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The Caspian Sea – Earth’s largest inland sea – is shrinking

Caspian Sea: Satellite view of an oblong dark blue lake with a lighter blue area at the top.
The Caspian Sea is shrinking. But the reasons for water loss in Earth’s largest inland sea have been poorly understood. A new study has assessed the pressures the sea is facing. Image via NASA Earth Observatory.

The Caspian Sea – Earth’s largest inland sea – is shrinking

The Caspian Sea is the world’s largest inland sea when measured by surface area. It spans 143,200 square miles (371,000 square km), or about the size of Japan. And it sits on the boundary of Asia and Europe, with five countries sharing its borders: Russia and Azerbaijan on the European side and Iran, Turkmenistan and Kazakhstan on the Asian side.

But the Caspian Sea is shrinking. The sea has been receding since the 1990s in fact, especially in its northern regions, but the reasons for this have poorly understood. Now, a new study by an international team of researchers has taken a closer look at the stresses this important body of water is under. They found that the Caspian Sea’s decline is largely being driven by reduced river inflow, especially from Russia’s Volga river. And both climate change and human activity appear to blame.

The American Geophysical Union said on June 18, 2026, that:

saving it will require international action.

The researchers published their peer-reviewed study in the journal Earth’s Future on June 5, 2026.

Map showing where Europe and Asia meet with an arrow pointing to a sea that stretches north-south.
The Caspian Sea is on the boundary of where Europe meets Asia. Image via DEMIS Mapserver.

A better understanding of an unfolding disaster

Even though the Caspian Sea has been shrinking since the 1990s, the reasons behind the water drying up have not been well understood. So an international team of researchers, led by Jesse Duku of UC Irvine, looked at satellite observations, river flow records and climate data for a better understanding.

They found that precipitation across the region has remained largely unchanged since the early 1990s. However, evaporation from the sea’s surface has increased. But this only accounts for about 37% to 40% of the observed water loss. Instead, the biggest change has been a decline in river inflow. In particular, Russia’s Volga River – which supplies most of the Caspian Sea’s freshwater – has experienced a substantial decrease in inflow.

And, according to the study, the total inflow from the sea’s five major rivers fell significantly between 1991 and 2020. The researchers said the findings point to not just climate influences but to human activities. In fact, they found that water consumption and river regulation seem to be playing a larger role than scientists previously recognized.

Satellite view of a long north-south lake with 5 labels for the countries surrounding it.
This map shows the locations of the 5 countries that have coastlines on the Caspian Sea. Image via ESA/ Copernicus.
A map of eastern Europe with long river snaking through it.
The Volga River drainage basin. Image via Wikipedia.

How much water is the Caspian Sea losing? Why is that important?

Since the mid-1990s, the Caspian Sea has lost about 5.5% of its surface area. That equals roughly 630 cubic kilometers (over 150 cubic miles) of water. And scientists project the sea could fall an additional 26 to 46 feet (8 to 14 meters) by 2100. The northern part of the Caspian Sea is already naturally shallow. And this is the region that has been especially vulnerable to falling water levels.

The researchers detected rising concentrations of chlorophyll-a in the northern Caspian. Scientists use this form of chlorophyll to measure the amount of algae and cyanobacteria, and the measurements suggest the waters are feeling an increase in ecological stress.

The Caspian Sea supports more than 850 endemic species, or species that are only found there. The species include the critically endangered Caspian seal and several species of sturgeon. Those sturgeon are the source of 90% of the world’s black caviar. Declining water levels also threaten wetlands, fish spawning grounds and coastal ecosystems.

But the impacts extend beyond wildlife. The Caspian Sea is vital for fisheries, trade and industry across the region. Lower water levels can disrupt ports and shipping routes. The study also said:

In addition, the Caspian Sea is a major hotspot for the oil and gas industry, where approximately 1 million tons of oil are estimated to leak into the sea annually. These combined pressures raise concerns about how hydrological shifts and human activities may influence water quality and ecosystem functioning.

The study’s authors warned that without coordinated management among the five nations bordering the sea, the region could face growing environmental and economic challenges.

Side-by-side satellite images of a lake that loses extent around the edges on the right.
The left side shows a view of the northern region of the Caspian Sea in 2006. The right side is how the same area looked in 2022. Image via NASA Earth Observatory.

How does this compare to the Aral Sea?

In the study, the authors compare the shrinking of the Caspian Sea to the Aral Sea. The Aral Sea is another large inland body of water in Central Asia. The Aral Sea once covered about 26,000 square miles (68,000 square km), making it the world’s 4th-largest lake. But beginning in the 1960s, Soviet irrigation projects diverted much of the water from the rivers that fed it. As a result, the Aral Sea lost about 90% of its volume over the following decades and split into several smaller lakes.

The Caspian Sea’s situation is not as severe. It remains far larger than the Aral Sea ever was, and scientists do not expect it to disappear. But both water bodies share a common challenge: reduced river inflow. In the Caspian Sea, declining flows from the Volga River and other tributaries, combined with rising evaporation linked to a warming climate, are contributing to falling water levels. Researchers said the comparison serves as a warning that human management of water resources can have long-lasting consequences for inland seas and the communities that depend on them.

They concluded that preventing further decline will require greater cooperation among Azerbaijan, Iran, Kazakhstan, Russia and Turkmenistan. Improved water management, better data sharing and policies that protect river inflows could help preserve the sea’s ecosystems and economies for future generations.

Bottom line: A new study finds that the Caspian Sea’s decline is being driven by both climate change and human activity. Reduced river inflow, especially from the Volga River, appears to be a major factor behind the shrinking of Earth’s largest inland sea.

Read more: Will Lake Mead – largest US reservoir – reach record lows?

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

The post The Caspian Sea – Earth’s largest inland sea – is shrinking first appeared on EarthSky.



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Caspian Sea: Satellite view of an oblong dark blue lake with a lighter blue area at the top.
The Caspian Sea is shrinking. But the reasons for water loss in Earth’s largest inland sea have been poorly understood. A new study has assessed the pressures the sea is facing. Image via NASA Earth Observatory.

The Caspian Sea – Earth’s largest inland sea – is shrinking

The Caspian Sea is the world’s largest inland sea when measured by surface area. It spans 143,200 square miles (371,000 square km), or about the size of Japan. And it sits on the boundary of Asia and Europe, with five countries sharing its borders: Russia and Azerbaijan on the European side and Iran, Turkmenistan and Kazakhstan on the Asian side.

But the Caspian Sea is shrinking. The sea has been receding since the 1990s in fact, especially in its northern regions, but the reasons for this have poorly understood. Now, a new study by an international team of researchers has taken a closer look at the stresses this important body of water is under. They found that the Caspian Sea’s decline is largely being driven by reduced river inflow, especially from Russia’s Volga river. And both climate change and human activity appear to blame.

The American Geophysical Union said on June 18, 2026, that:

saving it will require international action.

The researchers published their peer-reviewed study in the journal Earth’s Future on June 5, 2026.

Map showing where Europe and Asia meet with an arrow pointing to a sea that stretches north-south.
The Caspian Sea is on the boundary of where Europe meets Asia. Image via DEMIS Mapserver.

A better understanding of an unfolding disaster

Even though the Caspian Sea has been shrinking since the 1990s, the reasons behind the water drying up have not been well understood. So an international team of researchers, led by Jesse Duku of UC Irvine, looked at satellite observations, river flow records and climate data for a better understanding.

They found that precipitation across the region has remained largely unchanged since the early 1990s. However, evaporation from the sea’s surface has increased. But this only accounts for about 37% to 40% of the observed water loss. Instead, the biggest change has been a decline in river inflow. In particular, Russia’s Volga River – which supplies most of the Caspian Sea’s freshwater – has experienced a substantial decrease in inflow.

