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Possible Distributions of Some Orbital Elements of Interstellar Particles in the Solar System

Published online by Cambridge University Press:  12 April 2016

O.I. Belkovich  and
I.N. Potapov
O.I. Belkovich
Affiliation:
Engelhardt Astronomikal Observatory Kazan, SU-422526
I.N. Potapov
Affiliation:
Pedagogical Institute Vitebsk, SU-210036 U.S.S.R.

Abstract

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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.

Type
VII. Dynamics of Interplanetary Dust
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 421 - 424
Copyright
Copyright © Reidel 1985

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