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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.385100 Deuteron Mass | to common mass-weight units |
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385100 D | = 1.2876149682149E-21 kilograms (kg) |
385100 D | = 1.2876149682149E-18 grams (g) |
385100 D | = 1.2876149682149E-15 milligrams (mg) |
385100 D | = 2.8387074027207E-21 pounds (lbs) |
385100 D | = 4.5419318443532E-20 ounces (oz) |
385100 D | = 6.4380748410745E-18 carats (ct) |
385100 D | = 1.9870938676658E-17 grains (gr) |
385100 D | = 2.0276475062003E-22 stones (st) |
385100 D | = 9.9354678050518E-19 scruples (℈) |
385100 D | = 1.0138232454135E-22 quarters UK (1/4[UK]) |