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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.
High resolution observations reveal dust structure of the protoplanetary disk around HD 163296
icon1. 8. 2026
iconStars | Exoplanets | Planet formatio
Image: High resolution observations reveal dust structure of the protoplanetary disk around HD 163296
The protoplanetary disk surrounding the star HD 163296 contains complex structures that provide insight into the birthplace of planets. By analyzing new and archival data from the Atacama Large Millimeter/submillimeter Array (ALMA), researchers have characterized the temperature, density, and size of dust grains within this vast cloud of gas and debris. To study the disk, the analysis utilized spectral energy distribution fitting, a technique that examines how light is emitted across differen...
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WISPIT 2 revealed as a binary star system hosting two young protoplanets
icon1. 8. 2026
iconStars | Exoplanets | Young Stellar Obje
Image: WISPIT 2 revealed as a binary star system hosting two young protoplanets
The WISPIT 2 system, known for harboring two giant protoplanets within a multi-ringed disc of gas and dust, has been identified as a spectroscopic binary. This means the system consists of two stars orbiting one another, visible through changes in their light patterns rather than direct imaging of both stars. This discovery establishes the system as a primary location for studying how planets form in environments around two stars. The system c...
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High resolution imaging reveals structural details of the protoplanetary disk around TW Hydrae
icon1. 8. 2026
iconStars | Exoplanets | James Webb Space Telescope | Young Stellar Objects | Planet formatio
Image: High resolution imaging reveals structural details of the protoplanetary disk around TW Hydrae
The protoplanetary disk surrounding the star TW Hydrae, the nearest such disk to Earth, has been observed in unprecedented detail. Protoplanetary disks are rotating, flattened clouds of gas and dust that surround young stars, serving as the raw material for planet formation. By using the high-contrast imaging capabilities of the James Webb Space Telescope’s Near Infrared Camera, researchers have mapped the disk's architecture to better understand...
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Magnetospheric plasma sources around the ultra-cool dwarf LSR J1835+3259
icon1. 8. 2026
iconStars | Exoplanets | Brown dwarf
Image: Magnetospheric plasma sources around the ultra-cool dwarf LSR J1835+3259
Radio waves emitted by ultra-cool dwarf stars suggest these objects possess radiation belts similar to those found around Jupiter. These belts consist of plasma, a state of matter containing charged particles, trapped within the star's magnetic field. This study investigates the origin of this plasma for the ultra-cool dwarf LSR J1835+3259 by modeling potential sources, such as escaping atmospheric ions or material from a volcanic moon. The re...
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Inclined eccentric planet model explains moving dust clumps around the star AU Microscopii
icon1. 8. 2026
iconStars | Exoplanets | Planet formatio
Image: Inclined eccentric planet model explains moving dust clumps around the star AU Microscopii
The red dwarf star AU Microscopii is surrounded by a complex debris disk—a ring of dust and rocky debris—that features unusual clumps of dust moving at high speeds. These features, visible only when scattering light from the star, consist of tiny grains about 0.2 micrometers in size. New simulations suggest that the observed motion of these dust clumps may be caused by the gravitational influence of a yet-to-be-confirmed planet interacting with t...
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Dayside atmosphere of ultra-hot Jupiter WASP-178 b shows thermal inversion and neutral iron
icon1. 8. 2026
iconStars | Exoplanets | Planetary atmospheres | Hot Jupiter
Image: Dayside atmosphere of ultra-hot Jupiter WASP-178 b shows thermal inversion and neutral iron
WASP-178 b is an ultra-hot Jupiter, a gas giant planet that orbits extremely close to its parent star, resulting in scorching atmospheric temperatures. New high-resolution optical observations of the planet’s dayside reveal a thermal inversion, a state where the temperature in the upper atmosphere increases with altitude, opposite to the expected cooling trend. These findings help clarify the complex, three-dimensional processes driving extreme w...
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Azimuthal brightness modulation reveals hidden dust rings in the disk of CI Tauri
icon7. 7. 2026
iconStars | Young Stellar Objects | Planet formatio
Image: Azimuthal brightness modulation reveals hidden dust rings in the disk of CI Tauri
CI Tauri is a young star surrounded by a protoplanetary disk—a rotating, flattened cloud of gas and dust from which planets are born. While these disks often contain rings and gaps that signal planet formation, narrow structures can be too small for telescopes to resolve directly. A new method has now revealed hidden, fine-scale features within the disk of CI Tauri by measuring how brightness changes at different angles. The analysis focused o...
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Numerical simulations reveal outcomes of primordial black hole encounters with TOI 2796
icon7. 7. 2026
iconStars | Exoplanets | Black holes | TESS
Image: Numerical simulations reveal outcomes of primordial black hole encounters with TOI 2796
The TOI 2796 system, which is known to host a hot Jupiter—a massive gas giant planet orbiting very close to its parent star—faces potential disruption from encounters with primordial black holes. Primordial black holes are hypothetical objects thought to have formed in the very early universe, long before the first stars and galaxies emerged. Using numerical three-body simulations, the gravitational effects of such an encounter on the planetary s...
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Radial velocity reveals for the first time planetary mass object around brown dwarf CD-35 2722 B
icon7. 7. 2026
iconStars | Exoplanets | Brown dwarfs | Exomoo
Image: Radial velocity reveals for the first time planetary mass object around brown dwarf CD-35 2722 B
Evidence for satellites orbiting the brown dwarf CD-35 2722 B has been identified using precise light measurements. While thousands of planets have been found orbiting stars, satellites around objects outside our solar system—known as exosatellites—have remained elusive and controversial. This study presents a strong detection of at least one, and possibly two, massive objects circling this brown dwarf, providing new data on how such systems form...
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Inflated hot Neptune TOI-2195 A b likely formed from a massive gas giant
icon6. 7. 2026
iconStars | Exoplanets | TESS | Orange dwarf
Image: Inflated hot Neptune TOI-2195 A b likely formed from a massive gas giant
A newly identified planet, TOI-2195 A b, has been found orbiting an orange dwarf star. Classified as an inflated hot Neptune, this planet completes an orbit around its host star every 4.16 days. The discovery offers a new perspective on how such planets form, suggesting they may have once been much larger gas giants that lost a significant portion of their mass. Researchers analyzed the system using the Rossiter-McLaughlin effect, which measur...
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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.

KELT-2
439 ly
study icon Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity
today

HAT-P-18
527 ly
study icon ExoEcho: Exoplanet Ephemerides Change Observations. III. A JWST Survey for Transit Timing Variations of 37 Exoplanets
today

TOI-2257
189 ly
study icon The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b
today

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
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