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Fáìlì:000155-asteroid shape model (155) Scylla.png

000155-asteroid_shape_model_(155)_Scylla.png (250 × 250 pixel, ìtóbi faili: 16 KB, irú MIME: image/png)

Àkótán

Ìjúwe
English: 3D convex shape model of 155 Scylla, 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 (155) Scylla
Olùdá Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

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155 Scylla

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26 Oṣù Ẹ̀bìbì 2020

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5b71bfb7f891eaa935a55c14bf43bc3c70d3962f

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250 pixel

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lọ́wọ́09:21, 26 Oṣù Ẹ̀bìbì 2020Àwòrán kékeré fún ní 09:21, 26 Oṣù Ẹ̀bìbì 2020250 × 250 (16 KB)Rfassbind{{Information |description={{en|1=3D convex shape model of {{w|155 Scylla}}, 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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