			      THE ORRERY
			    Version 0.9.4

[ Version 0.9.5 is just an update to make sure that the Orrery still    ]
[ builds with Geomview >= V1.9.2.                                       ]
[                                                                       ]
[ cH Sat Jun 9 2007
[                                                                       ]
[ Version 0.9.4 is just an update to make sure that the Orrery still    ]
[ builds with Geomview >= V1.9.0.                                       ]
[                                                                       ]
[ cH Tue Apr 24 2007
[                                                                       ]
[ Note: This release of the Orrery, version 0.9.3, is the same as       ]
[ version 0.9.2 with the exception that I've changed some of the        ]
[ settings in the Makefiles and the configure script in order to allow  ]
[ this version to be configured and built outside the Geomview source   ]
[ tree.  I did this in order to facilitate creating source and binary   ]
[ RPMs for Orrery.                                                      ]
[                                                                       ]
[ mbp Thu Feb 21 16:30:00 2002                                          ]
[                                                                       ]
[ Release 0.9.2 of the Orrery was essentially the same as the original  ]
[ one that Stuart Levy released in 1997.  The only difference is in the ]
[ organization of the files --- this copy is modified to work with the  ]
[ new Geomview source tree and Makefile system.                         ]
[                                                                       ]
[ mbp Sun Mar 18 19:05:46 2001                                          ]

The Orrery is a digital model of the solar system, named for the mechanical
models of the same name (often you'll see one with just the Sun, Earth
and Moon, as little balls supported on wires); the first such was built
for the fourth Earl of Orrery in the 1700's.

It includes all nine planets, some of their satellites, and a few recent
comets.

If you have questions, problems, or comments relating to this software
(which probably deserves to be called a beta release), please write to us at:

   software@geomview.org


INSTALLATION

For installation instructions, see the file `INSTALL.Orrery'. The file
`INSTALL' contains generic installation instructions.

The .geomview-orrery file(s) mention "wish", the tcl/tk interpreter;
they assume it's on your UNIX search path.  You may want to change
this for a couple of reasons:

  - if you have a version 8.0 wish installed somewhere,
	and it's different from "wish", use that.  The pre-interpretation
	in tcl/tk 8.0 speeds up the orrery's calculations quite a bit.
  - if you don't have "wish" installed, but you do have one of the
	geomview 1.6.1 releases, you can use its built-in wish.
	Change "wish" to "emodule-wish.sh".

  In either case, you can just edit any of the
    modules/*/.geomview-orrery
  files; they're all linked together, so changing any of them changes all.

WHAT'S INCLUDED?

  You can invoke the orrery itself with

    geomview -start orrery

  or by picking "Orrery" from geomview's list of modules.
  See the "Help" button for explanations and suggestions on use.

  You'll also find some command-line-based tools in src/bin/orrery.
  Invoked with no parameters, each gives a brief usage message describing
  how to use it.

    peri2elem
	Add new comets.  Convert cometary orbital elements,
	with specified eccentricity, perihelion distance and date,
	into something which could be added to our orbital-elements file,
	data/modules/orrery/orrery.elements.

    stargv
	Make your own star field.  Read yale.star-format file,
	extracting stars brighter than a specified limit, and writing
	Geomview-readable file suitable to be placed in
	data/modules/orrery/stars-to-mag-N.oogl.
	If you have the SAO database in ".star"-format too (not included here),
	you can generate star charts down to mag 9 or so.

    mktxmesh
	Generate a spherical MESH object, with texture coordinates specified
	for one of several kinds of map projections.

  Also, there's some reusable tcl code in the data/modules/orrery
  directory:

    data/modules/orrery/vectext.tcl
	Vector text generator.  Contains a built-in Hershey font.

    data/modules/orrery/browser.tcl
	A simple file browser.



DEPENDENCIES

You'll need at least some variant of geomview 1.6, as some of
the bodies include texture maps, which geomview 1.5 couldn't parse.
Even in geomview 1.6.1, the plain-X renderer accepts but ignores texture
mapping.  Most of the geomview 1.6.1 binary distributions also include an
Open GL version, built using the Open-GL-like Mesa libraries.
You can see textured images with
  geomview -opengl -start orrery

Note that texture mapping is still off by default; see the Display... panel.


