Emergence of Protoplanetary Disks and Successive Formation of Gaseous Planets by Gravitational Instability

We use resistive magnetohydrodynamical (MHD) simulations with the nested grid technique to study the formation of protoplanetary disks around protostars from molecular cloud cores that provide the realistic environments for planet formation. We find that gaseous planetary-mass objects are formed in...

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Published inAstrophysical journal. Letters Vol. 718; no. 2; pp. L58 - L62
Main Authors Inutsuka, Shu-ichiro, Machida, Masahiro N, Matsumoto, Tomoaki
Format Journal Article
LanguageEnglish
Published United States IOP Publishing 01.08.2010
Subjects
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
FLUID MECHANICS
GRAVITATIONAL INSTABILITY
HYDRODYNAMICS
INSTABILITY
MAGNETIC DISKS
MAGNETIC STORAGE DEVICES
MAGNETOHYDRODYNAMICS
MASS
MECHANICS
MEMORY DEVICES
PLANETS
PLASMA INSTABILITY
PROTOPLANETS
PROTOSTARS
SIMULATION
STARS
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Abstract We use resistive magnetohydrodynamical (MHD) simulations with the nested grid technique to study the formation of protoplanetary disks around protostars from molecular cloud cores that provide the realistic environments for planet formation. We find that gaseous planetary-mass objects are formed in the early evolutionary phase by gravitational instability in regions that are decoupled from the magnetic field and surrounded by the injection points of the MHD outflows during the formation phase of protoplanetary disks. Magnetic decoupling enables massive disks to form and these are subject to gravitational instability, even at {approx}10 AU. The frequent formation of planetary-mass objects in the disk suggests the possibility of constructing a hybrid planet formation scenario, where the rocky planets form later under the influence of the giant planets in the protoplanetary disk.
AbstractList We use resistive magnetohydrodynamical (MHD) simulations with the nested grid technique to study the formation of protoplanetary disks around protostars from molecular cloud cores that provide the realistic environments for planet formation. We find that gaseous planetary-mass objects are formed in the early evolutionary phase by gravitational instability in regions that are decoupled from the magnetic field and surrounded by the injection points of the MHD outflows during the formation phase of protoplanetary disks. Magnetic decoupling enables massive disks to form and these are subject to gravitational instability, even at {approx}10 AU. The frequent formation of planetary-mass objects in the disk suggests the possibility of constructing a hybrid planet formation scenario, where the rocky planets form later under the influence of the giant planets in the protoplanetary disk.
Author Inutsuka, Shu-ichiro
Machida, Masahiro N
Matsumoto, Tomoaki
Author_xml – sequence: 1
  fullname: Inutsuka, Shu-ichiro
– sequence: 2
  fullname: Machida, Masahiro N
– sequence: 3
  fullname: Matsumoto, Tomoaki
BackLink https://www.osti.gov/biblio/21451020$$D View this record in Osti.gov
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Cites_doi 10.1086/507179
10.1088/0004-637X/704/1/L10
10.1006/icar.1996.0190
10.1126/science.1166609
10.1086/157986
10.1111/j.1365-2966.2005.09297.x
10.1086/308439
10.1088/0004-637X/695/2/1132
10.1016/j.icarus.2008.10.004
10.1111/j.1745-3933.2005.00105.x
10.1111/j.1745-3933.2008.00559.x
10.1086/528364
10.1046/j.1365-8711.1999.02211.x
10.1086/500496
10.1088/0004-637X/714/2/1343
10.1088/0004-637X/707/2/L123
10.1086/424830
10.1051/0004-6361:200811325
10.1086/341133
10.1016/j.icarus.2005.06.021
10.1086/157734
10.1051/0004-6361:20078309
10.1126/science.1166585
10.1086/305281
10.1086/529133
10.1111/j.1365-2966.2003.07317.x
10.1086/521779
10.1086/504423
10.1093/mnras/145.3.271
10.1086/340587
10.1086/344105
10.1086/309050
10.1086/320631
10.1111/j.1365-2966.2010.16527.x
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References 22
Gammie (4) 2002; 553
Machida (21) 2006; 645
24
29
André (1) 2008
Tomisaka (33) 2002; 575
Larson (14) 1969; 145
Machida (23) 2008; 677
Masunaga (26) 1998; 495
Banerjee (2) 2006; 641
Masunaga (25) 2000; 531
Thalmann (32) 2009; 707
Durisen (3) 2007
Ida (9) 2004; 616
