File:Comparison of Eccentricity.gif: Revision history

11 March 2022

• curprev 19:5119:51, 11 March 2022‎ Maintenance script talk contribs‎ 28 bytes +28‎ == Summary == Importing file Tag: Server-side upload

17 February 2011

• curprev 18:2518:25, 17 February 2011‎ imported>Dan Nessett‎ 1,921 bytes 0‎ uploaded a new version of "Image:Comparison of Eccentricity.gif": Reverted to version as of 10:24, 24 March 2010
• curprev 18:1418:14, 17 February 2011‎ imported>Dan Nessett‎ 1,921 bytes 0‎ uploaded a new version of "Image:Comparison of Eccentricity.gif": {{Image_Details |description = Animated Gif |author = |copyright = |source = |date-created = |pub-country = |notes = |versions = }}

6 April 2010

• curprev 12:0312:03, 6 April 2010‎ imported>Dan Nessett‎ 1,921 bytes +145‎ →‎Summary

24 March 2010

• curprev 05:2405:24, 24 March 2010‎ imported>Thomas Wright Sulcer‎ 1,776 bytes +1,776‎ {{Image_Details |description = Two orbits with otherwise identical Orbital elements differ in eccentricity |author = Garry R. Osgood |copyright = Garry R. Osgood |source = Wikimedia Commons |date-created = 31 August 2007 |pub-country = Unknown |notes = Two orbiting bodies have orbital elements that differ only in eccentricity. They are each independent two-body systems overlaid for purposes of illustration, and do not illustrate a three body system. The orbital period,...