Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit

Details Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.311..636h&link_type=abstract

Nature (ISSN 0028-0836), vol. 311, Oct. 18, 1984, p. 636-638.

Biology

25

Comets, Companion Stars, Nemesis (Star), Paleobiology, Perihelions, Stellar Mass, Stellar Rotation, Molecular Clouds, Motion Stability, Orbit Perturbation, Orbital Elements, Solar System

Scientific paper

It has been suggested that the observed periodic extinction of species at intervals of 26 Myr may be catalysed by a hypothetical stellar companion of the Sun, Nemesis, with an orbital period of 26 Myr. This letter investigates the effect of Nemesis on the comets in the inner comet cloud. This is used to determine the minimum required mass of Nemesis and its minimum required perihelion distance. The effect of passing stars on the stability of the orbit of Nemesis is investigated, and the probability of its having passed within the planetary system estimated.

Affiliated with

Also associated with

No associations

Rating

Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1229433