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29. 10. 2026
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Weighing potentially habitable planets around Sun-like stars remains surprisingly difficult: a methods test found that precise measurements often require planets weighing about 8 to 10 Earth masses. The latest reports also explore brilliant radio bursts from a rapidly spinning brown dwarf, a possible hotspot on another brown dwarf, and how transit changes can expose a planet that never crosses its star.

Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
icon6. 2. 2024 (accepted)
iconStars | Exoplane
Image: Second sub-Neptune exoplanet discovered around orange dwarf star TOI 238
The first planet TOI 238 b is a super-Earth with 1.4 Earth radii and was discovered just last year. Newly discovered TOI 238 c with 2.2 radii could be a water-rich world....
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New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
icon22. 1. 2024 (accepted)
iconStar
Image: New ultra-short-period exoplanet slightly bigger than Earth discovered orbiting the nearby star Wolf 327
The planet has a radius of 1.24 Earth radii, a mass of 2.53 Earth masses, and an equilibrium temperature of 996 degrees Kelvin. It is likely composed of a large iron core, a small rocky mantle, and a negligible atmosphere....
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How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
icon29. 11. 2023 (accepted)
iconStars | Exoplane
Image: How did exo-Venus TRAPPIST-1 c lose its carbon dioxide? Probably not through stellar winds
TRAPPIST-1 c receives almost the same bolometric flux as Venus. However JWST measurements show no sign of CO2 which is abundant in the atmosphere of our neighboring planet. According to a new study stellar winds cannot account for all the lost CO2. So astronomers believe that the planet was either born without significant CO2 atmosphere, or must have lost big portion of it through the escape of hydrogen. ...
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Retrieving planet formation parameters of WASP-77 A b
icon27. 11. 2023 (accepted)
iconStars | Exoplane
Image: Retrieving planet formation parameters of WASP-77 A b
WASP-77Ab likely formed in a disk with few planetesimals and underwent disk-free migration, starting within the CO ice line and ending beyond the water ice line...
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New study makes TOI-1670 c one of the longest-period planets to date to have its obliquity angle measured
icon27. 11. 2023 (accepted)
iconStars | Exoplane
Image: New study makes TOI-1670 c one of the longest-period planets to date to have its obliquity angle measured
The exoplanet joins a growing census of aligned warm Jupiters around single stars....
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Cold sub-Neptune planet discovered orbiting nearby star HD 88986
icon22. 11. 2023 (accepted)
iconStars | Exoplane
Image: Cold sub-Neptune planet discovered orbiting nearby star HD 88986
HD 88986 b has the longest orbital period among known transiting planets with known mass and less than 4 Earth radii....
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Sulfur dioxide and silicate clouds discovered in the atmosphere of the warm Neptune WASP-107 b
icon21. 11. 2023 (accepted)
iconStars | Exoplanets | Planetary atmosphere
Image: Sulfur dioxide and silicate clouds discovered in the atmosphere of the warm Neptune WASP-107 b
This is the first time these has been detected on a planet with a temperature below 1000 K...
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New study of nearby binary star LTT 3780 reveals clues to the formation of planets around red dwarfs
icon21. 11. 2023 (accepted)
iconStars | Exoplane
Image: New study of nearby binary star LTT 3780 reveals clues to the formation of planets around red dwarfs
The primary star is known to have 2 rocky exoplanets near radius valley which separates super-Earths and sub-Neptunes...
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Warm Jupiter with an orbital period of 15.27 days discovered orbiting a Sun-like star TOI 4515
icon20. 11. 2023 (accepted)
iconStars | Exoplanets | TESS
Image: Warm Jupiter with an orbital period of 15.27 days discovered orbiting a Sun-like star TOI 4515
Its high eccentricity may be the result of past violent scattering events ...
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icon15. 11. 2023 (accepted)
iconStars | Exoplanets | Kepler
Image:
Gas giant Kepler-1658 b is slowly spiraling inward due to tidal interactions with its host star. The observed rate of orbital decay cannot be explained by tidal dissipation in the star alone, but it can be explained if the planet rotates non-synchronously...
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Recently discovered exoplanets

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

Browse the latest scientific studies on stars and exoplanets in our galaxy. Stellar Catalog provides access to scientific data from astrophysics and stellar or planetary astronomy. It's a resource for anyone interested in the newest discoveries about what lies beyond our solar system.

Tau Ceti
11.9 ly
study icon Measuring masses of transiting Earth-like planets: first insights from the PLATO RV data challenge
yesterday

Kepler-88
1231 ly
study icon A Deep Learning Framework for TTV Characterization: A Case Study of the Kepler-88 System
28. 10. 2026

WISE J1517+0529
68.1 ly
study icon Periodic radio emission from a rapidly rotating T8 ultracool dwarf
28. 10. 2026

WD 1202-024
2757 ly
study icon A Model to Map Brown Dwarf Companions to White Dwarfs in Partial Secondary Eclipse
28. 10. 2026

V1298 Tauri
352 ly
study icon The GAPS Programme at TNG LXXXI. The puzzle of the HeI absorption signal in the atmosphere of V1298 Tau b with GIARPS@TNG
27. 10. 2026

CQ Tauri
487 ly
study icon A Warped Dust Ring in the CQ Tau Disk
27. 10. 2026

TOI 561
276 ly
study icon A Highly Reflective Atmosphere on the Lava World TOI-561b Revealed by JWST/NIRSpec Phase Curves
27. 10. 2026

HAT-P-11
124 ly
study icon Spatial variability of CH4-to-CO conversion pathways in irradiated gas giant atmospheres: implications for chemical relaxation and 1D quench schemes
27. 10. 2026

KIC 8462852
1470 ly
study icon The anomalously large transiting planet around Boyajian's star: evidence for a circumplanetary ring
27. 10. 2026

Circinus X-1
31000 ly
study icon Breaking the symmetry: X-ray polarization from a spreading layer on a tilted weakly magnetized neutron star
24. 10. 2026
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