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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 Decigrams (dg) is equal to 0.0001 kilograms, while 1 Sun Mass (M☉) = 1.999999999E+30 kilograms.| 1 Decigrams | to common mass-weight units |
|---|---|
| 1 dg | = 0.0001 kilograms (kg) |
| 1 dg | = 0.1 grams (g) |
| 1 dg | = 100 milligrams (mg) |
| 1 dg | = 0.00022046244201838 pounds (lbs) |
| 1 dg | = 0.003527399072294 ounces (oz) |
| 1 dg | = 0.5 carats (ct) |
| 1 dg | = 1.5432360734519 grains (gr) |
| 1 dg | = 1.5747312327469E-5 stones (st) |
| 1 dg | = 0.077161791764707 scruples (℈) |
| 1 dg | = 7.8736522208885E-6 quarters UK (1/4[UK]) |
| Decigrams | to Sun Mass (table conversion) |
|---|---|
| 1 dg | = 5.0000000025E-35 M☉ |
| 2 dg | = 1.0000000005E-34 M☉ |
| 3 dg | = 1.50000000075E-34 M☉ |
| 4 dg | = 2.000000001E-34 M☉ |
| 5 dg | = 2.50000000125E-34 M☉ |
| 6 dg | = 3.0000000015E-34 M☉ |
| 7 dg | = 3.50000000175E-34 M☉ |
| 8 dg | = 4.000000002E-34 M☉ |
| 9 dg | = 4.50000000225E-34 M☉ |
| 10 dg | = 5.0000000025E-34 M☉ |
| 20 dg | = 1.0000000005E-33 M☉ |
| 30 dg | = 1.50000000075E-33 M☉ |
| 40 dg | = 2.000000001E-33 M☉ |
| 50 dg | = 2.50000000125E-33 M☉ |
| 60 dg | = 3.0000000015E-33 M☉ |
| 70 dg | = 3.50000000175E-33 M☉ |
| 80 dg | = 4.000000002E-33 M☉ |
| 90 dg | = 4.50000000225E-33 M☉ |
| 100 dg | = 5.0000000025E-33 M☉ |
| 200 dg | = 1.0000000005E-32 M☉ |
| 300 dg | = 1.50000000075E-32 M☉ |
| 400 dg | = 2.000000001E-32 M☉ |
| 500 dg | = 2.50000000125E-32 M☉ |
| 600 dg | = 3.0000000015E-32 M☉ |
| 700 dg | = 3.50000000175E-32 M☉ |
| 800 dg | = 4.000000002E-32 M☉ |
| 900 dg | = 4.50000000225E-32 M☉ |
| 1000 dg | = 5.0000000025E-32 M☉ |
| 2000 dg | = 1.0000000005E-31 M☉ |
| 4000 dg | = 2.000000001E-31 M☉ |
| 5000 dg | = 2.50000000125E-31 M☉ |
| 7500 dg | = 3.750000001875E-31 M☉ |
| 10000 dg | = 5.0000000025E-31 M☉ |
| 25000 dg | = 1.250000000625E-30 M☉ |
| 50000 dg | = 2.50000000125E-30 M☉ |
| 100000 dg | = 5.0000000025E-30 M☉ |
| 1000000 dg | = 5.0000000025E-29 M☉ |
| 1000000000 dg | = 5.0000000025E-26 M☉ |