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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.| 71 Deuteron Mass | to common mass-weight units |
|---|---|
| 71 D | = 2.37394605929E-25 kilograms (kg) |
| 71 D | = 2.37394605929E-22 grams (g) |
| 71 D | = 2.37394605929E-19 milligrams (mg) |
| 71 D | = 5.2336594545098E-25 pounds (lbs) |
| 71 D | = 8.3738551272156E-24 ounces (oz) |
| 71 D | = 1.186973029645E-21 carats (ct) |
| 71 D | = 3.6635591951252E-21 grains (gr) |
| 71 D | = 3.7383270044203E-26 stones (st) |
| 71 D | = 1.8317793148758E-22 scruples (℈) |
| 71 D | = 1.8691625661998E-26 quarters UK (1/4[UK]) |