File:HR-sparse-de.svg
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
Size of this PNG preview of this SVG file: 506 × 600 pixels. Other resolutions: 202 × 240 pixels | 405 × 480 pixels | 648 × 768 pixels | 864 × 1,024 pixels | 1,727 × 2,048 pixels | 700 × 830 pixels.
Original file (SVG file, nominally 700 × 830 pixels, file size: 151 KB)
File information
Structured data
Captions
Summary
[edit]DescriptionHR-sparse-de.svg | This is an example of a Hertzsprung-Russell diagram; a plot of luminosity versus spectral class for a group of stars. The diagonal band labelled "main sequence" is where dwarf stars such as the Sun spend most of their active lifespan. Red giants and supergiants are evolved stars with a mass greater than a red dwarf, that are burning elements heavier than hydrogen. However, White Dwarfs are quite dense, non-luminous, but are still less in mass than supergiants. Once this supply of fuel is exhausted, these stars will migrate to the lower left on this diagram, becoming white dwarfs. |
Date | |
Source | derived from Image:HR-sparse.svg by User:Rursus. Text translated to German, some cosmetics applied, position of Sun corrected (spectral class G, not K) |
Author | User:Sch |
Other versions |
[edit]
|
Licensing
[edit]Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | ||
| ||
This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:38, 6 March 2008 | 700 × 830 (151 KB) | Sch (talk | contribs) | {{Information |Description=This is an example of a Hertzsprung-Russell diagram; a plot of luminosity versus spectral class for a group of stars. The diagonal band labelled "main sequence" is where dwarf stars such as the Sun spend most of their active lif |
You cannot overwrite this file.
File usage on Commons
The following 41 pages use this file:
- File:Diagram H-R2 PL.gif
- File:Diagrama H-R - Sirio y Sol.png
- File:ESO - Hertzsprung-Russell Diagram (by).jpg
- File:H-R diagram -edited-3-uz.png
- File:H-R diagram -edited-3-zh-hant.png
- File:H-R diagram -edited-3.gif
- File:H-R diagram -edited-3 (cs).png
- File:H-R diagram -edited-3 sv.gif
- File:H-R diagram afr.GIF
- File:H-R diagrama.png
- File:H-R diagrammi -edited-3 fin.png
- File:HR-sparse-Sirius e Sol.svg
- File:HR-sparse-de.svg
- File:HR-sparse-lb.svg
- File:HR-sparse.svg
- File:HR-sparse mk.svg
- File:HRD Sonne Sirius.png
- File:HRD Sonne Sirius ca.svg
- File:HRDiagram-Fr.png
- File:HRDiagram-ca.png
- File:HRDiagram-es.png
- File:HRDiagram-he-.gif
- File:HRDiagram-he-solaranalog.gif
- File:HRDiagram.png
- File:HRDiagram.sk.gif
- File:HRDiagram InsStrip-HU.gif
- File:HRDiagram af.png
- File:HRDiagram be.png
- File:HRDiagram in italian.gif
- File:HRDiagram mk.png
- File:HRDiagram ru.png
- File:HR図.png
- File:Hertsprung-Russell.jpg
- File:Hertzsprung-Russel StarData af.jpg
- File:Hertzsprung-Russel StarData de.jpg
- File:Hertzsprung-russel cizenegi.png
- File:Hertzsprung-russel diagram.png
- File:Mng'aro na joto.png
- File:RasmHersel.png
- File:Герцшпрунг-Рассел диаграммасы.png
- Template:Other versions/Hertzsprung-Russel
File usage on other wikis
The following other wikis use this file:
- Usage on de.wikipedia.org
- Usage on gl.wikipedia.org