PI: Eric Nielsen, SETI Institute/NASA Ames Research Center, email@example.com
Address: 189 N BERNARDO AVE, MOUNTAIN VIEW, CA 94043 United States
CoI: Alexandra Greenbaum, U. of Michigan
CoI: Quinn Konopacky, UC San Diego
CoI: Robert de Rosa, UC Berkeley
CoI: Jason Wang, UC Berkeley
CoI: Michael Ireland, MSSSO
CoI: Peter Tuthill, U. of Sydney
CoI: Sarah Blunt, Brown U.
CoI: Kimberly Ward-Duong, Arizona State U.
CoI: Franck Marchis, SETI Institute/NASA Ames Research Center
Title: Orbits of Moving Group Binaries: Constraining the Ages of Planet-Hosting Moving Groups using GPI NRM Astrometric Monitoring
Abstract: Resolved spectroscopic binaries in moving groups are a unique opportunity to place strong constraints on the age of those moving groups, and serve as an orthogonal measurement method to make the final age determination more robust. We propose here to monitor 9 moving group binaries with GPI NRM to characterize the orbits of these objects so that these stars may be used as calibrators for the ages of their host moving groups. Ages are vital for characterizing planet and brown dwarf companions, the majority of which are found around moving group stars, and so accurate ages for these groups strongly impact our understanding of directly imaged planets and brown dwarfs. We have recently demonstrated the viability of this method using two sets of binaries in the beta Pic moving group, and propose here to continue our program (approved for 2017A, observations not yet carried out) by monitoring stars in other groups and greatly reduce the uncertainties in quoted ages of nearby moving group stars and planets.
Program Type: Standard/Galactic
Run 1 (2017B): GEM-SQ/GPI -- 11.4hrs band 1 (GS-2017B-Q-22)
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360