Knowledge Resource Center for Ecological Environment in Arid Area
DOI | 10.1088/0004-637X/732/2/66 |
MODELING PLANETARY SYSTEM FORMATION WITH N-BODY SIMULATIONS: ROLE OF GAS DISK AND STATISTICS COMPARED TO OBSERVATIONS | |
Liu, Huigen1; Zhou, Ji-Lin; Wang, Su | |
通讯作者 | Liu, Huigen |
来源期刊 | ASTROPHYSICAL JOURNAL |
ISSN | 0004-637X |
出版年 | 2011 |
卷号 | 732期号:2 |
英文摘要 | During the late stage of planet formation, when Mars-sized cores appear, interactions among planetary cores can excite their orbital eccentricities, accelerate their merging, and thus sculpt their final orbital architecture. This study contributes to the final assembling of planetary systems with N-body simulations, including the type I or II migration of planets and gas accretion of massive cores in a viscous disk. Statistics on the final distributions of planetary masses, semimajor axes, and eccentricities are derived and are comparable to those of the observed systems. Our simulations predict some new orbital signatures of planetary systems around solar mass stars: 36% of the surviving planets are giant planets (> 10M(circle plus)). Most of the massive giant planets (> 30 M-circle plus) are located at 1-10 AU. Terrestrial planets are distributed more or less evenly at <1-2 AU. Planets in inner orbits may accumulate at the inner edges of either the protostellar disk (3-5 days) or its magnetorotational instability dead zone (30-50 days). There is a planet desert in the mass-eccentricity diagram, i.e., a lack of planets with masses 0.005-0.08M(J) in highly eccentric orbits (e > 0.3-0.4). The average eccentricity (similar to 0.15) of the giant planets (> 10M(circle plus)) is greater than that (similar to 0.05) of the terrestrial planets (< 10M(circle plus)). A planetary system with more planets tends to have smaller planet masses and orbital eccentricities on average. |
英文关键词 | celestial mechanics methods: numerical planetary systems planet-disk interactions planets and satellites: formation |
类型 | Article |
语种 | 英语 |
国家 | Peoples R China |
收录类别 | SCI-E |
WOS记录号 | WOS:000289935900006 |
WOS关键词 | T-TAURI STARS ; GIANT PLANETS ; DETERMINISTIC MODEL ; SNOW LINE ; PROTOPLANETARY DISKS ; ACCRETION DISKS ; MHD TURBULENCE ; M-DWARF ; MIGRATION ; MASS |
WOS类目 | Astronomy & Astrophysics |
WOS研究方向 | Astronomy & Astrophysics |
来源机构 | 南京大学 |
资源类型 | 期刊论文 |
条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/167201 |
作者单位 | 1.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China; 2.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Peoples R China |
推荐引用方式 GB/T 7714 | Liu, Huigen,Zhou, Ji-Lin,Wang, Su. MODELING PLANETARY SYSTEM FORMATION WITH N-BODY SIMULATIONS: ROLE OF GAS DISK AND STATISTICS COMPARED TO OBSERVATIONS[J]. 南京大学,2011,732(2). |
APA | Liu, Huigen,Zhou, Ji-Lin,&Wang, Su.(2011).MODELING PLANETARY SYSTEM FORMATION WITH N-BODY SIMULATIONS: ROLE OF GAS DISK AND STATISTICS COMPARED TO OBSERVATIONS.ASTROPHYSICAL JOURNAL,732(2). |
MLA | Liu, Huigen,et al."MODELING PLANETARY SYSTEM FORMATION WITH N-BODY SIMULATIONS: ROLE OF GAS DISK AND STATISTICS COMPARED TO OBSERVATIONS".ASTROPHYSICAL JOURNAL 732.2(2011). |
条目包含的文件 | 条目无相关文件。 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。