Results 1 to 10 of about 187 (113)
Close approach of a cloud of particles around an oblate planet [PDF]
Computational and Applied Mathematics, 2015 zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Vivian Martins Gomes, Antonio Prado
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Apsidal precession of orbits about an oblate planet
Astronomical Journal, 1981 It is noted that expressions for the apsidal precession rates to second order on J2 appear in the literature in at least three apparently mutually contradictory forms. The expressions are reconciled by accounting for subtle differences in the definitions of orbital elements.
exaly +2 more sources
The orbit of a satellite of an oblate planet
Astronomical Journal, 1959 Boris Garfinkel
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On the motion of a satellite of an oblate planet
Astronomical Journal, 1958 Boris Garfinkel
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Motion of a Satellite of a Very Oblate Planet
Astronomical Journal, 1968 J M A Danby
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The gravitational orbit of a satellite of an oblate planet
Astronomical Journal, 1958 Theodore E Sterne
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CONSTRAINING THE OBLATENESS OFKEPLERPLANETS [PDF]
The Astrophysical Journal, 2014 19 pages, 15 figures, 9 tables; accepted by ApJ; for a short video introducing the main results, please click https://www.youtube.com/watch?v ...
Wei Zhu +3 more
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Circular Rydberg states of helium atoms or helium-like ions in a high-frequency laser field
Open Physics, 2021 In the literature, there were studies of Rydberg states of hydrogenic atoms/ions in a high-frequency laser field. It was shown that the motion of the Rydberg electron is analogous to the motion of a satellite around an oblate planet (for a linearly ...
Kryukov Nikolay, Oks Eugene
doaj +1 more source
Computation of the perturbed locations of L1 for all Sun-Planet RTBP systems with oblate primaries
Results in Physics, 2019 The location of the equilibrium point ΔL1 in the restricted three body problem with oblate primaries is investigated. The zonal harmonic coefficients are retained up to the fourth harmonic coefficient of both primaries.
S.E. Abd El-Bar +2 more
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Constraining the oblateness of transiting planets with photometry and spectroscopy [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle ingress and egress features in photometric transit light curves, we investigate the effect of oblateness on the spectroscopic Rossiter–McLaughlin (RM) signals. We found that
B Akinsanmi +4 more
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