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9. 8. 2026
Sterne | Exoplaneten | Rote ZwergeThe exoplanet Ross 128 b, which orbits a nearby Red dwarf star, serves as a primary model for understanding the atmospheres of rocky worlds. By simulating various climate conditions and atmospheric compositions, new research assesses how these planets reflect light, a critical factor for future observations using high-contrast imaging and high-resolution spectroscopy—techniques that separate a planet's light from its host star to analyze its atmosphere.
The research team utilized three-dimens...
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9. 8. 2026Sterne | Exoplaneten | James-Webb-Weltraumteleskop | Planetenatmosphären | TESS | Rote ZwergeThe giant planet TOI-3235 b, which has a mass about two-thirds that of Jupiter and a temperature of 604 Kelvin, orbits a small Red dwarf star. Studying the atmospheres of such massive planets around small, cool stars is important for understanding how they formed, as current theories suggest they should be rare. However, light from the host star often interferes with these observations, creating signals that can be mistaken for atmospheric featur...
Read article 8. 8. 2026Sterne | ExoplaneteThe star TOI-3272 is currently under investigation for hosting a potential hot Jupiter, a massive gas giant planet that orbits extremely close to its host star. Researchers identified this candidate using data from the Transiting Exoplanet Survey Satellite (TESS), which detects the periodic dimming of stars caused by a planet passing in front of them. The system is particularly interesting because the host star appears to be relatively young, wit...
Read article 8. 8. 2026Sterne | Exoplaneten | PlanetenatmosphäreThe TRAPPIST-1 system contains seven Earth-sized planets orbiting a red dwarf star. Studying their atmospheres using transmission spectroscopy—a method where starlight passes through a planet's atmosphere during a transit—is complicated by the star itself. Active regions on the stellar surface, such as starspots, can mimic or mask the signals of atmospheric gases, making it difficult to distinguish between the planet's actual composition and the ...
Read article 8. 8. 2026Sterne | Exoplaneten | PlanetenatmosphäreThe 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 deep...
Read article 4. 8. 2026Sterne | | | ÜberrieseBetelgeuse, 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...
Read article 1. 8. 2026Sterne | Exoplaneten | TESSTOI-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...
Read article 1. 8. 2026Sterne | ExoplaneteClimate 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...
Read article 1. 8. 2026Sterne | Exoplaneten | Rote ZwergeGliese 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...
Read article 1. 8. 2026Sterne | Exoplaneten | PlanetenatmosphäreWASP-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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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 |
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