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         Solar System:     more books (106)
  1. Wonders (of the Planets: Visions of our solar system in the 21st Century) by Prinja, 2006
  2. The Solar System by Paul P. Sipiera, 1997-10
  3. The Pebble First Guide to the Solar System (Pebble First Guides) by Joanne Mattern, 2009-12
  4. Discover Science: Solar System by Dr. Mike Goldsmith, 2010-08-17
  5. Solarizing Your Present Home: Practical Solar Heating Systems You Can Build
  6. Determination of the Motion of the Solar System in Fixed Unalterable Space by Martin Gardiner, 2009-07-17
  7. Solar System Evolution: A New Perspective (Volume 0) by Stuart Ross Taylor, 2005-07-14
  8. Wind and Solar Power Systems: Design, Analysis, and Operation, Second Edition by Mukund R. Patel, 2005-07-15
  9. Explore the Solar System!: 25 Great Projects, Activities, Experiments (Explore Your World series) by Anita Yasuda, 2009-05-01
  10. Solar System (Extraordinary)
  11. Moon (Exploring the Solar System) by Giles Sparrow, 2002-02
  12. The Sun: Star of the Solar System (Our Solar System) by Lincoln James, 2010-08-15
  13. The Solar System: The Cosmic Perspective, Fourth Edition
  14. 3-D Thrillers! Solar System (Discovery Kids) by Marc Tyler Nobleman, 2001-06-04

81. Index Of /spacecraft_data/iras/solar_system/asteroid_and_comet_survey
Index of /spacecraft_data/iras/solar_system/asteroid_and_comet_survey. Parent Directory data/
http://128.183.114.83/spacecraft_data/iras/solar_system/asteroid_and_comet_surve
Index of /spacecraft_data/iras/solar_system/asteroid_and_comet_survey
Name Last modified Size Description ... data/ 03-Apr-2002 15:41

82. Solar System - Simple English Wikipedia, The Free Encyclopedia
This short article can be made longer. You can help Wikipedia by adding to it. Retrieved from http//simple.wikipedia.org/wiki/solar_system
http://simple.wikipedia.org/wiki/Solar_system
Solar system
From the Simple English Wikipedia, the free encyclopedia that anyone can change
Jump to: navigation search A to scale picture of the Solar System. Earth is number 3 A solar system is a phrase used in astronomy . It means a collection of planets comets and other objects moving around a star . The best known solar system is the one humans live in, the one Earth is in. The Earth moves around the Sun in an oval shaped, or "elliptical" orbit . The other planets in the solar system also move around the sun in elliptical orbits The biggest objects that go around the Sun are called planets . It took people many years of looking carefully through telescopes to find them. No new big ones have been found for a long time, but more small objects are found every year. Most of the planets have moons that orbit around them. There are 166 of these moons in the solar system.
Contents
change The order of planets
These are the 8 planets , 3 dwarf planets and other large objects moving around the Sun in order from closest to the sun to farthest away from the sun (numbers sign to the picture on the right):
change Structure
There are a few main parts of the Solar System. The terrestrial inner planets (

83. Glish Solar System Client
The immediate purposes for solar_system are to track the moon and planets with the The solar_system client program requires three data files in one
http://www.cv.nrao.edu/~rfisher/Glish/solar_system.html
Glish Client for Computing Positions of Planets, Pulsar Pulse Delays, LST, Precession, Nutation and Aberration
Table of Contents
Introduction
This document briefly desribes the events recognized by the glish "solar_system" client program. This client is based on the JPL solar system ephemerides and the StarLink 'slalib' function set. This client is probably a temporary one, which will be superseded by more elaborate functions in the AIPS++ Measures system. The immediate purposes for "solar_system" are to track the moon and planets with the GBT software and to provide a few functions of general utility such as precession/nutation, aberration, UTC to LST and LST to UTC conversion, doppler calculation, and pulsar pulse delay. The client events decribed in more detail below are Event Name Input Value Record object_track [object=, mjd=, utc=, num_pts=, interval=] object_doppler [object=, mjd=, utc=, num_pts=, interval=] doppler_fraction [ra=, dec=, mjd=, utc=, num_pts=, interval=] observer_position_velocity [mjd=, utc=, num_pts=, interval=] pulse_delay [ra=, dec=, mjd=, utc=, num_pts=, interval=] utc_to_tdb [mjd=, utc=] utc_to_last [mjd=, utc=] last_to_utc [mjd=, last=] j2000_to_epoch [ra=, dec=, mjd=, utc=] epoch_to_j2000 [ra=, dec=, mjd=, utc=] add_aberration [ra=, dec=, mjd=, utc=] remove_aberration [ra=, dec=, mjd=, utc=] set_observer_coord [x=, y=, z=] geocentric_observer_track [mjd=, utc=, num_pts=, interval=] barycentric_observer_track [mjd=, utc=, num_pts=, interval=] barycentric_earth_track [mjd=, utc=, num_pts=, interval=] barycentric_object_track [object=, mjd=, utc=, num_pts=, interval=]

84. The Colors Of The Moon
About This Photograph. Is the moon really this colorful? In a way, yes. The lunar surface actually does have quite a bit of color, although in reality it is
http://www.rc-astro.com/photo/id1018.html
Home Latest Popular Nebulae ... About
The Colors of the Moon
Interested in a print?
About This Photograph
Is the moon really this colorful? In a way, yes. The lunar surface actually does have quite a bit of color, although in reality it is very subtle. In this photograph, the color saturation has been enhanced to bring out the differences in the colors of the various areas of the surface. The hues are correct, just much more vivid than we usually see them. Aside from making an interesting aesthetic presentation, the colors also give clues as to the mineralogy of the moon's surface. Also, at the sites of many impact craters we can see that deeper material exposed (and in some cases scattered) by the impact is of a different composition than the material on the surface.
Technical Details
Optics: 20" f/8 RCOS Ritchey-Chrétien Cassegrain w/ Field Corrector. Mount: Software Bisque Paramount ME. Camera: SBIG STL-11000XM. Filters: SBIG Standard RGB. Dates/Times: 18 April 2005. Location: Dimension Point Observatory, Mayhill, New Mexico. Exposure Details: LRGB = 2:4:2:4 milliseconds, two-frame mosaic.

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