, astronomers who’d been studying this star found that it moves through space in the same direction and at the same speed as the Pleiades star cluster.

And the Pleiades is not far from Eridanus on the sky’s dome. GD 50 is also about the same age as stars in the Pleiades. Therefore, astronomers concluded that GD 50 was born in the Pleiades, then flung out, possibly after passing too close to another star.

Some other runaway stars

Further examples of runaway stars are AE Aurigae, 53 Arietis and Mu Columbae. In fact, they’re all moving away from each other at velocities of over 100 km/s (for comparison, our sun moves through the Milky Way at only about 20 km/s faster than the local average). Tracing their motions backwards on the sky’s dome, astronomers can see that – about 2 million years ago – the paths of these stars intersected near the Orion Nebula. There is a great loop or bubble of gas – called Barnard’s Loop – surrounding Orion’s three prominent Belt stars. Barnard’s Loop may be the remnant of the supernova that launched these stars as runaway stars.

Explore runaway stars on Wikipedia

4 panels with stars with arcs in front of them and tails behind, all in blue.
4 runaway stars plowing through regions of dense interstellar gas and creating bright bow waves and trailing tails of glowing gas. The stars in these NASA Hubble Space Telescope images are among 14 young runaway stars spotted by Hubble’s Advanced Camera for Surveys between October 2005 and July 2006. Image via Hubblesite/ Wikimedia Commons.

Bottom line: Runaway stars move differently from the general stream of stars in our Milky Way galaxy. The most compelling evidence suggests they were kicked out from their original star clusters by encounters between pairs of binary stars or by a supernova explosion.

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Runaway star: Colorful nebula sprinkled with stars, and inset with one labeled star and arrows.
This Hubble Space Telescope image shows a cloud in space where new stars are forming – called 30 Doradus – aka the Tarantula Nebula. The enlarged inset shows a star that appears to have been kicked out of the nebula. In the inset, an arrow points to the runaway star and a dashed arrow to its presumed direction of motion. Image via NASA.

A runaway star moves faster and in a different direction

The sun and all of the Milky Way’s stars are moving in orbit around the center of our galaxy. In fact, it’s more or less orderly, but there are local movements within this general stream of stars, too. Astronomers have identified some Milky Way stars that are moving faster than expected, or in a direction that seems unusual. In view of this unusual motion, they use the term runaway star to describe these renegades.

Stars form in clouds of gas and dust. Multiple stars form from a single cloud. Therefore, many Milky Way stars move through space in loose associations, or more tightly bound open star clusters. By tracking the motions of a runaway star, astronomers can sometimes determine its original stellar association. However, something must have happened to kick the star into fast motion, on a path through space different from its original cluster or association.

The 2025 EarthSky Lunar Calendar makes a great gift. Get yours today!

Astronomers point to 2 possible reasons for a runaway star

The first scenario involves two binary star systems – two systems, each containing two stars – that pass close to each other. The encounter can disrupt both systems and eject one or more stars at relatively high speeds.

The second idea involves a supernova explosion in a multiple star system. These powerful explosions can propel associated stars that didn’t explode along new paths, at much-higher speeds.

GD 50 might be from the Pleiades

One runaway star is GD 50, a white dwarf star with a bit more mass than our sun, but smaller than the Earth. A dime as dense as GD 50 would weigh 2,600 pounds (~1,200 kilos) on Earth. GD 50 is in the direction of the constellation Eridanus the River. But, around 2009, astronomers who’d been studying this star found that it moves through space in the same direction and at the same speed as the Pleiades star cluster.

And the Pleiades is not far from Eridanus on the sky’s dome. GD 50 is also about the same age as stars in the Pleiades. Therefore, astronomers concluded that GD 50 was born in the Pleiades, then flung out, possibly after passing too close to another star.

Some other runaway stars

Further examples of runaway stars are AE Aurigae, 53 Arietis and Mu Columbae. In fact, they’re all moving away from each other at velocities of over 100 km/s (for comparison, our sun moves through the Milky Way at only about 20 km/s faster than the local average). Tracing their motions backwards on the sky’s dome, astronomers can see that – about 2 million years ago – the paths of these stars intersected near the Orion Nebula. There is a great loop or bubble of gas – called Barnard’s Loop – surrounding Orion’s three prominent Belt stars. Barnard’s Loop may be the remnant of the supernova that launched these stars as runaway stars.

