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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 Deuteron Mass (D) is equal to 3.343585999E-27 kilograms, while 1 Sun Mass (M☉) = 1.999999999E+30 kilograms.| 9000000000000 Deuteron Mass | to common mass-weight units |
|---|---|
| 9000000000000 D | = 3.0092273991E-14 kilograms (kg) |
| 9000000000000 D | = 3.0092273991E-11 grams (g) |
| 9000000000000 D | = 3.0092273991E-8 milligrams (mg) |
| 9000000000000 D | = 6.634216209942E-14 pounds (lbs) |
| 9000000000000 D | = 1.0614745935907E-12 ounces (oz) |
| 9000000000000 D | = 1.50461369955E-10 carats (ct) |
| 9000000000000 D | = 4.6439482755109E-10 grains (gr) |
| 9000000000000 D | = 4.7387243718003E-15 stones (st) |
| 9000000000000 D | = 2.3219737794201E-11 scruples (℈) |
| 9000000000000 D | = 2.3693609994082E-15 quarters UK (1/4[UK]) |