Obliquity Determination
Obliquity Determination is a methodological framework in planetary science that quantifies the axial tilt of a celestial body relative to its orbital plane by analyzing rotational dynamics and gravitational interactions, distinguishing it from other geophysical inversion techniques through its specific focus on spin-axis orientation and its constraints on interior mass distribution.
104
Publications
10.4K
Citations
339
Authors
223
Institutions
Publications per year
2017–2026
29
Parents
104
A long-term numerical solution for the insolation quantities of the Earth
J. Laskar, Philippe Robutel, F. Joutel et al. · Astronomy and Astrophysics · 2004 · 4.3K citations · Full text
STARSPOTS AND SPIN-ORBIT ALIGNMENT IN THE WASP-4 EXOPLANETARY SYSTEM
The Astrophysical Journal · 2011 · 182 citations · Full text
Natural Sciences, Astronomy, Physics +10
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Massachusetts Institute of Technology
Cambridge, United States
15 h-index
27 publications
2.7K citations
Princeton University
Princeton, United States
11 h-index
21 publications
882 citations

Centre National de la Recherche Scientifique
Paris, France
10 h-index
32 publications
26.3K citations

Aarhus University
Aarhus, Denmark
9 h-index
48 publications
3.9K citations
California Institute of Technology
Pasadena, United States
8 h-index
10 publications
629 citations
University of California, Berkeley
Berkeley, United States
7 h-index
10 publications
952 citations

Pennsylvania State University
State College, United States
7 h-index
10 publications
695 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
8 publications
819 citations
1–8 of 223
AJ · 18 publications · 606 citations
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ApJ · 10 publications · 1K citations
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8 publications · 4.5K citations
8
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5 publications · 309 citations
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5 publications · 235 citations
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