Astronomical constant should not be confused with Cosmological constant.
An astronomical constant is any of several physical constants used in astronomy. Formal sets of constants, along with recommended values, have been defined by the International Astronomical Union (IAU) several times: in 1964[1] and in 1976[2] (with an update in 1994). In 2009 the IAU adopted a new current set, and recognizing that new observations and techniques continuously provide better values for these constants, they decided[3] to not fix these values, but have the Working Group on Numerical Standards continuously maintain a set of Current Best Estimates.[4] The set of constants is widely reproduced in publications such as the Astronomical Almanac of the United States Naval Observatory and HM Nautical Almanac Office.
Besides the IAU list of units and constants, also the International Earth Rotation and Reference Systems Service defines constants relevant to the orientation and rotation of the Earth, in its technical notes.[5]
The IAU system of constants defines a system of astronomical units for length, mass and time (in fact, several such systems), and also includes constants such as the speed of light and the constant of gravitation which allow transformations between astronomical units and SI units. Slightly different values for the constants are obtained depending on the frame of reference used. Values quoted in barycentric dynamical time (TDB) or equivalent time scales such as the Teph of the Jet Propulsion Laboratory ephemerides represent the mean values that would be measured by an observer on the Earth's surface (strictly, on the surface of the geoid) over a long period of time. The IAU also recommends values in SI units, which are the values which would be measured (in proper length and proper time) by an observer at the barycentre of the Solar System: these are obtained by the following transformations:
\tauA({\rmSI})=(1+L\rm
| ||||
| ) |
\tauA({\rmTDB})
GE({\rmSI})=(1+L\rm)GE({\rmTDB})
GS({\rmSI})=(1+L\rm)GS({\rmTDB})
See main article: article and Astronomical system of units. The astronomical unit of time is a time interval of one day (D) of 86400 seconds. The astronomical unit of mass is the mass of the Sun (S). The astronomical unit of length is that length (A) for which the Gaussian gravitational constant (k) takes the value when the units of measurement are the astronomical units of length, mass and time.
| Quantity | Symbol | Value | Relative uncertainty | Ref. | ||
|---|---|---|---|---|---|---|
| Defining constants | ||||||
| align=center | k | 0.017 202 098 95 A3/2 S-1/2 D-1 | defined | |||
| align=center | c | 299 792 458 m s-1 | defined | [6] | ||
| Mean ratio of the TCG second to the TT second | align=center | 1 - LG | 1 - 6.969 290 134 | defined | [7] | |
| align=center | 1 - LB | 1 - 1.550 519 767 72 | defined | [8] | ||
| Primary constants | ||||||
| align=center | 1 - LC | 1 - 1.480 826 867 41 | 1.4 | |||
| align=center | τA | 499.004 783 836 156 s | A/c | |||
| align=center | ae | 6.378 1366 m | 1.6 | |||
| Potential of the geoid | W0 | 6.263 685 60 m2 s-2 | 8.0 | |||
| J2 | 0.001 082 6359 | 9.2 | ||||
| align=center | 1/ƒ | 0.003 352 8197 = 1/298.256 42 | 3.4 | |||
| align=center | GE | 3.986 004 391 m3 s-2 | 2.0 | |||
| align=center | G | 6.674 30 m3 kg-1 s-2 | 1.5 | [9] | ||
| align=center | μ | 0.012 300 0383 = 1/81.300 56 | 4.0 | |||
| align=center | ρ | 5028.796 195″ | [10] | |||
| align=center | ε | 23° 26′ 21.406″ | ||||
| Derived constants | ||||||
| align=center | N | 9.205 2331″ | [11] | |||
| align=center | A | 149 597 870 700 m | defined | |||
| Solar parallax = arcsin(ae/A) | align=center | π☉ | 8.794 1433″ | 1.6 | † | |
| align=center | κ | 20.495 52″ | ||||
| Heliocentric gravitational constant = A3k2/D2 | align=center | GS | 1.327 2440 m3 s-2 | 3.8 | ||
| Ratio of mass of Sun to mass of Earth = (GS)/(GE) | align=center | S/E | 332 946.050 895 | |||
| Ratio of mass of Sun to mass of (Earth + Moon) | align=center | (S/E) (1 + μ) | 328 900.561 400 | |||
| Mass of Sun = (GS)/G | align=center | S | 1.98855 kg | 1.0 | † | |
| System of planetary masses: Ratios of mass of Sun to mass of planet | ||||||
| 6 023 600 | ||||||
| 408 523.71 | ||||||
| 328 900.561 400 | ||||||
| 3 098 708 | ||||||
| 1047.3486 | ||||||
| 3497.898 | ||||||
| 22 902.98 | ||||||
| 19 412.24 | ||||||
| 135 200 000 | ||||||
| Other constants (outside the formal IAU System) | ||||||
| Parsec = A/tan(1") | align=center | pc | 3.085 677 581 28×1016 m | 4.0 | † | |
| Light-year = 365.25cD | align=center | ly | 9.460 730 472 5808 m | defined | † | |
| align=center | H0 | 70.1 km s-1 Mpc-1 | 0.019 | |||
| align=center | 3.939 W = 2.107 S D-1 | variable, ±0.1% | ||||
† The definitions of these derived constants have been taken from the references cited, but the values have been recalculated to take account of the more precise values of the primary constants cited in the table.