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Stellar Brief: 19. 10. 2026
The cold brown dwarf WISE 0855 has weather that looks strikingly planet-like: James Webb observations reveal patchy water clouds and changing atmospheric gases, including carbon monoxide and phosphine. Read today's Stellar Brief

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Latest astronomy Новости

Infant planet TOI-837 b shows a mildly misaligned orbit around its star
icon20. 6. 2026
iconЗвезды | Экзопланеты
Image: Infant planet TOI-837 b shows a mildly misaligned orbit around its star
TOI-837 b is a young, Saturn-sized planet located in the IC 2602 cluster, which is only 35 million years old. By studying the spin-orbit obliquity—the angle between the axis of the planet's orbit and the axis of the host star's rotation—researchers can determine how planets migrated to their current positions. This planet is the first younger than 100 million years observed to have a measurable misalignment, providing a rare look at planetary evolution. The planet was observed during transit ...
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Thick carbon dioxide atmosphere confirmed for exoplanet 55 Cancri e
icon20. 6. 2026
iconЗвезды | Экзопланеты
Image: Thick carbon dioxide atmosphere confirmed for exoplanet 55 Cancri e
The exoplanet 55 Cancri e is a hot, rocky world with a complex atmosphere that has been the subject of recent study. New research using advanced three-dimensional climate models shows that the planet likely possesses a thick, carbon dioxide-rich atmosphere. This conclusion relies on simulations that account for heat distribution across the planet, providing a more detailed look than previous one-dimensional models allowed. The findings indicat...
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Statistical analysis confirms TOI-7701 b as a sub-Saturn planet orbiting a subgiant star
icon20. 6. 2026
iconЭкзопланеты | Звезды
Image: Statistical analysis confirms TOI-7701 b as a sub-Saturn planet orbiting a subgiant star
TOI-7701 b (TOI-7701.01) is a transiting object orbiting a bright F-type subgiant star. Initially identified as a candidate in a machine-learning survey, its true nature as a planet had remained uncertain until now. New statistical analysis has confirmed this object as a sub-Saturn, placing it at the critical boundary between giant planets and low-mass brown dwarfs, which are objects larger than planets but smaller than stars. The confirmation...
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Carbon isotope ratio measured in the atmosphere of planet Beta Pictoris b
icon19. 6. 2026
iconЗвезды | Экзопланеты | Атмосферы планет
Image: Carbon isotope ratio measured in the atmosphere of planet Beta Pictoris b
Beta Pictoris b is a young, giant planet located in a star system where astronomers can directly image its atmosphere. By studying the specific chemical makeup of this world, researchers can learn how it formed and how its composition compares to the raw materials found in the gas cloud that birthed the system. This study provides a detailed chemical profile of the planet, focusing on carbon isotopes and its overall atmospheric makeup. The pla...
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Atmosphere of the rocky exoplanet Gliese 486 b studied with infrared observations
icon17. 6. 2026
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Image: Atmosphere of the rocky exoplanet Gliese 486 b studied with infrared observations
Gliese 486 b is a rocky exoplanet orbiting a Red dwarf star at a distance of about 26 light-years from the Solar System. Because it orbits very close to its host star, the planet is extremely hot, with surface temperatures reaching approximately 700 Kelvin. Observations from the James Webb Space Telescope were used to examine the light from the star as the planet passed in front of it to search for an atmosphere. The research indicates that th...
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Transit depth variations in young multi-planetary system HIP 67522 reveal stellar surface activity
icon17. 6. 2026
iconЗвезды | Экзопланеты
Image: Transit depth variations in young multi-planetary system HIP 67522 reveal stellar surface activity
The HIP 67522 system, at approximately 17 million years old, is one of the youngest multi-planetary systems ever observed. This Sun-like star, located within the Scorpius-Centaurus OB association, hosts two Saturn-sized planets locked in a near 2:1 orbital resonance, meaning that for every orbit the outer planet completes, the inner planet completes roughly two. Scientists have conducted an analysis of photometric transit data—where the dimming o...
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Three massive planets discovered orbiting distant low luminosity red giant stars
icon12. 6. 2026
iconЗвезды | Экзопланеты
Image: Three massive planets discovered orbiting distant low luminosity red giant stars
Researchers have identified three massive planets orbiting two low luminosity red giant stars, marking a significant addition to our understanding of planetary systems around evolved stars. These stars, which have expanded and cooled after exhausting the hydrogen fuel in their cores, are a unique environment for planet formation and survival. The study, part of a long-term campaign using the CORALIE spectrograph, focused on observing changes in t...
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Two young giant planets discovered with the longest orbital periods for their class
icon6. 6. 2026
iconЗвезды | Экзопланеты
Image: Two young giant planets discovered with the longest orbital periods for their class
Astronomers have identified two young, large-radius planets orbiting the F-type star HD 114082, marking them as the longest-period young transiting exoplanets currently known. These planets, designated b and c, were detected through a collaborative effort using data from multiple space and ground-based telescopes, including TESS, the Next-Generation Transit Survey (NGTS), the Characterising Exoplanet Satellite (CHEOPS), and the Antarctic Search f...
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Three newly discovered hot Jupiters provide insights into late-stage planetary evolution
icon6. 6. 2026
iconЗвезды | Экзопланеты | TESS | Горячий юпитер | Солнцеподобные звёзды
Image: Three newly discovered hot Jupiters provide insights into late-stage planetary evolution
Understanding how giant planets evolve is essential for building a complete picture of planetary systems. While many exoplanets have been found, studying their changes over time requires observing systems in different stages of development. A recent discovery has added three new gas giant planets — known as hot Jupiters — orbiting stars that are approaching the end of their main sequence, a critical but less studied phase of planetary life. Th...
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UV radiation from host stars complicates search for life on TRAPPIST-1 e
icon6. 6. 2026
iconЗвезды | Экзопланеты | Атмосферы планет | Красные карлики
Image: UV radiation from host stars complicates search for life on TRAPPIST-1 e
The search for life on distant planets often relies on identifying biosignatures — gases like oxygen or methane that are produced by biological processes. However, a new study highlights how the specific ultraviolet (UV) radiation from a host star can significantly influence a planet's atmospheric chemistry, potentially creating false-positive signals that might be mistaken for life. The research focused on the planet TRAPPIST-1 e, which orbits a...
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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
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
TOI-4468 b 08 / 2026 170.1 M⊕ 1233.1 ly
TOI-4468 d 08 / 2026 311 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.

