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24. 10. 2026
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A planet’s helium atmosphere streams ahead of its orbit, while infrared observations reveal the hidden rhythms of its star. New work also shows how neutron-star tilt can reshape X-ray light, traces the past of massive blue supergiants, and maps cloudy and clear zones on the hot Jupiter WASP-43 b.
Fourth planetary system with nodal precession identified. TOI 1518 b grazes the disk of its parent star
icon27. 2. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Fourth planetary system with nodal precession identified. TOI 1518 b grazes the disk of its parent star
The planets orbit is not perfectly aligned with the stars equator, but tilted at a sharp angle. This tilt, combined with the stars rapid rotation, causes the planets trajectory to slowly wobble over time, a phenomenon called nodal precession....
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Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
icon6. 2. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
The first planet TOI 238 b is a super-Earth with 1.4 Earth radii and was discovered just last year. Newly discovered TOI 238 c with 2.2 radii could be a water-rich world....
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New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
icon22. 1. 2024 (Принял)
iconЗвезды
Image: New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
The planet has a radius of 1.24 Earth radii, a mass of 2.53 Earth masses, and an equilibrium temperature of 996 degrees Kelvin. It is likely composed of a large iron core, a small rocky mantle, and a negligible atmosphere....
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How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
icon29. 11. 2023 (Принял)
iconЗвезды | Экзопланеты
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 (Принял)
iconЗвезды | Экзопланеты
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 (Принял)
iconЗвезды | Экзопланеты
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 (Принял)
iconЗвезды | Экзопланеты
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 (Принял)
iconЗвезды | Экзопланеты | Атмосферы планет
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 (Принял)
iconЗвезды | Экзопланеты
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 (Принял)
iconЗвезды | Экзопланеты | 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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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

Просмотрите последние научные исследования звезд и экзопланет в нашей галактике. Откройте для себя новейшие исследования в области астрофизики и звездной астрономии.

Circinus X-1
31000 ly
study icon Breaking the symmetry: X-ray polarization from a spreading layer on a tilted weakly magnetized neutron star
yesterday

HD 74371
5445 ly
+5 study icon Photometric variability of blue supergiants: Constraints on stellar masses and evolutionary stages
yesterday

WASP 121
858 ly
study icon Detection of Solar-like Oscillations and Granulation at Infrared Wavelengths using JWST
23. 10. 2026

WASP-43
284 ly
study icon The coupled impacts of atmospheric dynamics and cloud microphysics on hot Jupiter atmospheres. I. An application to WASP-43b
23. 10. 2026

TOI 3884
141 ly
study icon A Headwind-like Helium Outflow from TOI-3884b
23. 10. 2026

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
22. 10. 2026

TYC 5709-354-1
437 ly
study icon Predictions for an unseen third planet in the WISPIT 2 system
22. 10. 2026

TIC 220432308
1129 ly
+1 study icon Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields
21. 10. 2026

TOI 431
106 ly
+4 study icon Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey
21. 10. 2026

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)
21. 10. 2026
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