Results 11 to 20 of about 129,106 (151)
Ephemerides of the main Uranian satellites [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 International ...
N V Emelyanov
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Existence of undiscovered Uranian satellites [PDF]
, 1986 Structure in the Uranian ring system as observed in recent occultations may contain indirect evidence for the existence of undiscovered satellites. Using the Alfven and Arrhenius (1975, 1976) scenario for the formation of planetary systems, the orbital radii of up to nine hypothetical satellites interior to Miranda are computed.
Boice, D.C.
openaire +4 more sources
Spectroscopic Links among Giant Planet Irregular Satellites and Trojans [PDF]
The Planetary Science Journal, 2023 We collect near-infrared spectra (∼0.75–2.55 μ m) of four Jovian irregular satellites and visible spectra (∼0.32–1.00 μ m) of two Jovian irregular satellites, two Uranian irregular satellites, and four Neptune Trojans.
Benjamin N. L. Sharkey +4 more
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Observations of Uranus and Main Uranian Satellites by Using Methane Filter from 2019 to 2025
The Astronomical JournalObservations of Uranus and Uranian satellites, aimed at improving the ephemerides, are fundamental to the dynamical realization of the celestial reference.
Jian Chen +6 more
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Predictions of the mutual events of the Uranian satellites occurring in 2006–2009 [PDF]
Astronomy and Astrophysics, 2006 Context. Every 42 years, the Earth and the Sun pass through the equatorial plane of Uranus allowing observations of mutual occultations and eclipses of the main satellites of Uranus. The next opportunity will occur in 2006-2009. Aims. Such events are uncommon and very rare, and they allow us to accurately determine the inclinations of the orbits of the
J -E Arlot, W Thuillot
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Astronomical Journal, 2014 French et al. determined the orbits of the Uranian rings, the orientation of the pole of Uranus, and the gravity harmonics of Uranus from Earth-based and Voyager ring occultations. Jacobson et al. determined the orbits of the Uranian satellites and the masses of Uranus and its satellites from Earth-based astrometry and observations acquired with the ...
exaly +2 more sources
THE ORBITS OF THE OUTER URANIAN SATELLITES
Astronomical Journal, 2009 M Brozović
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Tidal evolution of the Uranian satellites [PDF]
Icarus, 1988 Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric and Planetary Sciences, 1988. ; Vita. ; Includes bibliographical references. ; by William Charles Tittemore. ; Ph.D.
William C. Tittemore, Jack Wisdom
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Strong Tidal Dissipation at Uranus?
The Planetary Science Journal, 2023 Geophysical estimates of paleo heat fluxes on the Uranian moons Miranda and Ariel are in the range of 25–75 mW m ^−2 . For a canonical Uranus dissipation factor Q = 18,000, expected equilibrium tidal heating rates for these satellites are less than 6 mW ...
Francis Nimmo
doaj +1 more source
Control of colocated geostationary satellites [PDF]
, 1996 Control of the inter-satellite distances within a cluster of colocated satellites located in the same GEO window is examined with regards to the close approaches between pairs of satellites. Firstly, the orbital evolution and station keeping control of a
Hardacre, S.
core +7 more sources