And, according to the study, the total inflow from the sea’s five major rivers fell significantly between 1991 and 2020. The researchers said the findings point to not just climate influences but to human activities. In fact, they found that water consumption and river regulation seem to be playing a larger role than scientists previously recognized.

Satellite view of a long north-south lake with 5 labels for the countries surrounding it.
This map shows the locations of the 5 countries that have coastlines on the Caspian Sea. Image via ESA/ Copernicus.
A map of eastern Europe with long river snaking through it.
The Volga River drainage basin. Image via Wikipedia.

How much water is the Caspian Sea losing? Why is that important?

Since the mid-1990s, the Caspian Sea has lost about 5.5% of its surface area. That equals roughly 630 cubic kilometers (over 150 cubic miles) of water. And scientists project the sea could fall an additional 26 to 46 feet (8 to 14 meters) by 2100. The northern part of the Caspian Sea is already naturally shallow. And this is the region that has been especially vulnerable to falling water levels.

The researchers detected rising concentrations of chlorophyll-a in the northern Caspian. Scientists use this form of chlorophyll to measure the amount of algae and cyanobacteria, and the measurements suggest the waters are feeling an increase in ecological stress.

The Caspian Sea supports more than 850 endemic species, or species that are only found there. The species include the critically endangered Caspian seal and several species of sturgeon. Those sturgeon are the source of 90% of the world’s black caviar. Declining water levels also threaten wetlands, fish spawning grounds and coastal ecosystems.

But the impacts extend beyond wildlife. The Caspian Sea is vital for fisheries, trade and industry across the region. Lower water levels can disrupt ports and shipping routes. The study also said:

In addition, the Caspian Sea is a major hotspot for the oil and gas industry, where approximately 1 million tons of oil are estimated to leak into the sea annually. These combined pressures raise concerns about how hydrological shifts and human activities may influence water quality and ecosystem functioning.

The study’s authors warned that without coordinated management among the five nations bordering the sea, the region could face growing environmental and economic challenges.

Side-by-side satellite images of a lake that loses extent around the edges on the right.
The left side shows a view of the northern region of the Caspian Sea in 2006. The right side is how the same area looked in 2022. Image via NASA Earth Observatory.

How does this compare to the Aral Sea?

In the study, the authors compare the shrinking of the Caspian Sea to the Aral Sea. The Aral Sea is another large inland body of water in Central Asia. The Aral Sea once covered about 26,000 square miles (68,000 square km), making it the world’s 4th-largest lake. But beginning in the 1960s, Soviet irrigation projects diverted much of the water from the rivers that fed it. As a result, the Aral Sea lost about 90% of its volume over the following decades and split into several smaller lakes.

The Caspian Sea’s situation is not as severe. It remains far larger than the Aral Sea ever was, and scientists do not expect it to disappear. But both water bodies share a common challenge: reduced river inflow. In the Caspian Sea, declining flows from the Volga River and other tributaries, combined with rising evaporation linked to a warming climate, are contributing to falling water levels. Researchers said the comparison serves as a warning that human management of water resources can have long-lasting consequences for inland seas and the communities that depend on them.

They concluded that preventing further decline will require greater cooperation among Azerbaijan, Iran, Kazakhstan, Russia and Turkmenistan. Improved water management, better data sharing and policies that protect river inflows could help preserve the sea’s ecosystems and economies for future generations.

Bottom line: A new study finds that the Caspian Sea’s decline is being driven by both climate change and human activity. Reduced river inflow, especially from the Volga River, appears to be a major factor behind the shrinking of Earth’s largest inland sea.

Read more: Will Lake Mead – largest US reservoir – reach record lows?

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

The post The Caspian Sea – Earth’s largest inland sea – is shrinking first appeared on EarthSky.



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Back-to-back Venezuela earthquakes kill at least 164

Two devastating earthquakes struck Venezuela in the space of a minute last night, June 24, 2026. This is an intensity map of the second, which had a magnitude of 7.5. That’s the strongest quake to hit Venezuela since 1990. Read about the Venezuela earthquakes below. Image via USGS.

Back-to-back Venezuela earthquakes last night kill at least 164

Two powerful earthquakes struck Venezuela in the space of a minute last night, leaving at least 164 dead and over 700 injured as of 10:30 UTC, June 25.

The quakes struck at 6:04 p.m. local time (22:04 UTC). Centered on the state of Carabobo – some 12 miles (20 km) from the country’s capital, Caracas – they had magnitudes of 7.2 and 7.5. The second was the strongest to strike Venezuela since a magnitude 7.7 quake in 1900.

Many buildings in Caracas have been reduced to rubble. And, as reported by the BBC, Venezuela’s acting president Delcy Rodríguez has stated that the most affected state is La Guaira, just north of Caracas, where “dozens” of buildings have collapsed.

The number of lives lost will almost certainly rise as more information comes in. Shortly after the earthquake struck, the US Geological Survey (USGS) predicted a 33% chance of 1,000 to 10,000 fatalities, and a 42% chance of 10,000 to 100,000 fatalities.

BREAKING: USGS upgrades Venezuela earthquake to 7.5. Major damage to buildings.

AZ Intel (@azintel.bsky.social) 2026-06-24T23:16:42.984Z

Quakes came during holiday celebrations

June 24 is a national holiday in Venezuela, commemorating the victory of Venezuelan independence leader Simón Bolívar against Spain in the 1821 Battle of Carabobo. So the devastating quakes came with many people at home, celebrating with their families.

This morning, rescue attempts continue amid fears of possible aftershocks.

Leaders across the world have offered condolences and pledged support, with governments including that of the U.S., Germany and China volunteering to aid relief efforts.

Bottom line: Two back-to-back Venezuela earthquakes caused devastation last night. The current death toll is at least 164, with over 700 injured.

Read more: Yellowstone earthquakes rattle underground ecosystems

Read more: Can animals sense earthquakes? Science investigates

The post Back-to-back Venezuela earthquakes kill at least 164 first appeared on EarthSky.



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Two devastating earthquakes struck Venezuela in the space of a minute last night, June 24, 2026. This is an intensity map of the second, which had a magnitude of 7.5. That’s the strongest quake to hit Venezuela since 1990. Read about the Venezuela earthquakes below. Image via USGS.

Back-to-back Venezuela earthquakes last night kill at least 164

Two powerful earthquakes struck Venezuela in the space of a minute last night, leaving at least 164 dead and over 700 injured as of 10:30 UTC, June 25.

The quakes struck at 6:04 p.m. local time (22:04 UTC). Centered on the state of Carabobo – some 12 miles (20 km) from the country’s capital, Caracas – they had magnitudes of 7.2 and 7.5. The second was the strongest to strike Venezuela since a magnitude 7.7 quake in 1900.

Many buildings in Caracas have been reduced to rubble. And, as reported by the BBC, Venezuela’s acting president Delcy Rodríguez has stated that the most affected state is La Guaira, just north of Caracas, where “dozens” of buildings have collapsed.

The number of lives lost will almost certainly rise as more information comes in. Shortly after the earthquake struck, the US Geological Survey (USGS) predicted a 33% chance of 1,000 to 10,000 fatalities, and a 42% chance of 10,000 to 100,000 fatalities.

BREAKING: USGS upgrades Venezuela earthquake to 7.5. Major damage to buildings.

AZ Intel (@azintel.bsky.social) 2026-06-24T23:16:42.984Z

Quakes came during holiday celebrations

June 24 is a national holiday in Venezuela, commemorating the victory of Venezuelan independence leader Simón Bolívar against Spain in the 1821 Battle of Carabobo. So the devastating quakes came with many people at home, celebrating with their families.

This morning, rescue attempts continue amid fears of possible aftershocks.

Leaders across the world have offered condolences and pledged support, with governments including that of the U.S., Germany and China volunteering to aid relief efforts.

