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Today's spotlight falls on the fascinating white dwarf WD J1330, a star currently drawing significant attention from researchers and enthusiasts alike. While we often think of white dwarfs as plain, new research highlights their remarkable visual diversity, proving these dense stellar remnants can shimmer in vibrant hues from yellow to purple depending on their unique chemical signatures.
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Oxygen-rich atmospheres may develop much faster on planets orbiting red dwarfs than on Earth
icon28. 1. 2026
iconStar
Image: Oxygen-rich atmospheres may develop much faster on planets orbiting red dwarfs than on Earth
A new study focusing on the Earth-like exoplanet TRAPPIST-1e suggests that the transition to an oxygen-rich atmosphere, known as the Great Oxidation Event, could occur up to a billion years sooner than it did on our own planet. While Earth's atmosphere took hundreds of millions of years to accumulate oxygen after the appearance of life, the unique light from M-dwarf stars promotes more efficient ozone formation. This process lowers the barrier for full atmospheric oxidation, potentially allo...
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JWST Discovers a Potential Giant Planet Orbiting a Dead Star
icon28. 1. 2026
iconStars | Exoplanets | White dwarf
Image: JWST Discovers a Potential Giant Planet Orbiting a Dead Star
Using the James Webb Space Telescope, astronomers have discovered a significant infrared glow around white dwarf star WD 0644+025, an unusually heavy white dwarf located within 25 parsecs of Earth. This excess heat suggests the presence of a giant planet, roughly seven times the mass of Jupiter, orbiting the remains of this dead star. While white dwarfs are the final stage of stars like our Sun, this particular star is unique because it shows...
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Discovery of a New Earth-Sized Neighbor: A Potential Twin of Our Home Planet Found Orbiting a Sun-Like Star
icon28. 1. 2026
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Image: Discovery of a New Earth-Sized Neighbor: A Potential Twin of Our Home Planet Found Orbiting a Sun-Like Star
Astronomers have discovered a fascinating planet candidate, named HD 137010 b, which bears a striking resemblance to Earth. Located around a bright star similar to our Sun, this world is almost exactly the same size as Earth and orbits its star every 355 days—a year nearly identical to our own. Because it sits at the outer edge of the 'habitable zone,' it receives just enough light and heat that it could potentially host liquid water. This di...
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Discovery of TOI-6692b: A Giant Planet with a Highly Elliptical 130-Day Orbit
icon27. 1. 2026
iconStar
Image: Discovery of TOI-6692b: A Giant Planet with a Highly Elliptical 130-Day Orbit
Astronomers have discovered a new giant planet named TOI-6692b, which is similar to Jupiter but follows a much more elongated, eccentric path around its star. While Earth takes a year to orbit the Sun in a nearly circular path, this massive world completes its orbit in 130 days, swinging in and out due to its oval-shaped trajectory. Initially spotted by a single shadow it cast while passing in front of its star, its existence was confirmed usi...
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Light variations of LAMOST J235456.73+3356 point to intense heating from a neutron star
icon6. 1. 2026
iconStars | Neutron star
Image: Light variations of LAMOST J235456.73+3356 point to intense heating from a neutron star
Models favor a neutron star instead of a colder white dwarf. LAMOST J2354+3356 is over 400 light years away, and is the closest neutron star candidate....
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Spectral energy measurements of Tau Ceti and other exoplanet host stars
icon4. 1. 2026
iconStars | Exoplanets | Sun-like stars | James Webb Space Telescope
Image: Spectral energy measurements of Tau Ceti and other exoplanet host stars
Researchers have compiled detailed spectral energy distributions for 20 stars that hosted exoplanets studied by the James Webb Space Telescope. By measuring the X-ray and ultraviolet light emitted by these stars, the team highlights how intense radiation impacts the atmospheres of orbiting planets. This data includes vital information on stars like Tau Ceti, helping experts better understand the potential for atmospheric loss on these worlds....
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Astronomers identified two remarkably low-density, inflated planets TOI-1927 b and TOI-2643 b
icon22. 12. 2025
iconStars | Exoplane
Image: Astronomers identified two remarkably low-density, inflated planets TOI-1927 b and TOI-2643 b
TOI-1927 b and TOI-2643 b are the first puffy planets known to orbit stars in thick disc of the Milky Way. This is highly unexpected in such metal-poor environment of our galaxy....
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5 new Earth-sized exoplanets discovered orbiting small red dwarfs
icon16. 12. 2025
iconStars | Exoplanets | Super-Earths | Red dwarf
Image: 5 new Earth-sized exoplanets discovered orbiting small red dwarfs
These planets could be great targets for study of atmosphere loss on exoplanets close to their active stars....
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Hot Jupiter WASP-189 b shows a strong dayside glow but almost no nightside light
icon8. 12. 2025
iconStars | Exoplanets | TESS | Hot Jupiter
Image: Hot Jupiter WASP-189 b shows a strong dayside glow but almost no nightside light
TESS phase curve reveals extreme heat with poor redistribution. The planet orbits in a near-polar orbit around its rapidly rotating star...
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JWST detected phosphine in the atmosphere of cool brown dwarf Wolf 1130 C
icon9. 10. 2025
iconStars | Planetary atmospheres | Exoplane
Image: JWST detected phosphine in the atmosphere of cool brown dwarf Wolf 1130 C
The phosphine is detected in far higher quantities than in other brown dwarfs. The result matches disequilibrium chemistry seen in Jupiter and Saturn. The brown dwarf orbits white dwarf - red dwarf binary....
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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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