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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.| 4306132405 Deuteron Mass | to common mass-weight units |
|---|---|
| 4306132405 D | = 1.4397924019198E-17 kilograms (kg) |
| 4306132405 D | = 1.4397924019198E-14 grams (g) |
| 4306132405 D | = 1.4397924019198E-11 milligrams (mg) |
| 4306132405 D | = 3.1742014892675E-17 pounds (lbs) |
| 4306132405 D | = 5.078722382828E-16 ounces (oz) |
| 4306132405 D | = 7.1989620095991E-14 carats (ct) |
| 4306132405 D | = 2.2219395729246E-13 grains (gr) |
| 4306132405 D | = 2.2672860639747E-18 stones (st) |
| 4306132405 D | = 1.1109696150134E-14 scruples (℈) |
| 4306132405 D | = 1.1336424642994E-18 quarters UK (1/4[UK]) |