Please use this identifier to cite or link to this item: http://cmuir.cmu.ac.th/jspui/handle/6653943832/57893
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dc.contributor.authorS. Dueantakhuen_US
dc.contributor.authorS. Wannawichianen_US
dc.date.accessioned2018-09-05T03:52:41Z-
dc.date.available2018-09-05T03:52:41Z-
dc.date.issued2017-10-20en_US
dc.identifier.issn17426596en_US
dc.identifier.issn17426588en_US
dc.identifier.other2-s2.0-85034097688en_US
dc.identifier.other10.1088/1742-6596/901/1/012008en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85034097688&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/57893-
dc.description.abstract© Published under licence by IOP Publishing Ltd. The study of orbital elements of Asteroids in Cometary Orbits (ACOs) is based on images taken by a 0.7-m telescope to find positions of asteroids and calculate their orbital elements. This work focuses on variation of positions and orbital shape of an asteroid, 1667Pels, which is obtained by analyzing orbital elements and minimum orbital intersection distances. Each observation, those parameters are affected by the gravity from Jupiter on ACOs. The accuracy of single site data was calibrated by comparing the result from this work to other observations in Minor Planet Center database.en_US
dc.subjectPhysics and Astronomyen_US
dc.titleOrbital Shapes of Asteroids in Cometary Orbits based on 0.7m Telescope Imagingen_US
dc.typeConference Proceedingen_US
article.title.sourcetitleJournal of Physics: Conference Seriesen_US
article.volume901en_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsNational Astronomical Research Institute of Thailanden_US
Appears in Collections:CMUL: Journal Articles

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