Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2011-08-04
MNRAS, 418, (2011) 1335-1345
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
13 pages, 9 figures, accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2011.19585.x
In this work, we extensively investigate the terrestrial planetary formation for the inclined planetary systems (considering the OGLE-2006-BLG-109L system as prototype) in the late stage. In the simulations, we show that the occurrence of terrestrial planets is quite common, in the final assembly stage. Moreover, we find that 40% of the runs finally occupy one planet in the habitable zone (HZ). On the other hand, the numerical results also indicate that the inner region of the planetesimal disk, ranging from $\sim 0.1$ to 0.3 AU, plays an important role in building up terrestrial planets. By examining all simulations, we note that the survivals are located either between 0.1$\sim$1.0 AU or beyond 7 AU, or at the 1:1 mean motion resonance of OGLE-2006-BLG-109Lb at $\sim$2.20 AU. The outcomes suggest that it may exist moderate possibility for the inclined systems to harbor terrestrial planets, even planets in the HZs.
Ji Jianghui
Jin Sheng
No associations
LandOfFree
Terrestrial Planet Formation in the Inclined Systems: Application to OGLE-2006-BLG-109L 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 Terrestrial Planet Formation in the Inclined Systems: Application to OGLE-2006-BLG-109L System, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Terrestrial Planet Formation in the Inclined Systems: Application to OGLE-2006-BLG-109L System will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-14877