LIMITATIONS

The Orrery is very simple numerically; it just uses fixed Keplerian
orbital elements for each body.  Though there's no closed form for
position as a function of time on such an orbit, there *is* a closed form
for time as a function of position; it uses Newton's method to find the
inverse function for each body at each time step.
The orbital elements are, I suspect, osculating elements as of 1996.0,
though I'm not sure; they're expressed in epoch-2000 coordinates.
The only exception to this is the moon; see Credits below.

Accuracy seems moderately good; within a few years of the present,
positions (RA, Dec) among the inner planets seem within a minute of arc
or so of values from Elwood Downey's "ephem" program.
Cometary positions seem similarly accurate.  The outer planets (>= Jupiter)
are much worse -- off by several minutes of arc.  I don't know why.
Lunar positions are good enough to detect eclipses, but not to predict them;
the moon's longitude often seems to be off by an hour or two of lunar motion.

Accuracy gets much worse at times far from the present; positions centuries
from now disagree with "ephem" by a few degrees.


CREDITS

This Orrery module was written, originally as a demonstration of Geomview
texture mapping, by Stuart Levy (slevy@ncsa.uiuc.edu) at the Geometry Center,
University of Minnesota and is copyright (c) 1997, University of Minnesota.
It is free software, available under the terms of the GNU Public License;
see the file COPYING for details.

The formulae for calculating the Moon's position were adapted from Elwood
Downey's "ephem" program, <URL:ftp://iraf.noao.edu/contrib/xephem/ephem>;
he in turn translated them from Peter Duffet-Smith's book "Astronomy with
Your Personal Computer", Cambridge University Press, 1985.
I've omitted many small-amplitude terms, so this lunar ephemeris is less
accurate than theirs.

For all other bodies, planetary orbital elements and physical data
(pole direction, etc.) in data/modules/orrery/orrery.elements
were taken from JPL's program "quick"; I think they amount to osculating
elements as of 1996.0, in coordinate system 2000.0.  Orbital elements
are widely available, though I'm not sure where you can find physical
data in a convenient, publicly available place; maybe the US Govt.
Printing Office publication Astronomical Almanac?  (Some comets were added
by hand.  Note that the Orrery module deals only with elliptical orbits, e<1.)

The stars were taken from the Yale Bright Star Catalogue.  The version
used was the "yale.star" reduced file included as part of the
useful "starchart" package:
  <URL:ftp://ftp.uu.net/usenet/comp.sources.unix/volume12/starcharts/>
  <URL:ftp://ftp.uu.net/usenet/comp.sources.unix/volume13/starchart/>
That file is also included here, as src/bin/orrery/yale.tar.gz.



Most of the images included here in the data/modules/orrery directory,
used for texturing the surfaces of the planets, are copyrighted,
but may be used under fairly liberal conditions, naturally including proper
credit to their sources.  So, here are the credits for these fine images,
with the place from which each was retrieved.

The images weren't retrieved in precisely the form given here; often they
were JPEG or sometimes GIF images of some arbitrary size, which I've
scaled and converted into these power-of-two-sized .ppm.{Z,gz} files.

The images came from three sources:
 - NASA's Planetary Data System (PDS, <URL:http://www-pdsimage.wr.usgs.gov>)
 - the Clementine Lunar Image Browser (image of Earth's Moon);
 - the Geometry Center using public-domain CIA outline data for the Earth.

 * jupiter.ppm.gz  PDS image PIA00011, "Cylindrical Projection of Jupiter"
  Available (image and more details on its origin) from
   <URL:http://www-pdsimage.wr.usgs.gov/cgi-bin/PIAGenCatalogPage.pl?PIA0011>
  Produced by
   JPL, <URL:http://www.jpl.nasa.gov>
  Caption mentions
    ``... made from 10 color images of Jupiter taken Feb. 1, 1979, by
	Voyager 1, during a single 10-hour rotation of the planet. ...''

