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LIGHTCURVE ANALYSIS OF NEA 2015 HM10
Independent CCD photometry observations by the authors of the near-Earth asteroid 2015 HM10 were made in 2015 July. Analysis of both data sets found a synodic rotation period of approximately 0.376 h and amplitude of 1.47 ± 0.05 mag.
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| Udgivet i: | Minor Planet Bull |
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| Main Authors: | , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
2016
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| Fag: | |
| Online adgang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7244007/ https://ncbi.nlm.nih.gov/pubmed/32455366 |
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