do not follow here
Stellar Catalog more icon
Nouvelles
more icon

news icon
Latest astronomy nouvelles

Restez informé(e) des dernières actualités astronomiques, des découvertes sur les étoiles et les exoplanètes, et des recherches en cours. Découvrez de nouveaux articles sur l'astronomie.
Radio signal from HD 189733 system observed using NenuFAR telescope
icon1. 8. 2026
iconÉtoiles | Exoplanète
Image: Radio signal from HD 189733 system observed using NenuFAR telescope
Researchers have identified potential radio signals coming from the HD 189733 system, a discovery that may offer insights into the magnetic fields of planets outside our solar system. Detecting such auroral radio emissions—light produced when charged particles interact with magnetic fields—is a key method for understanding the interiors and potential habitability of distant worlds. The signal was recorded at low frequencies. The team analyzed data using a technique called beamforming, which c...
Read article tag icon
Advertisement
Orbital companion dynamics influence the dust disk structure around CQ Tauri
icon1. 8. 2026
iconÉtoiles | Exoplanètes | Objets stellaires jeunes | Formation des planète
Image: Orbital companion dynamics influence the dust disk structure around CQ Tauri
The star CQ Tauri shows indirect signs of a companion affecting its surrounding environment. Observations reveal a large cavity in the disk of material around the star, measuring approximately 25 astronomical units across, with a prominent ring of dust peaking at a distance of 53 astronomical units. An astronomical unit is the average distance from the Earth to the Sun. To understand this structure, researchers simulated how gas and dust behav...
Read article tag icon
Two low-density planets confirmed orbiting the bright star HD 148797
icon1. 8. 2026
iconÉtoiles | Exoplanète
Image: Two low-density planets confirmed orbiting the bright star HD 148797
The bright F-type star HD 148797 hosts two moderate-period planets, classified as sub-Jovian worlds with unusually low density. These planets reside in a region of space known as the Neptunian savanna, a classification for planets with specific ranges of size and orbital distance. The findings provide insights into how such systems form and evolve, suggesting they often develop in dynamically stable environments rather than through violent orbita...
Read article tag icon
Wide-orbit stellar companions influence formation of giant planets around Red dwarf stars
icon1. 8. 2026
iconÉtoiles | Exoplanètes | TESS | Naines rouges | Formation des planètes | Naines blanche
Image: Wide-orbit stellar companions influence formation of giant planets around Red dwarf stars
The giant planet TOI-5628Ab orbits a mid-type Red dwarf star every 4.34 days. This planet is part of a complex system that also includes a distant white dwarf companion, a remnant of a star that has exhausted its nuclear fuel. By studying this system and comparing it to a wider population of similar stars, the research identifies a strong connection between the presence of distant stellar companions and the existence of large planets orbiting ver...
Read article tag icon
Orbital analysis of π Mensae system updates parameters for three potential exoplanets
icon1. 8. 2026
iconÉtoiles | Exoplanète
Image: Orbital analysis of π Mensae system updates parameters for three potential exoplanets
The π Mensae star system, which hosts the first exoplanet detected by the Transiting Exoplanet Survey Satellite (TESS), has been the subject of a comprehensive new study. By combining six years of TESS photometry — the measurement of a star's brightness over time to detect dips caused by orbiting planets — with 22 years of radial velocity data, which tracks the tiny wobbles in a star’s motion caused by a planet’s gravitational pull, this research...
Read article tag icon
New modeling framework reveals complex dust structures in the HD 169142 disk
icon1. 8. 2026
iconÉtoiles | Exoplanètes | Formation des planète
Image: New modeling framework reveals complex dust structures in the HD 169142 disk
The protoplanetary disk surrounding the star HD 169142 contains complex dust structures that provide clues about how planets form. A new analytical framework has been developed to process data from the Atacama Large Millimeter/submillimeter Array (ALMA), an interferometer that combines radio telescopes to capture high-resolution images. This method improves upon traditional techniques by reducing biases caused by limited image resolution, allowin...
Read article tag icon
Refined mass and radius measurements for planets orbiting stars TOI-4438 and TOI-442
icon1. 8. 2026
iconÉtoiles | Exoplanètes | TESS
Image: Refined mass and radius measurements for planets orbiting stars TOI-4438 and TOI-442
Researchers have completed a detailed re-analysis of two planetary systems, TOI-4438 and TOI-442, providing more precise physical data for their orbiting planets. By combining new transit observations from the TESS space telescope with high-resolution infrared spectroscopy, the study clarifies the properties of these worlds. The analysis also investigated the magnetic activity of the host stars, which are both Red dwarf stars, to improve the accu...
Read article tag icon
Escaping helium atmosphere identified on the rocky exoplanet LHS 1140b
icon1. 8. 2026
iconÉtoiles | Exoplanètes | Atmosphères planétaires | Exoplanètes habitable
Image: Escaping helium atmosphere identified on the rocky exoplanet LHS 1140b
Spectroscopic observations have identified escaping helium from the atmosphere of LHS 1140b, a rocky exoplanet located within the habitable zone of its host star. While scientists have previously observed atmospheric loss on massive gas giants, such evidence for rocky, Earth-like worlds is rare. This finding provides significant insight into the evolution and composition of planetary atmospheres in systems orbiting low-mass stars. The findings...
Read article tag icon
Migration history of the super-eccentric planet TIC 241249530 b
icon1. 8. 2026
iconÉtoiles | Exoplanète
Image: Migration history of the super-eccentric planet TIC 241249530 b
TIC 241249530 b is a rare, highly eccentric planet often described as a hot Jupiter progenitor. Orbiting a star at a distance that varies significantly, this planet is currently in the process of migrating toward its host star. This transition is driven by high-eccentricity migration, a process where a planet’s orbit is stretched into a very elongated shape, eventually shrinking and circularizing due to intense tidal forces. The research exami...
Read article tag icon
Shadows in the protoplanetary disk around HD 142527 reveal dust grain sizes
icon1. 8. 2026
iconÉtoiles | Exoplanètes | Formation des planète
Image: Shadows in the protoplanetary disk around HD 142527 reveal dust grain sizes
Planet formation begins within protoplanetary disks, which are swirling clouds of gas and dust surrounding young stars. To understand how planets emerge, it is critical to determine the size of dust grains within these disks. A new method has been developed to estimate these sizes by measuring how quickly different regions of a disk cool down. This technique specifically analyzes transitional disks where an inner disk is tilted, casting a distinc...
Read article tag icon

Top article categories

Filtered articles by category.

Exoplanètes nouvellement découvertes

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
tag icon

Latest scientific studies

Parcourez les dernières études scientifiques sur les étoiles et les exoplanètes de notre galaxie. Découvrez les dernières recherches en astrophysique et en astronomie stellaire.

WASP-33
378 ly
study icon Identifying deformed exoplanets with JWST and Ariel: A target selection metric for phase curve observations
today

WASP 94
687 ly
study icon A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum
today

TOI-3118
1410 ly
study icon A Sample of Thick-Disk Stars Hosting Hot Jupiters
today

DM Tauri
470 ly
study icon Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+
yesterday

HD 152384
419 ly
study icon HD 152384: A 5 Myr old debris disk system showing a gaseous ring of refractory elements at the dust sublimation radius
yesterday

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
yesterday

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

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
yesterday

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
14. 10. 2026

HD 158485
390 ly
study icon TESS Pulsation Timing Reveals the JWST Calibration Star HD 158485 as a Double-pulsator Binary
14. 10. 2026
tag icon
Publications plus anciennes

Advertisement