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A Photometric Search for Extrasolar Planets Around White
Dwarfs
by Michael J. Wilson
Abstract:
This thesis is an observational survey, using the Iowa
Robotic Observatory,
with the goal of detecting an extrasolar planet around a white dwarf.
With the large
number of planets that have been discovered around solar-type stars,
a natural
assumption is that some of these planets may remain in orbit around
the remnant white
dwarf. A brief look at the conditions under which a Jovian planet orbiting
near a
white dwarf may form is taken in order to see that the drag force experienced
by the
orbiting planet causes it to spiral in. The Roche radius is considered
for how close
a potential planet can approach along with the probability of an eclipse
if the planet
is close to the star. An initial number of the local sample (within
20 parsecs) of
white dwarfs is chosen, with 84 targets remaining out of 105 initial
targets after known
binary systems are removed. Of these 84 white dwarfs, 75 were observed
and 128 light
curves generated over 578 good hours of observation out of 698 hours
total during survey
period of October 2002 until July 2003. No eclipse events were detected,
which led to
the conclusion that planets surviving very close to the Roche limit
(within a few
hundredths of an AU) are not common. In addition, a study of the variability
of
these white dwarfs was undertaken. It was found that a few possibilities
arose,
including the possibility of a variable that was not a white dwarf,
but was one of
the calibration stars used.
Download the final thesis:
Without Appendices:
PDF (2 MB)
MS Word (1.5 MB)
With Appendices:
PDF (32 MB)
MS Word (41 MB)
Sample White Dwarf Images
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RA 04:23 Dec 12:00
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RA 04:26 Dec 58:48
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Images and Charts:
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