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Uranus ring occultation observations: 1977-2006
DOI: 10.1016/j.icarus.2023.115474 Bibcode: 2023Icar..39515474F

Nicholson, Philip D.; French, Richard G.; Sicardy, Bruno +25 more

The Uranian rings were discovered serendipitously on 10 March 1977 during a stellar occultation (Elliot et al., 1977a; Millis et al., 1977), and a rich set of subsequent Earth-based occultations revealed that these narrow and sharp-edged rings were eccentric and inclined, precessing under the gravitational influence of the oblate central planet. C…

2023 Icarus
Gaia eHST 6
Spins and shapes of basaltic asteroids and the missing mantle problem
DOI: 10.1016/j.icarus.2023.115520 Bibcode: 2023Icar..39715520O

Hasegawa, Sunao; Oszkiewicz, Dagmara; Skiff, Brian A. +31 more

Basaltic V-type asteroids are common in the inner part of the Main Asteroid Belt and much less abundant in the mid and outer parts. They are of scientific interest because they sample crusts and mantles of theoretically plentiful differentiated planetesimals that existed in the Solar System four billion years ago. Some Solar System theories sugges…

2023 Icarus
Gaia 5
Astrometric observations of the main Saturnian satellites from 2004 to 2014 based on Gaia DR3
DOI: 10.1016/j.icarus.2023.115478 Bibcode: 2023Icar..39515478Y

Zhang, H. Y.; Yan, D.; Qiao, R. C. +1 more

A total of 3169 astrometric positions of the seven main satellites of Saturn: Enceladus, Tethys, Dione, Rhea, Titan, Hyperion and Iapetus were obtained in the time span 2004-2014 from observations made with 1.56 m telescope at Sheshan station of Shanghai Observatory, CAS. We compared our observations to the theoretical positions retrieved from IMC…

2023 Icarus
Gaia 1