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LIGHTCURVE ANALYSIS OF THE NEA BINARY ASTEROID 5381 SEKHMET
Radar observations in 2003 (Nolan et al., 2003) showed that the near-Earth asteroid (NEA) 5381 Sekhmet was a binary. CCD photometry observations made from the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) during the 2014 apparition confirmed the discovery and found the first precis...
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| Vydáno v: | Minor Planet Bull |
|---|---|
| Hlavní autoři: | , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
2014
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| Témata: | |
| On-line přístup: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7249533/ https://ncbi.nlm.nih.gov/pubmed/32457964 |
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