The formation of the planetary sequence in a rotating, self-gravitating disk of randomly colliding planetesimals

E Griv; M Gedalin; D Eichler; E Liverts

The formation of the planetary sequence in a rotating, self-gravitating disk of randomly colliding planetesimals

Research output: Chapter in Book/Report/Conference proceeding › Chapter › peer-review

Abstract

The kinetic theory is used to study the evolution of the self-gravitation disk of randomly colliding planetesimals. It is shown that as a result of an almost aperiodic Jeans-type instability of small-amplitude gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequance with mathematical reg

Original language	English
Title of host publication	Astrophysical Ages and Time Scales
Pages	138-140
Volume	245
State	Published - 2001

Publication series

Name	ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES

Cite this

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title = "The formation of the planetary sequence in a rotating, self-gravitating disk of randomly colliding planetesimals",

abstract = "The kinetic theory is used to study the evolution of the self-gravitation disk of randomly colliding planetesimals. It is shown that as a result of an almost aperiodic Jeans-type instability of small-amplitude gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequance with mathematical reg",

author = "E Griv and M Gedalin and D Eichler and E Liverts",

year = "2001",

language = "English",

isbn = "1583810838",

volume = "245",

series = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",

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TY - CHAP

T1 - The formation of the planetary sequence in a rotating, self-gravitating disk of randomly colliding planetesimals

AU - Griv, E

AU - Gedalin, M

AU - Eichler, D

AU - Liverts, E

PY - 2001

Y1 - 2001

N2 - The kinetic theory is used to study the evolution of the self-gravitation disk of randomly colliding planetesimals. It is shown that as a result of an almost aperiodic Jeans-type instability of small-amplitude gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequance with mathematical reg

AB - The kinetic theory is used to study the evolution of the self-gravitation disk of randomly colliding planetesimals. It is shown that as a result of an almost aperiodic Jeans-type instability of small-amplitude gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequance with mathematical reg

M3 - Chapter

SN - 1583810838

VL - 245

T3 - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES

SP - 138

EP - 140

BT - Astrophysical Ages and Time Scales

ER -

The formation of the planetary sequence in a rotating, self-gravitating disk of randomly colliding planetesimals

Abstract

Publication series

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