The growth of embryos considering SPH-collision studies

Elke Pilat-Lohinger; Thomas Maindl; David Bancelin; Christoph Schäfer

The growth of embryos considering SPH-collision studies

Elke Pilat-Lohinger
, Thomas Maindl
, David Bancelin
, Christoph Schäfer

Department of Astrophysics

Publications: Contribution to book › Contribution to proceedings

Abstract

To get more realistic results for terrestrial planet formation we combine N-body simulations with SPH collision studies. In this context we show the mass-loss and water-loss for Moon- and Mars-size bodies after collision where we consider various impact angles which have been determined in N-body simulations.

Original language	English
Title of host publication	EPSC-DPS Joint Meeting 2019
Volume	13
Publication status	Published - Sept 2019

Austrian Fields of Science 2012

103003 Astronomy
103004 Astrophysics

Access to Document

http://adsabs.harvard.edu/abs/2019EPSC...13.1760P

Cite this

@inproceedings{7c99db3b854e4295bc1201241a7a3a10,

title = "The growth of embryos considering SPH-collision studies",

abstract = "To get more realistic results for terrestrial planet formation we combine N-body simulations with SPH collision studies. In this context we show the mass-loss and water-loss for Moon- and Mars-size bodies after collision where we consider various impact angles which have been determined in N-body simulations.",

author = "Elke Pilat-Lohinger and Thomas Maindl and David Bancelin and Christoph Sch{\"a}fer",

year = "2019",

month = sep,

language = "English",

volume = "13",

booktitle = "EPSC-DPS Joint Meeting 2019",

}

TY - GEN

T1 - The growth of embryos considering SPH-collision studies

AU - Pilat-Lohinger, Elke

AU - Maindl, Thomas

AU - Bancelin, David

AU - Schäfer, Christoph

PY - 2019/9

Y1 - 2019/9

N2 - To get more realistic results for terrestrial planet formation we combine N-body simulations with SPH collision studies. In this context we show the mass-loss and water-loss for Moon- and Mars-size bodies after collision where we consider various impact angles which have been determined in N-body simulations.

AB - To get more realistic results for terrestrial planet formation we combine N-body simulations with SPH collision studies. In this context we show the mass-loss and water-loss for Moon- and Mars-size bodies after collision where we consider various impact angles which have been determined in N-body simulations.

M3 - Contribution to proceedings

VL - 13

BT - EPSC-DPS Joint Meeting 2019

ER -

The growth of embryos considering SPH-collision studies

Abstract

Austrian Fields of Science 2012

Access to Document

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Cite this