File:Sn2006gy light curve.jpg
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DescriptionSn2006gy light curve.jpg |
English: Original caption: "This graph shows the intrinsic brightness of SN 2006gy and how it changes over time. The graphic also demonstrates how much brighter SN 2006gy is when compared to typical examples of the two main supernova classes. Type Ia supernovas involve the thermonuclear explosion of a white dwarf and type II supernovas are the collapse of a massive star. The famous supernova SN 1987A is also shown. Not only does SN 2006gy get much brighter than other supernovas but it stays very bright for much longer." Français : « Ce graphique montre la brillance intrinsèque de SN 2006gy et comment celle-ci change dans le temps (...) » |
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Author | NASA/CXC/UC Berkeley/N.Smith et al. | ||
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Images credited first to NASA/CXC are in the public domain.
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Public domainPublic domainfalsefalse |
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 | 23:20, 9 May 2007 | 3,000 × 2,025 (421 KB) | Tom (talk | contribs) | {{Information |Description=Original caption: "This graph shows the intrinsic brightness of SN 2006gy and how it changes over time. The graphic also demonstrates how much brighter SN 2006gy is when compared to typical examples of the two main supernova |
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Width | 3,000 px |
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Height | 2,025 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS2 Windows |
File change date and time | 19:17, 9 May 2007 |
Color space | Uncalibrated |
Image width | 3,000 px |
Image height | 2,025 px |
Date and time of digitizing | 15:17, 9 May 2007 |
Date metadata was last modified | 15:17, 9 May 2007 |
IIM version | 2 |