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Latest astronomy nachricht

Bleiben Sie auf dem Laufenden mit den neuesten Astronomie-Nachrichten, Entdeckungen über Sterne und Exoplaneten sowie aktuellen Forschungsergebnissen. Entdecken Sie neue Artikel aus der Welt der Astronomie.
Observations of planet LHS 1140 b show no persistent signs of helium escape
icon23. 8. 2026
iconSterne | Exoplaneten | James-Webb-Weltraumtelesko
Image: Observations of planet LHS 1140 b show no persistent signs of helium escape
Recent observations of the temperate planet LHS 1140 b have provided new insights into its atmosphere. While previous data suggested the presence of helium escaping from the planet, detailed analysis of four planetary transits—the period when a planet passes in front of its star—reveals no consistent evidence of such activity, indicating that earlier detections may have been influenced by stellar changes or instrumental factors. Researchers examined the light from the star LHS 1140 during tra...
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Asymmetric aerosol distribution observed on the warm Saturn planet WASP-69 b
icon23. 8. 2026
iconSterne | Exoplaneten | James-Webb-Weltraumtelesko
Image: Asymmetric aerosol distribution observed on the warm Saturn planet WASP-69 b
The warm Saturn-sized exoplanet WASP-69 b exhibits significant atmospheric differences between its morning and evening sides. New observations reveal an asymmetric distribution of aerosols—tiny particles suspended in the atmosphere—which create distinct cloud conditions across the planet. This discovery helps explain how planets at temperatures near 1,000 Kelvin manage the cycle of cloud formation and evaporation as material travels around the gl...
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Geometric model explains the brightness temperature of planet 55 Cancri e
icon13. 8. 2026
iconSterne | Exoplanete
Image: Geometric model explains the brightness temperature of planet 55 Cancri e
The thermal characteristics of 55 Cancri e, an ultra-short period rocky planet, are better understood by accounting for the planet’s three-dimensional geometry and its rotation. By calculating how sunlight hits the planet at various angles throughout its day, it is possible to model the temperature distribution across its surface more accurately. This approach clarifies why the planet exhibits a specific thermal imprint observed by telescope meas...
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Sulfur-rich atmosphere of planet AF Lep b reveals history of solid accretion
icon13. 8. 2026
iconSterne | Exoplaneten | Planetenatmosphäre
Image: Sulfur-rich atmosphere of planet AF Lep b reveals history of solid accretion
AF Lep b is a young gas giant planet with a mass roughly three to four times that of Jupiter, orbiting its host star at a distance of approximately 9 astronomical units. Recent observations using the James Webb Space Telescope have allowed for a detailed look at the chemical composition of its atmosphere, providing new insights into how this massive planet formed and grew during the early stages of its solar system. The research team analyzed ...
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Formation of giant planets PDS 70 c and SR 12 c mirrors our solar system
icon13. 8. 2026
iconSterne | Exoplaneten | Planetenentstehu
Image: Formation of giant planets PDS 70 c and SR 12 c mirrors our solar system
The young planetary systems PDS 70 and SR 12 provide new insights into how giant planets and their moons form. By studying the dust disks surrounding the planets PDS 70 c and SR 12 c, it is clear that these distant worlds share significant similarities with the development of Jupiter and Saturn. These observations help explain how gas and dust accumulate to form planets and smaller satellites in the early stages of a star system's life. The pl...
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Two warm saturn-mass planets found orbiting the star TOI-3850
icon13. 8. 2026
iconSterne | Exoplaneten | TESS | Sonnähnliche Sterne
Image: Two warm saturn-mass planets found orbiting the star TOI-3850
A multi-planet system has been identified orbiting TOI-3850, a G0 dwarf star similar in metallicity to our Sun. The system contains two warm planets—gas-rich worlds that orbit closer to their star than Jupiter, but further than the extremely hot planets commonly found in close proximity to their hosts. These planets are currently situated near a gravitational configuration known as a 2:1 mean motion resonance, where the outer planet completes one...
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Radial velocity analysis characterizes planetary systems around DMPP-7 HD 67200 and HD 2134
icon13. 8. 2026
iconSterne | Exoplanete
Image: Radial velocity analysis characterizes planetary systems around DMPP-7 HD 67200 and HD 2134
Recent observations have analyzed the environments around three stars - DMPP-7, HD 67200, and HD 2134 — to search for evidence of orbiting planets. By studying radial velocity, which measures the tiny wobbles in a star’s position caused by the gravitational tug of an orbiting planet, the project examined these systems to distinguish between genuine planetary signals and the natural activity of the stars themselves. The researchers used a Bayes...
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Analysis of dust rings in the protoplanetary disk around LkCa 15
icon10. 8. 2026
iconSterne | Exoplaneten | Planetenentstehu
Image: Analysis of dust rings in the protoplanetary disk around LkCa 15
Protoplanetary disks are vast, swirling clouds of gas and dust surrounding young stars that eventually coalesce to form planets. A new method has been developed to analyze the physical properties of these disks by examining how their dust rings appear when viewed at an angle. By studying these shapes, researchers can determine the intrinsic width, thickness, and light-blocking capacity, known as optical depth, of the dust material within the disk...
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Lambda Bootis phenomenon identified in the massive early B-type star HD 37356
icon10. 8. 2026
iconSterne | Massereiche Hauptreihensterne
Image: Lambda Bootis phenomenon identified in the massive early B-type star HD 37356
The Lambda Bootis phenomenon is a unique chemical condition in stars where certain elements, known as refractory elements (materials that condense at high temperatures, such as iron), are significantly less abundant than expected, while volatile elements remain at normal levels. This feature has now been identified in the massive early B-type star HD 37356, marking the first time this characteristic has been observed in such a massive stellar obj...
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Evaporating planet explains gaseous disk formation around white dwarf WD J0914+1914
icon9. 8. 2026
iconSterne | Exoplaneten | Rote Zwerge
Image: Evaporating planet explains gaseous disk formation around white dwarf WD J0914+1914
The white dwarf WD J0914+1914 is surrounded by a ring of gas containing hydrogen, oxygen, and sulfur. This material originates from a nearby Neptune-like or super-puff planet—a planet with a very low density—that is losing its atmosphere due to intense radiation from the star. The escaping gas forms a disk around the star, which is then slowly pulled onto the white dwarf's surface, creating the unique light signals observed by instruments. Adv...
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Neu entdeckte Exoplaneten

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

Durchsuchen Sie die neuesten wissenschaftlichen Studien zu Sternen und Exoplaneten in unserer Galaxie. Entdecken Sie die neuesten Forschungsergebnisse zur Astrophysik und Sternastronomie.

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

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

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

DM Tauri
470 ly
study icon Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+
15. 10. 2026

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
15. 10. 2026

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
15. 10. 2026

HAT-P-18
527 ly
study icon ExoEcho: Exoplanet Ephemerides Change Observations. III. A JWST Survey for Transit Timing Variations of 37 Exoplanets
15. 10. 2026

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
15. 10. 2026

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
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