Wobble Motion
Wobble Motion is a geophysical phenomenon characterized by small, quasi-periodic deviations in the rotational axis of a planet relative to its crust, caused by the redistribution of mass and external gravitational torques, distinguishing it from steady rotational or orbital motion.
268
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12.4K
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712
Authors
327
Institutions
Publications per year
2017–2026
30
Parents
268
Five Planets Orbiting 55 Cancri
Debra A. Fischer, Geoffrey W. Marcy, R. Paul Butler et al. · The Astrophysical Journal · 2008 · 262 citations · Full text
Natural Sciences, Astronomy, Physics +15
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327

Centre National de la Recherche Scientifique
Paris, France
10 h-index
24 publications
1K citations
The University of Tokyo
Tokyo, Japan
9 h-index
16 publications
276 citations
Institute of Geodesy and Geophysics
Wuhan, China
7 h-index
13 publications
381 citations
Case Western Reserve University
Cleveland, United States
7 h-index
21 publications
873 citations
Massachusetts Institute of Technology
Cambridge, United States
6 h-index
7 publications
839 citations
GFZ Helmholtz Centre for Geosciences
Potsdam, Germany
6 h-index
13 publications
781 citations

Observatoire de Paris
Paris, France
6 h-index
7 publications
113 citations
Columbia University
New York, United States
6 h-index
8 publications
918 citations
1–8 of 327
GJI · 30 publications · 1.6K citations
21
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JGR · 25 publications · 1.9K citations
21
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9 publications · 258 citations
9
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7 publications · 265 citations
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ApJ · 6 publications · 608 citations
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