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 ...
Why do we find ourselves around a yellow star instead of a red star?
We present the discovery and validation of a three-planet system orbiting the nearby (31.1 pc) M2 dwarf star TOI-. 700 (TIC 150428135). TOI-700 lies in the ...
A giant planet candidate transiting a white dwarf
The F-dwarf planet required 108% of the modern solar constant to generate a global mean surface temperature of 287 K, similar to modern-day ...



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Planets and Astrobiology