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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 Sun Mass (M☉) is equal to 1.999999999E+30 kilograms, while 1 Decagrams (da g) = 0.01 kilograms.| 1 Sun Mass | to common mass-weight units |
|---|---|
| 1 M☉ | = 1.999999999E+30 kilograms (kg) |
| 1 M☉ | = 1.999999999E+33 grams (g) |
| 1 M☉ | = 1.999999999E+36 milligrams (mg) |
| 1 M☉ | = 4.4092488381629E+30 pounds (lbs) |
| 1 M☉ | = 7.0547981410607E+31 ounces (oz) |
| 1 M☉ | = 9.999999995E+33 carats (ct) |
| 1 M☉ | = 3.0864721453605E+34 grains (gr) |
| 1 M☉ | = 3.149462463919E+29 stones (st) |
| 1 M☉ | = 1.5432358345225E+33 scruples (℈) |
| 1 M☉ | = 1.5747304433903E+29 quarters UK (1/4[UK]) |
| Sun Mass | to Decagrams (table conversion) |
|---|---|
| 1 M☉ | = 1.999999999E+32 da g |
| 2 M☉ | = 3.999999998E+32 da g |
| 3 M☉ | = 5.999999997E+32 da g |
| 4 M☉ | = 7.999999996E+32 da g |
| 5 M☉ | = 9.999999995E+32 da g |
| 6 M☉ | = 1.1999999994E+33 da g |
| 7 M☉ | = 1.3999999993E+33 da g |
| 8 M☉ | = 1.5999999992E+33 da g |
| 9 M☉ | = 1.7999999991E+33 da g |
| 10 M☉ | = 1.999999999E+33 da g |
| 20 M☉ | = 3.999999998E+33 da g |
| 30 M☉ | = 5.999999997E+33 da g |
| 40 M☉ | = 7.999999996E+33 da g |
| 50 M☉ | = 9.999999995E+33 da g |
| 60 M☉ | = 1.1999999994E+34 da g |
| 70 M☉ | = 1.3999999993E+34 da g |
| 80 M☉ | = 1.5999999992E+34 da g |
| 90 M☉ | = 1.7999999991E+34 da g |
| 100 M☉ | = 1.999999999E+34 da g |
| 200 M☉ | = 3.999999998E+34 da g |
| 300 M☉ | = 5.999999997E+34 da g |
| 400 M☉ | = 7.999999996E+34 da g |
| 500 M☉ | = 9.999999995E+34 da g |
| 600 M☉ | = 1.1999999994E+35 da g |
| 700 M☉ | = 1.3999999993E+35 da g |
| 800 M☉ | = 1.5999999992E+35 da g |
| 900 M☉ | = 1.7999999991E+35 da g |
| 1000 M☉ | = 1.999999999E+35 da g |
| 2000 M☉ | = 3.999999998E+35 da g |
| 4000 M☉ | = 7.999999996E+35 da g |
| 5000 M☉ | = 9.999999995E+35 da g |
| 7500 M☉ | = 1.49999999925E+36 da g |
| 10000 M☉ | = 1.999999999E+36 da g |
| 25000 M☉ | = 4.9999999975E+36 da g |
| 50000 M☉ | = 9.999999995E+36 da g |
| 100000 M☉ | = 1.999999999E+37 da g |
| 1000000 M☉ | = 1.999999999E+38 da g |
| 1000000000 M☉ | = 1.999999999E+41 da g |