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Astronomers first discovered Cha 1107-7626 in 2008, and since then, they have observed it with different telescopes to learn more about how the infant planet evolves, as well as to study its surroundings.
тяжеловесные негабаритные перевозки
The research team observed the planet with Webb in 2024, making a clear detection of the surrounding disk. Next, the researchers studied it using the X-shooter spectrograph on the Very Large Telescope, which can capture different wavelengths of light emitted by an object ranging from ultraviolet to near-infrared.

The observations detected a puzzling event as the planet transitioned from a steady accretion rate in April and May to a burst of growth between June and August.
https://tlk-triga.ru/perevozka_opasnogo_gruza/
грузоперевозки по московской области цены
“I fully expected that this is a short-term event, because those are much more common,” Scholz said. “When the burst kept going through July and August, I was absolutely stunned.”

Follow-up observations made using the Webb telescope also showed that the chemistry of the disk had changed. Water vapor, present during the growth spurt, wasn’t in the disk before. Webb is the only telescope capable of capturing such detailed changes in the environment for such a faint object, Scholz said. Prior to this research, astronomers had only ever seen the chemistry of a disk change around a star, but not around a planet.

Comparing observations from before and during the event showed that magnetic activity seems to be the main driver behind how much gas and dust is falling on the planet — a phenomenon typically associated with stars as they grow.

But the new observations suggest that objects with much less mass than stars — the rogue world is less than 1% the mass of our sun — can have strong magnetic fields capable of driving the growth of the object, according to the study authors.

An infrared image taken with the Visible and Infrared Telescope for Astronomy shows Cha 1107-7626, a dot located in the center.
An infrared image taken with the Visible and Infrared Telescope for Astronomy shows Cha 1107-7626, a dot located in the center. ESO/Meingast et al.
A planet that acts like a star
The origin of rogue planets remains murky. It’s possible they are planets that are kicked out of orbit around stars due to the gravitational influence of other objects. Or perhaps they are the lowest-mass objects that happen to form like stars. For Cha 1107-7626, astronomers said they think it’s the latter.

“This object most likely formed in a way similar to stars — from the collapse and fragmentation of a molecular cloud,” Scholz said.

A molecular cloud is a massive, cold cloud of gas and dust that can stretch for hundreds of light-years, according to NASA.

“We’re struck by quite how much the infancy of free-floating planetary-mass objects resembles that of stars like the Sun,” Jayawardhana said in a statement. “Our new findings underscore that similarity, and imply that some objects comparable to giant planets form the way stars do, from contracting clouds of gas and dust accompanied by disks of their own, and they go through growth episodes just like newborn stars.”

Astronomers have observed a planet that in some ways behaves more like a star — including a massive growth spurt unlike anything witnessed before in a free-floating planet.
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The rogue planet, which does not orbit any star, is called Cha 1107-7626 and is outside of our solar system, 620 light-years from Earth in the Chamaeleon constellation. A single light-year, or the distance light travels in one year, is equal to 5.88 trillion miles (9.46 trillion kilometers).

The planet has a mass five to 10 times that of Jupiter, the largest planet in our solar system. And it’s getting bigger every second, according to new research published Thursday in The Astrophysical Journal Letters.

Estimated to be 1 million to 2 million years old, Cha 1107-7626 is still forming, said study coauthor Aleks Scholz, an astronomer at the University of St. Andrews in Scotland. It may sound old, but astronomically speaking, the planet is in its infancy. By contrast, the planets in our solar system are about 4.5 billion years old.
https://ms-stroy.ru/
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Cha 1107-7626 is surrounded by a disk of gas and dust, which constantly falls onto the planet and accumulates during a process that astronomers call accretion. But the rate at which the young planet is growing varies, the study authors said.

Observations with the European Southern Observatory’s Very Large Telescope in Chile’s Atacama Desert, along with follow-up views conducted by the James Webb Space Telescope, showed that the planet is adding material about eight times faster than a few months earlier and gobbling up gas and dust at a record rate of 6.6 billion tons (6 billion metric tons) per second.

