50 citations · 120 across the 5 of their papers we have counts for
5 papers
Runaway climate cooling of ocean planets in the habitable zone: a consequence of seafloor weathering enhanced by melting of high-pressure ice
Akifumi Nakayama, Takanori Kodama, Masahiro Ikoma +1
Terrestrial planets covered globally with thick oceans (termed ocean planets) in the habitable zone were previously inferred to have extremely hot climates in most cases. This is b…
Impact Erosion Model for Gravity-Dominated Planetesimals
H. Genda, T. Fujita, H. Kobayashi +3
Disruptive collisions have been regarded as an important process for planet formation, while non-disruptive, small-scale collisions (hereafter called erosive collisions) have been…
Rapid Water Loss can Extend the Lifetime of the Planetary Habitability
T. Kodama, H. Genda, Y. Abe +1
Two habitable planetary states are proposed: an aqua planet like the Earth and a land planet that has a small amount of water. Land planets keep liquid water under larger solar rad…
Resolution Dependence of Disruptive Collisions between Planetesimals in the Gravity Regime
H. Genda, T. Fujita, H. Kobayashi +2
Collisions are a fundamental process in planet formation. If colliding objects simply merge, a planetary object can grow. However, if the collision is disruptive, planetary growth…
Lifetime and Spectral Evolution of a Magma Ocean with a Steam Atmosphere: Its Detectability by Future Direct Imaging
Keiko Hamano, Hajime Kawahara, Yutaka Abe +2
We present the thermal evolution and emergent spectra of solidifying terrestrial planets along with the formation of steam atmospheres. The lifetime of a magma ocean and its spectr…