Bottom line: Two back-to-back Venezuela earthquakes caused devastation last night. The current death toll is at least 164, with over 700 injured.

Read more: Yellowstone earthquakes rattle underground ecosystems

Read more: Can animals sense earthquakes? Science investigates

The post Back-to-back Venezuela earthquakes kill at least 164 first appeared on EarthSky.



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Mammatus clouds are ominous and beautiful


Learn more about mammatus clouds and see stunning photos in this video. Watch in the player above or on YouTube.

Love wildlife and the natural world? Get the latest animal stories – as well as space and night sky updates – delivered to your inbox.

Mammatus clouds: Ominous and beautiful

Mammatus clouds are pouch-like protrusions hanging from the undersides of clouds. You’ll usually find them under thunderstorm anvil clouds, but you might see them under other clouds as well. They’re composed primarily of ice. And groups of them can extend hundreds of miles in any direction. But they’re fleeting, remaining visible in your local sky for perhaps 10 or 15 minutes at a time.

Most clouds are formed by rising air. But mammatus clouds are formed by sinking air. They appear ominous.

People associate these cloud pouches with severe weather. And it’s true; they typically appear before or after a storm. But, in a way that’s so common in nature, their dangerous aspect goes hand-in-hand with a magnificent beauty. Enjoy the pictures below.

Read more: Cloud shapes are a useful tool for predicting weather

Beautiful bubbling clouds

Many round, fluffy clouds above a house.
View at EarthSky Community Photos. | Deb King in Moundridge, Kansas, took this spectacular photo of mammatus clouds on June 10, 2026. Thank you, Deb!
Dark orange sky with mammatus clouds with buildings in foreground.
View at EarthSky Community Photos. | Vermont Jr. Coronel captured this photo from the Philippines on May 28, 2026, and wrote: “Mammatus clouds after the sudden thunderstorm on a very hot late afternoon. Thunderstorms are prevalent now in the Philippines during afternoon. A sign that the rainy season is about to begin.” Thank you, Vermont!
Trees in the foreground with clouds looking like they are bubbling downward from the bottom layer.
View at EarthSky Community Photos. | Aaron Watson captured this image on July 17, 2025, from Colorado and wrote: “Interesting mammatus clouds this morning. It looked like long, deep grooves across the sky.” Thank you, Aaron!

More from our Community photos

A house and trees in the foreground and above, a lumpy layer at the bottom of the cloud.
View at EarthSky Community Photos. | Michael O’Connor captured this image on July 12, 2025, from Michigan and wrote: “Mammatus clouds. First time ever seeing them.” Thank you, Michael!
Cloud bank overhead with orange bubbles underneath and darker blue behind.
View at EarthSky Community Photos. | Lina Tomlin in Texarkana, Texas, photographed these mammatus clouds on April 29, 2024. Lina wrote: “Stepped outside and my jaw dropped. I loved watching this massive storm cell roll by. I saw more ‘bubble’ clouds appear, and as the sun went down they lit up. I’ve never been this close to clouds like that. Thrilling!” Thank you, Lina!

Bottom line: Mammatus clouds look like bubbling, low-hanging clouds. They’re often associated with thunderstorms. Learn more about them and see photos here.

Read more: Lenticular clouds look like UFOs

Read more: What are hole-punch clouds, aka fallstreak holes?

The post Mammatus clouds are ominous and beautiful first appeared on EarthSky.



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Learn more about mammatus clouds and see stunning photos in this video. Watch in the player above or on YouTube.

Love wildlife and the natural world? Get the latest animal stories – as well as space and night sky updates – delivered to your inbox.

Mammatus clouds: Ominous and beautiful

Mammatus clouds are pouch-like protrusions hanging from the undersides of clouds. You’ll usually find them under thunderstorm anvil clouds, but you might see them under other clouds as well. They’re composed primarily of ice. And groups of them can extend hundreds of miles in any direction. But they’re fleeting, remaining visible in your local sky for perhaps 10 or 15 minutes at a time.

Most clouds are formed by rising air. But mammatus clouds are formed by sinking air. They appear ominous.

People associate these cloud pouches with severe weather. And it’s true; they typically appear before or after a storm. But, in a way that’s so common in nature, their dangerous aspect goes hand-in-hand with a magnificent beauty. Enjoy the pictures below.

Read more: Cloud shapes are a useful tool for predicting weather

Beautiful bubbling clouds

Many round, fluffy clouds above a house.
View at EarthSky Community Photos. | Deb King in Moundridge, Kansas, took this spectacular photo of mammatus clouds on June 10, 2026. Thank you, Deb!
Dark orange sky with mammatus clouds with buildings in foreground.
View at EarthSky Community Photos. | Vermont Jr. Coronel captured this photo from the Philippines on May 28, 2026, and wrote: “Mammatus clouds after the sudden thunderstorm on a very hot late afternoon. Thunderstorms are prevalent now in the Philippines during afternoon. A sign that the rainy season is about to begin.” Thank you, Vermont!
Trees in the foreground with clouds looking like they are bubbling downward from the bottom layer.
View at EarthSky Community Photos. | Aaron Watson captured this image on July 17, 2025, from Colorado and wrote: “Interesting mammatus clouds this morning. It looked like long, deep grooves across the sky.” Thank you, Aaron!

More from our Community photos

A house and trees in the foreground and above, a lumpy layer at the bottom of the cloud.
View at EarthSky Community Photos. | Michael O’Connor captured this image on July 12, 2025, from Michigan and wrote: “Mammatus clouds. First time ever seeing them.” Thank you, Michael!
Cloud bank overhead with orange bubbles underneath and darker blue behind.
View at EarthSky Community Photos. | Lina Tomlin in Texarkana, Texas, photographed these mammatus clouds on April 29, 2024. Lina wrote: “Stepped outside and my jaw dropped. I loved watching this massive storm cell roll by. I saw more ‘bubble’ clouds appear, and as the sun went down they lit up. I’ve never been this close to clouds like that. Thrilling!” Thank you, Lina!

Bottom line: Mammatus clouds look like bubbling, low-hanging clouds. They’re often associated with thunderstorms. Learn more about them and see photos here.

Read more: Lenticular clouds look like UFOs

Read more: What are hole-punch clouds, aka fallstreak holes?

The post Mammatus clouds are ominous and beautiful first appeared on EarthSky.



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Why aren’t the hottest days on the solstice?

Hottest day: Two lounging chairs on the beach with an umbrella; water and a pier in the distance.
The hottest days occur after the summer solstice. Image via Quang Nguyen Vinh/ Pexels.

It might seem logical for the hottest days in the Northern Hemisphere to fall around the June solstice, when the sun reaches its northernmost point for the year. But the hottest days in the north actually come a month or two after the solstice. And in the Southern Hemisphere, the coldest weather doesn’t arrive until a month or two after the June solstice. Why? It’s down to a phenomenon known as the lag of the seasons.

Why the north’s hottest days follow the solstice

You can understand this phenomenon if you’ve ever visited a beach in June. On Northern Hemisphere beaches around now, you’ll notice how cold the ocean feels. Or think about mountaintops in June, which can often still be blanketed by ice and snow. The summer sun still hasn’t had time to melt the ice and warm the oceans.

So that’s why the hot weather lags behind the year’s longest day and highest sun.

By August, ocean water on that same beach will be much warmer. And the snow line will have crept up the mountaintops. That’s why the hottest weather comes some months after the year’s longest day. The land and oceans simply need those extra months to warm up – to store heat – after the cold of winter.

And in the Southern Hemisphere

In the Southern Hemisphere now, the same phenomenon is occurring but in reverse. There, the lag of the seasons is delaying the year’s coldest weather. The June solstice, for the Southern Hemisphere, is the winter solstice. The coldest weather comes in July and August because the land and oceans in that part of the world take some extra weeks to give up their stored heat.

