File:RochePotential.jpg
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Original file (963 × 700 pixels, file size: 119 KB, MIME type: image/jpeg)
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Summary
| DescriptionRochePotential.jpg |
English: A three-dimensional representation of the Roche potential in a binary star with a mass ratio of 2, in the co-rotating frame. The droplet-shaped figures in the equipotential plot at the bottom of the figure are called the Roche lobes of each star. L1, L2 and L3 are the points of Lagrange where forces cancel out. Mass can flow through the saddle point L1 from one star to its companion, if the donor star fills its Roche lobe.
Esperanto: Tridimensia bildigo de la potencialo de Roche en dustela sistemo kies maskvocienco estas 2, en la kunturnema referenco. La guta formaro en la sampotenciala grafiko sube de la bildo nomiĝas la loboj de Roche de ambaŭ steloj. |
| Date | |
| Source | http://hemel.waarnemen.com/Informatie/Sterren/hoofdstuk6.html#h6.2 |
| Author | Marc van der Sluys |
| Other versions |
|
This graph image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with
{{vector version available|new image name}}.It is recommended to name the SVG file “RochePotential.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. |
This graph image was uploaded in the JPEG format even though it consists of non-photographic data. This information could be stored more efficiently or accurately in the PNG or SVG format. If possible, please upload a PNG or SVG version of this image without compression artifacts, derived from a non-JPEG source (or with existing artifacts removed). After doing so, please tag the JPEG version with {{Superseded|NewImage.ext}} and remove this tag. This tag should not be applied to photographs or scans. If this image is a diagram or other image suitable for vectorisation, please tag this image with {{Convert to SVG}} instead of {{BadJPEG}}. If not suitable for vectorisation, use {{Convert to PNG}}. For more information, see {{BadJPEG}}. |
Licensing
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| 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. | ||
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| 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 |
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2006
121,791 byte
700 pixel
963 pixel
image/jpeg
70b5368e7dd688e85d0b2379e081f0d1a1122bc0
File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 10:55, 23 May 2006 | 963 × 700 (119 KB) | wikimediacommons>Sluys | A three-dimensional representation of the Roche potential in a binary star with a mass ratio of 2, in the co-rotating frame. The droplet-shaped figures in the equipotential plot at the bottom of the figure are called the Roche lobes of each star. L1, L2 |
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