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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.
In relation to the base unit of [mass weight] => (kilograms), 1 Sun Mass (M☉) is equal to 1.999999999E+30 kilograms, while 1 Deuteron Mass (D) = 3.343585999E-27 kilograms.| 900 Sun Mass | to common mass-weight units |
|---|---|
| 900 M☉ | = 1.7999999991E+33 kilograms (kg) |
| 900 M☉ | = 1.7999999991E+36 grams (g) |
| 900 M☉ | = 1.7999999991E+39 milligrams (mg) |
| 900 M☉ | = 3.9683239543466E+33 pounds (lbs) |
| 900 M☉ | = 6.3493183269546E+34 ounces (oz) |
| 900 M☉ | = 8.9999999955E+36 carats (ct) |
| 900 M☉ | = 2.7778249308244E+37 grains (gr) |
| 900 M☉ | = 2.8345162175271E+32 stones (st) |
| 900 M☉ | = 1.3889122510703E+36 scruples (℈) |
| 900 M☉ | = 1.4172573990513E+32 quarters UK (1/4[UK]) |