How special is the Solar system?

被引：23

作者：

Beer, ME ^{[1
]}

King, AR

Livio, M

Pringle, JE

机构：

[1] Univ Leicester, Theoret Astrophys Grp, Leicester LE1 7RH, Leics, England

[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2004年 / 354卷 / 03期

关键词：

accretion; accretion discs; planets and satellites : formation;

D O I：

10.1111/j.1365-2966.2004.08237.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Most mechanisms proposed for the formation of planets are modified versions of the mechanism proposed for the formation of the Solar system. Here we argue that, with reference to those planetary systems that have been observed, it has yet to be established that the Solar system is a typical planetary system. We consider the possibility that most observed planetary systems formed in a different way. If this is so, it may be that none of the observed planetary systems is likely to harbour an Earth-like planet.

引用

页码：763 / 768

页数：6

共 69 条

[1] On the origin of ionizing photons emitted by T Tauri stars [J].

Alexander, RD ;

Clarke, CJ ;

Pringle, JE .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 348 (03) :879-884

[2] Migration and giant planet formation [J].

Alibert, Y ;

Mordasini, C ;

Benz, W .

ASTRONOMY & ASTROPHYSICS, 2004, 417 (01) :L25-L28

[3]

[Anonymous], 1996, NUMERICAL RECIPES FO

[4] Predictions for the frequency and orbital radii of massive extrasolar planets [J].

Armitage, PJ ;

Livio, M ;

Lubow, SH ;

Pringle, JE .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 334 (01) :248-256

[5]

ASGHARI N, 2004, IN PRESS A A

[6] Dynamical modeling of large scale asymmetries in the βPictoris dust disk [J].

Augereau, JC ;

Nelson, RP ;

Lagrange, AM ;

Papaloizou, JCB ;

Mouillet, D .

ASTRONOMY & ASTROPHYSICS, 2001, 370 (02) :447-455

[7] The formation of close binary systems by dynamical interactions and orbital decay [J].

Bate, MR ;

Bonnell, IA ;

Bromm, V .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 336 (03) :705-713

[8] The formation of a star cluster: predicting the properties of stars and brown dwarfs [J].

Bate, MR ;

Bonnell, IA ;

Bromm, V .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 339 (03) :577-599

[9] The formation mechanism of brown dwarfs [J].

Bate, MR ;

Bonnell, IA ;

Bromm, V .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 332 (03) :L65-U1

[10] Possible observational criteria for distinguishing brown dwarfs from planets [J].

Black, DC .

ASTROPHYSICAL JOURNAL, 1997, 490 (02) :L171-L174

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