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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.
Magnetic fields act as brakes and heaters in the atmosphere of ultra-hot Jupiter WASP-18 b
icon23. 2. 2026
iconStars | Exoplane
Image: Magnetic fields act as brakes and heaters in the atmosphere of ultra-hot Jupiter WASP-18 b
Researchers have discovered that the magnetic field of the giant planet WASP-18 b plays a dramatic role in controlling its weather. Because the planet is so close to its star, its atmosphere becomes 'ionized' or electrically charged. This allows the planet's magnetic field to act like a physical brake on high-altitude winds, creating a 'stop and go' effect in the atmospheric flow. This magnetic drag, combined with frictional heating, creates unusual temperature patterns, including two distin...
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Discovery of a hot rocky world with Earth-like density orbiting a young star
icon23. 2. 2026
iconStars | Exoplanets | TESS | Orange dwarf
Image: Discovery of a hot rocky world with Earth-like density orbiting a young star
Astronomers have confirmed the existence of TOI-5734b, a 'hot sub-Neptune' planet orbiting a star slightly smaller and cooler than our Sun. Despite being about twice the size of Earth and nine times its mass, the planet has a density remarkably similar to our home world. This suggests that TOI-5734b is likely a rocky planet that has lost most of its original atmosphere due to the heat of its nearby young star. Located in a system only about 5...
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Stellar paternity tests: Tracing runaway stars back to their galactic nurseries
icon22. 2. 2026
iconStars | Gaia | Massive main-sequence star
Image: Stellar paternity tests: Tracing runaway stars back to their galactic nurseries
Most massive stars are born within crowded clusters in the flat disk of our Milky Way, yet some are found drifting far above or below this plane. By tracing the movements of 39 high-latitude B-type stars and nearly 450 star clusters using Gaia satellite data, researchers have successfully linked five of these 'orphaned' stars to their original birthplaces. These stars were likely kicked out of their home clusters millions of years ago at high...
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Chandra telescope captures first image of a protective bubble around a Sun-like star
icon22. 2. 2026
iconStars | Chandra | Sun-like star
Image: Chandra telescope captures first image of a protective bubble around a Sun-like star
Astronomers using the Chandra X-ray Observatory have achieved a scientific first by resolving the 'astrosphere'—a protective bubble created by stellar winds—around a young, Sun-like star named HD 61005. Located about 119 light-years away, this star is a much more active version of our own Sun as it appeared in its youth. The study revealed a glowing halo of X-rays extending 220 astronomical units wide, caused by the star's wind crashing into t...
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Detailed analysis of WASP-31 b's atmosphere and orbital alignment
icon21. 2. 2026
iconStars | Exoplane
Image: Detailed analysis of WASP-31 b
A new study using the ESPRESSO spectrograph has provided a precise look at the giant exoplanet WASP-31 b. Researchers confirmed that the planet’s orbit is nearly perfectly aligned with its star's rotation. While attempting to scan the planet's atmosphere for chemical elements, the team found that the signal was heavily obscured by distortions caused by the planet passing in front of its star. Although previously suggested elements like potassium ...
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Discovery of two warm planets smaller than Saturn orbiting solar-type stars
icon21. 2. 2026
iconStars | Exoplanets | TESS
Image: Discovery of two warm planets smaller than Saturn orbiting solar-type stars
Researchers have discovered two new gas giant planets, TOI-883 b and TOI-899 b, which are similar in mass to a 'light' Saturn. These 'warm' giants orbit stars very much like our own Sun with orbital periods of approximately 10 and 11 days. Despite their similar sizes and environments, the two planets appear to have different internal compositions. This suggests they may have followed different evolutionary paths, providing a unique opportunit...
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Chemical traces of a hidden world: Silicon sulfide hints at a protoplanet in the PDS 66 disk
icon16. 2. 2026
iconStars | Exoplanets | Young Stellar Objects | Planet formatio
Image: Chemical traces of a hidden world: Silicon sulfide hints at a protoplanet in the PDS 66 disk
Astronomers using the ALMA telescope have detected rare molecules of silicon sulfide (SiS) in the dusty disk surrounding the young star PDS 66. This chemical signature is highly unusual because these molecules normally freeze onto dust grains in the cold reaches of a planetary system. The detection of a warm, compact source of SiS gas about 60 astronomical units from the star suggests the presence of a 'protoplanet'—a planet still in the proc...
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Discovery of NGTS-38 b: A rare warm super-Jupiter with a 180-day orbit
icon16. 2. 2026
iconStars | Exoplanets | Hot Jupiter | TESS
Image: Discovery of NGTS-38 b: A rare warm super-Jupiter with a 180-day orbit
Astronomers have discovered a massive gas giant planet, NGTS-38 b, orbiting a bright, metal-rich star similar to our Sun but slightly hotter. This 'warm super-Jupiter' stands out due to its unusually long orbital period of 180.5 days, which is much longer than most planets discovered by the transit method. Unlike the scorched 'hot Jupiters' that orbit their stars in just a few days, NGTS-38 b maintains a relatively cool equilibrium temperatur...
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Using intensity interferometry to double-check the size of Red Clump stars
icon15. 2. 2026
iconStar
Image: Using intensity interferometry to double-check the size of Red Clump stars
Scientists are testing a specialized method called intensity interferometry to measure the precise physical dimensions of 'Red Clump' stars, such as HD 17652. These aging stars are vital benchmarks used to calculate distances across the universe, including the gap between us and the Large Magellanic Cloud. By analyzing how light interferes at different wavelengths, researchers can map the stellar surface and account for 'limb darkening'—the e...
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Probing the magnetic field of a mysterious neutron star in a massive binary system
icon15. 2. 2026
iconStars | NuSTAR | Supergiants | Neutron star
Image: Probing the magnetic field of a mysterious neutron star in a massive binary system
Using the NuSTAR space telescope, researchers have performed a deep analysis of the X-ray binary 4U 1700-37, a system where a compact object—likely a neutron star—is pulling material from a massive supergiant star HD 153919. By studying the high-energy light emitted as this material falls toward the object, the team looked for 'cyclotron lines,' which act as a direct probe of a star's magnetic strength. While no rhythmic pulses were found, th...
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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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