Constraining the Shape Distribution of Near Earth Objects from Partial Lightcurves
Constraining the Shape Distribution of Near Earth Objects from Partial Lightcurves
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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In the absence of dense photometry for a large population of Near Earth Objects (NEOs), the best method of obtaining a shape distribution comes from sparse photometry and partial lightcurves. We have used 867 partial lightcurves obtained by Spitzer to determine a shape distribution for sub-kilometre NEOs. From this data we find a best fit average e...
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Constraining the Shape Distribution of Near Earth Objects from Partial Lightcurves
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TN_cdi_proquest_journals_2189903528
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2189903528
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1903.03159
