Precession Models
Precession Models is a theoretical framework in astrometry that describes the gradual, long-term changes in the orientation of a celestial body's rotational axis due to gravitational perturbations, distinguishing it from other astronomical reference corrections by specifically accounting for the slow conical motion of the Earth's polar axis over millennia within the context of reference frame and ephemeris computations.
138
Publications
6.1K
Citations
1.3K
Authors
333
Institutions
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2017–2026
26
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Precession of Mercury’s Perihelion from Ranging to the MESSENGER Spacecraft
Ryan S. Park, W. M. Folkner, Alexander S. Konopliv et al. · The Astronomical Journal · 2017 · 208 citations
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
13 h-index
30 publications
1.4K citations
Systèmes de Référence Temps-Espace
Paris, France
10 h-index
20 publications
883 citations

Observatoire de Paris
Paris, France
9 h-index
15 publications
804 citations
Jet Propulsion Laboratory
Pasadena, United States
9 h-index
14 publications
1.4K citations
Massachusetts Institute of Technology
Cambridge, United States
7 h-index
51 publications
7K citations

Sorbonne Université
Paris, France
7 h-index
16 publications
1.5K citations

Rutherford Appleton Laboratory
Didcot, United Kingdom
6 h-index
6 publications
480 citations
California Institute of Technology
Pasadena, United States
6 h-index
88 publications
14.1K citations
1–8 of 333
11 publications · 418 citations
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10 publications · 266 citations
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9 publications · 282 citations
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AJ · 8 publications · 424 citations
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PRD · 5 publications · 329 citations
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