File:001703-asteroid shape model (1703) Barry.png

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Summary

Description	English: 3D convex shape model of 1703 Barry, computed using light curve inversion techniques. J. Hanuš, J. Ďurech, M. Brož, B. D. Warner (June 2011). "A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method". Astronomy and Astrophysics 530: A134. DOI:10.1051/0004-6361/201116738. ISSN 0004-6361. arXiv
Date	16 March 2020
Source	DAMIT – Database of Asteroid Models from Inversion Techniques: for (1703) Barry
Author	Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	09:44, 17 March 2020		250 × 250 (16 KB)	Rfassbind	{{Information \|description={{en\|1=3D convex shape model of {{w\|1703 Barry}}, computed using {{w\|light curve}} inversion techniques.}} {{cite journal \|authors = {{w\|Josef Hanuš (astronomer)\|J. Hanuš}}, {{w\|Josef Ďurech\|J. Ďurech}}, {{w\|Miroslav Brož\|M. Brož}}, {{w\|Brian D. Warner\|B. D. Warner}} \|date = June 2011 \|title = A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method \|journal = Astronomy and Astrophysics \|volum...

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