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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 +2 more
exaly +4 more sources
Close approach maneuvers around an oblate planet
Journal of Physics: Conference Series, 2015 There are many applications of the close approach maneuvers in astronautics, and several missions used this technique in the last decades. In the present work, those close approach maneuvers are revisited, but now considering that the spacecraft passes around an oblate planet.
Antonio F B A Prado, D M Sanchez
exaly +2 more sources
Polarization of Starlight by an Unresolved and Oblate Extrasolar Planet in an Elliptical Orbit
Astrophysical Journal, 2006 We calculate the degree of linear polarization of radiation from stars having planets that may not be resolved spatially. We assume single scattering by water and silicate particulates in the planetary atmosphere. The dilution of the reflected polarized radiation of the planet by the unpolarized stellar radiation and the effect of oblateness of the ...
Sujan Sengupta
exaly +3 more sources
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
openaire +3 more sources
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
doaj +1 more source
Some remarks on the motion of a satellite of an oblate planet
Astronomical Journal, 1961 exaly +2 more sources
Inclination of satellite orbits about an oblate precessing planet
Astronomical Journal, 1965 Peter Goldreich
exaly +2 more sources
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
openaire +3 more sources
TESS phase curve of ultra-hot Jupiter WASP-189 b★
Astronomy & AstrophysicsContext. The thermal structures of highly irradiated ultra-hot Jupiters can deviate substantially from those of cooler hot Jupiters. For planets orbiting host stars that are rapidly rotating (and, thus, oblate), photometric light curves provide a unique ...
Patel J. A. +6 more
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