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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.
Magnetic activity cycles found in exoplanet-hosting red dwarf stars Gliese 617 A and Lalande 21185
icon5. 3. 2026
iconЗвезды | Экзопланеты | Красные карлики
Image: Magnetic activity cycles found in exoplanet-hosting red dwarf stars Gliese 617 A and Lalande 21185
M dwarf stars are small, cool stars that are popular targets for finding exoplanets because their size makes it easier to detect planets in their habitable zones. However, these stars often have magnetic activity that can mimic the signals of planets, making it important to understand their activity cycles. This study focused on two M dwarfs, Gliese 617 A and Lalande 21185 (Gliese 411), both known to host exoplanets. Researchers analyzed 13 years of high-resolution spectra from the SOPHIE spe...
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Vertical structure of the Beta Pictoris debris disk revealed across multiple wavelengths
icon5. 3. 2026
iconЗвезды | Формирование планет | Экзопланеты | Массивные звезды главной последовательности
Image: Vertical structure of the Beta Pictoris debris disk revealed across multiple wavelengths
β Pictoris is a well-known star surrounded by a disk of dust and debris, making it a prime example for studying how planetary systems evolve. By observing this disk at different wavelengths, scientists can learn about the structure and behavior of the material around the star. This study focused on measuring the vertical height of the disk using images from mid-infrared to millimeter wavelengths. Researchers used advanced modeling to analyze t...
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Methanol search in the water-rich planet-forming disk around HL Tauri
icon5. 3. 2026
iconЗвезды | Экзопланеты | Формирование планет | Молодые звездные объекты | Планеты-океаны
Image: Methanol search in the water-rich planet-forming disk around HL Tauri
HL Tauri is a young star surrounded by a disk of gas and dust where planets are forming. Scientists are interested in finding complex molecules like methanol in such disks because these molecules are important for the chemistry that could lead to life. Methanol is often found around other young stars, but its presence in planet-forming disks is rare. In this study, researchers looked for methanol in the disk around HL Tauri, motivated by the d...
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Volcanic activity and mantle dynamics shape the lava world K2-141 b
icon4. 3. 2026
iconЗвезды | Экзопланеты | Лавовые планеты
Image: Volcanic activity and mantle dynamics shape the lava world K2-141 b
K2-141 b is an ultra-short period planet, known as a lava world, that orbits very close to its star. This extreme environment causes one side of the planet to be extremely hot, covered by a magma ocean, while the other side remains much cooler and solid. Scientists used computer models to study how the planet's interior moves and how this affects volcanic activity, especially on the nightside, which is not directly heated by the star. The rese...
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The four planets in the TOI 2076 system reveal early atmospheric loss and fragile orbits
icon4. 3. 2026
iconЗвезды | Экзопланеты | Атмосферы планет
Image: The four planets in the TOI 2076 system reveal early atmospheric loss and fragile orbits
TOI-2076 is a young star system, about 200 million years old, that hosts four planets slightly larger than Earth. These planets, called sub-Neptunes, orbit close to their star and offer a unique look at how planetary systems change in their early stages. Unlike many young systems where planets are locked in precise orbital patterns called resonances, the planets in TOI-2076 are near but not exactly in resonance, making their arrangement less stab...
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JWST reveals planetary dynamics and possible hidden companion in TWA 7 system
icon4. 3. 2026
iconЭкзопланеты | Молодые звездные объекты | Формирование планет | Звезды | Космический телескоп имени Джеймса Уэбба
Image: JWST reveals planetary dynamics and possible hidden companion in TWA 7 system
TWA 7 is a young star surrounded by a debris disk, which is a ring of dust and small objects left over from planet formation. Recent observations with the JWST telescope have directly imaged a planet far from the star and revealed detailed features in the disk, such as a sharply defined inner edge and an unusual horseshoe-shaped structure. These features suggest that the system's planets are shaping the disk in complex ways. Researchers used c...
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TOI-1080 b: a small rocky planet around a quiet M4V star is validated for detailed study
icon3. 3. 2026
iconЗвезды | Экзопланеты | TESS | Красные карлики
Image: TOI-1080 b: a small rocky planet around a quiet M4V star is validated for detailed study
Researchers have detected and validated TOI-1080 b (SIPS J1825-5212 b), a small, temperate exoplanet that transits its quiet M4V host star every 3.97 days. The host star is located 25.6 parsecs away. The planet was first identified by the TESS mission and confirmed with both TESS and ground-based observations. Analysis of the light curves shows that TOI-1080 b has a radius of about 1.2 times that of Earth and an equilibrium temperature of 36...
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Ground-based spectroscopy reveals hydrogen sulfide in the atmosphere of super-Earth L 98-59 d
icon3. 3. 2026
iconЗвезды | Экзопланеты | Суперземля | Атмосферы планет
Image: Ground-based spectroscopy reveals hydrogen sulfide in the atmosphere of super-Earth L 98-59 d
Scientists have used high-resolution transmission spectroscopy from the Gemini-South telescope to study the atmosphere of the temperate super-Earth exoplanet L 98-59 d. This approach, typically used for larger and hotter planets, was successfully applied to a smaller, more temperate world, demonstrating the capability of ground-based facilities to characterize super-Earth atmospheres. The team confirmed the presence of hydrogen sulfide (H2S) i...
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TESS survey shows the radius valley vanishes for planets around mid-to-late M dwarfs
icon2. 3. 2026
iconЗвезды | Экзопланеты | TESS | Красные карлики
Image: TESS survey shows the radius valley vanishes for planets around mid-to-late M dwarfs
Researchers conducted the most comprehensive search for planets around mid-to-late M dwarf stars using data from the TESS mission. Surveying over 8,000 such stars, they identified 77 transiting planet candidates and measured how often planets occur as a function of their size, orbital period, and the amount of starlight they receive. The study found that each mid-to-late M dwarf hosts on average about 1.1 planets larger than Earth within 30 ...
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JWST reveals clues to the atmosphere of Jupiter-analog exoplanet epsilon Eridani b
icon2. 3. 2026
iconЗвезды | Экзопланеты | Атмосферы планет | Космический телескоп имени Джеймса Уэбба

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
today

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

WASP 121
858 ly
study icon Detection of Solar-like Oscillations and Granulation at Infrared Wavelengths using JWST
yesterday

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
yesterday

TOI 3884
141 ly
study icon A Headwind-like Helium Outflow from TOI-3884b
yesterday

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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