Higher-order Gravity Coefficients
Higher-Order Gravity Coefficients is a mathematical construct in planetary gravity modeling that represents the deviation of a celestial body's gravitational field from spherical symmetry, distinguished by its derivation from terms beyond the second degree in the spherical harmonic expansion of the gravitational potential.
21
Publications
746
Citations
29
Authors
27
Institutions
Publications per year
2017–2026
4
Variants
Higher-degree Gravity Coefficients
Parents
21
The Newtonian limit of fourth and higher order gravity
Astronomische Nachrichten · 1991 · 69 citations · Full text
The gravitational field of Phobos
B. F. Chao, David Parry Rubincam · Geophysical Research Letters · 1989 · 52 citations
Natural Sciences, Astronomy, Physics +16
1–5 of 21
29
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Italy
3 publications · 207 citations
3
h-index
2
h-index
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Italy
2 publications · 186 citations
2
h-index
2
h-index
1
h-index
1–5 of 29
27
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
Naples, Italy
3 h-index
4 publications
348 citations
University of Sussex
Brighton, United Kingdom
2 h-index
4 publications
120 citations
University of Colorado Boulder
Boulder, United States
1 h-index
2 publications
26 citations
University of Pennsylvania
Philadelphia, United States
1 h-index
3 publications
126 citations

University of Warsaw
Warsaw, Poland
1 h-index
3 publications
51 citations
Humboldt-Universität zu Berlin
Berlin, Germany
1 h-index
2 publications
84 citations
Shahid Beheshti University
Tehran, Iran
1 h-index
1 publications
62 citations

Tomsk State University of Control Systems and Radio-Electronics
Tomsk, Russia
1 h-index
1 publications
38 citations
1–8 of 27
4 publications · 138 citations
4
h-index
3 publications · 78 citations
3
h-index
2 publications · 186 citations
2
h-index
PRD · 1 publications · 42 citations
1
h-index
1 publications · 16 citations
1
h-index
1–5