Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...332.1147b&link_type=abstract
Astronomy and Astrophysics, v.332, p.1147-1153 (1998)
Astronomy and Astrophysics
Astrophysics
9
Celestial Mechanics, Stellar Dynamics, Binaries: Visual, Stars: Individual: Ads 12033, Planetary Systems
Scientific paper
Numerical simulations are made within the frame of the elliptic plane restricted three-body problem, in order to search if stable orbits exist for planets around one of the two components in double stars. The ADS 12033 system is investigated here. Large stable planetary orbits, already known to exist (more precisely, known to be possible from the dynamical point of view) through a systematic exploration of the circular model and for several cases of the elliptic model (Sun-Jupiter, alpha Centauri, Sirius and eta Coronae Borealis), are found to exist around ADS 12033 A and ADS 12033 B up to distances from each star of the order of more than half the binary's periastron separation. Moreover, nearly circular stable planetary orbits are found to exist in the so-called ``habitable zone" around each star.
No associations
LandOfFree
Planetary orbits in the elliptic restricted problem. IV. The ADS 12033 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 Planetary orbits in the elliptic restricted problem. IV. The ADS 12033 system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Planetary orbits in the elliptic restricted problem. IV. The ADS 12033 system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1601691