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19 April 2024 |
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Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest | | Stephen C. Unwin
; Michael Shao
; Angelle M. Tanner
; Ronald J. Allen
; Charles A. Beichman
; David Boboltz
; Joseph H. Catanzarite
; Brian C. Chaboyer
; David R. Ciardi
; Stephen J. Edberg
; Alan L. Fey
; Debra A. Fischer
; Christopher R. Gelino
; Andrew P. Gould
; Carl Grillmair
; Todd J. Henry
; Kathryn V. Johnston
; Kenneth J. Johnston
; Dayton L. Jones
; Shrinivas R. Kulkarni
; Nicholas M. Law
; Steven R. Majewski
; Valeri V. Makarov
; Geoffrey W. Marcy
; David L. Meier
; Rob P. Olling
; Xiaopei Pan
; Richard J. Patterson
; Jo Eliza Pitesky
; Andreas Quirrenbach
; Stuart B. Shaklan
; Edward J. Shaya
; Louis E. Strigari
; John A. Tomsick
; Ann E. Wehrle
; Guy Worthey
; | | Date: |
28 Aug 2007 | | Abstract: | Precision astrometry at microarcsecond accuracy has application to a wide
range of astrophysical problems. This paper is a study of the science questions
that can be addressed using an instrument that delivers parallaxes at about 4
microarcsec on targets as faint as V = 20, differential accuracy of 0.6
microarcsec on bright targets, and with flexible scheduling. The science topics
are drawn primarily from the Team Key Projects, selected in 2000, for the Space
Interferometry Mission PlanetQuest (SIM PlanetQuest). We use the capabilities
of this mission to illustrate the importance of the next level of astrometric
precision in modern astrophysics. SIM PlanetQuest is currently in the detailed
design phase, having completed all of the enabling technologies needed for the
flight instrument in 2005. It will be the first space-based long baseline
Michelson interferometer designed for precision astrometry. SIM will contribute
strongly to many astronomical fields including stellar and galactic
astrophysics, planetary systems around nearby stars, and the study of quasar
and AGN nuclei. SIM will search for planets with masses as small as an Earth
orbiting in the ’habitable zone’ around the nearest stars using differential
astrometry, and could discover many dozen if Earth-like planets are common. It
will be the most capable instrument for detecting planets around young stars,
thereby providing insights into how planetary systems are born and how they
evolve with time. SIM will observe significant numbers of very high- and
low-mass stars, providing stellar masses to 1%, the accuracy needed to
challenge physical models. Using precision proper motion measurements, SIM will
probe the galactic mass distribution and the formation and evolution of the
Galactic halo. (abridged) | | Source: | arXiv, 0708.3953 | | Services: | Forum | Review | PDF | Favorites | |
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