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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.| 3729450531 Deuteron Mass | to common mass-weight units |
|---|---|
| 3729450531 D | = 1.2469738579415E-17 kilograms (kg) |
| 3729450531 D | = 1.2469738579415E-14 grams (g) |
| 3729450531 D | = 1.2469738579415E-11 milligrams (mg) |
| 3729450531 D | = 2.7491090185485E-17 pounds (lbs) |
| 3729450531 D | = 4.3985744296777E-16 ounces (oz) |
| 3729450531 D | = 6.2348692897074E-14 carats (ct) |
| 3729450531 D | = 1.9243750402267E-13 grains (gr) |
| 3729450531 D | = 1.9636486805193E-18 stones (st) |
| 3729450531 D | = 9.6218737162513E-15 scruples (℈) |
| 3729450531 D | = 9.8182384859708E-19 quarters UK (1/4[UK]) |