Explore runaway stars on Wikipedia

4 panels with stars with arcs in front of them and tails behind, all in blue.
4 runaway stars plowing through regions of dense interstellar gas and creating bright bow waves and trailing tails of glowing gas. The stars in these NASA Hubble Space Telescope images are among 14 young runaway stars spotted by Hubble’s Advanced Camera for Surveys between October 2005 and July 2006. Image via Hubblesite/ Wikimedia Commons.

Bottom line: Runaway stars move differently from the general stream of stars in our Milky Way galaxy. The most compelling evidence suggests they were kicked out from their original star clusters by encounters between pairs of binary stars or by a supernova explosion.

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A mystery mollusk sea slug in the deep ocean


A video about the newly described sea slug Bathydevius caudactylus, from the Monterey Bay Aquarium Research Institute.

  • Scientists identified a new deep-sea sea slug species, Bathydevius caudactylus, using remotely operated vehicles (ROVs).
  • Bathydevius caudactylus, found in the dark, cold depths of the ocean, is the only known sea slug living in deep open waters.
  • This mostly gelatinous sea slug uses a unique head hood to catch crustaceans. It’s bioluminescent and can swim, or drift in the currents.

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A discovery 20 years in the making

In February 2000, scientists using cameras on a remotely operated vehicle (called ROV for short) spotted an unusual sea slug swimming in the deep sea. They nicknamed it the mystery mollusk. Since then, there have been over 150 ROV sightings of this animal. And scientists were able to collect several specimens for detailed study in laboratories. Now, more than 20 years since that first sighting, they have enough information to announce that this sea slug is in fact a new species.

Researchers at the Monterey Bay Aquarium Research Institute (MBARI) published their findings in the December 2024 issue of the peer-reviewed journal Deep-Sea Research Part I: Oceanographic Research Papers.

They named the sea slug species Bathydevius caudactylus. This animal lives in a deep ocean zone cast in perpetual darkness because sunlight never reaches such great depths. It has a head dominated by a large gelatinous hood, a trunk containing internal organs, and a tail that acts like a paddle. Bathydevius are small creatures, with captured specimens ranging in size from 2.2 to 5.7 inches (56 to 145 millimeters). Moreover, they are bioluminescent, meaning these organisms can light up in the dark due to light-producing chemicals in their bodies.

Paper co-author, Steven Haddock remarked in a statement:

What is exciting to me about the mystery mollusk is that it exemplifies how much we are learning as we spend more time in the deep sea, particularly below 2,000 meters [6,500 feet]. For there to be a relatively large, unique, and glowing animal that is in a previously unknown family really underscores the importance of using new technology to catalog this vast environment. The more we learn about deep-sea communities, the better we will be at ocean decision-making and stewardship.

Bathydevius is a sea slug known as a nudibranch

When scientists first saw Bathydevius, they did not know what to make of it. That’s because they were puzzled by its appearance. For instance, a hood-like structure dominated the animal’s head. Its flat tail had several tentacle-like protrusions. In addition, within its almost transparent trunk were reddish internal organs.

The sea slug appears as a ghostly transparent organism floating in water. It has a light whitish hood, a trunk with reddish internal organs, and a tail with tentacle-like projections.
A view of the newly identified sea slug species Bathydevius caudactylus. Image via MBARI. Used with permission.

Using ROVs, scientists carefully captured several of these delicate mystery mollusks for detailed anatomical and genetic studies. This work allowed them to confirm that their mystery mollusk was a nudibranch. Also known as sea slugs, nudibranchs are often found in shallower water such as tide pools and coral reefs. Some live in open water, near the ocean surface. In addition, a few nudibranch species live on the ocean floor.

However, Bathydevius was different. It was first encountered in the deep open waters of Monterey Bay. Since then, it has been observed in deep waters off the North American Pacific coast, ranging offshore from Oregon to Southern California. A similar-looking sea slug was spotted in the Mariana Trench, the deepest ocean trench, in the Western Pacific. Could that also be Bathydevius? Scientists aren’t sure, but if it is, that would greatly expand its range.

