File:An asteroid that has split due to rotational fission (artist’s impression).tif
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[edit]DescriptionAn asteroid that has split due to rotational fission (artist’s impression).tif | This artist’s impression shows an asteroid that has split up to due to rotational fission and become a binary. New work shows that such binaries will break apart and form two separate asteroids on similar, but independent, orbits around the Sun if the larger piece is more than five times as massive as the smaller. | ||||
Date | 26 August 2010, 10:00 | ||||
Source | https://www.eso.org/public/images/ann1051a/ | ||||
Author | ESO/M.Kornmesser/L. Calçada | ||||
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 20:11, 2 December 2023 | 4,000 × 2,827 (12.14 MB) | Юрий Д.К. (talk | contribs) | {{Information |Description=This artist’s impression shows an asteroid that has split up to due to rotational fission and become a binary. New work shows that such binaries will break apart and form two separate asteroids on similar, but independent, orbits around the Sun if the larger piece is more than five times as massive as the smaller. |Source=https://www.eso.org/public/images/ann1051a/ |Date=26 August 2010, 10:00 |Author=ESO/M.Kornmesser/L. Calçada |Permission={{eso}} |other_versions= }... |
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Width | 4,000 px |
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Height | 2,827 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 21 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | CINEMA 4D |
File change date and time | 10:21, 25 August 2010 |
Color space | Uncalibrated |