Jump to content

Fáìlì:004616-asteroid shape model (4616) Batalov.png

Page contents not supported in other languages.
Lát'ọwọ́ Wikipedia, ìwé ìmọ̀ ọ̀fẹ́

Fáìlì àtìbẹ̀rẹ̀ (1,024 × 1,024 pixel, ìtóbi faili: 142 KB, irú MIME: image/png)

Àkótán

Ìjúwe
English: 3D convex shape model of 4616 Batalov, 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 (4616) Batalov
Olùdá Astronomical Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin

Ìwé àṣẹ

w:en:Creative Commons
ìdárúkọ
This file is licensed under the Creative Commons Attribution 4.0 International license.
Ẹ ní ààyè:
  • láti pín pẹ̀lú ẹlòmíràn – láti ṣàwòkọ, pínkiri àti ṣàgbéká iṣẹ́ náà
  • láti túndàpọ̀ – láti mulò mọ́ iṣẹ́ míràn
Lábẹ́ àwọn àdéhùn wọ̀nyí:
  • ìdárúkọ – Ẹ gbọdọ̀ ṣe ọ̀wọ̀ tó yẹ, pèsè ìjápọ̀ sí ìwé-àṣe, kí ẹ sì sọ bóyá ìyípadà wáyé. Ẹ le ṣe èyí lórísi ọ̀nà tó bojúmu, sùgbọ́n tí kò ní dà bii pé oníìwé-àṣe fọwọ́ sí yín tàbí lílò yín.

akole

Ṣafikun alaye ila kan ti ohun ti faili yii duro

Awọn nkan ṣe afihan ninu faili yii

depicts Èdè Gẹ̀ẹ́sì

copyright status Èdè Gẹ̀ẹ́sì

copyrighted Èdè Gẹ̀ẹ́sì

copyright license Èdè Gẹ̀ẹ́sì

5 Oṣù Ọ̀pẹ̀ 2023

media type Èdè Gẹ̀ẹ́sì

image/png

checksum Èdè Gẹ̀ẹ́sì

ae828812966332e84062684cfd9912f71eac1f13

data size Èdè Gẹ̀ẹ́sì

145,757 byte

height Èdè Gẹ̀ẹ́sì

1,024 pixel

width Èdè Gẹ̀ẹ́sì

1,024 pixel

Ìtàn fáìlì

Ẹ kan kliki lórí ọjọ́ọdún/àkókò kan láti wo fáìlì ọ̀ún bó ṣe hàn ní àkókò na.

Ọjọ́ọdún/ÀkókòÀwòrán kékeréÀwọn ìwọ̀nOníṣeÀríwí
lọ́wọ́13:01, 9 Oṣù Ọ̀pẹ̀ 2023Àwòrán kékeré fún ní 13:01, 9 Oṣù Ọ̀pẹ̀ 20231,024 × 1,024 (142 KB)Svr-box{{Information |description={{en|1=3D convex shape model of {{w|4616 Batalov}}, 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...

Ojúewé kan yìí únlo fáìlì yí:

Ìlò fáìlì káàkiri

Àwọn wiki míràn wọ̀nyí lo fáìlì yìí: