The solar mass can be determined from the length of the year , the distance of the LOCATION@1 to the Sun -LRB- the astronomical unit -RRB- -LRB- AU -RRB- , and the gravitational constant -LRB- G -RRB- as .

It is equal to the mass of the MISC@1 , about NUMBER@1 times the mass of the LOCATION@1 , or NUMBER@2 times the mass of LOCATION@2 .
