Orbital stability of massive protoplanets in the terrestrial planet region of the solar system

Details Orbital stability of massive protoplanets in the terrestrial planet region of the solar system Orbital stability of massive protoplanets in the terrestrial planet region of the solar system

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....19..421d&link_type=abstract

Moon and the Planets, vol. 19, Dec. 1978, p. 421-424.

Computer Science

5

Orbital Mechanics, Planetary Evolution, Solar Orbits, Terrestrial Planets, Angular Momentum, Circular Orbits, Equations Of Motion, Solar System

Scientific paper

A number of theories of the formation of the planets advocate that the terrestrial planets were originally of cosmic composition and that it is only subsequent evolution that has removed their volatile components. This paper shows that such protoplanets could have remained in the terrestrial planet region without significant changes occurring in their orbits for an acceptable time interval.

Affiliated with

Also associated with

No associations

Rating

Orbital stability of massive protoplanets in the terrestrial planet region of the solar system 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 Orbital stability of massive protoplanets in the terrestrial planet region of the solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Orbital stability of massive protoplanets in the terrestrial planet region of the solar system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-888348