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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. Read today's Stellar Brief

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Latest astronomy Новости

Low density super earth TOI-2211 b characterized as a potential hot water world
icon9. 10. 2026
iconЗвезды | Экзопланеты | Оранжевый карлик | TESS | CHEOPS | Суперземля
Image: Low density super earth TOI-2211 b characterized as a potential hot water world
Researchers have performed a detailed characterization of the exoplanet TOI-2211 b, a super-Earth orbiting an orange dwarf star. By combining data from multiple telescopes, the study identified the planet as a promising candidate for a hot water world. Additionally, the team detected a second, non-transiting planetary candidate within the same system, providing new insights into the architecture of this distant star system....
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Orbital alignment of the hot Neptune planet orbiting WASP-195 confirmed
icon8. 10. 2026
iconЗвезды | Экзопланеты
Image: Orbital alignment of the hot Neptune planet orbiting WASP-195 confirmed
Researchers have measured the orbital alignment of a Neptune-mass planet around the hot star WASP-195. By observing the Rossiter-McLaughlin effect, the study confirms that the planet maintains a spin-orbit alignment, providing insight into the migration history of this specific planetary system and helping to fill a data gap regarding smaller planets orbiting stars hotter than the sun....
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Warm Jupiter HD 715 b orbits a massive subgiant star
icon7. 10. 2026
iconЗвезды | Экзопланеты | TESS | Субгиганты
Image: Warm Jupiter HD 715 b orbits a massive subgiant star
A new warm Jupiter named HD 715 b has been confirmed orbiting the bright subgiant star HD 715. Identified initially through a single transit event captured by the TESS mission, follow-up observations have revealed the planet's orbital characteristics. This system is particularly notable because the host star is among the most massive known to harbor a transiting warm Jupiter, providing new data on orbital diversity....
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Leave-one-out cross-validation provides clarity in radial velocity measurements of exoplanetary systems
icon7. 10. 2026
iconЗвезды | Экзопланеты | Солнцеподобные звёзды
Image: Leave-one-out cross-validation provides clarity in radial velocity measurements of exoplanetary systems
Advanced statistical methods help clarify planetary signals hidden within precise radial velocity data. By systematically testing how individual measurements influence a model, researchers have refined the mass estimate of HD 119130 b, clarified the orbital architecture of the Gliese 4276 system, and confirmed the three-planet structure orbiting Gliese 357 by testing for predictive consistency....
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Oxygen signatures in the rock vapor outflow of planet BD+05 4868 b
icon6. 10. 2026
iconЗвезды | Экзопланеты | Оранжевый карлик
Image: Oxygen signatures in the rock vapor outflow of planet BD+05 4868 b
Observations of the disintegrating rocky planet BD+05 4868 b reveal potential signatures of oxygen escaping from its surface. By analyzing the planet during transit, the recorded data suggest the presence of a mineral-vapor outflow. This finding provides insights into how intensely irradiated rocky worlds lose their material through evaporation processes....
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Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
icon6. 10. 2026
iconЗвезды | Экзопланеты | Красные карлики | Космический телескоп имени Джеймса Уэбба | Атмосферы планет | Планеты-океаны
Image: Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
Researchers have analyzed the atmospheres of eight sub-Neptune planets orbiting Red dwarf stars using the James Webb Space Telescope. By studying the mean molecular weight of their gaseous envelopes, the team identified a new category of intermediate planets, dubbed hybrid worlds, which do not fit the traditional definitions of simple gas-enveloped rocks or water-rich worlds formed in the outer solar system....
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Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
icon6. 10. 2026
iconЗвезды | Экзопланеты | Молодые звездные объекты
Image: Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
Observations of the protoplanetary disc surrounding the star HD 139614 reveal complex light patterns caused by an inclined planet. By analyzing scattered-light images, researchers identified shifting brightness in the inner ring and a distinct spiral structure. A physical model suggests that a tilted planet forces inner parts of the disc to warp and precess, casting long-lasting shadows across the outer regions....
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Magnetic field analysis of the ultra hot Jupiter KELT-9 b
icon6. 10. 2026
iconЗвезды | Экзопланеты | | Горячий юпитер
Image: Magnetic field analysis of the ultra hot Jupiter KELT-9 b
Magnetic fields play a vital role in shaping the atmospheres of planets, yet measuring them around close-in worlds remains difficult. A recent analysis of the ultra-hot Jupiter KELT-9 b sought to detect a magnetic field using the Zeeman effect in atomic lines. While a marginal signal was observed in 2025, subsequent observations failed to replicate the result, leaving the presence of the field unconfirmed....
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Twenty-nine giant planets confirmed around bright stars using TESS data
icon5. 10. 2026
iconЗвезды | Экзопланеты | TESS | Гиганты
Image: Twenty-nine giant planets confirmed around bright stars using TESS data
A large-scale analysis of TESS mission data has confirmed 29 new hot and warm Jupiter-sized planets orbiting bright stars. By using space-based transits and ground-based observations, the study provides a consistent dataset of these massive worlds, revealing new details about their orbits, masses, and stellar environments, including the identification of three new bound stellar companions in these systems....
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Astrometric data reveals 29 distant giant planet candidates in known planetary systems
icon5. 10. 2026
iconЗвезды | Экзопланеты | Гиганты
Image: Astrometric data reveals 29 distant giant planet candidates in known planetary systems
Researchers have identified 29 potential outer giant planets orbiting within existing exoplanetary systems by analyzing stellar motion data. By utilizing measurements from the Hipparcos and Gaia space missions, the team detected the subtle gravitational tugs these distant companions exert on their host stars, providing new targets for future observations to understand how these planets shape their systems....
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Недавно обнаруженные экзопланеты

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
Newly discovered exoplanets
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Latest scientific studies

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V1298 Tauri
352 ly
study icon Radio and high-energy variable emission from a multi-wavelength follow-up of the infant planet-hosting star V1298 Tau
today

TYC 5709-354-1
437 ly
study icon Predictions for an unseen third planet in the WISPIT 2 system
today

TIC 220432308
1129 ly
+1 study icon Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields
yesterday

TOI 431
106 ly
+4 study icon Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey
yesterday

L 115-21
41.9 ly
study icon A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274)
yesterday

TOI-3686
841 ly
study icon TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance
yesterday

TOI-270
73.3 ly
study icon Ammonia-Hydrogen Phase Equilibria in Planetary Envelopes from First-Principles-Based Machine-Learning Molecular Dynamics
yesterday

PDS 70
370 ly
study icon Kinematic structure and age of a Scorpius--Centaurus subcomponent: implications for PDS 70 planetary system
20. 10. 2026

TIC 402710280
218 ly
study icon A 36.34-day Sub-Neptune Candidate Transiting the Nearby K Dwarf TIC 402710280
20. 10. 2026

LTT 9779
264 ly
+1 study icon Granulation in Color: The Chromatic Stellar Flicker of LTT-9779 and WASP-121
20. 10. 2026
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