NOAO >   Observing Info >   Approved Programs >   2017B-0086

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Program Information for 2017B-0086


PI: Carl Melis, UC San Diego, cmelis@ucsd.edu
Address: Center for Astrophysics and Space Sciences, 9500 Gilman Drive, Code 0424, La Jolla, CA, 92093-0424 USA

CoI: Patrick Dufour, University of Montreal

Title: Does SDSSJ195750.83+340404.4 accrete from a circumstellar disk made of a planetary core?

Abstract: White dwarf stars are now known to regularly accrete material from their extant planetary systems. We have identified a new polluted white dwarf star that appears to be accreting extremely iron-rich material, suggesting that it is being polluted by the core of a massive, differentiated rocky body. We propose Gemini NIRI near-infrared imaging photometry observations of SDSSJ1957+3404 that will allow us to ensure that infrared excess emission detected toward the white dwarf by Spitzer truly emanates from a disk orbiting it and to better constrain the disk properties. These observations will be an essential part of a greater program targeting this white dwarf that will address questions pertaining to terrestrial planet structure and formation processes and the question of what mixture of elements is responsible for Earth's under-dense outer core.

Program Type: Standard/Galactic

Scheduled Nights:
Run 1 (2017B):  GEM-NQ/NIRI -- 0.9hrs band 1 (GN-2017B-Q-23)


National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360



NOAO >   Observing Info >   Approved Programs >   2017B-0086

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