File:003189-asteroid shape model (3189) Penza.png
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| Description | 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 (3189) Penza |
| Author | Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 22:21, 28 January 2023 | | 1,024 × 1,024 (151 KB) | Svr-box (talk | contribs) | {{Information |description={{en|1=3D convex shape model of {{w|3189 Penza}}, 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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