PI: Andrew Howard, University of California, Berkeley, email@example.com
Address: Astronomy Department, 601 Campbell Hall MC 3411, Berkeley, CA 94720, United States
CoI: Ian Crossfield, University of California, Los Angeles
CoI: Howard Isaacson, University of California, Berkeley
CoI: Stephen Kane, NASA Exoplanet Science Institute
Title: Properties and Ephemeris of HD 97658b
Abstract: Our team recently discovered the transiting extrasolar planet HD 97658b. This ``super-Earth'' has a mass of 6.4 Earth-masses and a radius of 2.9 Earth-radii, implying a low bulk density of 1.4 g cm^- 3. The size and mass are intermediate between the terrestrial and ice giants in our solar system. It is one of only three super-Earths known to transit a bright enough nearby star for which detailed follow-up atmospheric spectroscopy is feasible. We have planned transmission spectroscopy using Spitzer, Hubble, and the IRTF. These measurements are sensitive to atmospheric hydrogen, water, and CO_2, and will constrain the internal composition. Scheduling these measurements depends on a precise transit ephemeris, which our discovery data were insufficient to produce. The wide-field imager on the 0.9-m WIYN is ideal to measure a transit light curve with bright comparison stars separated by tens of arcminutes. We request two nights which will yield the planetary radius in R-band (anchoring atmospheric models) and an accurate transit ephemeris for scheduling the space-based and large aperture follow-up observations.
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