See also:
Most of the corrections detailed for version 1.2.5 are therefore not required and potentially in error when applied to 1.3.0. Below are some additions specific to 1.3.0 - do not use them with earlier versions.
Archive: saturnmoons-130.zip
Length Date Time Name
-------- ---- ---- ----
125599 02-04-03 02:42 models/epimetheus.3ds
125599 02-04-03 02:34 models/janus.3ds
125599 02-03-03 19:53 models/prometheus.3ds
0 04-15-03 19:12 models/
0 04-15-03 19:22 textures/lores/
3216 04-15-03 19:22 textures/lores/epimetheus.jpg
3985 04-15-03 19:22 textures/lores/janus.jpg
3271 04-15-03 19:22 textures/lores/prometheus.jpg
0 04-15-03 19:20 textures/medres/
13676 04-15-03 19:20 textures/medres/epimetheus.jpg
16569 04-15-03 19:18 textures/medres/janus.jpg
12876 04-15-03 19:19 textures/medres/prometheus.jpg
0 04-15-03 19:20 textures/
2630 04-15-03 20:11 SaturnMoons-readme.txt
-------- -------
433020 14 files
\extras directory.
It provides shape models and textures for three inner moons of Saturn,
adapted from public domain data and images provided by Phil Stooke
at his Cartography of Non-spherical Worlds website
http://publish.uwo.ca/~pjstooke/plancart.htm
and his Small World Atlas website
http://www.ssc.uwo.ca/geography/spacemap/contents.htm
I generated the 3ds mesh objects and modified and applied the texture
maps. Smoothing of the resulting objects was done by "Praesepe".
All of these satellites depart markedly from simple elliptical orbits -
Janus and Epimetheus interact strongly with each other during close
approaches, as do Prometheus and the satellite Pandora. The orbits
provided in Celestia's minormoons.ssc are correct for January 2000, but
will be significantly in error at other dates. However, all these moons
are in synchronous rotation with their orbital periods, so it adds
realism if the shape models are rotated to align their prime meridians
with Saturn.
To display them optimally in Celestia you should edit the texture and
mesh definitions, and also add the necessary RotationOffsets to
minormoons.ssc, as noted in CAPITAL LETTERS in the text that follows:
However, if you have not previously edited minormoons.ssc, and therefore
have no changes you wish to preserve, you may prefer to simply copy the
following version on top of the original file in the \extras folder - this
will automatically make all necessary changes.
"Prometheus" "Sol/Saturn"
{
Texture "prometheus.jpg" # CHANGE THIS LINE
Mesh "prometheus.3ds" # CHANGE THIS LINE
Radius 50.1
EllipticalOrbit
{
Period 0.612986
SemiMajorAxis 139350
Eccentricity 0.0023
Inclination 0.000
LongOfPericenter 32.879 # J2000.0
MeanAnomaly 22.695 #
}
RotationOffset 55.6 # ADD THIS LINE
Albedo 0.6
}
# ...Pandora is here in original file
"Epimetheus" "Sol/Saturn"
{
Texture "epimetheus.jpg" # CHANGE THIS LINE
Mesh "epimetheus.3ds" # CHANGE THIS LINE
Radius 59.5
EllipticalOrbit
{
Period 0.694590
SemiMajorAxis 151422
Eccentricity 0.0205
Inclination 0.337 #
AscendingNode 149.880 #
ArgOfPericenter 86.905 # J2000.0
MeanAnomaly 192.354 #
}
RotationOffset 69.1 # ADD THIS LINE
Albedo 0.5
}
"Janus" "Sol/Saturn"
{
Texture "janus.jpg" # CHANGE THIS LINE
Mesh "janus.3ds" # CHANGE THIS LINE
Radius 88.8
EllipticalOrbit
{
Period 0.694590
SemiMajorAxis 151472
Eccentricity 0.0073
Inclination 0.168 #
AscendingNode 120.557 #
ArgOfPericenter 43.066 # J2000.0
MeanAnomaly 79.973 #
}
RotationOffset 243.6 # ADD THIS LINE
Albedo 0.6
}
This Web page is maintained by Selden Ball
at Wilson Lab.
Please send any comments or corrections to
seb@lepp.cornell.edu