Rotation period and light curve of asteroid 423 Diotima

The asteroid 423 Diotima was observed photoelectrically in V filter during October 1987 at Observatorio Municipal de Mercedes. The synodic rotational period and amplitude obtained are: P=4.626 ± 0.002 hours and Δm=0.196 ± 0.014. The values confirm the solution proposed by Zappala et al. (1985) to th...

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Autor principal: Gil-Hutton, Ricardo Alfredo
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1990
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142717
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id I19-R120-10915-142717
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Gil-Hutton, Ricardo Alfredo
Rotation period and light curve of asteroid 423 Diotima
topic_facet Astronomía
Galaxia
description The asteroid 423 Diotima was observed photoelectrically in V filter during October 1987 at Observatorio Municipal de Mercedes. The synodic rotational period and amplitude obtained are: P=4.626 ± 0.002 hours and Δm=0.196 ± 0.014. The values confirm the solution proposed by Zappala et al. (1985) to the ambiguity presented in previous determinations of the rotational period and convert this asteroid in a peculiar object.
format Articulo
Comunicacion
author Gil-Hutton, Ricardo Alfredo
author_facet Gil-Hutton, Ricardo Alfredo
author_sort Gil-Hutton, Ricardo Alfredo
title Rotation period and light curve of asteroid 423 Diotima
title_short Rotation period and light curve of asteroid 423 Diotima
title_full Rotation period and light curve of asteroid 423 Diotima
title_fullStr Rotation period and light curve of asteroid 423 Diotima
title_full_unstemmed Rotation period and light curve of asteroid 423 Diotima
title_sort rotation period and light curve of asteroid 423 diotima
publishDate 1990
url http://sedici.unlp.edu.ar/handle/10915/142717
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