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Stellar Brief: 19. 10. 2026
The coldest known brown dwarf, WISE 0855, has patchy water clouds—and its atmosphere is changing before our eyes. James Webb observations found carbon monoxide absorption varying by as much as 10% over time, offering a rare glimpse of weather on an object between a giant planet and a star. Read today's Stellar Brief

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Latest astronomy news

James Webb Space Telescope has imaged a massive exoplanet orbiting nearby star Epsilon Indi A
icon5. 3. 2025
iconStars | Exoplane
Image: James Webb Space Telescope has imaged a massive exoplanet orbiting nearby star Epsilon Indi A
It’s one of the coolest directly imaged exoplanets ever, with hints of exotic chemistry in its atmosphere. ...
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New observations from Keck Telescope confirm mass of scorching Earth-sized planet TOI 6324 b
icon25. 2. 2025
iconStars | Exoplane
Image: New observations from Keck Telescope confirm mass of scorching Earth-sized planet TOI 6324 b
It’s the closest confirmed ultra-short-period planet to Earth’s size, with no thick atmosphere. The planet TOI 6324 b orbits a nearby (67 light years) red dwarf star with about 20 % solar mass. The planet's orbit is so tight, that the year on it lasts less than a day. Although the planet is similar in size and mass to Earth, its proximity to the star expose it to extreme temperature and radiation....
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JWST has detected a possible sub-Jupiter mass planet in the debris disk of the young star CE Antliae (TWA 7)
icon24. 2. 2025
iconStar
Image: JWST has detected a possible sub-Jupiter mass planet in the debris disk of the young star CE Antliae (TWA 7)
CE Antliae is a very young variable star of T Tauri class, meaning it is still in process of contracting to become the main sequence. There are multiple known rings orbiting the star. The position of newly discovered planet candidate may explain the unique rings around the star. ...
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JWST has detected hydrogen cyanide and acetylene in the brown dwarf binary WISE J0458+6434
icon20. 2. 2025
iconStars | Brown dwarf
Image: JWST has detected hydrogen cyanide and acetylene in the brown dwarf binary WISE J0458+6434
These molecules suggest intense vertical mixing in the atmosphere, challenging previous models of carbon chemistry in cold brown dwarfs. WISE J0458+6434 is a binary system with two T-type brown dwarfs separated by several AU. The pair lies 30 light years away....
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An ultra-hot Neptune in the Neptune desert LTT 9779 b has a metal-rich atmosphere with possible silicate clouds
icon2. 2. 2025
iconStars | Exoplane
Image: An ultra-hot Neptune in the Neptune desert LTT 9779 b has a metal-rich atmosphere with possible silicate clouds
No strong atmospheric signals were detected, suggesting high metallicity and hazes that obscure spectral features....
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Atmosphere of K2-18 b shows strong methane detection but no clear evidence of CO₂ or dimethyl sulfide
icon31. 1. 2025
iconStars | Exoplane
Image: Atmosphere of K2-18 b shows strong methane detection but no clear evidence of CO₂ or dimethyl sulfide
These findings contradict claims of a liquid water ocean or life signs. The planet is likely an oxygen-poor sub-Neptune....
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Rapidly rotating magnetic star HR 5907 emits unusual low-frequency radio signals
icon23. 1. 2025
iconStars | Massive main-sequence star
Image: Rapidly rotating magnetic star HR 5907 emits unusual low-frequency radio signals
Its circular polarization suggests persistent auroral activity via electron cyclotron maser emission...
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Three extremely metal-poor RR Lyrae stars were analyzed using high-resolution spectra
icon14. 1. 2025
iconStar
Image: Three extremely metal-poor RR Lyrae stars were analyzed using high-resolution spectra
Their movement suggests mixed origins - in galactic disk and halo....
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A disintegrating rocky planet discovered orbiting a bright K-dwarf BD+05 4868 A
icon10. 1. 2025
iconStars | Exoplane
Image: A disintegrating rocky planet discovered orbiting a bright K-dwarf BD+05 4868 A
When transiting in front of the star, comet-like tails both leading and trailing are visible, indicating large dust grains and rapid mass loss...
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Discovery of TOI 6038 A b - a dense sub-Saturn in the transition between the Neptunian ridge and savanna
icon7. 1. 2025
iconStars | TESS | Exoplane
Image: Discovery of TOI 6038 A b - a dense sub-Saturn in the transition between the Neptunian ridge and savanna
Its high-density core suggests tidal or disk migration to its current orbit....
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Recently discovered exoplanets

EK Chamaeleontis b 10 / 2026 2702.2 M⊕ 321.3 ly
HD 715 b 10 / 2026 201.9 M⊕ 542.8 ly
DENIS J1253-5709 b 10 / 2026 244.8 M⊕ 54.4 ly
TOI-6417 b 09 / 2026 349.7 M⊕ 1903.9 ly
TOI-6443 b 09 / 2026 1605.4 M⊕ 2051.6 ly
TOI-7219 b 09 / 2026 661 M⊕ 1074.2 ly
TOI-4079 B b 09 / 2026 1646.8 M⊕ 1185.6 ly
HD 45652 b 09 / 2026 1557.7 M⊕ 113.9 ly
LSPM J0804+1116 b 09 / 2026 6.4 M⊕ 82.6 ly
HR 8799 f 09 / 2026 524.5 M⊕ 133.3 ly
61 Cygni A b 09 / 2026 2543.3 M⊕ 11.4 ly
TOI-5646 b 08 / 2026 45.9 M⊕ 1352.3 ly
TOI-4468 c 08 / 2026 11.1 M⊕ 1233.1 ly
TOI-4468 b 08 / 2026 170.1 M⊕ 1233.1 ly
TOI-4468 d 08 / 2026 311 M⊕ 1233.1 ly
Newly discovered exoplanets
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