APS April Meeting 2010
Volume 55, Number 1
Saturday–Tuesday, February 13–16, 2010;
Washington, DC
Session V1: Plenary Session III
8:30 AM–10:18 AM,
Tuesday, February 16, 2010
Room: Marriott Ballroom Salon 1-2
Chair: Michael Turner, University of Chicago
Abstract ID: BAPS.2010.APR.V1.2
Abstract: V1.00002 : Status of Kepler Mission and Early Discoveries
9:06 AM–9:42 AM
Preview Abstract
Abstract
Author:
William J. Borucki
(NASA Ames Research Center)
Kepler is a Discovery-class mission designed to determine the
frequency of Earth-size planets in and near the habitable zone of
solar-like stars. The instrument consists of a 0.95 m aperture
photometer designed to obtain high precision photometric
measurement of $>$ 100,000 stars to search for patterns of
transits. The focal plane of the Schmidt-type telescope contains
42 CCDs with at total of 95 megapixels that cover 115 square
degrees of sky. The photometer was launched into an
Earth-trailing heliocentric orbit on March 6, 2009, finished its
commissioning on May 12, and is now in the science operations
mode. During the commissioning, data were obtained at a 30 minute
cadence for 53,000 stars for 9.7 days. During the first 33.5 days
of science-mode operation, 156,000 stars have been observed.
Discoveries based on these data are presented.
Although the data have not yet been corrected for the presence of
systematic errors and artifacts, the data show the presence of
hundreds of eclipsing binary stars and variable stars of amazing
variety. To provide some estimate of the capability of the
photometer, a quick analysis of the photometric precision was
made. Analysis of the commissioning data also show transits,
occultations and light emitted from the known exoplanet HAT-P7b.
The data show a smooth rise and fall of light from the planet as
it orbits its star, punctuated by a drop of 130$\pm$11 ppm in
flux when the planet passes behind its star. We interpret this as
the phase variation of the dayside thermal emission from the
planet plus reflected light as it orbits its star and is
occulted. The depth of the occultation is similar in amplitude to
that expected from a transiting Earth-size planet and
demonstrates that the Mission has the precision necessary to
detect such planets.
Discoveries of several new exoplanets are shown and compared with
known exoplanets with respect to mass, size, density, and
orbital period. Detection of stellar oscillations and unusual
objects are also presented.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2010.APR.V1.2