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HD 80606 Exoplanet Transit Campaign

Note: This observing campaign is now over.

The AAVSO is working with www.transitsearch.org to coordinate the observing campaign of HD 80606 and its most unusual extrasolar planet. With an orbital eccentricity of e ~ 0.93, HD 80606b ranks as the most eccentric planet known. HD 80606 has a visual binary companion called HD 80607. It has been suggested that HD 80606b's extreme eccentricity may be the result of a three-body interaction between the planet and these two stars (Wu & Murray 2003).

There are some challenges to this observing request, including a low probability of transit and a relatively bright star companion. However, detecting this transit would give us an unprecedented characaterization of this remote orbiting world, so we need your help!

We are recommending intense photometric monitoring of the star during the four-day window centered on 2005 Feb 25 19:39 UT. Please submit your photometry using WebObs, the AAVSO online data submission tool. It is easy to use and will help format all of the observations appropriately.

Highly eccentric orbit of HD 80606b. Click image to enlarge. See G. Laughlin, 2005 (pdf) for more info.
Last updated: Wed Feb 23 14:19:29 EST 2005

Background Information
      Original Announcement - Detailed Information from transitsearch.org (pdf file)
      HD 80606 Results page - transitsearch.org

Up-to-date Information
      
       AAVSO Photometry Discussion Group - General postings

Tips
      
Tips on Bright Star Photometry

Want to know more about Transit Search and other campaigns?
      Variable Star of the Season - Transiting Exoplanets HD 209458 and TrES-1
      HD 74156 and HD 37605 - Completed in December 2004
      IL Aqr/GJ 876 Transit Campaign - Completed in October 2004
      AAVSO Exoplanet Transit Search - Main observing program web pages
      Bruce Gary's Transitsearch Tips

HD 80606 Campaign Details

PlanetPeak WindowDepthDuration
HD 80606b JD 2453427.32 +/- .4 1.34%17.33 hours

transit histogram
Histogram of central transit times computed using 1-planet Keplerian fits to the combined Swiss and Keck radial velocity data, combined with a bootstrap Monte-Carlo method to compute transit times. More information is available in the Original Announcement
 
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