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In celestial mechanics, the plane of reference is the plane used to define orbital elements (positions). The two main orbital elements that are measured with respect to the plane of reference are the inclination and the longitude of the ascending node. Depending on the type of body being described, there are four different kinds of reference planes that are typically used: *Ecliptic or invariable plane for planets, asteroids, comets, etc. within the solar system, as these bodies generally have orbits that lie close to the ecliptic. *Equator of the orbited body for satellites with small semi-major axes *Local Laplace plane for satellites with intermediate-to-large semi-major axes *Plane tangent to celestial sphere for extrasolar objects On the plane of reference, a zero-point must be defined from which the angles of longitude are measured. This is usually defined as the point on the celestial sphere where the plane crosses the prime hour circle (the hour circle occupied by the First Point of Aries), also known as the equinox. ==See also== * Fundamental plane * Plane (geometry) 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Plane of reference」の詳細全文を読む スポンサード リンク
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