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THE HUNGARIA ASTEROID 4868 KNUSHEVIA: A POSSIBLE BINARY
CCD photometry observations of the Hungaria asteroid 4868 Knushevia were made in 2013 April-June at the Center for Solar System Studies. Analysis of the data indicates that the asteroid may be a binary with a primary period P(1) = 3.4122 ± 0.0001 h, A(1) = 0.05 ± 0.01 mag and a secondary period of P...
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| Publicat a: | Minor Planet Bull |
|---|---|
| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
2015
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7244136/ https://ncbi.nlm.nih.gov/pubmed/32455357 |
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