egasimus wrote:Well, I'm quite familiar with programming.
What I'm thinking of making is creating an entirely new universe which contains only the galaxies of the Local Group, maybe with some fancier models than the ones currently present, and the ability to travel from galaxy to galaxy, and also to observe all galaxies from a distant point of view. Which always looks at the selected galaxy, putting it in the centre of the screen, and can rotate around it. Also, maybe a circle representing the supergalactic plane, and lines straight up and straight down to galaxies to represent their Y coordinate... something roughly like this, but more realistic:
![Image](http://rst.gsfc.nasa.gov/Sect20/localgrpA.jpg)
Is that sort of thing possible?
Yes, that's easily possible.
My galaxies.dsc (= deepsky.dsc) database within the Celestia distribution contains
ALL known galaxies of the local group (including dwarfs in a Volume <~ (10 Mpc)^3) (Note the name of the galaxy data file changed after Celestia version 1.5.x). The citation of the many scientific catalogs used, you find in the "boiler plate" of my galaxy data file in the Celestia 1.6 distribution @SVN:
galaxies.dsc wrote:# Revised NGC and IC Catalog, Wolfgang Steinicke, January 6, 2006
#
http://www.ngcic.org/steinicke/default.htm#
# Augmented by galaxies from Local Group volume (V <~ (10 Mpc)^3)
# Catalog of Neighboring Galaxies (Karachentsev+, 2004)
#
http://cdsweb.u-strasbg.fr/viz-bin/Cat?J/AJ/127/2031#
# Augmented by averages of distance entries from
# NED-1D: NASA/IPAC Extragalactic Database of Distances
#
http://nedwww.ipac.caltech.edu/level5/NED1D/#
# Augmented by
# NASA/IPAC Extragalactic Database (NED, batch)
#
http://nedwww.ipac.caltech.edu/#
# Augmented by
# Revised 3rd Reference Catalog of Bright Galaxies (RC3,VII/155)
#
http://cdsweb.u-strasbg.fr/viz-bin/Cat?VII/155#
# Augmented by
# Mark III Catalog of Galaxy Peculiar Velocities (Willick+ 1997,VII/198)
#
http://cdsweb.u-strasbg.fr/viz-bin/Cat?VII/198#sRM2.18#
# Augmented by distances from
# The SBF Survey of Galaxy Distances. IV.
# SBF Magnitudes, Colors, and Distances,
# J.L. Tonry et al., Astrophys J 546, 681 (2001)
#
# Augmented by distances from
# Compilation of "200 Brightest Galaxies"
#
http://www.anzwers.org/free/universe/galax200.html#
# Augmented by redshifts-> distances from
# VII/193 The CfA Redshift Catalogue, Version June 1995 (Huchra+ 1995)
#
http://cdsweb.u-strasbg.fr/viz-bin/Cat?VII/193#
# Using today's Hubble constant = 73.2 [km/sec/Mpc]
# (WMAP 2007, 3 years running, legacy archive)
#
# Abreviations for various distance methods used:
# SBF= SBF (Surface Brightness Fluctuations), T-F= Tully-Fischer
# V_cmb = rad. velocity in CMB frame & Hubble law
# cep=Cepheids, P=photometric, N(G)=planetary nebula (globular cluster) luminosity function
#
# Adapted for Celestia with Perl script: deepsky.pl Revision: 1.50
# Processed 2007-5-18 5 137 0 18:10:24 UTC
#
# by Dr. Fridger Schrempp,
fridger.schrempp@desy.de# ------------------------------------------------------
The commented Perl script of > 1200 lines that I wrote for generating the database, you find in the Celestia sources (-> src/tools/galaxies).
There is the option of including custom templates for individual galaxies. The rest I would do with a simple celx script.
Yet, I am sceptical about your sentence " ...maybe with some fancier models than the ones currently present", since the present galaxies are more "fancy" than they might look on first sight
![Wink ;-)](./images/smilies/icon_wink.gif)
. Take for instance the MilkyWay itself: In the following screenshots, you see how well its arms are mapped out by the known locations of the pulsars (yellow & red squares):
Have a click for kingsize (important!)!
![Image](http://www.shatters.net/~t00fri/images/MW-topview-small.jpg)
The green cross marks the sun's position in Orion's arm of the MW. The line from there to the center of the MW corresponds to
zero galactic longitude.
The sideways views also confirm the thickness profile of our MilkyWay from the scatter of the pulsar locations! The yellow crosses mark the precise location of the galactic plane whence the perfect alignment of the Celestia MilkyWay becomes obvious...
Have a click for kingsize (important!)!
![Image](http://www.shatters.net/~t00fri/images/MW-sideways-small.jpg)
The second image shows sideways views of the alignment quality where the top and bottom images differ by a 90 degree rotation within the galactic plane. Look for the sun's position...
Finally, it takes some practice to achieve the correct display settings for galaxies (in terms of zoom factor and observer distance from a galaxy) ... See e.g.
viewtopic.php?f=2&t=13348Fridger