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ANOTHER TRIO OF POSSIBLE VERY WIDE BINARY ASTEROIDS
Lightcurve analysis of the near-Earth asteroids (442742) 2012 WP3, (523604) 2004 QB17, and 2018 RL indicate that they are potential members of a relatively rare class of “very wide binary asteroids.” These objects feature a primary rotational period of tens to hundreds of hours and a secondary rotat...
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| Pubblicato in: | Minor Planet Bull |
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| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
2019
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7192042/ https://ncbi.nlm.nih.gov/pubmed/32355918 |
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