Template:Infobox dwarf planet: Difference between revisions
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imported>Thorsten Alteholz (New page: {| class="infobox" style="font-size: 90%; width: 22em; text-align: left" |+ '''{{{name}}}''' |- ! colspan="2" cellspacing="0" cellpadding="2" style="background:#FFDEAD; text-align: center"...) |
imported>Thorsten Alteholz No edit summary |
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Revision as of 13:12, 21 October 2007
| Epoch: | {{{epoch}}} |
|---|---|
| M | {{{mano}}} |
| n: | {{{mmot}}} |
| a: | {{{maax}}} |
| e: | {{{ecc}}} |
| P: | {{{orbper}}} |
| Perihelion: | {{{peri2000}}} |
| Node: | {{{node2000}}} |
| Inclination: | {{{incl2000}}} |
| H: | {{{avmag}}} |
| G: | {{{slope}}}
|
| M | Mean anomaly at the epoch. |
| n | Mean daily motion (in degrees/day). |
| a | Semimajor axis (in AU). |
| z | Reciprocal semimajor axis (in 1/AU). |
| q | Perihelion distance (in AU). |
| e | Orbital eccentricity. |
| P | Orbital period (in years). |
| Perihelion | The J2000.0 argument of perihelion (in degrees). |
| Node | The J2000.0 longitude of the ascending node (in degrees). |
| Inclination | The J2000.0 inclination (in degrees). |
| H | Absolute visual magnitude. |
| G | Slope parameter. For an explanation of the H,G magnitude system refer to Application of Photometric Models to Asteroids, Bowell et al., in Asteroids II, 524-556 (published by the University of Arizona Press, ISBN 0-8165-1123-3) and the references therein. |