Bathydevius is a unique sea slug

What makes Bathydevius unique? It is the only sea slug known to live in deep open water. This animal has been found in depths from 3,300 to 13,100 feet (1,000 to 4,000 meters) in ocean waters known as the bathypelagic zone. This section of the ocean is always dark because sunlight never reaches such great depths. It is also very cold, about 39° Fahrenheit (4° Celsius). Pressures ranges from 100 to 400 atmospheres, depending on depth.

Like other nudibranchs, Bathydevius is a hermaphrodite, which means that it has both male and female sex organs. Scientists have observed them spawning, by attaching themselves to the seafloor with their muscular foot and laying ribbons of eggs.

The scientists also found, based on genetic studies of specimens they caught, that this creature is unique enough to belong to its own taxonomic family. (Family is a higher-level classification rank for closely related species. In this case, Bathydevius caudactylus is the only species in the family Bathydeviidae.)

A sea slug adapted for deep ocean waters

Most sea slugs feed using a rough-surfaced tongue, called a radula, taking prey attached to objects such as rocks. Bathydevius, however, uses its hood as a trap to catch crustaceans like shrimp, not unlike a Venus flytrap.

The sea slug appears as a ghostly transparent organism floating in water. Its light whitish hood is wide open, reddish internal organs are visible in its trunk, and a tail with tentacle-like projections.
The sea slug species Bathydevius caudactylus with its hood extended open. Image via MBARI. Used with permission.

It swims slowly in the water by undulating its body. Sometimes, it simply drifts in the currents. Because Bathydevius has an almost transparent body, it is able to go largely undetected by predators. But if it needs to make an escape, it closes its hood rapidly, which propels its body backward.

Bathydevius is bioluminescent. It can create a light display, possibly to deter predators. The light comes from granules embedded in its body and appears like tiny blue stars illuminating the shape of the animal.

An animation of bioluminescence, appearing as tiny bright dots, in the sea slug that shows its shape as it moves in the water.
Bioluminescent spots in Bathydevius caudactylus, captured using a low-light camera system. Image via MBARI. Used with permission.

Haddock remarked in the statement:

Only recently have cameras become capable of filming bioluminescence in high-resolution and in full color. MBARI is one of the only places in the world where we have taken this new technology into the deep ocean, allowing us to study the luminous behavior of deep-sea animals in their natural habitat.

Bottom line: After 20 years of research, scientists have identified and named a new species of sea slug that lives in the deep ocean. They’ve called it Bathydevius caudactylus.

Source: Discovery and description of a remarkable bathypelagic nudibranch, Bathydevius caudactylus, gen. et. sp. nov.

Via Monterey Bay Aquarium Research Institute (MBARI)

Read more: The adorable leaf sheep sea slug: Lifeform of the week

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A video about the newly described sea slug Bathydevius caudactylus, from the Monterey Bay Aquarium Research Institute.

  • Scientists identified a new deep-sea sea slug species, Bathydevius caudactylus, using remotely operated vehicles (ROVs).
  • Bathydevius caudactylus, found in the dark, cold depths of the ocean, is the only known sea slug living in deep open waters.
  • This mostly gelatinous sea slug uses a unique head hood to catch crustaceans. It’s bioluminescent and can swim, or drift in the currents.

The 2025 EarthSky lunar calendar makes a great gift. Get yours today!

A discovery 20 years in the making

In February 2000, scientists using cameras on a remotely operated vehicle (called ROV for short) spotted an unusual sea slug swimming in the deep sea. They nicknamed it the mystery mollusk. Since then, there have been over 150 ROV sightings of this animal. And scientists were able to collect several specimens for detailed study in laboratories. Now, more than 20 years since that first sighting, they have enough information to announce that this sea slug is in fact a new species.

Researchers at the Monterey Bay Aquarium Research Institute (MBARI) published their findings in the December 2024 issue of the peer-reviewed journal Deep-Sea Research Part I: Oceanographic Research Papers.

They named the sea slug species Bathydevius caudactylus. This animal lives in a deep ocean zone cast in perpetual darkness because sunlight never reaches such great depths. It has a head dominated by a large gelatinous hood, a trunk containing internal organs, and a tail that acts like a paddle. Bathydevius are small creatures, with captured specimens ranging in size from 2.2 to 5.7 inches (56 to 145 millimeters). Moreover, they are bioluminescent, meaning these organisms can light up in the dark due to light-producing chemicals in their bodies.

