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Making More Terrestrial Planets

Icarus, 2001
The results of 16 new 3D N-body simulations of the final stage of the formation of the terrestrial planets are presented. These Nbody integrations begin with 150‐160 lunar-to-Mars size planetary embryos, with semi-major axes 0.3< a < 2.0 AU, and include perturbations from Jupiter and Saturn.
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The Strangest Terrestrial Planet

Science, 2012
NASA's MESSENGER mission previously revealed that Mercury has a volcanic crust; now it finds evidence for an inner “anticrust.”
openaire   +1 more source

A wide-orbit giant planet in the high-mass b Centauri binary system

Nature, 2021
Markus Janson   +2 more
exaly  

Terrestrial planets

2015
Vadym Kaydash   +3 more
openaire   +1 more source

Climates of terrestrial planets

2016
Suppose we detect a planet half the size of Venus orbiting a 5 billion year old M-type star at 0.5 AU. To our surprise the planet has detectable radiation belts. How might the planet's climate and surface habitability differ from that of Venus? The prospect that the scientific community might be faced in the next decade or two with questions like the
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High atmospheric metal enrichment for a Saturn-mass planet

Nature, 2023
Jacob Bean, Qiao Xue, J L Lunine
exaly  

A planet within the debris disk around the pre-main-sequence star AU Microscopii

Nature, 2020
Peter Plavchan   +2 more
exaly  

Understanding planet formation using microgravity experiments

Nature Reviews Physics, 2021
Gerhard Wurm, Jens Teiser
exaly  

A temperate Earth-sized planet with tidal heating transiting an M6 star

Nature, 2023
Björn Benneke   +2 more
exaly  

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