Results 91 to 100 of about 5,831 (201)
* Tromikosoma uranus (Thomson, 1877) Fig. 21 A–C. Phormosoma uranus: A. Agassiz, 1881: 103. Echinosoma uranus: H.L. Clark, 1925a: 57. Tromikosoma uranus: Mortensen, 1935: 168 –170. Pl. VI, Figs 2–3. Pl.
Filander, Zoleka, Griffiths, Charles
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Using sophisticated computer enhancement techniques, two astronomers have been able to clearly “photograph” the rings of Uranus (Figure 1). The photographs show that the rings are made of particles that are perhaps the darkest found in the solar system. Creating clear images of the rings is a feat that has proved extremely difficult in the past because
openaire +1 more source
Crantor, a short-lived horseshoe companion to Uranus?
Context. Stable co-orbital motion with Uranus is vulnerable to planetary migration but temporary co-orbitals may exist today. So far only two candidates have been suggested, both moving on horseshoe orbits: 83982 Crantor (2002 GO9) and 2000 SN331. Aims. (
R. De La Fuente Marcos +1 more
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Gravity Science With the Uranus Orbiter
Uranus Flagship 2023, Pasadena, CA, July 25-27, 2023The Cassini and Juno missions have considerably expanded our understanding of Saturn, Jupiter, and their moons.
Goossens, Sander +4 more
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Inaccuracy in our knowledge of the transport properties of relevant mixtures under planetary interior conditions is a roadblock in predicting the observable properties of planets in our solar system and beyond.
Argha Jyoti Roy +3 more
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Facts on this site about Uranus include mean distance from Sun, length of year, rotation period, mean orbital velocity, inclination of axis, average temperature (day and night), diameter, and number of observed satellites.
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Insights on the Formation Conditions of Uranus and Neptune from Their Deep Elemental Compositions
This study, placed in the context of the preparation for the Uranus Orbiter Probe mission, aims to predict the bulk volatile compositions of Uranus and Neptune.
Olivier Mousis +8 more
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Uranus after Solstice: Results from the 1998 November 6 Occultation
this paper are given relative to the rotational North pole of Uranus, following the notation in Baron et al. 1989 and Sicardy et al. 1985.) All published occultations of the Uranian atmosphere at 1-- 100 bar occurred before Uranus' southern summer ...
Leslie A. Young +3 more
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Atmospheric Entry Studies for Uranus [PDF]
The Objectives of this work are: 1) Establish a range of probe atmospheric entry environments based on the Uranus Flagship mission outlined in the Planetary Science Decadal Survey for two launch windows: Year 2021 and 2034.
Garcia, Joseph +11 more
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This page of Nine Planets highlights details about the gas giant planet Uranus and its moons. Information includes planet diameter, mass, distance from the Sun, orbit, and mythology.
Bill Arnett
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