File:HR-sparse-Sirius e Sol.svg

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file (SVG file, nominally 700 × 830 pixels, file size: 178 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 File:HR-sparse.svg
Author User:Rursus
Other versions
  • Colored version with text
    Colored version with text
  • Without
    Without

[edit]

Hertzsprung–Russell diagram
  • Afrikaans
    Afrikaans
  • Afrikaans (alt)
    Afrikaans (alt)
  • català
    català
  • čeština
    čeština
  • English
    English
  • English (alt)
    English (alt)
  • español
    español
  • français
    français
  • galego
    galego
  • italiano
    italiano
  • magyar
    magyar
  • македонски
    македонски
  • oʻzbekcha
    oʻzbekcha
  • polski
    polski
  • slovenčina
    slovenčina
  • suomi (alt)
    suomi (alt)
  • svenska
    svenska
  • беларуская
    беларуская
  • қазақша
    қазақша
  • русский
    русский
  • հայերեն
    հայերեն
  • 日本語
    日本語
  • 中文（繁體）
    中文（繁體）
  • עברית
    עברית
  • עברית
    עברית
  • العربية
    العربية
Sun + Sirius sparse
  • català
    català
  • Deutsch (PNG)
    Deutsch (PNG)
  • Deutsch
    Deutsch
  • English (PNG)
    English (PNG)
  • English
    English
  • español
    español
  • galego
    galego
  • Lëtzebuergesch
    Lëtzebuergesch
  • македонски
    македонски
  • Türkçe
    Türkçe
Well-known stars in the Milky Way
  • Afrikaans
    Afrikaans
  • English
    English
  • English (alt)
    English (alt)
  • Kiswahili
    Kiswahili
  • Deutsch
    Deutsch
  • български
    български

Licensing

[edit]
GNU head 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.
w:en:Creative Commons
attribution share alike 		This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
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/TimeThumbnailDimensionsUserComment
current00:36, 28 January 2020Thumbnail for version as of 00:36, 28 January 2020700 × 830 (178 KB)Magog the Ogre (talk | contribs)fix order
16:12, 13 August 2014Thumbnail for version as of 16:12, 13 August 2014700 × 830 (178 KB)HombreDHojalata (talk | contribs)== {{int:filedesc}} == {{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 spen...
15:27, 13 August 2014Thumbnail for version as of 15:27, 13 August 2014700 × 830 (175 KB)HombreDHojalata (talk | contribs)retoques na posición dos textos
15:25, 13 August 2014Thumbnail for version as of 15:25, 13 August 2014700 × 830 (175 KB)HombreDHojalata (talk | contribs)axustando tamaño de texto
15:21, 13 August 2014Thumbnail for version as of 15:21, 13 August 2014700 × 830 (174 KB)HombreDHojalata (talk | contribs)== {{int:filedesc}} == {{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 spen...

You cannot overwrite this file.

File usage on other wikis

The following other wikis use this file:

  • Usage on gl.wikipedia.org

Metadata

This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.

Retrieved from "https://commons.wikimedia.org/w/index.php?title=File:HR-sparse-Sirius_e_Sol.svg&oldid=796569584"