Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Robin M. Canup"'
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 1, p 9 (2024)
The amount of vapor in the impact-generated protolunar disk carries implications for the dynamics, devolatilization, and moderately volatile element isotope fractionation during lunar formation. The equation of state (EoS) used in simulations of the
Externí odkaz:
https://doaj.org/article/70988f8a08aa4ce2a5c431e0ee5d4260
Autor:
Simon B. Porter, Robin M. Canup
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 7, p 120 (2023)
We present a new orbit and mass solution for the four small satellites of Pluto: Styx, Nix, Kerberos, and Hydra. We have reanalyzed all available observations of the Pluto system obtained by the Hubble Space Telescope from 2005 to 2019 with the ACS,
Externí odkaz:
https://doaj.org/article/ceb0b5d1e3344e5984f5a06ceec0850a
Autor:
Alex N. Halliday, Robin M. Canup
Publikováno v:
Nature Reviews Earth & Environment. 4:19-35
Autor:
Raluca Rufu, Robin M. Canup
The origin of the Uranian satellite system remains uncertain. The four major satellites have nearly circular, coplanar orbits, and the ratio of the satellite system to planetary mass resembles Jupiter’s satellite system, suggesting the Uranian syst
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32b68c54063dc4e437a5ca3a3c5af168
http://arxiv.org/abs/2204.00124
http://arxiv.org/abs/2204.00124
Autor:
Robin M. Canup, Raluca Rufu
Publikováno v:
Journal of Geophysical Research: Planets. 125
Forming the Moon by a high-angular momentum impact may explain the Earth-Moon isotopic similarities, however, the post-impact angular momentum needs to be reduced by a factor of 2 or more to the current value (1 L_EM) after the Moon forms. Capture in
Publikováno v:
Journal of geophysical research. Planets
A high-angular momentum giant impact with the Earth can produce a Moon with a silicate isotopic composition nearly identical to that of Earth’s mantle, consistent with observations of terrestrial and lunar rocks. However, such an event requires sub
The goal of this chapter is to review hypotheses for the origin of the Pluto system in light of observational constraints that have been considerably refined over the 85-year interval between the discovery of Pluto and its exploration by spacecraft.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::038eb96bcf5d63f31745ecc6b1509d6a
https://doi.org/10.2458/azu_uapress_9780816540945-ch021
https://doi.org/10.2458/azu_uapress_9780816540945-ch021
Publikováno v:
Nature geoscience. 8
The Moon may have formed from an Earth-orbiting disk of vapor and melt produced by a giant impact.(1) The Moon and Earth’s mantles have similar compositions. However, it is unclear why lunar samples are more depleted in volatile elements than terre
Publikováno v:
Science Advances
A few early, large collisions on Mars may be responsible for heterogeneity in tungsten and platinum in martian meteorites.
The approximately chondritic estimated relative abundances of highly siderophile elements (HSE) in the bulk martian mantle
The approximately chondritic estimated relative abundances of highly siderophile elements (HSE) in the bulk martian mantle
Autor:
Julien Salmon, Robin M. Canup
Publikováno v:
Science Advances
Phobos and Deimos are likely remnants of a low-mass disk generated by the impact of a Vesta to Ceres-sized body with Mars.
It has been proposed that Mars’ moons formed from a disk produced by a large impact with the planet. However, whether su
It has been proposed that Mars’ moons formed from a disk produced by a large impact with the planet. However, whether su