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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.| 103000 Deuteron Mass | to common mass-weight units |
|---|---|
| 103000 D | = 3.44389357897E-22 kilograms (kg) |
| 103000 D | = 3.44389357897E-19 grams (g) |
| 103000 D | = 3.44389357897E-16 milligrams (mg) |
| 103000 D | = 7.5924918847114E-22 pounds (lbs) |
| 103000 D | = 1.2147987015538E-20 ounces (oz) |
| 103000 D | = 1.721946789485E-18 carats (ct) |
| 103000 D | = 5.3147408041958E-18 grains (gr) |
| 103000 D | = 5.4232067810604E-23 stones (st) |
| 103000 D | = 2.657369992003E-19 scruples (℈) |
| 103000 D | = 2.7116020326561E-23 quarters UK (1/4[UK]) |