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Latest astronomy noticias

Manténgase al día con las últimas noticias astronómicas, descubrimientos sobre estrellas y exoplanetas, e investigaciones actuales. Explore artículos recientes del mundo de la astronomía.
Transmission spectrum of the sub-Neptune HD 191939 b reveals no clear atmospheric signals
icon8. 8. 2026
iconEstrellas | Exoplanetas | Atmósferas planetari
Image: Transmission spectrum of the sub-Neptune HD 191939 b reveals no clear atmospheric signals
The sub-Neptune exoplanet HD 191939 b, a world larger than Earth but smaller than Neptune, has been examined to understand its atmospheric composition. Observations were conducted to analyze how light filters through the planet's atmosphere, a method known as transmission spectroscopy, which helps identify the gases present. The results show a flat spectrum with no distinct signatures, suggesting the presence of clouds or hazes that hide the deeper atmospheric layers. Researchers utilized the...
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Observations reveal evidence of a potential stellar companion for the red supergiant Betelgeuse
icon4. 8. 2026
iconEstrellas | | | Supergigante
Image: Observations reveal evidence of a potential stellar companion for the red supergiant Betelgeuse
Betelgeuse, one of the most prominent red supergiant stars in the night sky, has long been a subject of intense scientific inquiry. Recent analysis has sought to verify the existence of a secondary star orbiting this massive primary. By examining the star’s long secondary period of variability, which suggested the presence of an orbiting body, researchers targeted the system to confirm if a companion star was indeed present in the vicinity of thi...
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Planet engulfment remains a possible cause for lithium enhancement in TOI-5882
icon1. 8. 2026
iconEstrellas | Exoplanetas | TESS
Image: Planet engulfment remains a possible cause for lithium enhancement in TOI-5882
TOI-5882 is a subgiant star—a star in the later stages of its life—that is notably rich in lithium. This star hosts a massive brown dwarf, an object larger than a giant planet but smaller than a star, orbiting every 7.1 days. The high levels of lithium found in the star have led to the hypothesis that the star may have recently consumed a smaller planet, such as a super-Earth or a Neptune-sized world, whose material would alter the star's chemica...
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Helium-dominated atmospheres on rocky planets provide unique climate conditions for potential life
icon1. 8. 2026
iconEstrellas | Exoplane
Image: Helium-dominated atmospheres on rocky planets provide unique climate conditions for potential life
Climate models of rocky planets with helium-dominated atmospheres suggest these worlds may possess distinct thermal characteristics compared to planets with more common gases like nitrogen or hydrogen. Because helium is a simple atom with fewer internal ways to store energy, it creates a specific temperature profile that influences how heat is distributed and retained on a planet's surface. The study compared the warming effects of helium to n...
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Magnetic field and potential planet candidates of the nearby Red dwarf Gliese 729
icon1. 8. 2026
iconEstrellas | Exoplanetas | Enanas roj
Image: Magnetic field and potential planet candidates of the nearby Red dwarf Gliese 729
Gliese 729 (Ross 154) is the seventh closest Red dwarf to the Sun and serves as a significant subject for exoplanet research. Because Red dwarfs are typically very active, their magnetic fields can create noise that masks the subtle signals of orbiting planets. By analyzing a decade of data, the magnetic field of Gliese 729 has been mapped, revealing how its activity affects the search for small, rocky worlds in its vicinity. The research util...
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Horizontal quenching explains missing methane in the atmosphere of planet WASP-43 b
icon1. 8. 2026
iconEstrellas | Exoplanetas | Atmósferas planetari
Image: Horizontal quenching explains missing methane in the atmosphere of planet WASP-43 b
WASP-43 b is a hot Jupiter—a gas giant planet orbiting extremely close to its parent star. By using sophisticated three-dimensional computer simulations to analyze data from the James Webb Space Telescope, researchers have modeled the complex chemistry of the planet's atmosphere. The study focused on understanding how atmospheric circulation and chemical reactions influence the distribution of gases across the planet's day and night sides. The...
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Radio signal from HD 189733 system observed using NenuFAR telescope
icon1. 8. 2026
iconEstrellas | Exoplane
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 ...
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Orbital companion dynamics influence the dust disk structure around CQ Tauri
icon1. 8. 2026
iconEstrellas | Exoplanetas | Objetos estelares jóvenes | Formación planetari
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...
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Two low-density planets confirmed orbiting the bright star HD 148797
icon1. 8. 2026
iconEstrellas | Exoplane
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...
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Wide-orbit stellar companions influence formation of giant planets around Red dwarf stars
icon1. 8. 2026
iconEstrellas | Exoplanetas | TESS | Enanas rojas | Formación planetaria | Enanas b
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...
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Exoplanetas recién descubiertos

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

Explore los últimos estudios científicos sobre estrellas y exoplanetas en nuestra galaxia. Descubra las últimas investigaciones sobre astrofísica y astronomía estelar.

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
today

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
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