File:Sn2006gy light curve.jpg

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Description

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 (...) »

Date

Unknown date

Source

More Images of SN 2006gy. Harvard-Smithsonian Center for Astrophysics (2007-05-07).
- NASA/CXC/UC Berkeley/N.Smith et al.. Light Curve of SN 2006gy. Harvard-Smithsonian Center for Astrophysics.

Author

NASA/CXC/UC Berkeley/N.Smith et al.

Permission
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	Warnings: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

File history

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	23:20, 9 May 2007		3,000 × 2,025 (421 KB)	Tom	{{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

File usage

The following page uses this file:

SN 2006gy

Global file usage

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Usage on ar.wikipedia.org
- مستعر أعظم
- منحنى ضوئي
Usage on be.wikipedia.org
- Сусвет
Usage on bs.wikipedia.org
- SN 2006gy
Usage on ca.wikipedia.org
- SN 2006gy
Usage on de.wikipedia.org
Usage on en.wikiversity.org
- Stars/Supernovas
Usage on es.wikipedia.org
- SN 2006gy
Usage on eu.wikipedia.org
- Supernoba
Usage on fr.wikipedia.org
- SN 2006gy
- Supernova par production de paires
Usage on it.wikipedia.org
- SN 2006gy
Usage on ja.wikipedia.org
- SN 2006gy
Usage on ko.wikipedia.org
- SN 2006gy
Usage on nl.wikipedia.org
- SN 2006gy
Usage on ru.wikipedia.org
- Вселенная
- Шкала расстояний в астрономии
Usage on uk.wikipedia.org
- Наднова, що вибухає внаслідок нестабільності народження електрон-позитронних пар
- SN 2006gy
Usage on zh.wikipedia.org
- SN 2006gy

Metadata

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Width	3,000 px
Height	2,025 px
Bits per component	8 8 8
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

File:Sn2006gy light curve.jpg

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public domain

Wikimedia VRTS ticket number

2007050910013359

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