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Stellar Brief: 21. 10. 2026
A new age estimate changes the story of PDS 70: the star is 12 to 16 million years old, roughly three times older than earlier estimates. Its planet PDS 70 b may have formed millions of years after the star. Read today's Stellar Brief

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Latest astronomy nouvelles

Three super-Earths TOI-260 b, TOI-286 b, and TOI-286 c confirmed
icon11. 6. 2024
iconÉtoiles | Exoplanètes | Super-Terre | Planètes océ
Image: Three super-Earths TOI-260 b, TOI-286 b, and TOI-286 c confirmed
Astronomers used combinined high-precision data from TESS space telescope for transits and ESPRESSO instrument on VLT in Chile for radial velocity, that allowed them to measure mass and radius....
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icon8. 6. 2024
iconÉtoiles | Exoplanète
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Radius and temperature measured for stars in binary system EBLM J0608-59 (TOI-1338, BEBOP-1). Both stars in this system are orbited by at least two exoplanets....
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Exoplanet hidden in DM Tauri disc might be less massive than previously thought
icon5. 6. 2024
iconÉtoiles | Exoplanète
Image: Exoplanet hidden in DM Tauri disc might be less massive than previously thought
Magnetized winds play a crucial role in shaping the disc and its interaction with the planet. DM Tauri is a young forming star 470 light years away. It still has an accretion disc in which there is an exoplanet with mass around 53 Earths....
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By analyzing images taken years ago astronomers successfully revealed the presence of a giant exoplanet AF Leporis b
icon5. 6. 2024
iconÉtoiles | Exoplanète
Image: By analyzing images taken years ago astronomers successfully revealed the presence of a giant exoplanet AF Leporis b
A new machine learning method used to better separate the faint planet signal from the noisy starlight in images....
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icon3. 6. 2024
iconÉtoiles | Exoplanète
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Exoplanet HIP 41378 d was previously observed transiting its star twice, three years apart. Astronomers now aimed the CHEOPS telescope for another observation, but surprisingly, no transit was detected...
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New warm-Neptune TOI 5076 b confirmed with a mass about 16 times Earth's and a radius slightly over 3 times Earth's
icon30. 5. 2024
iconÉtoiles | Exoplanètes | TESS
Image: New warm-Neptune TOI 5076 b confirmed with a mass about 16 times Earth
Its density suggests a significant amount of volatile materials surrounding a rocky core....
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Tiny wobbles of a bright star HD 73344 have revealed the mass of a nearby sub-Neptune exoplanet
icon27. 5. 2024 (accepté)
iconÉtoiles | Exoplanète
Image: Tiny wobbles of a bright star HD 73344 have revealed the mass of a nearby sub-Neptune exoplanet
Additionally, another signal hints at the presence of a previously undetected planet orbiting farther from the star. HD 73344 is an F-type star approximately 115 light-years away. At roughly 20% larger than our Sun, it hosts a sub-Neptune exoplanet with a density similar to Saturns. The possible second planet has been detected with a minimum mass around one-third that of Jupiter...
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A mini-Neptune discovered in the habitable zone of star TOI 4633
icon29. 4. 2024 (accepté)
iconÉtoiles | Exoplanète
Image: A mini-Neptune discovered in the habitable zone of star TOI 4633
Also another non-transiting planet candidate lurks closer to the star...
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The famous planet thought to orbit 40 Eridani A does not exist. Its signal can be explained with stellar activity
icon26. 4. 2024 (accepté)
iconÉtoiles | Exoplanète
Image: The famous planet thought to orbit 40 Eridani A does not exist. Its signal can be explained with stellar activity
In the Star Trek universe the planet Vulcan (also NiVar) orbits one of the three stars in 40 Eridani system that lies 40 light years from the Sun....
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Planet confirmed orbiting one of three red dwarfs in the nearby system TOI 4336
icon19. 4. 2024 (accepté)
iconÉtoiles | Exoplanète
Image: Planet confirmed orbiting one of three red dwarfs in the nearby system TOI 4336
It is bigger than Earth and orbits near the habitable zone of its star....
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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
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