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- W3118546231 abstract "A Monte Carlo model of stellar perturbations of the Oort cloud is used to study the distributions in energy and perihelion of comets entering the planetary region for the first time. The model is run for a variety of initial states and a range of velocity perturbations. In all cases the resulting orbits are uniformly distributed in perihelion distance in the planetary region, q less than 20 AU. Most orbits are confined to a fairly narrow range in 1/a and hyperbolic orbits are rare." @default.
- W3118546231 created "2021-01-18" @default.
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- W3118546231 date "1977-01-01" @default.
- W3118546231 modified "2023-09-26" @default.
- W3118546231 title "Initial energy and perihelion distributions of Oort-cloud comets" @default.
- W3118546231 hasPublicationYear "1977" @default.
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