Nakano (28) 2002; 573
31
Kokubo (12) 2002; 581
11
Rice (30) 2005; 364
Ikoma (10) 2000; 537
34
13
Muto (27) 2009; 695
35
36
15
Machida (16) 2006; 647
Hori (7) 2008; 714
Machida (17) 2007; 670
Machida (19) 2009; 704
Machida (18) 2008; 676
5
6
8
20
References_xml – volume: 647
  start-page: L151
  issn: 1538-4357
  year: 2006
  ident: 16
  publication-title: ApJ
  doi: 10.1086/507179
– volume: 704
  start-page: L10
  issn: 1538-4357
  year: 2009
  ident: 19
  publication-title: ApJ
  doi: 10.1088/0004-637X/704/1/L10
– ident: 29
  doi: 10.1006/icar.1996.0190
– ident: 11
  doi: 10.1126/science.1166609
– ident: 36
  doi: 10.1086/157986
– ident: 22
  doi: 10.1111/j.1365-2966.2005.09297.x
– volume: 531
  start-page: 350
  issn: 0004-637X
  year: 2000
  ident: 25
  publication-title: ApJ
  doi: 10.1086/308439
– volume: 695
  start-page: 1132
  issn: 0004-637X
  year: 2009
  ident: 27
  publication-title: ApJ
  doi: 10.1088/0004-637X/695/2/1132
– ident: 15
  doi: 10.1016/j.icarus.2008.10.004
– volume: 364
  start-page: L56
  issn: 0035-8711
  year: 2005
  ident: 30
  publication-title: MNRAS
  doi: 10.1111/j.1745-3933.2005.00105.x
– ident: 5
  doi: 10.1111/j.1745-3933.2008.00559.x
– volume: 676
  start-page: 1088
  issn: 0004-637X
  year: 2008
  ident: 18
  publication-title: ApJ
  doi: 10.1086/528364
– ident: 34
  doi: 10.1046/j.1365-8711.1999.02211.x
– volume: 641
  start-page: 949
  issn: 0004-637X
  year: 2006
  ident: 2
  publication-title: ApJ
  doi: 10.1086/500496
– start-page: 607
  year: 2007
  ident: 3
  publication-title: Protostars and Planets V
– volume: 714
  start-page: 1343
  year: 2008
  ident: 7
  publication-title: ApJ
  doi: 10.1088/0004-637X/714/2/1343
– volume: 707
  start-page: L123
  issn: 1538-4357
  year: 2009
  ident: 32
  publication-title: ApJ
  doi: 10.1088/0004-637X/707/2/L123
– volume: 616
  start-page: 567
  issn: 0004-637X
  year: 2004
  ident: 9
  publication-title: ApJ
  doi: 10.1086/424830
– ident: 13
  doi: 10.1051/0004-6361:200811325
– volume: 575
  start-page: 306
  issn: 0004-637X
  year: 2002
  ident: 33
  publication-title: ApJ
  doi: 10.1086/341133
– ident: 8
  doi: 10.1016/j.icarus.2005.06.021
– start-page: 254
  year: 2008
  ident: 1
  publication-title: Structure Formation in Astrophysics
– ident: 35
  doi: 10.1086/157734
– ident: 6
  doi: 10.1051/0004-6361:20078309
– ident: 24
  doi: 10.1126/science.1166585
– volume: 495
  start-page: 346
  issn: 0004-637X
  year: 1998
  ident: 26
  publication-title: ApJ
  doi: 10.1086/305281
– volume: 677
  start-page: 327
  issn: 0004-637X
  year: 2008
  ident: 23
  publication-title: ApJ
  doi: 10.1086/529133
– ident: 31
  doi: 10.1111/j.1365-2966.2003.07317.x
– volume: 670
  start-page: 1198
  issn: 0004-637X
  year: 2007
  ident: 17
  publication-title: ApJ
  doi: 10.1086/521779
– volume: 645
  start-page: 1227
  issn: 0004-637X
  year: 2006
  ident: 21
  publication-title: ApJ
  doi: 10.1086/504423
– volume: 145
  start-page: 271
  issn: 0035-8711
  year: 1969
  ident: 14
  publication-title: MNRAS
  doi: 10.1093/mnras/145.3.271
– volume: 573
  start-page: 199
  issn: 0004-637X
  year: 2002
  ident: 28
  publication-title: ApJ
  doi: 10.1086/340587
– volume: 581
  start-page: 666
  issn: 0004-637X
  year: 2002
  ident: 12
  publication-title: ApJ
  doi: 10.1086/344105
– volume: 537
  start-page: 1013
  issn: 0004-637X
  year: 2000
  ident: 10
  publication-title: ApJ
  doi: 10.1086/309050
– volume: 553
  start-page: 174
  year: 2002
  ident: 4
  publication-title: ApJ
  doi: 10.1086/320631
– ident: 20
  doi: 10.1111/j.1365-2966.2010.16527.x
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Snippet We use resistive magnetohydrodynamical (MHD) simulations with the nested grid technique to study the formation of protoplanetary disks around protostars from...
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SubjectTerms ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
FLUID MECHANICS
GRAVITATIONAL INSTABILITY
HYDRODYNAMICS
INSTABILITY
MAGNETIC DISKS
MAGNETIC STORAGE DEVICES
MAGNETOHYDRODYNAMICS
MASS
MECHANICS
MEMORY DEVICES
PLANETS
PLASMA INSTABILITY
PROTOPLANETS
PROTOSTARS
SIMULATION
STARS
Title Emergence of Protoplanetary Disks and Successive Formation of Gaseous Planets by Gravitational Instability
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