A note on the cosmogony of the asteroidal belt

W. H. Ip

doi:10.1007/BF00642157

A note on the cosmogony of the asteroidal belt

W. H. Ip

Graduate Institute of Astronomy

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.

Original language	English
Pages (from-to)	235-241
Number of pages	7
Journal	Astrophysics and Space Science
Volume	45
Issue number	1
DOIs	https://doi.org/10.1007/BF00642157
State	Published - Nov 1976

Access to Document

10.1007/BF00642157

Cite this

@article{335c9b02860d4ccd83b12842e390ff5a,

title = "A note on the cosmogony of the asteroidal belt",

abstract = "Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.",

author = "Ip, {W. H.}",

year = "1976",

month = nov,

doi = "10.1007/BF00642157",

language = "???core.languages.en_GB???",

volume = "45",

pages = "235--241",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

number = "1",

}

TY - JOUR

T1 - A note on the cosmogony of the asteroidal belt

AU - Ip, W. H.

PY - 1976/11

Y1 - 1976/11

N2 - Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.

AB - Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.

UR - http://www.scopus.com/inward/record.url?scp=34250381742&partnerID=8YFLogxK

U2 - 10.1007/BF00642157

DO - 10.1007/BF00642157

M3 - 期刊論文

AN - SCOPUS:34250381742

SN - 0004-640X

VL - 45

SP - 235

EP - 241

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1

ER -

A note on the cosmogony of the asteroidal belt

Abstract

Access to Document

Fingerprint

Cite this