Zobrazeno 1 - 10
of 201
pro vyhledávání: '"Reinhardt, Christian"'
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
We investigate mantle stripping giant impacts (GI) between super-Earths with masses between 1 M$_{\oplus}$ and 20 M$_{\oplus}$. We infer new scaling laws for the mass of the largest fragment and its iron mass fraction, as well as updated fitting coef
Externí odkaz:
http://arxiv.org/abs/2204.04925
Autor:
Woo, Jason Man Yin, Reinhardt, Christian, Cilibrasi, Marco, Chau, Alice, Helled, Ravit, Stadel, Joachim
The formation of Uranus' regular moons has been suggested to be linked to the origin of its enormous spin axial tilt (~98^o). A giant impact between proto-Uranus and a 2-3 M_Earth impactor could lead to a large tilt and to the formation of an impact
Externí odkaz:
http://arxiv.org/abs/2105.13663
Publikováno v:
MNRAS 505.2 (2021) 1806-1816
We investigate how the choice of equation of state (EOS) and resolution conspire to affect the outcomes of giant impact (GI) simulations. We focus on the simple case of equal mass collisions of two Earth-like $0.5\,M_\oplus$ proto-planets showing tha
Externí odkaz:
http://arxiv.org/abs/2104.03559
Autor:
Grün, Borghild, Windsheim, Bad, Dargel, Stefan, Ludwig, Katarina, Roux, Andrés de, Otto-Knapp, Ralf, Lode, Hartmut, Gogoll, Christian, Probst, Meike, Herrmann, Frank, Overlack, Axel, Pabst, Stefan, Sommerwerck, Urte, Vehar, Köln; Harald, Blaas, Stefan, Schaaf, Bernhard, Kolditz, Martin, Sutharsan, Sivagurunathan, Kardos, Essen; Peter, Grünewaldt, Achim, Sorichter, Stephan, Scholz, Tobias, Idzko, Marco, Mohadjer, Moritz, Eisenmann, Stephan, Aries, Sven P., Lauer-Hermfisse, Johannes, Kampf, Sabine, Ringshausen, Felix C., Wege, Sabine, Herth, Felix, Ewig, Santiago, Reinhardt, Christian, Andreas, Stefan, Schumann, Christian, Bobis, Ingrid, Bahmer, Thomas, Fey, Kiel; Rita, Jüch, Martin, Kempa, Lostau; Axel T., Piirsoo, Erika, Klapdor, Benjamin, Mertsch, Pontus, Schmidt, Bernhard, Hein, Holger, Haidl, Peter, Gamarra, Jorge Fernando, Ewen, Raphael, Pink, Isabell, Shoemark, Amelia, Staar, Ben O., Rademacher, Jessica
Publikováno v:
In Chest
The origin of Uranus and Neptune remains a challenge for planet formation models. A potential explanation is that the planets formed from a population of a few planetary embryos with masses of a few Earth masses which formed beyond Saturn's orbit and
Externí odkaz:
http://arxiv.org/abs/2009.10100
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
European Journal of Marketing, 2022, Vol. 56, Issue 13, pp. 78-104.
Externí odkaz:
http://www.emeraldinsight.com/doi/10.1108/EJM-10-2020-0750
Despite many similarities, there are significant observed differences between Uranus and Neptune: while Uranus is tilted and has a regular set of satellites, suggesting their accretion from a disk, Neptune's moons are irregular and are captured objec
Externí odkaz:
http://arxiv.org/abs/1907.09809
Autor:
Deng, Hongping, Ballmer, Maxim D., Reinhardt, Christian, Meier, Matthias M. M., Mayer, Lucio, Stadel, Joachim, Benitez, Federico
The giant impact hypothesis for Moon formation successfully explains the dynamic properties of the Earth-Moon system but remains challenged by the similarity of isotopic fingerprints of the terrestrial and lunar mantles. Moreover, recent geochemical
Externí odkaz:
http://arxiv.org/abs/1904.02407