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- W2235355655 abstract "Distribution of eccentricities, perihelion distances of interstellar particles and their concentrations in the Solar system have been computed in the assumption that their velocities are similar to ones of the nearby stars of late spectral classes. More than 75% of orbits have eccentricities not exceeding the value 1.1 and concentration of particles at the Earth’s orbit 3.5 times greater than in the interstellar space.KeywordsSolar SystemVolume DensityOrbital ElementCentral StarAstronomical UnitThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W2235355655 date "1985-01-01" @default.
- W2235355655 modified "2023-10-16" @default.
- W2235355655 title "Possible Distributions of Some Orbital Elements of Interstellar Particles in the Solar System" @default.
- W2235355655 doi "https://doi.org/10.1007/978-94-009-5464-9_80" @default.
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