chris wrote:I need to add support for splash images to the Windows version. I may have time for that tonight (though working on extended star systems is much more fun . . .
)
--Chris
Aha! What about a "random splash selector feature"
picking images from some pool directory, such that the users can enjoy some real surprise each time Celestia starts up...
Bye Fridger
PS:
I am enjoying the new "binary orbit" developments very much...
If there is demand, I could easily hack another Perl script to generate at once
thousands of binary orbits in the adequate Celestia input format from the
official double star catalogs. As you know, Perl can calculate very well and accurately. It's easy to make the script decide on the fly what parameters to use to derive the orbits in each case...
Yet, after finishing up with a most exciting international conference on
Particle Cosmology last weekend at my laboratory [DESY] (organized in part by my theoretical physics department),
http://www.desy.de/desy-th/workshop2004/index.html
I am increasingly sad that the "cosmology mode" idea of Celestia does seem to stagnate entirely.
Incidentally:
For people interested in some of the excellent talks, just click on "Transparencies" for downloading the plenary talks. They are typically in PDF format, so Acrobat Reader will be fine.
In the light of the cosmic neutrino discussion we are having in the Physics and Astronomy department, looking into the talks by C. Spiering and (famous) G.Sigl would certainly be worthwhile...
Also the introductory lecture by Ruth Durrer, about the status of extracting the basic cosmological parameters from the WMAP data is excellent! In her talk as well as in the talk on "Large Scale Structure and Sloan Digital Sky Survey" by J. Friemann, it becomes dramatically obvious how crucially the merging of the information
from Sloan about the mass power spectrum with the WMAP results for the cosmic microwave background, eliminates remaining ambiguities about the cosmologigal parameters and inflation.
Bye Fridger