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24. 10. 2026
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A blue supergiant’s changing light reveals that it is moving back toward hotter temperatures after a red-supergiant phase. New findings also trace infrared ripples on WASP 121, map the uneven clouds of WASP-43 b, and reveal helium escaping ahead of TOI-3884 b. Meanwhile, observations of the young star V1298 Tauri show how magnetic activity can make a star brighten and fade across radio and X-ray light.
AU Mic’s young planets show aligned orbits, but stellar activity complicates measurements
icon30. 5. 2026
iconЗвезды | Экзопланеты
Image: AU Mic’s young planets show aligned orbits, but stellar activity complicates measurements
AU Mic is a young, nearby star with two Neptune-sized planets and a debris disk. Researchers observed back-to-back transits of both planets, AU Mic b and c, using multiple telescopes and measured their spin-orbit alignment with the Rossiter-McLaughlin effect. They confirmed that planet b’s orbit is well aligned with the star’s rotation, while planet c’s orbit is likely aligned but a polar orbit cannot be ruled out due to data limitations. The study found that stellar activity, especially duri...
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14 Herculis: Eccentric giants hint at an ejected massive planet
icon30. 5. 2026
iconЗвезды | Экзопланеты
Image: 14 Herculis: Eccentric giants hint at an ejected massive planet
The 14 Herculis system contains two super-Jupiter planets on eccentric, misaligned orbits—a configuration that is difficult to explain with standard planet formation models. Researchers used N-body simulations to study the system’s history and found that its current architecture can be reproduced if the system originally hosted additional massive planets that were later ejected through planet-planet scattering. The mass of the ejected planet help...
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HD 20794 d: a stable, eccentric planet crossing the habitable zone
icon27. 5. 2026
iconЗвезды | Экзопланеты | Oбитаемые экзопланеты
Image: HD 20794 d: a stable, eccentric planet crossing the habitable zone
This study analyzes the orbital dynamics and habitability of the HD 20794 planetary system, which contains three confirmed planets orbiting a nearby G-type star. Of particular interest is HD 20794 d, a terrestrial planet with a minimum mass of 5.82 Earth masses on a highly eccentric orbit that passes through the star’s habitable zone (HZ). The research calculates the HZ boundaries and determines how much time planet d spends within these limits. ...
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TRAPPIST-1 f, g, and h may have subsurface oceans and detectable cryovolcanic water vapor
icon27. 5. 2026
iconЗвезды | Экзопланеты
Image: TRAPPIST-1 f, g, and h may have subsurface oceans and detectable cryovolcanic water vapor
Scientists modeled the interiors and atmospheres of the exoplanets TRAPPIST-1f, g, and h to see if they could sustain subsurface oceans and produce detectable water vapor through cryovolcanism. Using simulations, they found that all three planets’ internal heat is mainly generated by radioactive decay and tidal forces. TRAPPIST-1f and g are likely to have thin outer ice shells and shallow subsurface oceans, while TRAPPIST-1h may have a thicker ic...
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AB Aurigae’s disk shows complex dynamics and accretion activity
icon27. 5. 2026
iconЗвезды | Экзопланеты
Image: AB Aurigae’s disk shows complex dynamics and accretion activity
Researchers observed the protoplanetary disk around the young star AB Aurigae using near-infrared polarized imaging and H-alpha observations over several years. Their study reveals that while most of the disk follows Keplerian rotation, the inner regions (within about 60 astronomical units) show significant deviations, including sub-Keplerian motion. Two bright spiral arms inside the disk’s millimeter cavity display different dynamic behaviors, p...
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WASP-156 b’s orbit is aligned, not polar, new data show
icon27. 5. 2026
iconЗвезды | Экзопланеты
Image: WASP-156 b’s orbit is aligned, not polar, new data show
WASP-156 b is a short-period exo-Neptune, a planet similar in size to Neptune but much closer to its star. Scientists studied the planet’s orbit using new high-precision spectroscopic and photometric observations. They measured the Rossiter-McLaughlin effect, which reveals the angle between the planet’s orbit and the star’s rotation. The results show that WASP-156 b’s orbit is well aligned with the star’s equator, with a projected obliquity of ab...
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Magnetic interactions found between Proxima Centauri and its planets
icon25. 5. 2026
iconЗвезды | Экзопланеты
Image: Magnetic interactions found between Proxima Centauri and its planets
Proxima Centauri, the closest star to the Sun, hosts at least two planets: Proxima b and Proxima d. Using high-resolution optical observations, astronomers searched for signs of magnetic interactions between the star and its planets. They measured the star’s rotation period as about 85 days and found that Proxima Centauri experiences frequent flares, with about 5 percent of the observing time showing flare activity. Statistical analysis revealed ...
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Eclipse mapping with SPIRou reveals first CO signal on WASP-33b’s dayside
icon25. 5. 2026
iconЗвезды | Экзопланеты | Горячий юпитер
Image: Eclipse mapping with SPIRou reveals first CO signal on WASP-33b’s dayside
WASP-33b is an ultra-hot Jupiter, a giant planet orbiting very close to its star. Scientists used high-resolution spectroscopy with the SPIRou instrument to observe eight eclipses of WASP-33b, focusing on the moments when the planet passes behind its star (ingress and egress). This technique, called eclipse mapping, can reveal details about the planet’s dayside atmosphere. The team analyzed the data using advanced software and combined it with pr...
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GJ 710’s rare close approach highlights stellar encounters near the Sun
icon22. 5. 2026
iconЗвезды
Image: GJ 710’s rare close approach highlights stellar encounters near the Sun
This study examines how often stars pass close to the Sun and puts the upcoming fly-by of GJ 710 into context. GJ 710 is expected to come within about 0.0621 parsecs (roughly 10,000 astronomical units) of the Solar System in about 1.3 million years, making it one of the closest known future encounters. The researchers analyzed the motions of nearby stars to identify both past and future close approaches within one parsec of the Sun. They correcte...
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Bright ancient star G256353 shows strong r-process element enrichment
icon22. 5. 2026
iconЗвезды
Image: Bright ancient star G256353 shows strong r-process element enrichment
Astronomers have studied four extremely metal-poor stars, which are among the oldest and most primitive in our galaxy. The main focus is on G256353, a star with a very low iron content and a strong enhancement of elements created by the rapid neutron-capture process, known as the r-process. Using high-resolution spectra from the GHOST instrument on Gemini South, the team measured the abundances of 15 neutron-capture elements in G256353. The patte...
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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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HD 74371
5445 ly
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

TOI-3686
841 ly
study icon TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance
21. 10. 2026
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