[FPSPACE] Finding Solar System Analogs With SIM and HIPPARCOS: A White Paper for the ExoPl
LARRY KLAES
ljk4 at msn.com
Tue Apr 24 15:06:46 EDT 2007
Finding Solar System Analogs With SIM and HIPPARCOS: A White Paper for the
ExoPlanet Task Force
Authors: Rob P. Olling
(Submitted on 23 Apr 2007)
Abstract: The astrometric signature imposed by a planet on its primary
increases substantially towards longer periods (proportinal to P^2/3), so
that long-period planets can be more easily detected, in principle. For
example, a one Solar-mass (M_Sun) star would be pulled by roughly 1 mas by a
one Jupiter-mass (M_J) planet with a period of one-hundred years at a
distance of 20 pc. Such position accuracies can now be obtained with both
ground-based and space-based telescopes. The difficulty was that it often
takes many decades before a detectable position shift will occur. However,
by the time the next generation of astrometric missions such as SIM will be
taking data, several decades will have past since the first astrometric
mission, HIPPARCOS. Here we propose to use a new astrometric method that
employs a future, highly accurate SIM Quick-Look survey and HIPPARCOS data
taken twenty years prior. Using position errors for SIM of 4 muas, this
method enables the detection and characterization of Solar-system analogs
(SOSAs) with periods up to 240 (500) years for 1 (10) M_J companions.
Because many tens of thousands nearby stars can be surveyed this way for a
modest expenditure of SIM time and SOSAs may be quite abundant, we expect to
find many hundreds of extra-solar planets with long-period orbits. Such a
data set would nicely complement the short-period systems found by the
radial-velocity method. Brown dwarfs and low-mass stellar companions can be
found and characterized if their periods are shorter than about 500 years.
This data set will provide invaluable constraints on models of planet
formation, as well as a database for systems where the location of the giant
planets allow for the formation of low-mass planets in the habitable zone.
[Abridged]
Comments:
A White Paper for the ExoPlanet Task Force: 7 pages
Subjects:
Astrophysics (astro-ph)
Cite as:
arXiv:0704.3059v1 [astro-ph]
Submission history
From: Rob P. Olling [view email]
[v1] Mon, 23 Apr 2007 18:42:10 GMT (22kb)
http://arxiv.org/abs/0704.3059
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