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Fáìlì:003428-asteroid shape model (3428) Roberts.png

003428-asteroid_shape_model_(3428)_Roberts.png (250 × 250 pixel, ìtóbi faili: 13 KB, irú MIME: image/png)

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Ìjúwe
English: 3D convex shape model of 3428 Roberts, 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
Ọjọ́ọdún
Orísun DAMIT – Database of Asteroid Models from Inversion Techniques: for (3428) Roberts
Olùdá Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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lọ́wọ́05:56, 19 Oṣù Ẹ̀rẹ̀nà 2020Àwòrán kékeré fún ní 05:56, 19 Oṣù Ẹ̀rẹ̀nà 2020250 × 250 (13 KB)Rfassbind{{Information |description={{en|1=3D convex shape model of {{w|3428 Roberts}}, 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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