File:HR-sparse.svg
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: 177 KB)
Captions
Captions
Add a one-line explanation of what this file represents
Summary
edit| 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 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 | (UTC) |
| Source | Image:Hertzsprung-russel diagram.png |
| Author | User:Rursus |
| Other versions |
[]
|
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. |
  
|
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. |
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 19:38, 24 June 2009 | | 700 × 830 (177 KB) | Rursus (talk | contribs) | Change sun position to something more realistical: c:a G2 |
| 19:58, 30 April 2007 |  | 700 × 830 (168 KB) | Rursus (talk | contribs) | {{Information |Description= |Source= |Date= |Author= }} | |
| 19:52, 30 April 2007 |  | 700 × 830 (168 KB) | Rursus (talk | contribs) | {{Information |Description= |Source= |Date= |Author= }} | |
| 19:45, 30 April 2007 |  | 700 × 830 (165 KB) | Rursus (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 45 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-diag-instability-strip.svg
- File:HR-diag-no-text-2.svg
- File:HR-diag-no-text.svg
- File:HR-diag-w-text.svg
- 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 en.wikipedia.org
- Usage on tr.wikipedia.org
