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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.| 120000 Sun Mass | to common mass-weight units |
|---|---|
| 120000 M☉ | = 2.3999999988E+35 kilograms (kg) |
| 120000 M☉ | = 2.3999999988E+38 grams (g) |
| 120000 M☉ | = 2.3999999988E+41 milligrams (mg) |
| 120000 M☉ | = 5.2910986057955E+35 pounds (lbs) |
| 120000 M☉ | = 8.4657577692728E+36 ounces (oz) |
| 120000 M☉ | = 1.1999999994E+39 carats (ct) |
| 120000 M☉ | = 3.7037665744326E+39 grains (gr) |
| 120000 M☉ | = 3.7793549567028E+34 stones (st) |
| 120000 M☉ | = 1.851883001427E+38 scruples (℈) |
| 120000 M☉ | = 1.8896765320684E+34 quarters UK (1/4[UK]) |