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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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Dades bibliogràfiques
Publicat a:Minor Planet Bull
Autors principals: Warner, Brian D., Stephens, Robert D.
Format: Artigo
Idioma:Inglês
Publicat: 2015
Matèries:
Accés en línia:https://ncbi.nlm.nih.gov/pmc/articles/PMC7244136/
https://ncbi.nlm.nih.gov/pubmed/32455357
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