Greetings, Chuft-Captain and lidocorc,
Chuft,
For demonstration purposes, the only things your
ssc needed were a closing } (curly bracket) and the addition of a 180? Mean Longitude. The latter is because Earth and the Moon are on opposite sides of their barycenter. I've revised your
ssc file and attached it.
lidocorc,
All you need to do is unzip the
ssc file and copy it into CELESTIA 1.6.0's
extras folder. Then restart CELESTIA and you're ready to go.
After you've done the above, here are a few cel:url's you can run to see the effects immediately. The motion of Earth around the barycenter is evident even when we zoom out enough to see both Earth and Moon. Very cool indeed, Chuft!
Earth-Moon Barycenter Demo (Showing Earth and Moon from side)
cel://Follow/Sol:Earth-Moon/2010-03-05T00:35:15.85262?x=AClce8+jxRc&y=EOZVPdTdJf///////////w&z=gOlMxQjxU/L//////////w&ow=0.500664&ox=-0.00806286&oy=-0.865502&oz=0.0132773&select=Sol:Earth-Moon&fov=34.5394&ts=1e+006<d=0&p=0&rf=105875&lm=32772&tsrc=0&ver=3Earth-Moon Barycenter Demo (Showing Earth and Moon from above)
cel://Follow/Sol:Earth-Moon/2010-02-06T06:47:46.20984?x=gOkJcELQ7Qg&y=ADNYhQTMXR8&z=APTb2uAdM/T//////////w&ow=0.331475&ox=0.27136&oy=-0.772326&oz=-0.469043&select=Sol:Earth-Moon&fov=34.5394&ts=1e+006<d=0&p=0&rf=105875&lm=32772&tsrc=0&ver=3Earth-Moon Barycenter Demo (from side and closer to Earth)
cel://Follow/Sol:Earth-Moon/2010-06-08T09:09:49.17210?x=ABaOQMA8ARw&y=wJx8p6hlo/z//////////w&z=AIKJMHPK0ev//////////w&ow=0.453526&ox=0.00706285&oy=-0.889319&oz=0.058099&select=Sol:Earth-Moon&fov=1.52125&ts=500000<d=0&p=0&rf=105875&lm=32772&tsrc=0&ver=3A few considerations:
This particular
ssc should be used only for demonstration purposes because it simplifies the Moon's highly irregular orbit to a great degree. The Moon's perigee (average about 363,400 km) and apogee (average about 405,400 km) actually change quite a bit even over relatively short periods (several months), so the barycenter's depth below Earth's surface varies more than that rendered when using a strictly elliptical orbit. In addition, the plane and direction of the axes of the lunar orbit are constantly changing. The inclination of its average plane relative to the Ecliptic varies between about 4.95° and 5.33°, and the orbital axis rotates around the Earth once every 8.9 years. Moreover, the lunar orbit’s ecliptic line of nodes—the line connecting the points where the Moon’s orbit crosses the Ecliptic—rotates westward or backwards (regresses) once every 18.6 years!
Therefore, when you want CELESTIA to accurately show the Moon's position again, just rename the file to something like
EarthMoon rev 01.sscDEMO and restart CELESTIA. This keeps the file in your extras folder for future demonstration, but makes it unreadable by CELESTIA until you're ready to use it again.
But anytime you want to demonstrate the motions around the barycenter, just rename the file to
EarthMoon rev 01.ssc and restart CELESTIA.
This gives you the best of both worlds.
If you ever need to show the motions of the Earth-Moon barycenter with continuing accuracy over time, you can use the JPL Ephemerides.
http://en.wikibooks.org/wiki/Celestia/JPL_EphemeridesBut if you just need to demonstrate Earth's and the Moon's motions around the barycenter, CC's
ssc does a great job.
Enjoy!
Gary