Related article
The Earth-size exoplanet TRAPPIST-1 e, depicted at the lower right, is silhouetted as it passes in front of its flaring host star in this artist’s concept of the TRAPPIST-1 system.
Earth-like exoplanet could be habitable, and astronomers may know soon

The unusual burst of activity is the strongest growth rate ever recorded for a planet of any kind, said lead study author Victor Almendros-Abad, an astronomer at the Palermo Astronomical Observatory of the National Institute for Astrophysics in Italy, and is shedding light on the tumultuous formation and evolution of planets.

“We’ve caught this newborn rogue planet in the act of gobbling up stuff at a furious pace,” said senior coauthor Ray Jayawardhana, provost and professor of physics and astronomy at Johns Hopkins University, in a statement.

“Monitoring its behavior over the past few months, with two of the most powerful telescopes on the ground and in space, we have captured a rare glimpse into the baby phase of isolated objects not much heftier than Jupiter. Their infancy appears to be much more tumultuous than we had realized.”

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Don Mueang International Airport, Thailand (DMK)
трипскан сайт
Are you an avgeek with a mean handicap? Then it’s time to tee off in Bangkok, where Don Mueang International Airport has an 18-hole golf course between its two runways. If you’re nervous from a safety point of view, don’t be — players at the Kantarat course must go through airport-style security before they hit the grass. Oh, you meant safety on the course? Just beware of those flying balls, because there are no barriers between the course and the runways. Players are, at least, shown a red light when a plane is coming in to land so don’t get too distracted by the game.
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Although Suvarnabhumi (BKK) is Bangkok’s main airport these days — it opened in 2006 —Don Mueang, which started out as a Royal Thai Air Force base in 1914, remains Bangkok’s budget airline hub, with brands including Thai Air Asia and Thai Lion Air using it as their base. Although you’re more likely to see narrowbodies these days, you may just get lucky — in 2022, an Emirates A380 made an emergency landing here. Imagine the views from the course that day.

Related article
Sporty airport outfit being worn by writer
CNN Underscored: Flying sucks. Make it better with these comfy airport outfits for women

Sumburgh Airport, Scotland (LSI)
The road south from Lerwick cuts across the runway of Sumburgh Airport on Shetland.
The road south from Lerwick cuts across the runway of Sumburgh Airport on Shetland. Alan Morris/iStock Editorial/Getty Images
Planning a trip to Jarlshof, the extraordinarily well-preserved Bronze Age settlement towards the southern tip of Shetland? You may need to build in some extra time. The ancient and Viking-era ruins, called one of the UK’s greatest archaeological sites, sit just beyond one of the runways of Sumburgh, Shetland’s main airport — and reaching them means driving, cycling or walking across the runway itself.

There’s only one road heading due south from the capital, Lerwick; and while it ducks around most of the airport’s perimeter, skirting the two runways, the road cuts directly across the western end of one of them. A staff member occupies a roadside hut, and before take-offs and landings, comes out to lower a barrier across the road. Once the plane is where it needs to be, up come the barriers and waiting drivers get a friendly thumbs up.

Amata Kabua International Airport, Marshall Islands (MAJ)
Fly into Majuro and you'll skim across the Pacific and land on the runway that's just about as wide as the sandbar-like island itself.
Fly into Majuro and you'll skim across the Pacific and land on the runway that's just about as wide as the sandbar-like island itself. mtcurado/iStockphoto/Getty Images
Imagine flying into Majuro, the capital of the Marshall Islands in Micronesia. You’re descending down, down, and further down towards the Pacific, no land in sight. Then you’re suddenly above a pencil-thin atoll — can you really be about to land here? Yes you are, with cars racing past the runway no less, matching you for speed.

