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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.
Exoplanet hidden in DM Tauri disc might be less massive than previously thought
icon5. 6. 2024
iconЗвезды | Экзопланеты
Image: Exoplanet hidden in DM Tauri disc might be less massive than previously thought
Magnetized winds play a crucial role in shaping the disc and its interaction with the planet. DM Tauri is a young forming star 470 light years away. It still has an accretion disc in which there is an exoplanet with mass around 53 Earths....
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By analyzing images taken years ago astronomers successfully revealed the presence of a giant exoplanet AF Leporis b
icon5. 6. 2024
iconЗвезды | Экзопланеты
Image: By analyzing images taken years ago astronomers successfully revealed the presence of a giant exoplanet AF Leporis b
A new machine learning method used to better separate the faint planet signal from the noisy starlight in images....
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icon3. 6. 2024
iconЗвезды | Экзопланеты
Image:
Exoplanet HIP 41378 d was previously observed transiting its star twice, three years apart. Astronomers now aimed the CHEOPS telescope for another observation, but surprisingly, no transit was detected...
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New warm-Neptune TOI 5076 b confirmed with a mass about 16 times Earth's and a radius slightly over 3 times Earth's
icon30. 5. 2024
iconЗвезды | Экзопланеты | TESS
Image: New warm-Neptune TOI 5076 b confirmed with a mass about 16 times Earth
Its density suggests a significant amount of volatile materials surrounding a rocky core....
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Tiny wobbles of a bright star HD 73344 have revealed the mass of a nearby sub-Neptune exoplanet
icon27. 5. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Tiny wobbles of a bright star HD 73344 have revealed the mass of a nearby sub-Neptune exoplanet
Additionally, another signal hints at the presence of a previously undetected planet orbiting farther from the star. HD 73344 is an F-type star approximately 115 light-years away. At roughly 20% larger than our Sun, it hosts a sub-Neptune exoplanet with a density similar to Saturns. The possible second planet has been detected with a minimum mass around one-third that of Jupiter...
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A mini-Neptune discovered in the habitable zone of star TOI 4633
icon29. 4. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: A mini-Neptune discovered in the habitable zone of star TOI 4633
Also another non-transiting planet candidate lurks closer to the star...
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The famous planet thought to orbit 40 Eridani A does not exist. Its signal can be explained with stellar activity
icon26. 4. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: The famous planet thought to orbit 40 Eridani A does not exist. Its signal can be explained with stellar activity
In the Star Trek universe the planet Vulcan (also NiVar) orbits one of the three stars in 40 Eridani system that lies 40 light years from the Sun....
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Planet confirmed orbiting one of three red dwarfs in the nearby system TOI 4336
icon19. 4. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Planet confirmed orbiting one of three red dwarfs in the nearby system TOI 4336
It is bigger than Earth and orbits near the habitable zone of its star....
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Tidal pull from close orbiting giant planet creates turbulence within the WASP-18
icon10. 4. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Tidal pull from close orbiting giant planet creates turbulence within the WASP-18
This turbulence might suppress the formation of sunspots, explaining the low stellar activity....
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Observations suggest the atmosphere of HAT-P-67 b might be evaporating due to a detected helium signal
icon4. 4. 2024 (Принял)
iconЗвезды | Экзопланеты
Image: Observations suggest the atmosphere of HAT-P-67 b might be evaporating due to a detected helium signal
HAT-P-67 b is one of the lowest-density gas giants....
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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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