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File:002144-asteroid shape model (2144) Marietta.png

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English: 3D convex shape model of 2144 Marietta, 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
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Source DAMIT – Database of Asteroid Models from Inversion Techniques: for (2144) Marietta
Author Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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current10:46, 3 December 2022Thumbnail for version as of 10:46, 3 December 20221,024 × 1,024 (157 KB)Svr-box (talk | contribs){{Information |description={{en|1=3D convex shape model of {{w|2144 Marietta}}, 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 |vo...

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