Majuro’s Amata Kabua International Airport gives a whole new meaning to the phrase “water landing”. Its single runway, just shy of 8,000ft, is a slim strip of asphalt over the sandbar that’s barely any wider than the atoll itself — and the island is so remote that when the runway was resurfaced, materials had to be transported from the Philippines, Hong Kong and Korea, according to the constructors. “Lagoon Road” — the 30-mile road that runs from top to toe on Majuro — skims alongside the runway.
Don’t think about pulling over, though — there’s only sand and sea on one side, and that runway the other.

Related article
Barra Airport, Scotland
At Scotland’s beach airport, the runway disappears at high tide

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Michelle Pfeiffer shares she’s now a grandmother
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Hollywood star Michelle Pfeiffer has announced that she has become a grandmother, and spoken about how it has affected her working life.

Speaking on the “Smartless” podcast on Monday, three-time Oscar nominee Pfeiffer told hosts Jason Bateman, Sean Hayes and Will Arnett that having a grandchild was “heaven.”

“I’ve been very quiet about it and it is – it’s heaven. It’s ridiculous,” said Pfeiffer, 67, who has an adopted daughter Claudia Rose and a son named John Henry.

“And if I had known that I was going to be a grandmother, I wouldn’t have taken on so much work, but I’ve enjoyed everything and I’m really grateful,” she said.
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“I love each of these projects,” said Pfeiffer, referencing her recent work on projects including “Yellowstone” spin-off series “The Madison” on Paramount+, Christmas comedy “Oh. What. Fun” and the TV adaptation of Rufi Thorpe’s novel “Margo’s Got Money Troubles.”

“I’m so grateful. I’m so grateful because I love acting… in fact, I probably, enjoy it more now than I ever have because I’m sort of more relaxed with it,” said Pfeiffer.

The Hollywood star has had a long and storied career both in movies and on TV, including appearances in “Scarface” (1983), “Batman Returns” (1992) and Showtime series “The First Lady” (2022).

“I don’t really have time to be thinking about anything but the task at hand,” she said, highlighting the fact that she also set up a fragrance company a few years ago.

Related article
LOS ANGELES, CALIFORNIA - APRIL 14: Michelle Pfeiffer arrives at Showtime's FYC event and premiere for 'The First Lady' at DGA Theater Complex on April 14, 2022 in Los Angeles, California. (Photo by Emma McIntyre/WireImage)
Michelle Pfeiffer would consider playing Catwoman again

“But when I had all these acting jobs coming up, I thought, ‘Okay, okay, how are you going to manage this and have a life?’ Because that hasn’t always been easy for me. I’m an all or nothing kind of girl,” added Pfeiffer.

“I always like taking on challenges and then I get into it and it’s sort of sink or swim and for whatever reason I kind of feed on that,” she said, before going on to suggest that her priorities have shifted recently.

“I don’t have the time nor the desire to go that deep for that long and not be present,” said Pfeiffer.

Экскурсии по Казани — обзор маршрутов и лучших туров по Казани
Казань — жемчужина Поволжья с богатой историей и неповторимой культурой. Если вы ищете интересные экскурсии по Казани, на нашем сайте представлены лучшие маршруты — от обзорных программ до авторских прогулок.
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Astronomers first discovered Cha 1107-7626 in 2008, and since then, they have observed it with different telescopes to learn more about how the infant planet evolves, as well as to study its surroundings.
перевозка экскаватора стоимость
The research team observed the planet with Webb in 2024, making a clear detection of the surrounding disk. Next, the researchers studied it using the X-shooter spectrograph on the Very Large Telescope, which can capture different wavelengths of light emitted by an object ranging from ultraviolet to near-infrared.

The observations detected a puzzling event as the planet transitioned from a steady accretion rate in April and May to a burst of growth between June and August.
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“I fully expected that this is a short-term event, because those are much more common,” Scholz said. “When the burst kept going through July and August, I was absolutely stunned.”

Follow-up observations made using the Webb telescope also showed that the chemistry of the disk had changed. Water vapor, present during the growth spurt, wasn’t in the disk before. Webb is the only telescope capable of capturing such detailed changes in the environment for such a faint object, Scholz said. Prior to this research, astronomers had only ever seen the chemistry of a disk change around a star, but not around a planet.

