File:The near-nucleus region of comet Hale-Bopp (eso9624a).tiff
The_near-nucleus_region_of_comet_Hale-Bopp_(eso9624a).tiff (505 × 480 pixels, file size: 101 KB, MIME type: image/tiff)
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Summary
[edit]DescriptionThe near-nucleus region of comet Hale-Bopp (eso9624a).tiff |
English: A series of CCD frames, showing the inner coma of Comet Hale-Bopp, was obtained with the SUSI high angular resolution camera at the ESO 3.5-metre New Technology Telescope (NTT) under very good seeing conditions in the morning of March 20, 1996. The photo shows a composite of nine 1-min exposures through a red filtre. The telescope was set to follow the motion of the comet and the stars are therefore seen as nine small trails (the intervals correspond to the time needed for the read-out from the CCD). The field shown measures about 55 x 55 arcsec across. North is up and East is left. |
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Date | 22 March 1996 (upload date) | ||
Source |
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Author | ESO | ||
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Licensing
[edit]This media was created by the European Southern Observatory (ESO).
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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current | 19:54, 21 June 2024 | 505 × 480 (101 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://www.eso.org/public/archives/images/original/eso9624a.tif via Commons:Spacemedia |
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Image title | A series of CCD frames, showing the inner coma of Comet Hale-Bopp, was obtained with the SUSI high angular resolution camera at the ESO 3.5-metre New Technology Telescope (NTT) under very good seeing conditions in the morning of March 20, 1996. The photo shows a composite of nine 1-min exposures through a red filtre. The telescope was set to follow the motion of the comet and the stars are therefore seen as nine small trails (the intervals correspond to the time needed for the read-out from the CCD). The field shown measures about 55 x 55 arcsec across. North is up and East is left. |
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Width | 505 px |
Height | 480 px |
Bits per component | 8 |
Compression scheme | LZW |
Pixel composition | Black and white (Black is 0) |
Orientation | Normal |
Number of components | 1 |
Number of rows per strip | 16 |
Data arrangement | chunky format |
White point chromaticity |
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Chromaticities of primarities |
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