Enormous white splash as an ocean wave hits a gray rock under a cloudy sky.
View at EarthSky Community Photos. | Cecille Kennedy captured this spectacular wave in Oregon on December 14, 2024. It takes a few months for the ocean to warm up in summer and cool down in winter, contributing to the so-called lag of the seasons. Thank you, Cecille!

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

Bottom line: The June solstice marks the height of the sun in the Northern Hemisphere, but the hottest weather comes a month or two later. The phenomenon is called the lag of the seasons, and the same process occurs in reverse in the Southern Hemisphere.

Read more: June solstice 2026: All you need to know

Watch: Solstices and equinoxes seen from space

The post Why aren’t the hottest days on the solstice? first appeared on EarthSky.



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Hottest day: Two lounging chairs on the beach with an umbrella; water and a pier in the distance.
The hottest days occur after the summer solstice. Image via Quang Nguyen Vinh/ Pexels.

It might seem logical for the hottest days in the Northern Hemisphere to fall around the June solstice, when the sun reaches its northernmost point for the year. But the hottest days in the north actually come a month or two after the solstice. And in the Southern Hemisphere, the coldest weather doesn’t arrive until a month or two after the June solstice. Why? It’s down to a phenomenon known as the lag of the seasons.

Why the north’s hottest days follow the solstice

You can understand this phenomenon if you’ve ever visited a beach in June. On Northern Hemisphere beaches around now, you’ll notice how cold the ocean feels. Or think about mountaintops in June, which can often still be blanketed by ice and snow. The summer sun still hasn’t had time to melt the ice and warm the oceans.

So that’s why the hot weather lags behind the year’s longest day and highest sun.

By August, ocean water on that same beach will be much warmer. And the snow line will have crept up the mountaintops. That’s why the hottest weather comes some months after the year’s longest day. The land and oceans simply need those extra months to warm up – to store heat – after the cold of winter.

And in the Southern Hemisphere

In the Southern Hemisphere now, the same phenomenon is occurring but in reverse. There, the lag of the seasons is delaying the year’s coldest weather. The June solstice, for the Southern Hemisphere, is the winter solstice. The coldest weather comes in July and August because the land and oceans in that part of the world take some extra weeks to give up their stored heat.

Enormous white splash as an ocean wave hits a gray rock under a cloudy sky.
View at EarthSky Community Photos. | Cecille Kennedy captured this spectacular wave in Oregon on December 14, 2024. It takes a few months for the ocean to warm up in summer and cool down in winter, contributing to the so-called lag of the seasons. Thank you, Cecille!

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

Bottom line: The June solstice marks the height of the sun in the Northern Hemisphere, but the hottest weather comes a month or two later. The phenomenon is called the lag of the seasons, and the same process occurs in reverse in the Southern Hemisphere.

Read more: June solstice 2026: All you need to know

Watch: Solstices and equinoxes seen from space

The post Why aren’t the hottest days on the solstice? first appeared on EarthSky.



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Boötes the Herdsman and its bright star Arcturus

Star chart: Constellation Boötes shaped like long narrow kite with 5 labeled stars.
The constellation Boötes the Herdsman is an excellent target for June nights. Arcturus is the brightest star in the constellation. Chart via EarthSky.

Boötes the Herdsman is a Northern Hemisphere constellation best seen in the late spring or early summer. It’s one of the largest constellations in the sky, ranking 13th out of 88. Boötes is most famous for its bright star Arcturus, which is the 4th-brightest star in the night sky.

Locating the constellation Boötes

You can find Boötes south of Ursa Major the Great Bear, off the handle of the Big Dipper. Boötes’ brightest star, Arcturus, is part of a mnemonic device used to orient people to the night sky. The saying goes, Arc to Arcturus, speed on to Spica. This means that as you follow the curve in the dipper’s handle away from Ursa Major, you will run into a bright star: Arcturus in Boötes. Continue the curve along and you’ll find Spica, which is a part of Virgo.

Man on rooftop of city looking at outlines of Boötes, Virgo and Corona Borealis.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, Madhya Pradesh, India, captured this photo of Boötes, Virgo and Corona Borealis on March 5, 2021. He wrote: “Spring constellations twinkling in the eastern horizon.” Thank you, Prateek!

Tracing out the shape of Boötes

Boötes is supposed to be the figure of a man, which is somewhat recognizable with its tall diamond shape and two stick legs jutting out at the bottom.

The point at which the tall diamond shape and stick legs intersect is the star Arcturus. In addition, the Herdsman also appears to have his left arm raised over his head. Some say it’s easy to pick out as a kite-shaped group of stars.

The stars in the Herdsman

Arcturus, the brightest star in Boötes, shines at magnitude -0.04, making it the 4th-brightest star in the night sky.

The name Arcturus means bear watcher or bear guard, referring to its closeness to the Great Bear, Ursa Major. Lying 37 light-years away from Earth, Arcturus glows with a faint orange hue.

The second brightest star in Boötes lies on the left side of the diamond shape. It’s called Izar, or Epsilon Boötis, and is 10 degrees up from Arcturus. It’s a magnitude 2.37 star lying 203 light-years away.

The third brightest star in Boötes is his left knee, which is found to the lower right of Arcturus. This star is Muphrid, or Eta Boötis, at magnitude 2.68. Muphrid lies 37 light-years away.

White star chart with black lines and dots drawing out Boötes.
The stars of Boötes. Image via IAU/ Sky and Telescope/ Wikimedia Commons/ CC BY-SA 3.0.

Fainter stars in Boötes

The other stars in the body of the Herdsman are all of comparable brightness. Starting above Izar and working up, around and back toward Arcturus are the stars Delta Boötis, Beta Boötis aka Nekkar (consider this Boötes’ neck), Gamma Boötis (or Seginus) and Rho Boötis.

Delta Boötis shines at magnitude 3.46 at a distance of 121 light-years. Nekkar shines at magnitude 3.49 and lies 219 light-years distant. Seginus has the brightest magnitude of these four stars, at 3.04. It is also the closest of the four at 84 light-years. Finally, Rho Boötis, which lies almost even with Izar, shines at magnitude 3.57 and lies 149 light-years away.

Arcturus shows large proper motion

The bright orange star Arcturus is especially noteworthy for its large proper motion, or sideways motion as seen on the dome of Earth’s sky.

Arcturus is actually moving at a tremendous speed (122 km/s or 76 miles/s) relative to our solar system. And from the vantage point of Earth, Arcturus is rapidly moving in a southerly direction at a rate of 3.9 arcminutes per century.

Its closest point to Earth will be about 4,000 years from now. Then as it moves away, it will vanish from visibility to the unaided eye in about 500,000 years.

Why does it move so much faster than the other stars in Boötes? It’s because Arcturus is much closer to us than the constellation’s other stars. That’s also why it’s so much brighter than its companions.

Bottom line: Boötes the Herdsman is a large constellation that holds one of the brightest stars in the sky, Arcturus.

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Star chart: Constellation Boötes shaped like long narrow kite with 5 labeled stars.
The constellation Boötes the Herdsman is an excellent target for June nights. Arcturus is the brightest star in the constellation. Chart via EarthSky.

Boötes the Herdsman is a Northern Hemisphere constellation best seen in the late spring or early summer. It’s one of the largest constellations in the sky, ranking 13th out of 88. Boötes is most famous for its bright star Arcturus, which is the 4th-brightest star in the night sky.

Locating the constellation Boötes

You can find Boötes south of Ursa Major the Great Bear, off the handle of the Big Dipper. Boötes’ brightest star, Arcturus, is part of a mnemonic device used to orient people to the night sky. The saying goes, Arc to Arcturus, speed on to Spica. This means that as you follow the curve in the dipper’s handle away from Ursa Major, you will run into a bright star: Arcturus in Boötes. Continue the curve along and you’ll find Spica, which is a part of Virgo.