Comparing observations from before and during the event showed that magnetic activity seems to be the main driver behind how much gas and dust is falling on the planet — a phenomenon typically associated with stars as they grow.

But the new observations suggest that objects with much less mass than stars — the rogue world is less than 1% the mass of our sun — can have strong magnetic fields capable of driving the growth of the object, according to the study authors.

An infrared image taken with the Visible and Infrared Telescope for Astronomy shows Cha 1107-7626, a dot located in the center.
An infrared image taken with the Visible and Infrared Telescope for Astronomy shows Cha 1107-7626, a dot located in the center. ESO/Meingast et al.
A planet that acts like a star
The origin of rogue planets remains murky. It’s possible they are planets that are kicked out of orbit around stars due to the gravitational influence of other objects. Or perhaps they are the lowest-mass objects that happen to form like stars. For Cha 1107-7626, astronomers said they think it’s the latter.

“This object most likely formed in a way similar to stars — from the collapse and fragmentation of a molecular cloud,” Scholz said.

A molecular cloud is a massive, cold cloud of gas and dust that can stretch for hundreds of light-years, according to NASA.

“We’re struck by quite how much the infancy of free-floating planetary-mass objects resembles that of stars like the Sun,” Jayawardhana said in a statement. “Our new findings underscore that similarity, and imply that some objects comparable to giant planets form the way stars do, from contracting clouds of gas and dust accompanied by disks of their own, and they go through growth episodes just like newborn stars.”

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Astronomers have observed a planet that in some ways behaves more like a star — including a massive growth spurt unlike anything witnessed before in a free-floating planet.
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The rogue planet, which does not orbit any star, is called Cha 1107-7626 and is outside of our solar system, 620 light-years from Earth in the Chamaeleon constellation. A single light-year, or the distance light travels in one year, is equal to 5.88 trillion miles (9.46 trillion kilometers).

The planet has a mass five to 10 times that of Jupiter, the largest planet in our solar system. And it’s getting bigger every second, according to new research published Thursday in The Astrophysical Journal Letters.

Estimated to be 1 million to 2 million years old, Cha 1107-7626 is still forming, said study coauthor Aleks Scholz, an astronomer at the University of St. Andrews in Scotland. It may sound old, but astronomically speaking, the planet is in its infancy. By contrast, the planets in our solar system are about 4.5 billion years old.
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Cha 1107-7626 is surrounded by a disk of gas and dust, which constantly falls onto the planet and accumulates during a process that astronomers call accretion. But the rate at which the young planet is growing varies, the study authors said.

Observations with the European Southern Observatory’s Very Large Telescope in Chile’s Atacama Desert, along with follow-up views conducted by the James Webb Space Telescope, showed that the planet is adding material about eight times faster than a few months earlier and gobbling up gas and dust at a record rate of 6.6 billion tons (6 billion metric tons) per second.

Related article
The Earth-size exoplanet TRAPPIST-1 e, depicted at the lower right, is silhouetted as it passes in front of its flaring host star in this artist’s concept of the TRAPPIST-1 system.
Earth-like exoplanet could be habitable, and astronomers may know soon

The unusual burst of activity is the strongest growth rate ever recorded for a planet of any kind, said lead study author Victor Almendros-Abad, an astronomer at the Palermo Astronomical Observatory of the National Institute for Astrophysics in Italy, and is shedding light on the tumultuous formation and evolution of planets.

“We’ve caught this newborn rogue planet in the act of gobbling up stuff at a furious pace,” said senior coauthor Ray Jayawardhana, provost and professor of physics and astronomy at Johns Hopkins University, in a statement.

“Monitoring its behavior over the past few months, with two of the most powerful telescopes on the ground and in space, we have captured a rare glimpse into the baby phase of isolated objects not much heftier than Jupiter. Their infancy appears to be much more tumultuous than we had realized.”

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