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celestial sphere |
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celestial sphere, imaginary sphere of infinite radius with the earth at its center. It is used for describing the positions and motions of stars and other objects. For these purposes, any astronomical object can be thought of as being located at the point where the line of sight from the earth through the object intersects the surface of the celestial sphere. In astronomical coordinate systems astronomical coordinate systems. A coordinate system is a method of indicating positions. Each coordinate is a quantity measured from some starting point along some line or curve, called a coordinate axis. ..... Click the link for more information. , the coordinate axes are great circles on the celestial sphere. In most systems of this type, the reference points are fixed on the sphere, so the two coordinates needed to locate a body are relatively constant. celestial sphereApparent surface of the heavens, on which the stars seem to be fixed. For the purpose of establishing celestial coordinate systems to mark the positions of heavenly bodies, it can be thought of as a real sphere at an infinite distance from Earth. Earth's rotational axis, extended to infinity, touches this sphere at the northern and southern celestial poles, around which the heavens seem to turn. The intersection of the plane of Earth's Equator with the sphere marks the celestial equator. celestial sphere an imaginary sphere of infinitely large radius enclosing the universe so that all celestial bodies appear to be projected onto its surface How to thank TFD for its existence? Tell a friend about us, add a link to this page, add the site to iGoogle, or visit webmaster's page for free fun content. |
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Just as scientists had planned, the craft rose out of the equatorial plane and for the next 5 months viewed the rings from above and below the planet's equator. The only place you can keep a satellite stationary over the earth is if it is orbiting the earth on the equatorial plane. 2][psi] method" [17-18], based on the collection of diffraction data at various tilts of the specimen about the axis perpendicular to the scattering direction and lying in the equatorial plane ([psi] angle). |
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