Man on rooftop of city looking at outlines of Boötes, Virgo and Corona Borealis.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, Madhya Pradesh, India, captured this photo of Boötes, Virgo and Corona Borealis on March 5, 2021. He wrote: “Spring constellations twinkling in the eastern horizon.” Thank you, Prateek!

Tracing out the shape of Boötes

Boötes is supposed to be the figure of a man, which is somewhat recognizable with its tall diamond shape and two stick legs jutting out at the bottom.

The point at which the tall diamond shape and stick legs intersect is the star Arcturus. In addition, the Herdsman also appears to have his left arm raised over his head. Some say it’s easy to pick out as a kite-shaped group of stars.

The stars in the Herdsman

Arcturus, the brightest star in Boötes, shines at magnitude -0.04, making it the 4th-brightest star in the night sky.

The name Arcturus means bear watcher or bear guard, referring to its closeness to the Great Bear, Ursa Major. Lying 37 light-years away from Earth, Arcturus glows with a faint orange hue.

The second brightest star in Boötes lies on the left side of the diamond shape. It’s called Izar, or Epsilon Boötis, and is 10 degrees up from Arcturus. It’s a magnitude 2.37 star lying 203 light-years away.

The third brightest star in Boötes is his left knee, which is found to the lower right of Arcturus. This star is Muphrid, or Eta Boötis, at magnitude 2.68. Muphrid lies 37 light-years away.

White star chart with black lines and dots drawing out Boötes.
The stars of Boötes. Image via IAU/ Sky and Telescope/ Wikimedia Commons/ CC BY-SA 3.0.

Fainter stars in Boötes

The other stars in the body of the Herdsman are all of comparable brightness. Starting above Izar and working up, around and back toward Arcturus are the stars Delta Boötis, Beta Boötis aka Nekkar (consider this Boötes’ neck), Gamma Boötis (or Seginus) and Rho Boötis.

Delta Boötis shines at magnitude 3.46 at a distance of 121 light-years. Nekkar shines at magnitude 3.49 and lies 219 light-years distant. Seginus has the brightest magnitude of these four stars, at 3.04. It is also the closest of the four at 84 light-years. Finally, Rho Boötis, which lies almost even with Izar, shines at magnitude 3.57 and lies 149 light-years away.

Arcturus shows large proper motion

The bright orange star Arcturus is especially noteworthy for its large proper motion, or sideways motion as seen on the dome of Earth’s sky.

Arcturus is actually moving at a tremendous speed (122 km/s or 76 miles/s) relative to our solar system. And from the vantage point of Earth, Arcturus is rapidly moving in a southerly direction at a rate of 3.9 arcminutes per century.

Its closest point to Earth will be about 4,000 years from now. Then as it moves away, it will vanish from visibility to the unaided eye in about 500,000 years.

Why does it move so much faster than the other stars in Boötes? It’s because Arcturus is much closer to us than the constellation’s other stars. That’s also why it’s so much brighter than its companions.

Bottom line: Boötes the Herdsman is a large constellation that holds one of the brightest stars in the sky, Arcturus.

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Nancy Grace Roman Space Telescope arrives at KSC

A large white tube at harbor with American flag and a sign for the Nancy Grace Roman telescope.
On June 21, 2026, the Nancy Grace Roman Space Telescope arrived at Kennedy Space Center (KSC) in Florida in preparation for its August launch. Image via NASA/Amber Jean Notvest.

The Nancy Grace Roman Space Telescope arrives at KSC

On June 21, 2026, the Nancy Grace Roman Space Telescope arrived at Kennedy Space Center (KSC) in Florida ahead of its launch this summer. The new telescope completed testing at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, before being loaded on NASA’s Pegasus barge for its shipment to Florida. Amazingly, the space telescope is eight months ahead of schedule! Currently, NASA said the schedule for launch is no earlier than Sunday, August 30. That launch will be on a SpaceX Falcon Heavy rocket from Launch Complex 39A at KSC.

What’s next for the Nancy Grace Roman Space Telescope? Roman still has more testing ahead. Those tests will include work on its solar panels, insulation and thermal blankets. Eventually, workers will load about 290 gallons of hydrazine fuel into the spacecraft’s tanks.

After launch, the next stop for Roman will be L2, or the second sun-Earth Lagrange point. You may already be familiar with this location because the James Webb Space Telescope is also here, sending back infrared images of the universe. The Roman telescope also has infrared eyes. NASA said:

Roman’s wide field of view and rapid survey capabilities will reveal billions of galaxies, hundreds of thousands of new exoplanets, hundreds of blackholes, and will provide vast volumes of daily data for astronomers to study.

The Nancy Grace Roman Space Telescope is complete

NASA said back on December 4, 2025, that the construction of the Nancy Grace Roman Space Telescope was complete. Julie McEnery, Roman’s senior project scientist at NASA Goddard, said:

With Roman’s construction complete, we are poised at the brink of unfathomable scientific discovery. In the mission’s first five years, it’s expected to unveil more than 100,000 distant worlds, hundreds of millions of stars, and billions of galaxies. We stand to learn a tremendous amount of new information about the universe very rapidly after Roman launches.

Two people in white clean suits inside a large building looking up at three solar panels.
This is the fully assembled Nancy Grace Roman Space Telescope. Image via NASA/ Jolearra Tshiteya.
A graphic showing what the telescope will be looking at and the number of objects it might find.
The Nancy Grace Roman Space Telescope by the numbers. Graphic via NASA’s Goddard Space Flight Center.

Meet the Nancy Grace Roman space telescope

Remember what astronomical images were like before we had the Hubble space telescope? Hubble was the first large optical telescope to be launched into space, above Earth’s obscuring atmosphere. And it fundamentally changed our view of the cosmos. Astronomers say the Nancy Grace Roman space telescope will do that, too, giving us a view of the universe we’ve never had before. The telescope will have a primary mirror of 7.9 feet in diameter (2.4 meters). That’s the same size as Hubble. But a single image from the Nancy Grace Roman space telescope will equal the sky coverage of 100 Hubble images.

Scientists expect the telescope to answer fundamental questions about distant planets orbiting stars in our Milky Way galaxy, about the dark energy we haven’t yet detected directly but believe makes up a substantial portion of our cosmos … and about what astronomers call the cosmic dawn.

The telescope’s Wide Field Instrument, its primary instrument, will have a field of view 100 times greater than Hubble’s infrared instrument. Roman’s large field of view means it can capture more sky in less time. The Wide Field Instrument will scan the Milky Way for exoplanets, or planets orbiting distant stars. Over the past 30 years, since the early 1990s until now, we’ve discovered more than 5,000 exoplanets. The Nancy Grace Roman space telescope is expected to increase that number to some 100,000 exoplanets in the next five years.

Roman’s other instrument is the Coronagraph Instrument. The Coronagraph Instrument will perform high contrast imaging and spectroscopy to gather more knowledge of individual exoplanets. More on the coronagraph below.

Interview with Néstor Espinoza


Watch this 52-second clip of astronomer Néstor Espinoza of the Space Telescope Science Institute talking with EarthSky’s Deborah Byrd. Néstor told us this telescope should increase the number of known exoplanets – or planets orbiting distant suns – from 5,000 now to 100,000 in just 5 years!

The Roman telescope’s 100,000 new exoplanets

The Roman space telescope will survey our galaxy, taking observations every 15 minutes for more than a year. What a mass of data it’ll collect in just that first year! The data will enable astronomers to track the brightness changes in stars, which could lead to discoveries of exoplanets, rogue planets, isolated black holes and more.

So how will the Roman space telescope find its 100,000 exoplanets? With the aid of the Roman Coronagraph, the first high-contrast active wavefront-control coronagraph to fly in space. NASA said:

The Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars. Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet [next to the bright object].

The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs.

