Rogue planet moons may harbor life for billions of years

Moons orbiting rogue planets could maintain liquid water oceans for up to 4.3 billion years through tidal heating and hydrogen-rich atmospheres. Researchers from Ludwig Maximilian University of Munich and the Max Planck Institute for Extraterrestrial Physics reached this conclusion in a new study.

Rogue planets, also known as free-floating planets, are worlds ejected from their original solar systems. They travel through interstellar space without orbiting a star. Previous research indicated that some of these planets can retain moons despite the chaotic ejection process. Those moons often end up in elongated orbits that generate internal heat through gravitational stretching and squeezing, known as tidal heating.

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A team led by Professor Lisa Kaltenegger at Cornell University has pinpointed 45 rocky exoplanets in the habitable zones of their stars, where liquid water might exist. The research, drawing on data from ESA's Gaia mission and NASA's Exoplanet Archive, highlights prime targets for the search for extraterrestrial life. Published in Monthly Notices of the Royal Astronomical Society, the study also notes 24 additional candidates in a stricter habitable zone.

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Astronomers have found a planetary system around a red dwarf star where a rocky world orbits beyond two gas giants, challenging standard models of how planets form. The discovery around LHS 1903 suggests planets may arise sequentially rather than all at once.

Astronomers have identified a rare planetary system 190 light-years from Earth featuring a hot Jupiter sharing its orbit with a mini-Neptune closer to the star. This configuration was once considered nearly impossible. New observations from the James Webb Space Telescope provide fresh insights into how the planets formed.

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Scientists have found that localized dust storms on Mars can drive water vapor into the upper atmosphere, where it breaks apart and escapes into space. The discovery, based on observations from multiple Mars orbiters, challenges prior assumptions about when and how the planet loses water. Researchers link the effect to an intense regional storm during the Northern Hemisphere summer.

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