S. Kenyon, J. Najita, und B. Bromley. (2016)cite arxiv:1608.05410Comment: 34 pages of text, 8 figures, ApJ, in press.
Zusammenfassung
We reconsider the commonly held assumption that warm debris disks are tracers
of terrestrial planet formation. The high occurrence rate inferred for
Earth-mass planets around mature solar-type stars based on exoplanet surveys
(roughly 20%) stands in stark contrast to the low incidence rate (less than
2-3%) of warm dusty debris around solar-type stars during the expected epoch of
terrestrial planet assembly (roughly 10 Myr). If Earth-mass planets at AU
distances are a common outcome of the planet formation process, this
discrepancy suggests that rocky planet formation occurs more quickly and/or is
much neater than traditionally believed, leaving behind little in the way of a
dust signature. Alternatively, the incidence rate of terrestrial planets has
been overestimated or some previously unrecognized physical mechanism removes
warm dust efficiently from the terrestrial planet region. A promising removal
mechanism is gas drag in a residual gaseous disk with a surface density of
roughly or somewhat more than 0.001% of the minimum mass solar nebula.
%0 Generic
%1 kenyon2016rocky
%A Kenyon, Scott J.
%A Najita, Joan R.
%A Bromley, Benjamin C.
%D 2016
%K exoplanet
%T Rocky Planet Formation: Quick and Neat
%U http://arxiv.org/abs/1608.05410
%X We reconsider the commonly held assumption that warm debris disks are tracers
of terrestrial planet formation. The high occurrence rate inferred for
Earth-mass planets around mature solar-type stars based on exoplanet surveys
(roughly 20%) stands in stark contrast to the low incidence rate (less than
2-3%) of warm dusty debris around solar-type stars during the expected epoch of
terrestrial planet assembly (roughly 10 Myr). If Earth-mass planets at AU
distances are a common outcome of the planet formation process, this
discrepancy suggests that rocky planet formation occurs more quickly and/or is
much neater than traditionally believed, leaving behind little in the way of a
dust signature. Alternatively, the incidence rate of terrestrial planets has
been overestimated or some previously unrecognized physical mechanism removes
warm dust efficiently from the terrestrial planet region. A promising removal
mechanism is gas drag in a residual gaseous disk with a surface density of
roughly or somewhat more than 0.001% of the minimum mass solar nebula.
@misc{kenyon2016rocky,
abstract = {We reconsider the commonly held assumption that warm debris disks are tracers
of terrestrial planet formation. The high occurrence rate inferred for
Earth-mass planets around mature solar-type stars based on exoplanet surveys
(roughly 20%) stands in stark contrast to the low incidence rate (less than
2-3%) of warm dusty debris around solar-type stars during the expected epoch of
terrestrial planet assembly (roughly 10 Myr). If Earth-mass planets at AU
distances are a common outcome of the planet formation process, this
discrepancy suggests that rocky planet formation occurs more quickly and/or is
much neater than traditionally believed, leaving behind little in the way of a
dust signature. Alternatively, the incidence rate of terrestrial planets has
been overestimated or some previously unrecognized physical mechanism removes
warm dust efficiently from the terrestrial planet region. A promising removal
mechanism is gas drag in a residual gaseous disk with a surface density of
roughly or somewhat more than 0.001% of the minimum mass solar nebula.},
added-at = {2016-08-22T14:54:38.000+0200},
author = {Kenyon, Scott J. and Najita, Joan R. and Bromley, Benjamin C.},
biburl = {https://www.bibsonomy.org/bibtex/22b865d1fc8a061791a2537252319187e/superjenwinters},
description = {Rocky Planet Formation: Quick and Neat},
interhash = {a0ee97fb0f0112cb55f93d0b560c259d},
intrahash = {2b865d1fc8a061791a2537252319187e},
keywords = {exoplanet},
note = {cite arxiv:1608.05410Comment: 34 pages of text, 8 figures, ApJ, in press},
timestamp = {2016-08-22T14:54:38.000+0200},
title = {Rocky Planet Formation: Quick and Neat},
url = {http://arxiv.org/abs/1608.05410},
year = 2016
}