The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature and distance from its parent star.

Roman space telescope: A bulky, cylindrical, metallic object with solar panels in space.
An artist’s concept of the Nancy Grace Roman Space Telescope. Image via NASA.

The Roman telescope and the cosmic dawn

After the Big Bang that set our universe into motion, the cosmos was dark for some 380,000 to 200 million years. Yes, dark. Even though stars had already begun to shine, neutral atoms would absorb their light, leaving the cosmos in a kind of obscuring fog. Then neutral atoms began to break apart, and the fog began to lift. The light of stars broke through and began traveling throughout space. Astronomers call this transition from dark to light the cosmic dawn. Takahiro Morishita of Caltech said:

Roman will excel at finding the building blocks of cosmic structures like galaxy clusters that later form. It will quickly identify the densest regions, where more ‘fog’ is being cleared, making Roman a key mission to probe early galaxy evolution and the cosmic dawn.

Roman’s wide field of view will help determine how common quasars are and whether certain types of galaxies played a larger role in clearing the fog. It will also look for “cosmic daybreakers” that illuminated our universe.

Many wispy, purplish bubbles filled with clusters of stars in black space.
Artist’s concept of the cosmic dawn. This is how the universe may have looked at less than a billion years old. Image via NASA/ ESA/ and A. Schaller (for STScI).

The Roman space telescope and dark energy

Dark energy is a mysterious force that makes up about 68% of the total energy content of our universe. Dark energy is responsible for the acceleration of our expanding universe. Roman will help astronomers understand just what dark energy is by taking a closer look at how the universe has evolved. Roman’s wide field will allow us a bigger picture of the universe. Mapping the distribution of matter and measuring distant supernovae will help show how dark energy might have changed over time.

Graphic showing a plot with a swoosh-shaped curve and an inset with galaxies connected by a blue abstract net.
In the universe’s past, expansion occurred at a slower rate than what we see in our universe today. Dark energy is behind the accelerated expansion. Image via NASA Scientific Visualization Studio.

Who was Nancy Grace Roman?

Nancy Grace Roman has the honorary title of Mother of the Hubble Space Telescope. Born in 1925, Roman became one of the few female astronomers in a male-dominated science. Among other accomplishments, she became the first female executive at NASA and NASA’s first Chief of Astronomy. She earned her nickname by helping get the Hubble Space Telescope approved by Congress. Roman was most excited for Hubble’s discoveries on dark energy. The telescope that will now bear Roman’s name will increase our understanding of dark energy, the universe and our place in it.

Read more about Nancy Grace Roman

Woman holding a notebook and looking up at readouts from a giant computer in the 1960s.
Nancy Grace Roman, “mother of the Hubble space telescope,” during her career at NASA. Image via NASA.

Bottom line: The Nancy Grace Roman Space Telescope has now arrived at Kennedy Space Center. It will be prepped for launch this summer, eight months ahead of schedule.

Via NASA

Via NASA JPL

Read more: 3 years of the Webb telescope: Here’s what it’s discovered

Read more: Alien life? Mammoth new telescope could find it in hours

The post Nancy Grace Roman Space Telescope arrives at KSC first appeared on EarthSky.



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A large white tube at harbor with American flag and a sign for the Nancy Grace Roman telescope.
On June 21, 2026, the Nancy Grace Roman Space Telescope arrived at Kennedy Space Center (KSC) in Florida in preparation for its August launch. Image via NASA/Amber Jean Notvest.

The Nancy Grace Roman Space Telescope arrives at KSC

On June 21, 2026, the Nancy Grace Roman Space Telescope arrived at Kennedy Space Center (KSC) in Florida ahead of its launch this summer. The new telescope completed testing at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, before being loaded on NASA’s Pegasus barge for its shipment to Florida. Amazingly, the space telescope is eight months ahead of schedule! Currently, NASA said the schedule for launch is no earlier than Sunday, August 30. That launch will be on a SpaceX Falcon Heavy rocket from Launch Complex 39A at KSC.

What’s next for the Nancy Grace Roman Space Telescope? Roman still has more testing ahead. Those tests will include work on its solar panels, insulation and thermal blankets. Eventually, workers will load about 290 gallons of hydrazine fuel into the spacecraft’s tanks.

After launch, the next stop for Roman will be L2, or the second sun-Earth Lagrange point. You may already be familiar with this location because the James Webb Space Telescope is also here, sending back infrared images of the universe. The Roman telescope also has infrared eyes. NASA said:

Roman’s wide field of view and rapid survey capabilities will reveal billions of galaxies, hundreds of thousands of new exoplanets, hundreds of blackholes, and will provide vast volumes of daily data for astronomers to study.

The Nancy Grace Roman Space Telescope is complete

NASA said back on December 4, 2025, that the construction of the Nancy Grace Roman Space Telescope was complete. Julie McEnery, Roman’s senior project scientist at NASA Goddard, said:

With Roman’s construction complete, we are poised at the brink of unfathomable scientific discovery. In the mission’s first five years, it’s expected to unveil more than 100,000 distant worlds, hundreds of millions of stars, and billions of galaxies. We stand to learn a tremendous amount of new information about the universe very rapidly after Roman launches.

Two people in white clean suits inside a large building looking up at three solar panels.
This is the fully assembled Nancy Grace Roman Space Telescope. Image via NASA/ Jolearra Tshiteya.
A graphic showing what the telescope will be looking at and the number of objects it might find.
The Nancy Grace Roman Space Telescope by the numbers. Graphic via NASA’s Goddard Space Flight Center.

Meet the Nancy Grace Roman space telescope

Remember what astronomical images were like before we had the Hubble space telescope? Hubble was the first large optical telescope to be launched into space, above Earth’s obscuring atmosphere. And it fundamentally changed our view of the cosmos. Astronomers say the Nancy Grace Roman space telescope will do that, too, giving us a view of the universe we’ve never had before. The telescope will have a primary mirror of 7.9 feet in diameter (2.4 meters). That’s the same size as Hubble. But a single image from the Nancy Grace Roman space telescope will equal the sky coverage of 100 Hubble images.

Scientists expect the telescope to answer fundamental questions about distant planets orbiting stars in our Milky Way galaxy, about the dark energy we haven’t yet detected directly but believe makes up a substantial portion of our cosmos … and about what astronomers call the cosmic dawn.

The telescope’s Wide Field Instrument, its primary instrument, will have a field of view 100 times greater than Hubble’s infrared instrument. Roman’s large field of view means it can capture more sky in less time. The Wide Field Instrument will scan the Milky Way for exoplanets, or planets orbiting distant stars. Over the past 30 years, since the early 1990s until now, we’ve discovered more than 5,000 exoplanets. The Nancy Grace Roman space telescope is expected to increase that number to some 100,000 exoplanets in the next five years.

Roman’s other instrument is the Coronagraph Instrument. The Coronagraph Instrument will perform high contrast imaging and spectroscopy to gather more knowledge of individual exoplanets. More on the coronagraph below.

Interview with Néstor Espinoza


Watch this 52-second clip of astronomer Néstor Espinoza of the Space Telescope Science Institute talking with EarthSky’s Deborah Byrd. Néstor told us this telescope should increase the number of known exoplanets – or planets orbiting distant suns – from 5,000 now to 100,000 in just 5 years!

The Roman telescope’s 100,000 new exoplanets

The Roman space telescope will survey our galaxy, taking observations every 15 minutes for more than a year. What a mass of data it’ll collect in just that first year! The data will enable astronomers to track the brightness changes in stars, which could lead to discoveries of exoplanets, rogue planets, isolated black holes and more.

So how will the Roman space telescope find its 100,000 exoplanets? With the aid of the Roman Coronagraph, the first high-contrast active wavefront-control coronagraph to fly in space. NASA said:

The Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars. Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet [next to the bright object].

The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs.

