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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

The longest-period M dwarf exoplanet found orbiting TOI 904
icon23. 10. 2023 (accepted)
iconStars | Exoplane
Image: The longest-period M dwarf exoplanet found orbiting TOI 904
Two new sub-Neptunes, TOI-904 b and c, have been discovered orbiting the early M dwarf TOI-904. The outer planet, TOI-904 c, is the longest-period M dwarf exoplanet found by TESS, with period 84 days and an estimated equilibrium temperature of 217 K. Future mass measurements and transmission spectroscopy of the similar-sized planets in this system could determine whether they are also similar in density and composition, suggesting a common formation pathway, or whether they have distinct origins...
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HD 152843 c has the longest orbital period of any known low-density exoplanet
icon23. 10. 2023 (accepted)
iconStars | Exoplane
Image: HD 152843 c has the longest orbital period of any known low-density exoplanet
The two planets in the HD 152843 system have nearly equal masses but differing radii, and the outer planet HD 152843 c has the longest orbital period of any known low-density exoplanet. HD 152843 c is also located in the Saturn valley, the observed lack of planets larger than Neptune but smaller than Saturn. The orbital periods of the planets suggest they are near a 5:3 mean motion resonance, and the brightness of the host star and the low densit...
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Second exoplanet discovered around star TOI 2134
icon20. 10. 2023 (accepted)
iconStars | Exoplanets | TESS
Image: Second exoplanet discovered around star TOI 2134
A temperate, highly eccentric sub-Saturn has been discovered orbiting the bright K-dwarf TOI-2134, in addition to an inner mini-Neptune that was discovered three years ago. The outer planet has a radius of 7.27 R⊕ and a mass of 41.86 M⊕, and a high eccentricity of 0.67, positioning it in the habitable zone of its system for part of its orbit. Further observations are needed to fully constrain the orbit of the outer planet and to study the spin-or...
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New warm Neptune discovered orbiting nearby red dwarf TOI 2015
icon18. 10. 2023 (accepted)
iconStars | TESS | Exoplane
Image: New warm Neptune discovered orbiting nearby red dwarf TOI 2015
The planet has more than 3 Earth radii and a 16 Earth masses, suggesting a likely volatile-rich planet. Transit timing variations in the system suggest the presence of an outer planet candidate near a 2:1 resonance, with a mass of 6.8 Earths. Further observations are needed to explicitly identify the resonance and further characterize the properties of the system....
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Exoplanets similar to Neptune have cloudy atmospheres and high metalicity
icon11. 10. 2023 (accepted)
iconStars | Exoplane
Image: Exoplanets similar to Neptune have cloudy atmospheres and high metalicity
A new analysis of exo-Neptune transmission spectra reveals that these planets have very cloudy atmospheres and high metallicity. Colder exo-Neptunes may have clearer atmospheres, making them better targets for future studies and the search for life beyond Earth...
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2 exoplanets discovered orbiting red dwarfs Gliese 724 and Gliese 3988
icon9. 10. 2023 (accepted)
iconStars | Exoplane
Image: 2 exoplanets discovered orbiting red dwarfs Gliese 724 and Gliese 3988
Both planets have short periods and relatively low masses, but Gliese 724 b is the most eccentric single exoplanet yet discovered around an M dwarf....
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The most promising ways to confirm Gaia astrometric planetary candidates and obtain follow-up data
icon9. 10. 2023 (accepted)
iconStars | Exoplanets | White dwarf
Image: The most promising ways to confirm Gaia astrometric planetary candidates and obtain follow-up data
Astrometric planet candidates around white dwarfs can be confirmed and characterized by combining astrometric data with spectroscopic and photometric data. Radial velocity and infrared photometry can be used to probe the mass of the objects producing some of the astrometric signals, and rule out parts of the brown dwarf and planet mass parameter space....
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Exomoon signal in the Kepler 1513 system might be caused by a second exoplanet
icon5. 10. 2023 (accepted)
iconStars | Exoplanets | Kepler | Exomoo
Image: Exomoon signal in the Kepler 1513 system might be caused by a second exoplanet
Exoplanet Kepler 1513 b was discovered in 2016. Observed transit timing variations were thought to be originating in planet-moon interaction. New observations show that better explanation for the variations is an existence of a second, non-transiting planet in the system....
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Stellar companions can affect planet formation
icon5. 10. 2023 (accepted)
iconStar
Image: Stellar companions can affect planet formation
Study of 66 stars with planets and planet candidates found that those with stellar companions have more false positive planet detections and shorter orbital periods for their planets. This suggests that stellar companions can truncate planet-forming disks and affect planet formation....
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JWST found heavy elements in atmosphere of exoplanet HD 209458 b
icon5. 10. 2023 (accepted)
iconStar
Image: JWST found heavy elements in atmosphere of exoplanet HD 209458 b
JWST has observed the atmosphere of HD 209458b, a hot Jupiter exoplanet. The observations reveal that the planet has a super-solar metallicity and a very low C/O ratio, suggesting that it has undergone significant contamination by evaporating planetesimals while migrating inward....
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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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