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Stellar Brief: 20. 10. 2026
The planet-forming disk around HD 100546 contains an unexpectedly high amount of methyl formate: ALMA measured a methyl-formate-to-methanol ratio of about 2, hinting that active chemistry is reshaping the ingredients from which planets form. Read today's Stellar Brief

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Latest astronomy zprávy

How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
icon29. 11. 2023 (přijato)
iconHvězdy | Exoplanety
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 (přijato)
iconHvězdy | Exoplanety
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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New study makes TOI-1670 c one of the longest-period planets to date to have its obliquity angle measured
icon27. 11. 2023 (přijato)
iconHvězdy | Exoplanety
Image: New study makes TOI-1670 c one of the longest-period planets to date to have its obliquity angle measured
The exoplanet joins a growing census of aligned warm Jupiters around single stars....
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Cold sub-Neptune planet discovered orbiting nearby star HD 88986
icon22. 11. 2023 (přijato)
iconHvězdy | Exoplanety
Image: Cold sub-Neptune planet discovered orbiting nearby star HD 88986
HD 88986 b has the longest orbital period among known transiting planets with known mass and less than 4 Earth radii....
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Sulfur dioxide and silicate clouds discovered in the atmosphere of the warm Neptune WASP-107 b
icon21. 11. 2023 (přijato)
iconHvězdy | Exoplanety | Atmosféry plane
Image: Sulfur dioxide and silicate clouds discovered in the atmosphere of the warm Neptune WASP-107 b
This is the first time these has been detected on a planet with a temperature below 1000 K...
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New study of nearby binary star LTT 3780 reveals clues to the formation of planets around red dwarfs
icon21. 11. 2023 (přijato)
iconHvězdy | Exoplanety
Image: New study of nearby binary star LTT 3780 reveals clues to the formation of planets around red dwarfs
The primary star is known to have 2 rocky exoplanets near radius valley which separates super-Earths and sub-Neptunes...
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Warm Jupiter with an orbital period of 15.27 days discovered orbiting a Sun-like star TOI 4515
icon20. 11. 2023 (přijato)
iconHvězdy | Exoplanety | TESS
Image: Warm Jupiter with an orbital period of 15.27 days discovered orbiting a Sun-like star TOI 4515
Its high eccentricity may be the result of past violent scattering events ...
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icon15. 11. 2023 (přijato)
iconHvězdy | Exoplanety | Kepler
Image:
Gas giant Kepler-1658 b is slowly spiraling inward due to tidal interactions with its host star. The observed rate of orbital decay cannot be explained by tidal dissipation in the star alone, but it can be explained if the planet rotates non-synchronously...
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AU Microscopii has at least two spectral components: a 4000 K ambient photosphere and cool spots that have a temperature of 3000 K
icon25. 10. 2023 (přijato)
iconHvězdy | Exoplanety
Image: AU Microscopii has at least two spectral components: a 4000 K ambient photosphere and cool spots that have a temperature of 3000 K
Researchers have used ground-based photometry and spectra to study the unocculted starspots on the young star AU Mic. They find that AU Mic has at least two spectral components: a 4000 K ambient photosphere and cool spots that have a temperature of 3000 K and cover 39% of the surface. They also detect a third flux component, which they attribute to flare flux. This study will help us better understand the starspot coverage on AU Mic and other sta...
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A new study has discovered an inner ring in the disk in young binary system HD 34700
icon25. 10. 2023 (přijato)
iconHvězdy
Image: A new study has discovered an inner ring in the disk in young binary system HD 34700
HD 34700 is a young binary system with a complex protoplanetary disk. A new study has discovered an inner ring in the disk, as well as extended logarithmic spiral arms and misaligned gas rotation patterns. These features suggest that the disk is being shaped by one or more physical mechanisms, such as the presence of an undetected planet or interaction with the surroundings. Further observations are needed to confirm these scenarios....
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Nově objevené exoplanety

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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