Virolithopanspermia: Might viruses be transported in rocks through space? [PDF]
PLoS PathogBushman FD.
europepmc +1 more source
Core-envelope miscibility in sub-Neptunes and super-Earths. [PDF]
NatureGilmore T, Stixrude L.
europepmc +1 more source
Improvement of merging processes in N-body simulations in circumstellar disks
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
Constructing the secular architecture of the solar system II: the terrestrial planets [PDF]
Astronomy and Astrophysics, 2009 We investigate the dynamical evolution of the terrestrial planets during the planetesimal-driven migration of the giant planets. A basic assumption of this work is that giant planet migration occurred after the completion of terrestrial planet formation, such as in the models that link the former to the origin of the Late Heavy Bombardment.
Rodney Gomes +2 more
exaly +4 more sources
Building the terrestrial planets: Constrained accretion in the inner Solar System [PDF]
Icarus, 2009 Accepted to Icarus. 21 pages, 12 figures, 5 tables in emulateapj format. Figures 3 and 4 degraded.
Alessandro Morbidelli, Sean Raymond
exaly +3 more sources
Can narrow discs in the inner Solar system explain the four terrestrial planets? [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT A successful Solar system model must reproduce the four terrestrial planets. Here, we focus on (1) the likelihood of forming Mercury and the four terrestrial planets in the same system (a 4-P system); (2) the orbital properties and masses of each terrestrial planet; and (3) the timing of Earth’s last giant impact and the mass ...
Patryk Sofia Lykawka
exaly +3 more sources
Formation of terrestrial planets in disks evolving via disk winds and implications for the origin of the solar system’s terrestrial planets [PDF]
Astronomy and Astrophysics, 2015 8 pages, 4 figures, accepted for publication in A& ...
Takeru Suzuki, Masahiro Ogihara
exaly +3 more sources
Constraining the Formation of the Four Terrestrial Planets in the Solar System [PDF]
Astrophysical Journal, 2019 Abstract To reproduce the orbits and masses of the terrestrial planets (analogs) of the solar system, most studies scrutinize simulations for success as a batch. However, there is insufficient discussion in the literature on the likelihood of forming planet analogs simultaneously in the same system (analog system). To address this issue,
Takashi Itô, Patryk Sofia Lykawka
exaly +3 more sources
Did the terrestrial planets of the solar system form by pebble accretion?
Earth and Planetary Science LettersThe dominant accretion process leading to the formation of the terrestrial planets of the Solar System is a subject of intense scientific debate. Two radically different scenarios have been proposed. The classic scenario starts from a disk of planetesimals which, by mutual collisions, produce a set of Moon to Mars-mass planetary embryos.
Alessandro Morbidelli +2 more
exaly +4 more sources