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pro vyhledávání: '"Timpe, Miles"'
In the leading theory of lunar formation, known as the giant impact hypothesis, a collision between two planet-size objects resulted in a young Earth surrounded by a circumplanetary debris disk from which the Moon later accreted. The range of giant i
Externí odkaz:
http://arxiv.org/abs/2409.02746
In the leading theory of lunar formation, known as the giant impact hypothesis, a collision between two planet-size objects resulted in a young Earth surrounded by a circumplanetary debris disk from which the Moon later accreted. The range of giant i
Externí odkaz:
http://arxiv.org/abs/2307.06078
Recent improvements to GPU hardware and the symplectic N-body code GENGA allow for unprecedented resolution in simulations of planet formation. In this paper, we report results from high-resolution N-body simulations of terrestrial planet formation t
Externí odkaz:
http://arxiv.org/abs/2109.03650
In the late stages of terrestrial planet formation, pairwise collisions between planetary-sized bodies act as the fundamental agent of planet growth. These collisions can lead to either growth or disruption of the bodies involved and are largely resp
Externí odkaz:
http://arxiv.org/abs/2001.09542
Publikováno v:
A&A 621, A125 (2019)
During their formation and early evolution, rocky planets undergo multiple global melting events due to accretionary collisions with other protoplanets. The detection and characterization of their post-collision afterglows (magma oceans) can yield im
Externí odkaz:
http://arxiv.org/abs/1811.07411
Akademický článek
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Autor:
Timpe, Miles, Barnes, Rory, Kopparapu, Ravikumar, Raymond, Sean N., Greenberg, Richard, Gorelick, Noel
If mutual gravitational scattering among exoplanets occurs, then it may produce unique orbital properties. For example, two-planet systems that lie near the boundary between circulation and libration of their periapses could result if planet-planet s
Externí odkaz:
http://arxiv.org/abs/1307.4761