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Latest astronomy news

Stay updated with the latest astronomy news, discoveries about stars and exoplanets, and current research. Explore fresh articles from the world of astronomy.
Observations of Gliese 1132 b reveal a planet likely lacking an atmosphere
icon31. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope | Planetary atmosphere
Image: Observations of Gliese 1132 b reveal a planet likely lacking an atmosphere
Recent analysis of data from the James Webb Space Telescope, the Hubble Space Telescope, and ground-based observations suggests that the exoplanet Gliese 1132 b is likely a bare rocky world. By examining the light filtering through the planet’s edges as it passes in front of its host star, the data reveals a featureless transmission spectrum, meaning no clear chemical fingerprints of an atmosphere were detected. The study compared various models, including clear and cloudy atmospheres, agains...
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Third hidden planet perturbs the orbit of two known planets around Kepler-50
icon31. 8. 2026
iconStars | Exoplanets | Kepler
Image: Third hidden planet perturbs the orbit of two known planets around Kepler-50
The star Kepler-50 hosts two known planets that pass in front of their host star from our perspective, an event known as a transit. These two planets are locked in a near-resonant relationship, meaning their orbital periods are mathematically related. Analysis of their transit times reveals small, irregular timing variations, which indicate the presence of a third, non-transiting planet tugging on them through gravity. Researchers examined dat...
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Two planets discovered orbiting the star TOI-4468 including a hot Jupiter
icon31. 8. 2026
iconStars | Exoplanets | TESS | Hot Jupiter
Image: Two planets discovered orbiting the star TOI-4468 including a hot Jupiter
A new planetary system has been identified orbiting the star TOI-4468, featuring a hot Jupiter and a nearby outer sub-Neptune. This system is unique because it includes a close outer companion to a hot Jupiter without any inner planets, a configuration not typically seen in the current census of known worlds. These findings provide new insights into how these massive, short-period planets form and evolve over time. The research confirmed the p...
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Chemical composition of TRAPPIST-1 measured using high-resolution infrared light
icon31. 8. 2026
iconStars | Exoplane
Image: Chemical composition of TRAPPIST-1 measured using high-resolution infrared light
TRAPPIST-1 is a small, cool star known for hosting several Earth-sized planets. Because very low-mass stars do not change much over time, they preserve the chemical signature of the cloud of gas and dust from which they formed. Understanding the chemical makeup of such a star provides essential clues about the building materials available to its planets during their formation process. The chemical composition was determined by analyzing high-r...
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Stellar flares explain missing methane in the atmosphere of exoplanet V1298 Tauri b
icon31. 8. 2026
iconStars | Exoplanets | Planetary atmosphere
Image: Stellar flares explain missing methane in the atmosphere of exoplanet V1298 Tauri b
The young exoplanet V1298 Tauri b is a warm sub-Neptune orbiting a very young orange dwarf star. Recent observations from the James Webb Space Telescope have revealed an atmospheric mystery: the planet contains far less methane than expected, while showing surprising levels of carbon dioxide. This phenomenon, known as the missing methane problem, has been observed in several cool planets, where standard chemical models fail to predict the observe...
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Stellar dynamics in CH Ind and SW CMa disprove need for circumbinary planets
icon23. 8. 2026
iconStars | Exoplane
Image: Stellar dynamics in CH Ind and SW CMa disprove need for circumbinary planets
Eclipsing binary stars—systems where two stars periodically pass in front of each other from our perspective—often show small shifts in their orbital timings. These shifts, known as apsidal motion, are sometimes used to search for third objects like planets orbiting both stars. This study evaluates two such systems, CH Ind and SW CMa, to determine if their observed orbital changes truly indicate the presence of external planets or if they are sim...
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Climate simulations reveal possible habitability conditions on planet Gliese 514 b
icon23. 8. 2026
iconStars | Exoplane
Image: Climate simulations reveal possible habitability conditions on planet Gliese 514 b
The exoplanet Gliese 514 b orbits within the habitable zone of a Red dwarf star located approximately 25 light-years from Earth. Because the planet follows an eccentric path—meaning its orbit is more oval-shaped than circular—it experiences significant seasonal changes in the amount of stellar light it receives. These conditions make it an important target for future direct-imaging missions, prompting an assessment of its potential surface climat...
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70 Ophiuchi and 36 Ophiuchi binary systems show potential for supporting stable habitable planets
icon23. 8. 2026
iconStars | Exoplane
Image: 70 Ophiuchi and 36 Ophiuchi binary systems show potential for supporting stable habitable planets
Numerical simulations have evaluated whether planets in the 70 Ophiuchi, 36 Ophiuchi, and Gamma Leonis binary systems can remain stable in their habitable zones. The habitable zone is the range of distances from a star where conditions might allow liquid water to exist on a planet's surface. While Gamma Leonis is unlikely to support stable planets due to its extreme orbital dynamics, the 70 Ophiuchi and 36 Ophiuchi systems show promising conditio...
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Atmospheric composition of stars AF Leporis A and Epsilon Indi A characterized
icon23. 8. 2026
iconStars | Exoplanets | Planetary atmosphere
Image: Atmospheric composition of stars AF Leporis A and Epsilon Indi A characterized
Understanding how planets form requires detailed knowledge of the chemical makeup of their host stars. This study provides a comprehensive analysis of the host stars AF Leporis A and Epsilon Indi A, which are known to harbor cold, directly imaged planets. By examining the light from these stars with high-resolution spectroscopy—a technique that breaks down starlight into its component colors to identify chemical elements—the composition of their ...
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Precision timing of planet HD 80606b reveals orbital stability and constraints on companions
icon23. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope
Image: Precision timing of planet HD 80606b reveals orbital stability and constraints on companions
The exoplanet HD 80606b is a massive gas giant known for its extreme eccentricity, meaning its path around its host star is highly elongated rather than circular. Because it transits and is eclipsed by its host star, the G5V star HD 80606, it serves as a unique laboratory for studying planetary dynamics. New high-precision data from the James Webb Space Telescope, combined with 25 years of previous radial velocity measurements, were used to exami...
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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
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

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.

HD 203771
184 ly
study icon An Intermediate-orbit Brown Dwarf Confirmed with Astrometry+Radial Velocity Joint Analysis, and the Eccentricity Distribution of Brown Dwarfs Across Different Locations
yesterday

HD 158485
390 ly
study icon TESS Pulsation Timing Reveals the JWST Calibration Star HD 158485 as a Double-pulsator Binary
yesterday

KELT-18
1032 ly
study icon High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm
yesterday

WASP 17
1315 ly
study icon A Spatial Map of the Atmospheric Limb of a Hot Jupiter
yesterday

Gliese 892
21.3 ly
study icon Detailed study of HD 219134: a benchmark K-dwarf with a compact planetary system
12. 10. 2026

WASP-39
702 ly
study icon Limb Asymmetries on WASP-39b: A Multi-GCM Comparison of Chemistry, Clouds, and Hazes
12. 10. 2026

WASP-13
753 ly
study icon The GAPS programme at TNG LXXXII. The first atmospheric investigation of the gas giant WASP-13b at high resolution with GIARPS
12. 10. 2026

EK Chamaeleontis
321 ly
study icon EK Cha b: multi-tracer detection of a protoplanet candidate in a gas-rich environment
9. 10. 2026

HD 89744
126 ly
+2 study icon Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs
9. 10. 2026

LTT 9779
264 ly
study icon Exploring the ultrahot Neptune LTT 9779 b with CRIRES+. Non-detection of helium transmission spectra and detection of H2O on the dayside
9. 10. 2026
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