Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufm.g51a0804h&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #G51A-0804
Physics
0726 Ice Sheets, 1236 Rheology Of The Lithosphere And Mantle (7218, 8160), 1621 Cryospheric Change (0776), 5450 Orbital And Rotational Dynamics (1221), 6225 Mars
Scientific paper
Secular obliquity variations due to climate friction on Mars are calculated. Martian interior is considered to be a three-layered structure. A viscosity of each layer is treated as a parameter. The results give knowledge as follows. First, under an internal structure with a crust of ``finite viscosity'' and/or a ``solid'' core, the effect of the climate friction becomes greater than that concluded by previous research. Second, under an internal structure with a mantle of ``heterogeneous viscosity'' the possibility of the great effect of the climate friction becomes stronger than that concluded by previous research.
Harada Yoshifumi
Heki Kosuke
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