 * mars+90.ppm.gz  PDS image PIA00193, "Latitude 90 Degrees North to
		90 Degrees South and Longitude 0 degrees to 180 degrees"
 * mars+270.ppm.gz PDS image PIA00194, "Latitude 90 Degrees North to
		90 Degrees South and Longitude -180 Degrees to 0 Degrees"
  Available (image and more on its origin) from
   <URL:http://www-pdsimage.wr.usgs.gov/cgi-bin/PIAGenCatalogPage.pl?PIA00193>
   <URL:http://www-pdsimage.wr.usgs.gov/cgi-bin/PIAGenCatalogPage.pl?PIA00194>
  Produced by
   USGS Flagstaff, <URL:http://wwwflag.wr.usgs.gov>
   from Viking orbiter 1 data
  Captions mention
	... Lambert azimuthal equal area projection ...


 * venus.pgm.gz was assembled from two cylindrical-projection PDS images:

		PIA00255 (Western hemisphere: left 240E, right 67.5E)
		PIA00256 (Eastern hemisphere; left edge 52.5E, right 240E)
  Available (image and more on its origin) from
   <URL:http://www-pdsimage.wr.usgs.gov/cgi-bin/PIAGenCatalogPage.pl?PIA00255>
   <URL:http://www-pdsimage.wr.usgs.gov/cgi-bin/PIAGenCatalogPage.pl?PIA00256>
  Produced by
   Solar System Visualization Project and Magellan science team
   at JPL Multimission Image Processing Laboratory, from
   Magellan synthetic-aperture radar mosaics.

There's one non-PDS image, the index map for the Clementine Lunar Image
Browser, <URL:http://www.nrl.navy.mil/clementine/clib>.

 * moon.pgm.gz  Clementine image
    Available from
     <URL:http://www.nrl.navy.mil/clementine/clib>

    This appears to be the same image as the USGS global albedo map,
    <URL:http://wwwflag.wr.usgs.gov/USGSFlag/Space/clementine/images/albedo.simp750.jpeg>
    Like other items on the wwwflag.wr.usgs.gov web page, it's in
    the public domain.  It was:

    Produced by
      USGS Flagstaff, assembled into global albedo map, from Clementine data
    Caption includes
      About 50,000 Clementine images have been processed and mosaicked to
      produce a global map of the Moon's albedo (normalized brightness or
      reflectivity) at a wavelength of 750 nm (just longward of visible red).


 * earth.ppm.Z
    I (slevy@ncsa.uiuc.edu) produced this Earth image using the public-domain
    CIA World Bank II outline database, with a program derived from one
    written by Joe Dellinger of Stanford.  The adapted program, with data,
    is available from <URL:ftp://geom.umn.edu/priv/slevy/worldmap.tar.gz>.
    Basically it wrote a collection of Postscript outlines for a
    rectangular projection of the earth; these were converted to an image,
    then manually patched up and flood-filled using ImageMagick.

Here's the copyright statement for the PDS images, as obtained from
<URL:http://www.jpl.nasa.gov/archive/copyright.html>, 10/31/1996.

   Image Copyright Information

   NASA generally has no objection to the reproduction and use of such
   NASA materials (audio transmissions and recordings; video transmission
   or recordings; or still or motion picture photography), subject to the
   following conditions:

     * NASA material may not be used to state or imply the endorsement by
       NASA or by any NASA employee of a commercial product, service or
       activity, or used in any manner that might mislead.
     * NASA should be acknowledged as the source of the material.
     * It is unlawful to falsely claim copyright or other rights in NASA
       material.
     * NASA shall in no way be liable for any costs, expenses or demands
       arising out of the use of NASA material by a recipient or a
       recipient's distributees.
     * NASA does not indemnify nor hold harmless users of NASA material,
       nor release such users from copyright infringement, nor grant
       exclusive use rights with respect to NASA material.
     * NASA material is not protected by copyright unless noted. If
       copyrighted, permission should be obtained from the copyright
       owner prior to use. If not copyrighted, NASA material may be
       reproduced and distributed without further permission from NASA.
     * If a recognizable person, or talent (e.g., a noted personality
       engaged to narrate a film) appears in NASA material, use for
       commercial purposes of that person's or talent's name, photograph
       likeness, voice, or biographical material may infringe a right of
       privacy or publicity. Therefore, permission should be obtained
       from the recognizable person or talent.
     * Some NASA material may incorporate music or footage which is
       copyrighted and licensed for the particular NASA work. Any editing
       or otherwise altering of the work may not be covered under the
       original license, and therefore would require permission of the
       copyright owner.

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