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Stellar Brief: 19. 10. 2026
The cold brown dwarf WISE 0855 has weather that looks strikingly planet-like: James Webb observations reveal patchy water clouds and changing atmospheric gases, including carbon monoxide and phosphine. Read today's Stellar Brief

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Latest astronomy news

Brown dwarf / giant exoplanet BD-14 3065 b has double the radius of Jupiter and is the largest object detected around post-main sequence star
icon18. 3. 2024 (accepted)
iconStars | Exoplanets | Brown dwarf
Image: Brown dwarf / giant exoplanet BD-14 3065 b has double the radius of Jupiter and is the largest object detected around post-main sequence star
The inflated size could be sign of deuterium burning....
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Newly discovered Neptune-sized planet TOI 4438 b orbits a nearby star every 7.44 days
icon14. 3. 2024 (accepted)
iconStars | Exoplane
Image: Newly discovered Neptune-sized planet TOI 4438 b orbits a nearby star every 7.44 days
It is likely rich in volatile elements like water and may have a thick atmosphere, which makes it great target for further study....
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Third planet confirmed orbiting red dwarf LHS 1678 A
icon29. 2. 2024 (accepted)
iconStars | Exoplane
Image: Third planet confirmed orbiting red dwarf LHS 1678 A
It is similar in size to Earth and to another planet in the system which makes it a great target for comparing evolution of planets in different orbits around star....
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Astronomers investigated 6 young stars with protoplanetary discs in nearby Taurus stellar nursery
icon28. 2. 2024 (accepted)
iconStar
Image: Astronomers investigated 6 young stars with protoplanetary discs in nearby Taurus stellar nursery
Most disks show complex structures like rings and cavities, hinting at planet formation...
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Observations of WASP 77 A b show water vapor, carbon monoxide, and titanium oxide in the atmosphere
icon28. 2. 2024 (accepted)
iconStars | Exoplane
Image: Observations of WASP 77 A b show water vapor, carbon monoxide, and titanium oxide in the atmosphere
The ratio of carbon to oxygen suggests the planet formed close to its star...
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Fourth planetary system with nodal precession identified. TOI 1518 b grazes the disk of its parent star
icon27. 2. 2024 (accepted)
iconStars | Exoplane
Image: Fourth planetary system with nodal precession identified. TOI 1518 b grazes the disk of its parent star
The planets orbit is not perfectly aligned with the stars equator, but tilted at a sharp angle. This tilt, combined with the stars rapid rotation, causes the planets trajectory to slowly wobble over time, a phenomenon called nodal precession....
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Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
icon6. 2. 2024 (accepted)
iconStars | Exoplane
Image: Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
The first planet TOI 238 b is a super-Earth with 1.4 Earth radii and was discovered just last year. Newly discovered TOI 238 c with 2.2 radii could be a water-rich world....
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New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
icon22. 1. 2024 (accepted)
iconStar
Image: New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
The planet has a radius of 1.24 Earth radii, a mass of 2.53 Earth masses, and an equilibrium temperature of 996 degrees Kelvin. It is likely composed of a large iron core, a small rocky mantle, and a negligible atmosphere....
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How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
icon29. 11. 2023 (accepted)
iconStars | Exoplane
Image: How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
TRAPPIST-1 c receives almost the same bolometric flux as Venus. However JWST measurements show no sign of CO2 which is abundant in the atmosphere of our neighboring planet. According to a new study stellar winds cannot account for all the lost CO2. So astronomers believe that the planet was either born without significant CO2 atmosphere, or must have lost big portion of it through the escape of hydrogen. ...
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Retrieving planet formation parameters of WASP-77 A b
icon27. 11. 2023 (accepted)
iconStars | Exoplane
Image: Retrieving planet formation parameters of WASP-77 A b
WASP-77Ab likely formed in a disk with few planetesimals and underwent disk-free migration, starting within the CO ice line and ending beyond the water ice line...
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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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