Paper co-author, Steven Haddock remarked in a statement:

What is exciting to me about the mystery mollusk is that it exemplifies how much we are learning as we spend more time in the deep sea, particularly below 2,000 meters [6,500 feet]. For there to be a relatively large, unique, and glowing animal that is in a previously unknown family really underscores the importance of using new technology to catalog this vast environment. The more we learn about deep-sea communities, the better we will be at ocean decision-making and stewardship.

Bathydevius is a sea slug known as a nudibranch

When scientists first saw Bathydevius, they did not know what to make of it. That’s because they were puzzled by its appearance. For instance, a hood-like structure dominated the animal’s head. Its flat tail had several tentacle-like protrusions. In addition, within its almost transparent trunk were reddish internal organs.

The sea slug appears as a ghostly transparent organism floating in water. It has a light whitish hood, a trunk with reddish internal organs, and a tail with tentacle-like projections.
A view of the newly identified sea slug species Bathydevius caudactylus. Image via MBARI. Used with permission.

Using ROVs, scientists carefully captured several of these delicate mystery mollusks for detailed anatomical and genetic studies. This work allowed them to confirm that their mystery mollusk was a nudibranch. Also known as sea slugs, nudibranchs are often found in shallower water such as tide pools and coral reefs. Some live in open water, near the ocean surface. In addition, a few nudibranch species live on the ocean floor.

However, Bathydevius was different. It was first encountered in the deep open waters of Monterey Bay. Since then, it has been observed in deep waters off the North American Pacific coast, ranging offshore from Oregon to Southern California. A similar-looking sea slug was spotted in the Mariana Trench, the deepest ocean trench, in the Western Pacific. Could that also be Bathydevius? Scientists aren’t sure, but if it is, that would greatly expand its range.

Bathydevius is a unique sea slug

What makes Bathydevius unique? It is the only sea slug known to live in deep open water. This animal has been found in depths from 3,300 to 13,100 feet (1,000 to 4,000 meters) in ocean waters known as the bathypelagic zone. This section of the ocean is always dark because sunlight never reaches such great depths. It is also very cold, about 39° Fahrenheit (4° Celsius). Pressures ranges from 100 to 400 atmospheres, depending on depth.

Like other nudibranchs, Bathydevius is a hermaphrodite, which means that it has both male and female sex organs. Scientists have observed them spawning, by attaching themselves to the seafloor with their muscular foot and laying ribbons of eggs.

The scientists also found, based on genetic studies of specimens they caught, that this creature is unique enough to belong to its own taxonomic family. (Family is a higher-level classification rank for closely related species. In this case, Bathydevius caudactylus is the only species in the family Bathydeviidae.)

A sea slug adapted for deep ocean waters

Most sea slugs feed using a rough-surfaced tongue, called a radula, taking prey attached to objects such as rocks. Bathydevius, however, uses its hood as a trap to catch crustaceans like shrimp, not unlike a Venus flytrap.

The sea slug appears as a ghostly transparent organism floating in water. Its light whitish hood is wide open, reddish internal organs are visible in its trunk, and a tail with tentacle-like projections.
The sea slug species Bathydevius caudactylus with its hood extended open. Image via MBARI. Used with permission.

It swims slowly in the water by undulating its body. Sometimes, it simply drifts in the currents. Because Bathydevius has an almost transparent body, it is able to go largely undetected by predators. But if it needs to make an escape, it closes its hood rapidly, which propels its body backward.

Bathydevius is bioluminescent. It can create a light display, possibly to deter predators. The light comes from granules embedded in its body and appears like tiny blue stars illuminating the shape of the animal.

An animation of bioluminescence, appearing as tiny bright dots, in the sea slug that shows its shape as it moves in the water.
Bioluminescent spots in Bathydevius caudactylus, captured using a low-light camera system. Image via MBARI. Used with permission.

Haddock remarked in the statement:

Only recently have cameras become capable of filming bioluminescence in high-resolution and in full color. MBARI is one of the only places in the world where we have taken this new technology into the deep ocean, allowing us to study the luminous behavior of deep-sea animals in their natural habitat.

Bottom line: After 20 years of research, scientists have identified and named a new species of sea slug that lives in the deep ocean. They’ve called it Bathydevius caudactylus.

Source: Discovery and description of a remarkable bathypelagic nudibranch, Bathydevius caudactylus, gen. et. sp. nov.

Via Monterey Bay Aquarium Research Institute (MBARI)

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