HD 112485
5881 ly
study icon Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission
yesterday

HD 100546
359 ly
study icon An ALMA view on molecular complexity: water, methanol, and methyl formate in the HD 100546 and IRS 48 disks
yesterday

HD 120678
5829 ly
study icon HD 120678: a classical Be star with a tilting heartbeat disk
18. 10. 2026

33 G. Librae
19.2 ly
+1 study icon EPRV Asteroseismology of the K dwarfs GJ 570 A and GJ 783 A with ESPRESSO. Empirical mode-amplitude scaling in tension with 3D convection simulations
18. 10. 2026

WISE 0855-0714
7.3 ly
study icon Water Cloud and Chemical Modulations in the Coldest Brown Dwarf
17. 10. 2026

TOI-5322
1560 ly
+1 study icon A Sample of Thick-Disk Stars Hosting Hot Jupiters
17. 10. 2026

WD J1330+6435
282 ly
study icon Any colour you like: the diverse chromaticities of white dwarfs
17. 10. 2026

WASP-33
378 ly
study icon Identifying deformed exoplanets with JWST and Ariel: A target selection metric for phase curve observations
16. 10. 2026

WASP 94
687 ly
study icon A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum
16. 10. 2026

TOI-3118
1410 ly
study icon A Sample of Thick-Disk Stars Hosting Hot Jupiters
16. 10. 2026
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