Long-term evolution of the spin of Venus-Reference-Cited by-同舟云学术

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Long-term evolution of the spin of Venus

Published:2003-05 Issue:1 Volume:163 Page:1-23
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Correia Alexandre C.M.,Laskar Jacques,de Surgy Olivier Néron

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference76 articles.

1. Cours de Mécanique Céleste;Andoyer,1923

2. Thermal evolution of Venus;Arkani-Hamed;Phys. Earth Planet. Inter.,1984

3. Preliminary results of an investigation of the light regime in the atmosphere and on the surface of Venus;Avduevskii;Kosmicheskie Issledovaniia,1976

4. Steady fluid flow in a precessing spheroidal shell;Busse;J. Fluid Mech.,1968

5. Study of Venus by CW radar;Carpenter;Astron. J.,1964

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1. The viscosity of Venus’ mantle inferred from its rotational state;Icarus;2024-11

2. Tidal evolution of Earth-like planets in the habitable zone of low-mass stars;Astronomy & Astrophysics;2024-06-28

3. Thermal tides in neutrally stratified atmospheres: Revisiting the Earth’s Precambrian rotational equilibrium;Astronomy & Astrophysics;2024-04

4. Spin Dynamics of Planets in Resonant Chains;The Astrophysical Journal;2024-01-26

5. Venus;Reference Module in Earth Systems and Environmental Sciences;2024

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