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The solar mass (M☉) is a standard unit of mass in astronomy, equal to approximately 2×1030 kg. It is used to indicate the masses of other stars, as well as clusters, nebulae, and galaxies.
1 Newton in Earth gravity is the equivalent weight of 1/9.80665 kg on Earth. This is derived using Newton's second law f=ma and assuming Earth gravity of 9.80665 m/s2. 1 N (on Earth) = 0.101971621297793 kg.
In relation to the base unit of [mass weight] => (kilograms), 1 Sun Mass (M☉) is equal to 1.999999999E+30 kilograms, while 1 Newtons[Earth Gravity] (N) = 0.10197162129779 kilograms.| 21 Sun Mass | to common mass-weight units |
|---|---|
| 21 M☉ | = 4.1999999979E+31 kilograms (kg) |
| 21 M☉ | = 4.1999999979E+34 grams (g) |
| 21 M☉ | = 4.1999999979E+37 milligrams (mg) |
| 21 M☉ | = 9.2594225601422E+31 pounds (lbs) |
| 21 M☉ | = 1.4815076096227E+33 ounces (oz) |
| 21 M☉ | = 2.09999999895E+35 carats (ct) |
| 21 M☉ | = 6.481591505257E+35 grains (gr) |
| 21 M☉ | = 6.6138711742298E+30 stones (st) |
| 21 M☉ | = 3.2407952524973E+34 scruples (℈) |
| 21 M☉ | = 3.3069339311197E+30 quarters UK (1/4[UK]) |