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Photometric lightcurve and rotation period of Himalia (Jupiter VI)

Pilcher, Frederick and Mottola, Stefano and Denk, Tilmann (2012) Photometric lightcurve and rotation period of Himalia (Jupiter VI). Icarus: International Journal of Solar System Studies (219), pp. 741-742. Elsevier. DOI: http://dx.doi.org/10.1016/j.icarus.2012.03.021

Full text not available from this repository.

Official URL: http://www.sciencedirect.com/science/article/pii/S0019103512001145

Abstract

Due to their great distance from their primaries and rapid solar perturbations of their orbits, the outer irregular satellites of the giant planets are not in tidal rotational lock. They are generally thought to be asteroid-like bodies with irregular shapes and rotation periods much shorter than the orbital ones, whose rotational properties can be found by the methods used to study asteroids. We report here the results of two sets of independent photometric CCD observations overlapping in time that were obtained using 0.35- and 1.23-m telescopes. The combined data set yields for Himalia a unique synodic rotation period of 7.7819 ± 0.0005 h, with a lightcurve amplitude of 0.20 ± 0.01 magnitudes. This determination corrects the erroneous period of 9.5 h published by Degewij et al. (Degewij, J., Andersson, L.E., Zellner, B. [1980a]. Icarus 44, 520–540).

Item URL in elib:https://elib.dlr.de/77110/
Document Type:Article
Title:Photometric lightcurve and rotation period of Himalia (Jupiter VI)
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Pilcher, FrederickOrgan Mesa ObservatoryUNSPECIFIED
Mottola, Stefanostefano.mottola (at) dlr.deUNSPECIFIED
Denk, TilmannFreie Universität BerlinUNSPECIFIED
Date:2012
Journal or Publication Title:Icarus: International Journal of Solar System Studies
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
DOI :http://dx.doi.org/10.1016/j.icarus.2012.03.021
Page Range:pp. 741-742
Publisher:Elsevier
Status:Published
Keywords:Irregular satellites, Jupiter, Satellites, Photometry
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Exploration des Sonnensystems (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Asteroids and Comets
Deposited By: Mottola, Dr.phys. Stefano
Deposited On:19 Sep 2012 08:22
Last Modified:10 Jan 2019 15:47

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