Obliquity Variations
Obliquity Variations is a geophysical construct that quantifies the temporal changes in the axial tilt of a planet relative to its orbital plane, distinguishing it from static obliquity by characterizing the dynamic evolution of rotational orientation over astronomical timescales.
135
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8.1K
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423
Authors
253
Institutions
Publications per year
2017–2026
34
Parents
135
S. J. Peale · The Astronomical Journal · 1969 · 270 citations
Natural Sciences, Astronomy, Physics +17
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Institut de Mécanique Céleste et de Calcul des Éphémérides, France
4 publications · 373 citations
4
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1–5 of 423
253

Centre National de la Recherche Scientifique
Paris, France
13 h-index
39 publications
1.7K citations
Princeton University
Princeton, United States
9 h-index
17 publications
1.2K citations

Ames Research Center
Mountain View, United States
7 h-index
9 publications
343 citations
Goddard Space Flight Center
Greenbelt, United States
7 h-index
7 publications
391 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
6 h-index
11 publications
307 citations
Utrecht University
Utrecht, The Netherlands
6 h-index
21 publications
1.7K citations
California Institute of Technology
Pasadena, United States
5 h-index
8 publications
624 citations

Université Paris Sciences et Lettres
Paris, France
5 h-index
10 publications
324 citations
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AJ · 15 publications · 776 citations
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JGR · 11 publications · 1.2K citations
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ApJ · 8 publications · 571 citations
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8 publications · 431 citations
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6 publications · 374 citations
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