File:Spectacular jet in comet Hale-Bopp (eso9522a).tiff
Spectacular_jet_in_comet_Hale-Bopp_(eso9522a).tiff (520 × 589 pixels, file size: 89 KB, MIME type: image/tiff)
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Summary
[edit]DescriptionSpectacular jet in comet Hale-Bopp (eso9522a).tiff |
English: This false-colour image of the large jet now observed in bright comet Hale-Bopp is a computer-enhanced version of a near-IR CCD-frame. It was obtained on August 31 1995 with the multi-mode DFOSC instrument at the Danish 1.5-m telescope on La Silla by Emilio Molinari from Osservatorio di Brera, Milano-Merate, Italy. On this photo, North is up and East is to the left. One pixel measures 0.5 arcsec and the circular field has a diameter of 65 arcsec. The intensity scale is indicated with the colour bar at the bottom; the intensity increases towards the right |
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Date | 1 September 1995 (upload date) | ||
Source |
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Author | ESO | ||
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current | 22:52, 14 June 2024 | ![]() | 520 × 589 (89 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://www.eso.org/public/archives/images/original/eso9522a.tif via Commons:Spacemedia |
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Image title | This false-colour image of the large jet now observed in bright comet Hale-Bopp is a computer-enhanced version of a near-IR CCD-frame. It was obtained on August 31 1995 with the multi-mode DFOSC instrument at the Danish 1.5-m telescope on La Silla by Emilio Molinari from Osservatorio di Brera, Milano-Merate, Italy. On this photo, North is up and East is to the left. One pixel measures 0.5 arcsec and the circular field has a diameter of 65 arcsec. The intensity scale is indicated with the colour bar at the bottom; the intensity increases towards the right |
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Width | 520 px |
Height | 589 px |
Bits per component | 8 |
Compression scheme | LZW |
Pixel composition | Palette |
Orientation | Normal |
Number of components | 1 |
Number of rows per strip | 15 |
Data arrangement | chunky format |
White point chromaticity |
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Chromaticities of primarities |
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