Troubleshooting the 24-inch Telescope and Photometric System at Hobbs Observatory

dc.contributor.advisorFord, Lyle A.
dc.contributor.advisorStecher, George J.
dc.contributor.authorCook, Cole
dc.contributor.authorRoot, Geoffrey
dc.date.accessioned2011-12-19T20:49:47Z
dc.date.available2011-12-19T20:49:47Z
dc.date.issued2011-05
dc.descriptionColor poster with text and images.en
dc.description.abstractAsteroids are remnants from the formation of the solar system. By studying the properties of asteroids, insights about this period of time and the solar system itself can be gained. In order to study the rotational properties of asteroids, photometric observations are made using the 24-inch telescope at Hobbs Observatory. After recent modifications to this telescope, inconsistencies were observed within the photometric data. The possible causes of these inconsistencies are examined.en
dc.description.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programsen
dc.identifier.urihttp://digital.library.wisc.edu/1793/55610
dc.language.isoen_USen
dc.relation.ispartofseriesUSGZE AS589en
dc.subjectTelescopesen
dc.subjectAsteroids--Brightnessen
dc.subjectAstronomical photometryen
dc.subjectHobbs Observatory (Eau Claire, Wis.)en
dc.subjectPostersen
dc.titleTroubleshooting the 24-inch Telescope and Photometric System at Hobbs Observatoryen
dc.typePresentationen

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