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003822-asteroid_shape_model_(3822)_Segovia.png (250 × 250 pixels, file size: 17 KB, MIME type: image/png)

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English: 3D convex shape model of 3822 Segovia, 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
Source DAMIT – Database of Asteroid Models from Inversion Techniques: for (3822) Segovia
Author Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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current07:57, 19 March 2020Thumbnail for version as of 07:57, 19 March 2020250 × 250 (17 KB)Rfassbind{{Information |description={{en|1=3D convex shape model of {{w|3822 Segovia}}, 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 |vol...

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