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Ìjúwe
English: 3D convex shape model of 5314 Wilkickia, 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 (5314) Wilkickia
Olùdá Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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5314 Wilkickia

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12 Oṣù Èrèlé 2024

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Ọjọ́ọdún/ÀkókòÀwòrán kékeréÀwọn ìwọ̀nOníṣeÀríwí
lọ́wọ́09:12, 17 Oṣù Èrèlé 2024Àwòrán kékeré fún ní 09:12, 17 Oṣù Èrèlé 20241,024 × 1,024 (125 KB)Svr-box{{Information |description={{en|1=3D convex shape model of {{w|5314 Wilkickia}}, 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 |v...

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