The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature and distance from its parent star.

Roman space telescope: A bulky, cylindrical, metallic object with solar panels in space.
An artist’s concept of the Nancy Grace Roman Space Telescope. Image via NASA.

The Roman telescope and the cosmic dawn

After the Big Bang that set our universe into motion, the cosmos was dark for some 380,000 to 200 million years. Yes, dark. Even though stars had already begun to shine, neutral atoms would absorb their light, leaving the cosmos in a kind of obscuring fog. Then neutral atoms began to break apart, and the fog began to lift. The light of stars broke through and began traveling throughout space. Astronomers call this transition from dark to light the cosmic dawn. Takahiro Morishita of Caltech said:

Roman will excel at finding the building blocks of cosmic structures like galaxy clusters that later form. It will quickly identify the densest regions, where more ‘fog’ is being cleared, making Roman a key mission to probe early galaxy evolution and the cosmic dawn.

Roman’s wide field of view will help determine how common quasars are and whether certain types of galaxies played a larger role in clearing the fog. It will also look for “cosmic daybreakers” that illuminated our universe.

Many wispy, purplish bubbles filled with clusters of stars in black space.
Artist’s concept of the cosmic dawn. This is how the universe may have looked at less than a billion years old. Image via NASA/ ESA/ and A. Schaller (for STScI).

The Roman space telescope and dark energy

Dark energy is a mysterious force that makes up about 68% of the total energy content of our universe. Dark energy is responsible for the acceleration of our expanding universe. Roman will help astronomers understand just what dark energy is by taking a closer look at how the universe has evolved. Roman’s wide field will allow us a bigger picture of the universe. Mapping the distribution of matter and measuring distant supernovae will help show how dark energy might have changed over time.

Graphic showing a plot with a swoosh-shaped curve and an inset with galaxies connected by a blue abstract net.
In the universe’s past, expansion occurred at a slower rate than what we see in our universe today. Dark energy is behind the accelerated expansion. Image via NASA Scientific Visualization Studio.

Who was Nancy Grace Roman?

Nancy Grace Roman has the honorary title of Mother of the Hubble Space Telescope. Born in 1925, Roman became one of the few female astronomers in a male-dominated science. Among other accomplishments, she became the first female executive at NASA and NASA’s first Chief of Astronomy. She earned her nickname by helping get the Hubble Space Telescope approved by Congress. Roman was most excited for Hubble’s discoveries on dark energy. The telescope that will now bear Roman’s name will increase our understanding of dark energy, the universe and our place in it.

Read more about Nancy Grace Roman

Woman holding a notebook and looking up at readouts from a giant computer in the 1960s.
Nancy Grace Roman, “mother of the Hubble space telescope,” during her career at NASA. Image via NASA.

Bottom line: The Nancy Grace Roman Space Telescope has now arrived at Kennedy Space Center. It will be prepped for launch this summer, eight months ahead of schedule.

Via NASA

Via NASA JPL

Read more: 3 years of the Webb telescope: Here’s what it’s discovered

Read more: Alien life? Mammoth new telescope could find it in hours

The post Nancy Grace Roman Space Telescope arrives at KSC first appeared on EarthSky.



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Meet the exotic Pink Planet with salty clouds

Large pinkish planet with banded clouds. Its yellowish sun is in the distance.
Artist’s illustration of the Pink Planet, also known as GJ504b. New observations from the James Webb Space Telescope show that this “cold” planet has salty clouds. Image via NASA/ Goddard Space Flight Center/ Northwestern University.
  • GJ504b is a gas giant exoplanet about 57 light-years from Earth. It’s called the Pink Planet due to its rosy color.
  • The Pink Planet’s exotic atmosphere has clouds composed of salt, new Webb space telescope observations have revealed.
  • The Pink Planet lies near the boundary between planets and brown dwarfs. Scientists still aren’t sure how it formed.

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

The Pink Planet with salty clouds

GJ504b is a gas giant planet orbiting a sun-like star about 57 light-years from Earth. It is huge, 25 times the mass of Jupiter. And it has a rosy color, leading astronomers to nickname it the Pink Planet.

The Pink Planet has been difficult for astronomers to study. It’s cold and dim, meaning it appears as just a very faint dot in most telescopes. But now, the James Webb Space Telescope has taken a closer look and found something surprising.

A team of researchers said on June 18, 2026, that salty clouds wrap around this world. Scientists had theorized that salty clouds could exist in the atmospheres of cold planets like this one. But this is some of the first direct evidence.

Cold planets like GJ504b are too dim to study with ground-based telescopes. So these new observations are an important step in being able to find out more about them.

The researchers published their peer-reviewed results in The Astronomical Journal on June 18, 2026.

Is the Pink Planet really a planet?

Astronomers first discovered the Pink Planet back in 2013. But is it really a planet? At 25 times the mass of Jupiter, it’s so massive that it comes close to the dividing line between planets and brown dwarfs. Brown dwarfs are typically larger than planets, but smaller than stars. They are called “failed stars” because they don’t have quite enough nuclear energy inside to ignite into actual stars.

Because of this, astronomers technically refer to the Pink Planet as a “planetary-mass companion.”

The Pink Planet is a cold world

The planet is dim due to its distance from Earth and its temperature. Hot planets, like hot Jupiters, are easier to directly image. And so far, most directly imaged exoplanets have been about 1,000 to 2,000 degrees Fahrenheit (540 to 1,100 degrees Celsius). But the Pink Planet is much cooler, only about 550 degrees Fahrenheit (290 degrees Celsius). That’s still hot by human standards, of course, but a lot cooler than the other hot planets.

In fact, the Pink Planet is the coldest exoplanet ever found so far by ground-based telescopes. Lead author Aneesh Baburaj at Northwestern University in Evanston, Illinois, said:

The Pink Planet is the coldest companion ever discovered using ground-based instruments. Many teams all around the world performed follow-up observations to study its light, but it was too faint for ground-based instruments. That made it a perfect target for JWST. When we finally obtained its spectrum, it immediately looked interesting. But once we started digging deeper into the data, we realized it was not like anything we have analyzed before.

Why is the Pink Planet so relatively cold? Scientists say it’s its age. Hot giant planets like this are born scorching hot. But they cool down as they get older. And scientists estimate that the Pink Planet is between 2.5 billion and 4 billion years old. Plenty of time to cool down.

Small black circle surrounded by bright, multi-colored and pixelated rays stretching outward from it. A smaller whitish dot is in the upper right.
A direct image of the Pink Planet (upper right), which the Subaru Telescope in Hawaii obtained in May 2011. It is still just a faint dot due to its distance and coldness. Image via NASA/ Goddard Space Flight Center/ NOAJ.

How do you reveal a world so faint?

So studying the Pink Planet with ground-based telescopes is not an easy task. But that’s where the James Webb Space Telescope comes in. It is much better at gathering the faint light from the planet. The glare from its nearby star still gets in the way though. So the researchers used advanced data-processing techniques to remove much of that glare.

By doing so, scientists could finally see the spectrum of the planet’s atmosphere. That’s where light is broken down into its individual component colors. Each color indicates a different element in the atmosphere. The results were way better than any previous attempts to analyze the Pink Planet’s atmosphere. Baburaj said:

In the past, other astronomers observed the companion for an entire night with some of the biggest telescopes in the world to obtain a spectrum. And they could not see the object. With JWST, our entire observation took around two hours, and we were successful.

Smiling man wearing a dark blue shirt.
Aneesh Baburaj at Northwestern University is the lead author of the new study about the Pink Planet. Image via Northwestern University.

Discovering the Pink Planet’s salty clouds

When they analyzed the atmosphere of the Pink Planet, the researchers found something unexpected. It has clouds composed of salt. The first results showed evidence for water vapor, methane, carbon dioxide, ammonia and other molecules. But that didn’t fully match the atmosphere that the computer simulations came up with. The simulations matched the observations only when there were other “physically implausible features” in the atmosphere. Why?

