Zobrazeno 1 - 10
of 148
pro vyhledávání: '"Matsuyama, Isamu"'
Autor:
Hamilton, Christopher W., McEwen, Alfred S., Keszthelyi, Laszlo, Carter, Lynn M., Davies, Ashley G., de Kleer, Katherine, Jessup, Kandis Lea, Jia, Xianzhe, Keane, James T., Mandt, Kathleen, Nimmo, Francis, Paranicas, Chris, Park, Ryan S., Perry, Jason E., Pommier, Anne, Radebaugh, Jani, Sutton, Sarah S., Vorburger, Audrey, Wurz, Peter, Borlina, Cauê, Haapala, Amanda F., DellaGiustina, Daniella N., Denevi, Brett W., Hörst, Sarah M., Kempf, Sascha, Khurana, Krishan K., Likar, Justin J., Masters, Adam, Mousis, Olivier, Polit, Anjani T., Bhushan, Aditya, Bland, Michael, Matsuyama, Isamu, Spencer, John
Jupiter's moon Io is a highly compelling target for future exploration that offers critical insight into tidal dissipation processes and the geology of high heat flux worlds, including primitive planetary bodies, such as the early Earth, that are sha
Externí odkaz:
http://arxiv.org/abs/2408.08334
Publikováno v:
The Planetary Science Journal, 5(5), 129
Body tides reveal information about planetary interiors and affect their evolution. Most models to compute body tides rely on the assumption of a spherically-symmetric interior. However, several processes can lead to lateral variations of interior pr
Externí odkaz:
http://arxiv.org/abs/2311.15710
Isostatic equilibrium is commonly defined as the state achieved when there are no lateral gradients in hydrostatic pressure, and thus no lateral flow, at depth within the lower viscosity mantle that underlies a planetary body's outer crust. In a cons
Externí odkaz:
http://hdl.handle.net/10150/625778
http://arizona.openrepository.com/arizona/handle/10150/625778
http://arizona.openrepository.com/arizona/handle/10150/625778
The goal of this work is to investigate under which circumstances the tidal response of a stratified body can be approximated by that of a homogeneous body. We show that any multilayered planet model can be approximated by a homogeneous body, with th
Externí odkaz:
http://arxiv.org/abs/2303.05253
Autor:
Matsuyama, Isamu, Nimmo, Francis, Keane, James T., Chan, Ngai H., Taylor, G. Jeffrey, Wieczorek, Mark A., Kiefer, Walter S., Williams, James G.
The interior structure of the Moon is constrained by its mass, moment of inertia, and k(2) and h(2) tidal Love numbers. We infer the likely radius, density, and (elastic limit) rigidity of all interior layers by solving the inverse problem using thes
Externí odkaz:
http://hdl.handle.net/10150/621595
http://arizona.openrepository.com/arizona/handle/10150/621595
http://arizona.openrepository.com/arizona/handle/10150/621595
Various theories have been proposed to explain the Moon's current inclined orbit. We test the viability of these theories by reconstructing the thermal-orbital history of the Moon. We build on past thermal-orbital models and incorporate the evolution
Externí odkaz:
http://arxiv.org/abs/2209.00935
Publikováno v:
Planet. Sci. J., 2, 194 (2021)
We present a coupled reorientation and climate model, to understand how true polar wander (TPW) and atmospheric condensation worked together to create the Sputnik Planitia (SP) ice sheet and reorient it to its present-day location on Pluto. SP is loc
Externí odkaz:
http://arxiv.org/abs/2109.11479
Publikováno v:
MNRAS 499 (2020) 40-51
Callisto is thought to possess a subsurface ocean, which will dissipate energy due to obliquity tides. This dissipation should have damped any primordial inclination within 1 Gyr - and yet Callisto retains a present-day inclination. We argue that Cal
Externí odkaz:
http://arxiv.org/abs/2009.05002
Publikováno v:
Geophysical Research Letters, 47, 2020, e2020GL088317
There is compelling evidence for subsurface water oceans among the three outer Galilean satellites, and evidence for an internal magma ocean in the innermost moon, Io. Tidal forces from Jupiter periodically deform these bodies, causing heating and de
Externí odkaz:
http://arxiv.org/abs/2008.02825
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