File:Supernovas Portrait Gallery (1999-snrg - pulsarV2BBB).tiff
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![File:Supernovas Portrait Gallery (1999-snrg - pulsarV2BBB).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/8/81/Supernovas_Portrait_Gallery_%281999-snrg_-_pulsarV2BBB%29.tiff/lossy-page1-725px-Supernovas_Portrait_Gallery_%281999-snrg_-_pulsarV2BBB%29.tiff.jpg?20240528093607)
Size of this JPG preview of this TIF file: 725 × 599 pixels. Other resolutions: 290 × 240 pixels | 581 × 480 pixels | 929 × 768 pixels | 1,239 × 1,024 pixels | 2,100 × 1,736 pixels.
Original file (2,100 × 1,736 pixels, file size: 1.41 MB, MIME type: image/tiff)
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Structured data
Captions
Captions
Chandra X-ray Image of PSR 0540-69
Summary
[edit]DescriptionSupernovas Portrait Gallery (1999-snrg - pulsarV2BBB).tiff |
English: PSR 0540-69 is a neutron star, or pulsar, that is rotating very rapidly, making a complete rotation every one-twentieth of a second. It is similar in many ways to the famous Crab Nebula pulsar. Both objects are spinning rapidly, are about 1,000 years old and are surrounded by a large cloud of gas and high-energy particles. The surrounding cloud in both cases is powered by the conversion of rotational energy of the neutron star into high energy particles through the combined action of rapid rotation and a strong magnetic field. PSR 0540-69 is 160,000 light years away in the Large Magellanic Cloud, one the Milky Way's small satellite galaxies. |
Date | 20 September 1999 (upload date) |
Source | Supernovas Portrait Gallery |
Author | NASA/SAO |
Other versions |
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Category InfoField | Supernovas & Supernova Remnants, Neutron Stars/X-ray Binaries |
Color Code InfoField | Intensity |
Constellation InfoField | Dorado |
Coordinates (J2000) InfoField | RA 05h 40m 11s |
Distance Estimate InfoField | 160,000 light years |
Scale InfoField | 2 arcmin across. |
Instruments InfoField | HRC |
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This media is a product of the Chandra X-ray Observatory Credit and attribution belongs to the Chandra X-ray Center, NASA/SAO |
Licensing
[edit]Public domainPublic domainfalsefalse |
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ![]() |
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current | 09:36, 28 May 2024 | ![]() | 2,100 × 1,736 (1.41 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://chandra.si.edu/photo/1999/snrg/pulsarV2BBB.tif via Commons:Spacemedia |
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Image title | PSR 0540-69 is a neutron star, or pulsar, that is rotating very rapidly, making a complete rotation every one-twentieth of a second. It is similar in many ways to the famous Crab Nebula pulsar. Both objects are spinning rapidly, are about 1,000 years old and are surrounded by a large cloud of gas and high-energy particles. The surrounding cloud in both cases is powered by the conversion of rotational energy of the neutron star into high energy particles through the combined action of rapid rotation and a strong magnetic field. PSR 0540-69 is 160,000 light years away in the Large Magellanic Cloud, one the Milky Way's small satellite galaxies. |
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Author | Chandra X-ray Observatory Center |
Width | 2,100 px |
Height | 1,736 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 | 41 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS4 Windows |
File change date and time | 10:03, 21 February 2013 |
Exif version | 2.21 |
Color space | sRGB |