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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.
First detection of a distinct silicate clouds on the day side of hot Jupiter
icon18. 9. 2024
iconЗвезды | Экзопланеты
Image: First detection of a distinct silicate clouds on the day side of hot Jupiter
James Webb detected quartz in the atmosphere of exoplanet HD 189733 b. Hot Jupiter HD 189733 b orbits a nearby star HD 189733 that is smaller than the Sun and lies only 64 light years away. The planet orbits close to the star with period only 2.2 days. The temperature in its atmosphere rises to scorching 1000 °C....
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Simulations suggest that rare Neptune-like planets orbiting close to their stars can form through a series of collisions between smaller planets
icon15. 9. 2024
iconЗвезды | Экзопланеты
Image: Simulations suggest that rare Neptune-like planets orbiting close to their stars can form through a series of collisions between smaller planets
This process could explain the existence of LHS 3154 b....
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New analysis of planets orbiting in habitable zones of small stars estimates minimum planetary magnetic field to protect their atmospheres
icon15. 9. 2024
iconЗвезды | Экзопланеты
Image: New analysis of planets orbiting in habitable zones of small stars estimates minimum planetary magnetic field to protect their atmospheres
Exoplanets Kepler 186 f and TOI 700 d might have magnetic fields sufficiently strong to protect their atmospheres and surfaces from stellar magnetic fields....
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Three Jupiter-like planets confirmed orbiting close to Sun-like stars
icon13. 9. 2024
iconЗвезды | Экзопланеты
Image: Three Jupiter-like planets confirmed orbiting close to Sun-like stars
One of the stars, TOI-4914 b, is more inflated than what is supported by current theoretical models. Warm Jupiter TOI 4914 b has about 70 % of Jupiter's mass, but its radius is 15 % bigger. That gives it about half of Jupiter's density....
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Second planet discovered in the young system TOI 4562 via timing variations in transits of the first planet
icon12. 9. 2024
iconЗвезды | Экзопланеты | TESS | Kepler
Image: Second planet discovered in the young system TOI 4562 via timing variations in transits of the first planet
This newly found exoplanet TOI 4562 c has the longest orbital period of any planet discovered via transit timing variations....
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Super-puff exoplanet Kepler 51 d is rotating surprisingly slowly
icon11. 9. 2024
iconЗвезды | Экзопланеты
Image: Super-puff exoplanet Kepler 51 d is rotating surprisingly slowly
More than 40-hour day could mean that the planet has a very thick atmosphere or a ring system...
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ALMA observations measure sulfur isotope ratios in a planet-forming disk around young star Oph-IRS 48
icon9. 9. 2024
iconЗвезды | Экзопланеты
Image: ALMA observations measure sulfur isotope ratios in a planet-forming disk around young star Oph-IRS 48
The results suggest that sulfur in this disk may have a different isotopic composition than in our solar system....
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Rare planet discovered orbiting near the Neptunian desert of a star TOI-3568
icon6. 9. 2024
iconЗвезды | Экзопланеты
Image: Rare planet discovered orbiting near the Neptunian desert of a star TOI-3568
It is a hot planet, bigger than Neptune with one of the highest luminosities in extreme ultraviolet for planets of this size. TOI-3568 b is 50% heavier than Neptune and its radius is 40% bigger. With an orbit lasting 4.4 days, it sits just outside the Neptunian desert, where the star evaporates the atmospheres of planets smaller than Jupiter and where only a few planets of this size have been found....
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A low-density gas giant exoplanet discovered orbiting a high-metallicity red dwarf star TOI-5688 A
icon4. 9. 2024
iconЗвезды | Экзопланеты | TESS
Image: A low-density gas giant exoplanet discovered orbiting a high-metallicity red dwarf star TOI-5688 A
TOI-5688 is a binary star almost 750 light years away from the Sun. The newly discovered planet orbits the primary star every 2.9 days and has radius 10 times bigger than Earth which is similar to Saturn....
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James Webb observations of the nearby rocky exoplanet Gliese 486 b suggest it has no thick atmosphere
icon28. 8. 2024
iconЗвезды | Экзопланеты
Image: James Webb observations of the nearby rocky exoplanet Gliese 486 b suggest it has no thick atmosphere
This is the most precise measurement yet of terrestrial exoplanet's thermal emission with JWST. Gliese 486 is a red dwarf only 26 light years from the Sun. The exoplanet Gliese 486 b orbits the star once every 36 hours. It is bigger, denser and hotter than Earth....
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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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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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