File:Stellarparallax2 fr.svg
Size of this PNG preview of this SVG file: 382 × 598 pixels. Other resolutions: 153 × 240 pixels | 306 × 480 pixels | 490 × 768 pixels | 653 × 1,024 pixels | 1,307 × 2,048 pixels | 480 × 752 pixels.
Original file (SVG file, nominally 480 × 752 pixels, file size: 16 KB)
File information
Structured data
Captions
Summary edit
DescriptionStellarparallax2 fr.svg |
This image is a French and vector version of Image:Stellarparallax2.png English: Stellar Parallax diagram
The apparent motion of a near by star is a small ellipse in the sky relative to background stars over the period of a year. The angle representing major axis radius of the elliptical path is the parallax angle. The minor axis radius angle is simply related to the direction of the star relative to the earth's orbital axis. Stars near the north and south poles will make perfect circles, while stars near the ecliptic will make flat ellipses. |
Date | 30 May 2006 (original upload date) |
Source | Originally from en.wikipedia; description page is/was here. |
Author | Booyabazooka at English Wikipedia |
Other versions |
|
Licensing edit
Public domainPublic domainfalsefalse |
I, the copyright holder of this work, release this work into the public domain. This applies worldwide. In some countries this may not be legally possible; if so: I grant anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law. |
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 05:10, 9 October 2007 | 480 × 752 (16 KB) | Ianare (talk | contribs) | |Description=:''This image is a vector version of en::Image:Stellarparallax2.png'' {{en|Stellar Parallax diagram The apparent motion of a near by star is a small ellipse in the sky relative to background stars over the period of a year. The angle r |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.