[University of Chicago] In the search for extraterrestrial life, it makes sense to first look for rocky planets with an atmosphere, like Earth. Without an atmosphere, a planet can’t have […]
HD 3167 b
Posted inAstrogeology, Biogeochemical Cycles & Geobiology, Lava / magma ocean / Volcanic Worlds, Status Report
Coupled Orbital And Interior Structure Evolution Of Lava Planets
Lava planets likely did not form in their current orbits, instead migrating inward via orbital decay, which influenced the evolution of their magma oceans.
Posted inAtmospheres, Climate, Weather, Biosignatures & Paleobiology, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Lava / magma ocean / Volcanic Worlds, Status Report
An Atmosphere On The Ultra-Short Period Super-Earth HD 3167 b
‘Lava worlds’-Earth-sized planets hot enough (Teq >~ 1100 K) to melt their dayside silicate surfaces-have emerged as promising candidates for atmospheric detection and characterization. Thermal emission observations show an apparent […]
