Latest astronomy Новости

Observations of the 5-million-year-old star HD 152384 have revealed a thin, gaseous ring composed of refractory elements. Located near the star's dust sublimation radius, this ring likely formed from the collisions of rocky planetesimals. This system provides a unique glimpse into the early, violent processes of planet formation and the evolution of debris disks around young stars....

Observations of the hot Jupiter KELT-2A b using the Gemini-North telescope confirm the presence of water vapor in its atmosphere. By analyzing its chemical makeup, researchers found that the carbon-to-oxygen ratio matches its host star, while overall metallic elements appear depleted. This unique chemical profile suggests the planet likely formed far from its star before migrating inward through a high-eccentricity path....

Researchers have used the James Webb Space Telescope to monitor the transit timings of 37 exoplanets. Among the findings, the Neptune-like planet HAT-P-18 b displays a periodic signal in the timing of its transits, suggesting complex planetary dynamics. These observations highlight the telescope's ability to track subtle orbital changes across various types of planets....

The exoplanet TOI-2257 b orbits its host star every 35 days with a highly eccentric path. New simulations show the planet sits near a critical boundary where tidal forces and atmospheric escape processes transition. Depending on whether the planet is a gaseous mini-Neptune or a rocky super-Earth, it may retain a significant hydrogen envelope or maintain conditions potentially suitable for liquid water....

Researchers have measured the mass of HD 203771 b, a rare brown dwarf orbiting an orange dwarf star. By combining precise astrometry and radial velocity data, the study confirms the companion has a mass roughly 70 times that of Jupiter. The analysis also explores how brown dwarfs migrate inward over time, suggesting that disk friction plays a key role in shaping their final orbital paths....

The star HD 158485, used to calibrate the James Webb Space Telescope, has been identified as a binary system. By analyzing light fluctuations from two pulsating stars in the pair, researchers calculated the orbital characteristics of the system. This finding is significant because the presence of an unseen companion star can alter the expected brightness data used for astronomical observations....

Observations of the ultrahot Jupiter KELT-18 b confirm that the planet is losing its atmosphere. By using high-resolution spectroscopy, researchers detected a signature of metastable helium escaping from the planet. This finding highlights the intense photoevaporation occurring on the massive gas giant as it orbits its host star....

Researchers have mapped the three-dimensional atmospheric structure of the hot Jupiter WASP-17 b. By observing the planet as it transits its star, the data reveals a stark 650 Kelvin temperature difference between the planet's morning and evening limbs. These results provide new insights into the complex dynamics and chemical distribution within the atmospheres of giant gas planets orbiting distant stars....

New analysis of the nearby orange dwarf HD 219134 refines its physical dimensions and age. By applying advanced seismic modeling, this study resolves previous disagreements regarding the star's radius and offers a clearer look at how high-energy radiation has shaped the atmospheres of its orbiting planets over nearly nine billion years....