In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 36, no. 3
L. Neslušan - T. Paulech
Detaily:
Rok, strany: 2006, 158 - 170
Kľúčové slová:
Kuiper belt, edge beyond 50 AU, stellar perturbations
O článku:
Through a numerical integration of the orbits of test particles
proto-planetary disc, which were perturbed by a nearly passing star
and Neptune, we answer the question on a possibility that the observed
truncation of the Kuiper belt at 50 AU was caused just by a close
encounter of the Solar System with a star. We consider a spectrum of
possible encounter relative velocities, geometries, and masses of the
perturbing star. Though the stellar perturbation tends to increase
the number density of the classical Kuiper-belt objects (CKBOs) inside
50 AU in some cases, Neptune simultaneously reduces again this
number density. The ratio of the discovery probabilities of CKBOs within
50 AU and beyond this distance appears to be comparable, for several
combinations of the encounter parameters, to a critical ratio at which
the truncation could be explained by a perturbative stellar passage.
However, even these interesting combinations are not acceptable, because
the simultaneous change of the velocity of the Sun turns out here to be so
large that the Oort cloud would have been stripped and no dynamically
new comets could be observed. In conclusion, no stellar encounter, with
a relative velocity comparable or larger than about
5 km s-1,
could cause the truncation of the Kuiper belt after the epoch when
the macroscopic bodies in the belt and a significant fraction of the
Oort cloud were formed.
Ako citovať:
ISO 690:
Neslušan, L., Paulech, T. 2006. The study of a gravitational influence of a nearly passing star on the primordial Kuiper belt. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 36, no.3, pp. 158-170. 1335-1842.
APA:
Neslušan, L., Paulech, T. (2006). The study of a gravitational influence of a nearly passing star on the primordial Kuiper belt. Contributions of the Astronomical Observatory Skalnaté Pleso, 36(3), 158-170. 1335-1842.