Stellar Brief: 22. 10. 2026
A young, planet-hosting star called V1298 Tauri is showing how fiercely active infant planetary systems can be: radio emissions appeared in 90 percent of monitoring visits, while its X-ray brightness also changed and showed a stellar flare.
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Latest astronomy noticias
13. 3. 2025
Estrellas | ExoplaneBarnard's Star is now one of the most compact low-mass planetary systems known. Barnard's Star is a small red dwarf only 6 light years away from the Solar System. One confirmed planet and two candidates orbiting the star were already known. New observations now confirm the three objects and add a new one....
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5. 3. 2025
Estrellas | ExoplaneIt’s one of the coolest directly imaged exoplanets ever, with hints of exotic chemistry in its atmosphere. ...
25. 2. 2025
Estrellas | ExoplaneIt’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....
24. 2. 2025
EstreCE 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. ...
20. 2. 2025
Estrellas | Enanas marroneThese 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....
2. 2. 2025
Estrellas | ExoplaneNo strong atmospheric signals were detected, suggesting high metallicity and hazes that obscure spectral features....
31. 1. 2025
Estrellas | ExoplaneThese findings contradict claims of a liquid water ocean or life signs. The planet is likely an oxygen-poor sub-Neptune....
23. 1. 2025
Estrellas | Estrellas masivas de la secuencia princiIts circular polarization suggests persistent auroral activity via electron cyclotron maser emission...
14. 1. 2025
EstreTheir movement suggests mixed origins - in galactic disk and halo....
10. 1. 2025
Estrellas | ExoplaneWhen 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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Exoplanetas recién descubiertos
| 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 | |
| L 115-21 b | 10 / 2026 | 0.4 M⊕ | 41.9 ly | |
| TIC 219893931 b | 09 / 2026 | 8.9 M⊕ | 1319.5 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 |
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