File:Bright comet 1995 Q1 (eso9516a).tiff
Bright_comet_1995_Q1_(eso9516a).tiff (511 × 509 pixels, file size: 106 KB, MIME type: image/tiff)
Captions
Summary
[edit]DescriptionBright comet 1995 Q1 (eso9516a).tiff |
English: This image of Bright Comet 1995 Q1 shows the comet head (coma) and the intricate structure of the innermost part of the long, narrow tail that points towards SE, i.e. away from the Sun. This photo was made with an emulsion-filtre combination that registers blue light from the molecules and ions in the coma and tail. The appearance of the tail changes rapidly due to the strong influence of the solar wind at the comet's relatively close location to the Sun, about 75 million kilometres. This corresponds to half the distance between the Earth and the Sun. |
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Date | 22 August 1995 (upload date) | ||
Source |
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Author | ESO | ||
Other versions |
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Licensing
[edit]This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 01:52, 1 April 2024 | 511 × 509 (106 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://www.eso.org/public/archives/images/original/eso9516a.tif via Commons:Spacemedia |
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Metadata
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Image title | This image of Bright Comet 1995 Q1 shows the comet head (coma) and the intricate structure of the innermost part of the long, narrow tail that points towards SE, i.e. away from the Sun. This photo was made with an emulsion-filtre combination that registers blue light from the molecules and ions in the coma and tail. The appearance of the tail changes rapidly due to the strong influence of the solar wind at the comet's relatively close location to the Sun, about 75 million kilometres. This corresponds to half the distance between the Earth and the Sun. |
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Width | 511 px |
Height | 509 px |
Bits per component | 8 |
Compression scheme | LZW |
Pixel composition | Palette |
Image data location | 23,612 |
Orientation | Normal |
Number of components | 1 |
Number of rows per strip | 509 |
Bytes per compressed strip | 77,916 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS4 Macintosh |
File change date and time | 10:25, 26 January 2011 |
Color space | Uncalibrated |