File:004492-asteroid shape model (4492) Debussy.png
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Summary
| Description |
English: 3D convex shape model of 4492 Debussy, 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 (4492) Debussy |
| Author | Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:33, 19 March 2020 | 250 × 250 (16 KB) | Rfassbind | {{Information |description={{en|1=3D convex shape model of {{w|4492 Debussy}}, 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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