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.
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Latest astronomy zprávy
29. 11. 2023 (přijato)
Hvězdy | ExoplanetyTRAPPIST-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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27. 11. 2023 (přijato)
Hvězdy | ExoplanetyWASP-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...
27. 11. 2023 (přijato)
Hvězdy | ExoplanetyThe exoplanet joins a growing census of aligned warm Jupiters around single stars....
22. 11. 2023 (přijato)
Hvězdy | ExoplanetyHD 88986 b has the longest orbital period among known transiting planets with known mass and less than 4 Earth radii....
21. 11. 2023 (přijato)
Hvězdy | Exoplanety | Atmosféry planeThis is the first time these has been detected on a planet with a temperature below 1000 K...
21. 11. 2023 (přijato)
Hvězdy | ExoplanetyThe primary star is known to have 2 rocky exoplanets near radius valley which separates super-Earths and sub-Neptunes...
20. 11. 2023 (přijato)
Hvězdy | Exoplanety | TESSIts high eccentricity may be the result of past violent scattering events
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15. 11. 2023 (přijato)
Hvězdy | Exoplanety | KeplerGas 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...
25. 10. 2023 (přijato)
Hvězdy | ExoplanetyResearchers 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...
25. 10. 2023 (přijato)
HvězdyHD 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 |
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