Английская Википедия:COCONUTS-2b

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Шаблон:Short description Шаблон:Infobox planetCOCONUTS-2 b, or WISEPA J075108.79-763449.6, is a gas giant exoplanet that orbits the M-type star L 34-26. With a mass of 6.3 Jupiters, it takes over one million years to complete one orbit around the star, and it is 7,506 AU away from it.[1]

The planet was discovered in 2011 and was initially identified as a T9 free-floating brown dwarf WISEPA J075108.79−763449.6.[2] During the COol Companions ON Ultrawide orbiTS (COCONUTS) survey, its association with L 34-26 was announced in 2021.[3] At a distance of 10.9 pc, COCONUTS-2b is the closest directly imaged exoplanet to Earth known to date.[4]

The researchers found that it is unlikely that COCONUTS-2b was formed inside the protoplanetary disk of the host star and it is more likely that the planet formed on its own via high entropy formation (aka hot-start process).[5][6]

Atmosphere

The planet has a spectral type of T9, based on a low signal-to-noise near-infrared spectrum with Magellan/FIRE.[2][5] This spectral type suggests high amounts of methane, water vapor and low amounts of carbon monoxide in the atmosphere of COCONUTS-2b.

COCONUTS-2b might have both clouds and a non-equilibrium process in its atmosphere.[5]

Due to its large orbital separation, COCONUTS-2b is a great laboratory to study the atmosphere and composition of young gas-giant exoplanets.[7] Astronomers estimate the planet’s temperature to be around Шаблон:Convert.[5]

Host star

Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end

L 34-26, also known as COCONUTS-2A and TYC 9381-1809-1, is a M3-type dwarf star located 35 light-years away, in the constellation of Chamaeleon. The star is about one-third the mass of the Sun, with an age between 150 and 800 million years old.[8]

Researchers using TESS found that L 34-26 showed stellar flares about every 0.48 days. It was the most active planet hosting star in their sample. The team studying the host star also found that L 34-26 is fast rotating with a rotation period of 2.83 days. The planet should not be influenced by the flares, because of the large orbital separation.[9]

Gallery

References

Шаблон:Reflist

External links

Шаблон:2021 in space Шаблон:Stars of Chamaeleon

  1. Шаблон:Cite news
  2. 2,0 2,1 Ошибка цитирования Неверный тег <ref>; для сносок :0 не указан текст
  3. Шаблон:Cite web
  4. Шаблон:Cite web
  5. 5,0 5,1 5,2 5,3 Шаблон:Cite journal
  6. Шаблон:Cite journal
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  8. Шаблон:Cite web
  9. Шаблон:Cite journal