IAU (1976) System of Astronomical Constants


The International Astronomical Union at its XVIth General Assembly in Grenoble in 1976, accepted System of Astronomical Constants. In 1994
the IAU recognized that the parameters became outdated, but retained the 1976 set for sake of continuity, but also recommended to start maintaining a set of "current best estimates"
;
this "sub group for numerical standards" had published a list, which included new constants
The system of constants was prepared
by Commission 4 on ephemerides led by P. Kenneth Seidelmann.
At the time, a new standard epoch was accepted; followed later
by a new reference system with fundamental catalogue, and expressions for precession of the equinoxes,
and in 1979 by new expressions for the relation between Universal Time and sidereal time
, and in 1979 and 1980 by a theory of nutation
. There were no reliable rotation elements for most planets, but a joint working group on Cartographic Coordinates and Rotational Elements was installed to compile recommended values

Units

The IAU system is based on the astronomical system of units:

Other quantities for use in the preparation of ephemerides

3.Equatorial radii
ObjectEquatorial radius
Mercury2 439 ±1
Venus6 052 ±6
Earth6 378.140 ±0.005
Mars3 397.2 ±1
Jupiter71 398
Saturn60 000
Uranus25 400
Neptune24 300
Pluto2 500
Moon1 738
Moon's disk, ratio to Earth's equatorial radiusk = 0.272 5076 ae
Sun696 000