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Understanding planet formation using microgravity experiments
Nature Reviews Physics, 2021Gerhard Wurm, Jens Teiser
exaly
2016
Planets are thought to form in the circumstellar disks orbiting young stars in formation. According to the core-accretion model, a candidate scenario for Earth-like planets, the interstellar sub-$\mu$m-sized dust particles grow thanks to collisions to mm/cm size and then form km-sized planetesimals via dynamical encounters.
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Planets are thought to form in the circumstellar disks orbiting young stars in formation. According to the core-accretion model, a candidate scenario for Earth-like planets, the interstellar sub-$\mu$m-sized dust particles grow thanks to collisions to mm/cm size and then form km-sized planetesimals via dynamical encounters.
openaire +1 more source
A wide-orbit giant planet in the high-mass b Centauri binary system
Nature, 2021Markus Janson +2 more
exaly
Extrasolar planets and planet formation
Planetary and Space Science, 2007Heike Rauer, Artie Hatzes
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Analysis of lunar samples: Implications for planet formation and evolution
Science, 2019Richard Carlson
exaly
Possible planet formation in the young, low-mass, multiple stellar system GG Tau A
Nature, 2014Stephane Guilloteau +2 more
exaly

