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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.
Mantle composition and mineralogy of super-Earth Gliese 486b characterised through stellar abundance
icon23. 8. 2026
iconStars | Exoplanets | Super-Earth
Image: Mantle composition and mineralogy of super-Earth Gliese 486b characterised through stellar abundance
The internal makeup of the super-Earth Gliese 486b has been estimated by analyzing the chemical properties of its host star. Because rocky planets typically inherit their chemical composition from the materials that formed their parent stars, understanding the composition of a star provides a window into the building blocks of its orbiting planets. This research provides a new framework that links stellar chemical data to the internal structure and mineralogy of distant rocky worlds. To deter...
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Analysis of existing JWST data attempts to detect outer planets of Trappist-1
icon23. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope
Image: Analysis of existing JWST data attempts to detect outer planets of Trappist-1
The Trappist-1 system, a small star orbited by seven Earth-sized planets, has been a major target for the James Webb Space Telescope. While the inner planets have been studied directly, the potential to detect thermal emission—the heat energy radiated by a planet—from the outer planets remains a significant challenge due to interference from the host star itself. This analysis compiled existing observations from five separate projects to see i...
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Observations of planet LHS 1140 b show no persistent signs of helium escape
icon23. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope
Image: Observations of planet LHS 1140 b show no persistent signs of helium escape
Recent observations of the temperate planet LHS 1140 b have provided new insights into its atmosphere. While previous data suggested the presence of helium escaping from the planet, detailed analysis of four planetary transits—the period when a planet passes in front of its star—reveals no consistent evidence of such activity, indicating that earlier detections may have been influenced by stellar changes or instrumental factors. Researchers ex...
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Asymmetric aerosol distribution observed on the warm Saturn planet WASP-69 b
icon23. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope
Image: Asymmetric aerosol distribution observed on the warm Saturn planet WASP-69 b
The warm Saturn-sized exoplanet WASP-69 b exhibits significant atmospheric differences between its morning and evening sides. New observations reveal an asymmetric distribution of aerosols—tiny particles suspended in the atmosphere—which create distinct cloud conditions across the planet. This discovery helps explain how planets at temperatures near 1,000 Kelvin manage the cycle of cloud formation and evaporation as material travels around the gl...
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Geometric model explains the brightness temperature of planet 55 Cancri e
icon13. 8. 2026
iconStars | Exoplane
Image: Geometric model explains the brightness temperature of planet 55 Cancri e
The thermal characteristics of 55 Cancri e, an ultra-short period rocky planet, are better understood by accounting for the planet’s three-dimensional geometry and its rotation. By calculating how sunlight hits the planet at various angles throughout its day, it is possible to model the temperature distribution across its surface more accurately. This approach clarifies why the planet exhibits a specific thermal imprint observed by telescope meas...
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Sulfur-rich atmosphere of planet AF Lep b reveals history of solid accretion
icon13. 8. 2026
iconStars | Exoplanets | Planetary atmosphere
Image: Sulfur-rich atmosphere of planet AF Lep b reveals history of solid accretion
AF Lep b is a young gas giant planet with a mass roughly three to four times that of Jupiter, orbiting its host star at a distance of approximately 9 astronomical units. Recent observations using the James Webb Space Telescope have allowed for a detailed look at the chemical composition of its atmosphere, providing new insights into how this massive planet formed and grew during the early stages of its solar system. The research team analyzed ...
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Formation of giant planets PDS 70 c and SR 12 c mirrors our solar system
icon13. 8. 2026
iconStars | Exoplanets | Planet formatio
Image: Formation of giant planets PDS 70 c and SR 12 c mirrors our solar system
The young planetary systems PDS 70 and SR 12 provide new insights into how giant planets and their moons form. By studying the dust disks surrounding the planets PDS 70 c and SR 12 c, it is clear that these distant worlds share significant similarities with the development of Jupiter and Saturn. These observations help explain how gas and dust accumulate to form planets and smaller satellites in the early stages of a star system's life. The pl...
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Two warm saturn-mass planets found orbiting the star TOI-3850
icon13. 8. 2026
iconStars | Exoplanets | TESS | Sun-like star
Image: Two warm saturn-mass planets found orbiting the star TOI-3850
A multi-planet system has been identified orbiting TOI-3850, a G0 dwarf star similar in metallicity to our Sun. The system contains two warm planets—gas-rich worlds that orbit closer to their star than Jupiter, but further than the extremely hot planets commonly found in close proximity to their hosts. These planets are currently situated near a gravitational configuration known as a 2:1 mean motion resonance, where the outer planet completes one...
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Radial velocity analysis characterizes planetary systems around DMPP-7 HD 67200 and HD 2134
icon13. 8. 2026
iconStars | Exoplane
Image: Radial velocity analysis characterizes planetary systems around DMPP-7 HD 67200 and HD 2134
Recent observations have analyzed the environments around three stars - DMPP-7, HD 67200, and HD 2134 — to search for evidence of orbiting planets. By studying radial velocity, which measures the tiny wobbles in a star’s position caused by the gravitational tug of an orbiting planet, the project examined these systems to distinguish between genuine planetary signals and the natural activity of the stars themselves. The researchers used a Bayes...
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Analysis of dust rings in the protoplanetary disk around LkCa 15
icon10. 8. 2026
iconStars | Exoplanets | Planet formatio
Image: Analysis of dust rings in the protoplanetary disk around LkCa 15
Protoplanetary disks are vast, swirling clouds of gas and dust surrounding young stars that eventually coalesce to form planets. A new method has been developed to analyze the physical properties of these disks by examining how their dust rings appear when viewed at an angle. By studying these shapes, researchers can determine the intrinsic width, thickness, and light-blocking capacity, known as optical depth, of the dust material within the disk...
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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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