Formation of trans-Neptunian satellite systems at the stage of condensations
نویسندگان
چکیده
منابع مشابه
Formation and migration of trans-Neptunian objects
s of the Conference ”Celestial Mechanics 2002: Results and Prospects” (10 14 September 2002, St. Petersburg, Russia), Institute of Applied Astronomy of Russian Academy of Sciences. We support the Eneev’s idea [1] that the largest (with diameter d>100 km) trans-Neptunian objects (TNOs) moving now in not very eccentric orbits could be formed directly by the compression of rarefied dust condensati...
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15 صفحه اولFormation and Evolution of the Trans-neptunian Belt and Dust
Trans-Neptunian objects (TNOs) with diameter greater than 100 km currently moving in not too eccentric orbits could be formed directly by the contraction of large rarefied condensations. Along with the gravitational influence of planets, gravitational interactions of TNOs played a certain role in their orbital evolution as well. More than 20% of Earth-crossing objects could have come from the t...
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In 1992, Jewitt and Luu (1993) carried out a survey of 0.7 square degrees of the sky to a limiting magnitude of We present B–V and V–R colors for trans-neptunian objects (TNOs) 1994 TB and 1993 SC. We have found that these TNOs R p 25 and discovered the first TNO (1992 QB1). Thirtyhave colors almost as red as 5145 Pholus which are therefore six TNOs have been discovered as of June, 1996. The co...
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ژورنال
عنوان ژورنال: Solar System Research
سال: 2017
ISSN: 0038-0946,1608-3423
DOI: 10.1134/s0038094617040013