detecting exoplanets and exomoons

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Detecting Exoplanets and Exomoons By Kimberly Ward-Duong Mentor: Dr. Stephen C. Tegler NAU Dept. of Physics and Astronomy Arizona/NASA Space Grant Research Symposium Tucson, Arizona April 17, 2010 With the Lutz 0.5-Meter Telescope

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With the Lutz 0.5-Meter Telescope. Detecting Exoplanets and Exomoons. By Kimberly Ward-Duong Mentor: Dr. Stephen C. Tegler NAU Dept. of Physics and Astronomy Arizona/NASA Space Grant Research Symposium Tucson, Arizona April 17, 2010. Exoplanets and Their Transits. Extrasolar Planets - PowerPoint PPT Presentation

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Page 1: Detecting Exoplanets and Exomoons

Detecting Exoplanets and Exomoons

By Kimberly Ward-DuongMentor: Dr. Stephen C. Tegler

NAU Dept. of Physics and Astronomy

Arizona/NASA Space Grant Research SymposiumTucson, ArizonaApril 17, 2010

With the Lutz 0.5-Meter Telescope

Page 2: Detecting Exoplanets and Exomoons

Exoplanets and Their Transits

Extrasolar Planets 443 systems 71 known to transit Transit/lightcurve relation Tc

Image credit: http://www.astro.virginia.edu/class/oconnell/astr121/

Our project: 1. Observe stars with known

exoplanet transits 2. Analyze transit lightcurves

Page 3: Detecting Exoplanets and Exomoons

Transit Timing Variation (TTV)

Periodic changes in Tc

New technique to detect multiple planet systems Ideal for the detection of other Earths, super-Earths

○ None yet discovered by these means!

http://images.iop.org/objects/phw/world/22/3/36/PWbra1_03-09.jpg

Page 4: Detecting Exoplanets and Exomoons

Data Collection

Atmospheric Research Observatory at NAU

Barry Lutz Telescope• 0.5-m (20-in) Ritchey-Chrétien

telescope• Apogee CCD Camera• 150-600+ images • 5-7 hours of data per night

Images courtesy of Dr. Stephen Tegler

Page 5: Detecting Exoplanets and Exomoons

Data Reduction Process

Creation of detailed analysis procedure

IRAFDifferential photometry

Plot and model lightcurves using MATLAB

WASP-11/HAT-P-10

Page 6: Detecting Exoplanets and Exomoons

ResultsWASP-11/HAT-P-10

•Quadratic limb darkening model fit to data (Mandel & Agol 2002)

•Parameters from discovery paper (West et al. 2009)

•Free parameter: Tc

•Standard deviation: 3 mmag

Page 7: Detecting Exoplanets and Exomoons

Discussion/Conclusion Observed transit timing variation?

Yes! Best fit model Tc early by 5 minutes

1.8 sec period difference

Possible explanations

More observations needed to verify/explain findings

Long term project plansGoal: Observe 50-100 transits/objectFurther refine modeling specificationsTechnique may also prove useful

for finding an exomoon

Image credit: http://www.astro.virginia.edu/class/oconnell/astr121/

Page 8: Detecting Exoplanets and Exomoons

Thank you!

And many thanks to:Dr. Stephen TeglerDr. Nadine Barlow

Ms. Kathleen StigmonArron Shiffer

David TollefsenAlex McCanna

NASA and the Arizona Space Grant Consortium

Questions?Artist’s impression of exoplanet HD 189733b

(Giovanni Tinetti)

(Title slide image credit: STScI artist rendition)