The reason was clouds. The researchers tried adding clouds to the computer model of the atmosphere. They added three different kinds of clouds, and found that the “unusual features” vanished. They were no longer needed to explain the observations. But what did explain them was clouds, and one type of cloud in particular: salt. As Baburaj explained:

We ran simulations with clouds, and the results aligned with what we know about cold planets. We tried three different types of clouds, and salt clouds fit best. When we accounted for salt clouds, it subdued the signature of molecules hidden deeper in the companion’s atmosphere. Then, the results became physically possible.

This is the first time we’ve found that salt clouds are critical to explaining the spectrum of an object. It’s a good reminder to account for clouds in our models.

Metals and the origin of the Pink Planet

Another finding is that the planet’s atmosphere is unusually rich in heavy elements, or metals.

The salt clouds explain the atmospheric observations. But they still don’t explain how the Pink Planet formed. Did it form like a planet or a small star? Only additional observations of this exotic pink world will help to answer that question.

Bottom line: New observations by the Webb space telescope of the giant exoplanet GJ504b – aka the Pink Planet – show that it has clouds made of salt.

Source: JWST-TST High Contrast: First Direct Spectroscopy of GJ 504 b Reveals Clouds and Possible Metal Enrichment

Via Northwestern University

Read more: Colorful life on exoplanets might be lurking in clouds

Read more: See colorful giant exoplanets in astonishing new Webb images

The post Meet the exotic Pink Planet with salty clouds first appeared on EarthSky.



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Large pinkish planet with banded clouds. Its yellowish sun is in the distance.
Artist’s illustration of the Pink Planet, also known as GJ504b. New observations from the James Webb Space Telescope show that this “cold” planet has salty clouds. Image via NASA/ Goddard Space Flight Center/ Northwestern University.
  • GJ504b is a gas giant exoplanet about 57 light-years from Earth. It’s called the Pink Planet due to its rosy color.
  • The Pink Planet’s exotic atmosphere has clouds composed of salt, new Webb space telescope observations have revealed.
  • The Pink Planet lies near the boundary between planets and brown dwarfs. Scientists still aren’t sure how it formed.

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

The Pink Planet with salty clouds

GJ504b is a gas giant planet orbiting a sun-like star about 57 light-years from Earth. It is huge, 25 times the mass of Jupiter. And it has a rosy color, leading astronomers to nickname it the Pink Planet.

The Pink Planet has been difficult for astronomers to study. It’s cold and dim, meaning it appears as just a very faint dot in most telescopes. But now, the James Webb Space Telescope has taken a closer look and found something surprising.

A team of researchers said on June 18, 2026, that salty clouds wrap around this world. Scientists had theorized that salty clouds could exist in the atmospheres of cold planets like this one. But this is some of the first direct evidence.

Cold planets like GJ504b are too dim to study with ground-based telescopes. So these new observations are an important step in being able to find out more about them.

The researchers published their peer-reviewed results in The Astronomical Journal on June 18, 2026.

Is the Pink Planet really a planet?

Astronomers first discovered the Pink Planet back in 2013. But is it really a planet? At 25 times the mass of Jupiter, it’s so massive that it comes close to the dividing line between planets and brown dwarfs. Brown dwarfs are typically larger than planets, but smaller than stars. They are called “failed stars” because they don’t have quite enough nuclear energy inside to ignite into actual stars.

Because of this, astronomers technically refer to the Pink Planet as a “planetary-mass companion.”

The Pink Planet is a cold world

The planet is dim due to its distance from Earth and its temperature. Hot planets, like hot Jupiters, are easier to directly image. And so far, most directly imaged exoplanets have been about 1,000 to 2,000 degrees Fahrenheit (540 to 1,100 degrees Celsius). But the Pink Planet is much cooler, only about 550 degrees Fahrenheit (290 degrees Celsius). That’s still hot by human standards, of course, but a lot cooler than the other hot planets.

In fact, the Pink Planet is the coldest exoplanet ever found so far by ground-based telescopes. Lead author Aneesh Baburaj at Northwestern University in Evanston, Illinois, said:

The Pink Planet is the coldest companion ever discovered using ground-based instruments. Many teams all around the world performed follow-up observations to study its light, but it was too faint for ground-based instruments. That made it a perfect target for JWST. When we finally obtained its spectrum, it immediately looked interesting. But once we started digging deeper into the data, we realized it was not like anything we have analyzed before.

Why is the Pink Planet so relatively cold? Scientists say it’s its age. Hot giant planets like this are born scorching hot. But they cool down as they get older. And scientists estimate that the Pink Planet is between 2.5 billion and 4 billion years old. Plenty of time to cool down.

Small black circle surrounded by bright, multi-colored and pixelated rays stretching outward from it. A smaller whitish dot is in the upper right.
A direct image of the Pink Planet (upper right), which the Subaru Telescope in Hawaii obtained in May 2011. It is still just a faint dot due to its distance and coldness. Image via NASA/ Goddard Space Flight Center/ NOAJ.

How do you reveal a world so faint?

So studying the Pink Planet with ground-based telescopes is not an easy task. But that’s where the James Webb Space Telescope comes in. It is much better at gathering the faint light from the planet. The glare from its nearby star still gets in the way though. So the researchers used advanced data-processing techniques to remove much of that glare.

By doing so, scientists could finally see the spectrum of the planet’s atmosphere. That’s where light is broken down into its individual component colors. Each color indicates a different element in the atmosphere. The results were way better than any previous attempts to analyze the Pink Planet’s atmosphere. Baburaj said:

In the past, other astronomers observed the companion for an entire night with some of the biggest telescopes in the world to obtain a spectrum. And they could not see the object. With JWST, our entire observation took around two hours, and we were successful.

Smiling man wearing a dark blue shirt.
Aneesh Baburaj at Northwestern University is the lead author of the new study about the Pink Planet. Image via Northwestern University.

Discovering the Pink Planet’s salty clouds

When they analyzed the atmosphere of the Pink Planet, the researchers found something unexpected. It has clouds composed of salt. The first results showed evidence for water vapor, methane, carbon dioxide, ammonia and other molecules. But that didn’t fully match the atmosphere that the computer simulations came up with. The simulations matched the observations only when there were other “physically implausible features” in the atmosphere. Why?

The reason was clouds. The researchers tried adding clouds to the computer model of the atmosphere. They added three different kinds of clouds, and found that the “unusual features” vanished. They were no longer needed to explain the observations. But what did explain them was clouds, and one type of cloud in particular: salt. As Baburaj explained:

We ran simulations with clouds, and the results aligned with what we know about cold planets. We tried three different types of clouds, and salt clouds fit best. When we accounted for salt clouds, it subdued the signature of molecules hidden deeper in the companion’s atmosphere. Then, the results became physically possible.

This is the first time we’ve found that salt clouds are critical to explaining the spectrum of an object. It’s a good reminder to account for clouds in our models.

Metals and the origin of the Pink Planet

Another finding is that the planet’s atmosphere is unusually rich in heavy elements, or metals.

The salt clouds explain the atmospheric observations. But they still don’t explain how the Pink Planet formed. Did it form like a planet or a small star? Only additional observations of this exotic pink world will help to answer that question.

Bottom line: New observations by the Webb space telescope of the giant exoplanet GJ504b – aka the Pink Planet – show that it has clouds made of salt.

Source: JWST-TST High Contrast: First Direct Spectroscopy of GJ 504 b Reveals Clouds and Possible Metal Enrichment

Via Northwestern University

Read more: Colorful life on exoplanets might be lurking in clouds

Read more: See colorful giant exoplanets in astonishing new Webb images

The post Meet the exotic Pink Planet with salty clouds first appeared on EarthSky.



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