File:M84, NGC 4374 (noao-m84).tiff
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![File:M84, NGC 4374 (noao-m84).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/2/24/M84%2C_NGC_4374_%28noao-m84%29.tiff/lossy-page1-730px-M84%2C_NGC_4374_%28noao-m84%29.tiff.jpg?20230917195919)
Size of this JPG preview of this TIF file: 730 × 600 pixels. Other resolutions: 292 × 240 pixels | 585 × 480 pixels | 828 × 680 pixels.
Original file (828 × 680 pixels, file size: 1.62 MB, MIME type: image/tiff)
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M84 is an elliptical galaxy of type E1 and a member of the large Virgo Cluster of galaxies. There are also some suggestions that it is actually a face-on lenticular galaxy.
Summary
[edit]DescriptionM84, NGC 4374 (noao-m84).tiff |
English: M84 is an elliptical galaxy of type E1 and a member of the large Virgo Cluster of galaxies. There are also some suggestions that it is actually a face-on lenticular galaxy. Lenticulars, type S0, are mostly smooth and featureless, like elliptical galaxies, but have a significant amount of dust and often some disk-like component, similar to the disk of a spiral galaxy without the arms. M84 contains a small central active region, with two oppositely directed jets visible at radio wavelengths. This image was taken at the KPNO 0.9-meter telescope in December 1996. The Virgo cluster also includes Messier galaxies M49, M58, M59, M60, M61, M85, M86, M87, M88, M89, M90, M91, M98, M99, and M100. |
Date | 30 June 2020, 21:33:00 (upload date) |
Source | M84, NGC 4374 |
Author | NOIRLab/NSF/AURA |
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This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 19:59, 17 September 2023 | ![]() | 828 × 680 (1.62 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-m84.tif via Commons:Spacemedia |
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Image title | M84 is an elliptical galaxy of type E1 and a member of the large Virgo Cluster of galaxies. There are also some suggestions that it is actually a face-on lenticular galaxy. Lenticulars, type S0, are mostly smooth and featureless, like elliptical galaxies, but have a significant amount of dust and often some disk-like component, similar to the disk of a spiral galaxy without the arms. M84 contains a small central active region, with two oppositely directed jets visible at radio wavelengths. This image was taken at the KPNO 0.9-meter telescope in December 1996. The Virgo cluster also includes Messier galaxies M49, M58, M59, M60, M61, M85, M86, M87, M88, M89, M90, M91, M98, M99, and M100. |
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Width | 828 px |
Height | 680 px |
Bits per component |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 3 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | ImageMagick 5.5.1 10/20/02 Q16 http://www.imagemagick.org |