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The astronomical system of units, formally called the IAU (1976) System of Astronomical Constants, is a system of measurement developed for use in astronomy. It was adopted by the International Astronomical Union (IAU) in 1976,〔Resolution No. 10 of the (XVIth General Assembly of the International Astronomical Union ), Grenoble, 1976.〕 and has been significantly updated in 1994 and 2009 (see astronomical constant). The system was developed because of the difficulties in measuring and expressing astronomical data in International System of Units (SI units). In particular, there is a huge quantity of very precise data relating to the positions of objects within the solar system which cannot conveniently be expressed or processed in SI units. Through a number of modifications, the astronomical system of units now explicitly recognizes the consequences of general relativity, which is a necessary addition to the International System of Units in order to accurately treat astronomical data. The astronomical system of units is a tridimensional system, in that it defines units of length, mass and time. The associated astronomical constants also fix the different frames of reference that are needed to report observations.〔 In particular, there is the ''barycentric celestial reference system'' (BCRS) centered at the barycenter of the solar system, and the ''geocentric celestial reference system'' (GCRS) centered at the center of mass of the Earth (including its fluid envelopes) 〕 The system is a conventional system, in that neither the unit of length nor the unit of mass are true physical constants, and there are at least three different measures of time. == Astronomical unit of time == (詳細はday, defined as seconds. 365.25 days make up one Julian year.〔 The symbol ''D'' is used in astronomy to refer to this unit. 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「Astronomical system of units」の詳細全文を読む スポンサード リンク
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