GAUSS - genesis of asteroids and evolution of the solar system

Exoplanet searches have found that roughly half of all Sun-like stars have one or more planets with radii of 1?4 Earth radii and orbital periods.







Planets and Astrobiology
The atmospheric substellar absorption of M-dwarf radiation on an Earth-like planet is stronger than for F- or G-dwarf instellation (Shields ...
The Habitability of Planets Orbiting M-dwarf Stars - SciSpace
From our joint analysis, we found the host TOI-6894 to be a M5. 0 ± 0.5 dwarf star with a radius of 0.2276 ± 0.0057 R? and a mass of 0.207 ± 0.011 M?, a very ...
2. Minor Planets and Asteroids - Astroshop.eu
The goal of Project GAUSS (Genesis of Asteroids and evolUtion of the Solar Sys- tem) is to return samples from the dwarf planet Ceres. Ceres is ...



Autres Cours:

The habitability of planets orbiting M-dwarf stars - eScholarship