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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 Daltons (Da) = 1.66053E-27 kilograms.| 279000 Sun Mass | to common mass-weight units |
|---|---|
| 279000 M☉ | = 5.57999999721E+35 kilograms (kg) |
| 279000 M☉ | = 5.57999999721E+38 grams (g) |
| 279000 M☉ | = 5.57999999721E+41 milligrams (mg) |
| 279000 M☉ | = 1.2301804258475E+36 pounds (lbs) |
| 279000 M☉ | = 1.9682886813559E+37 ounces (oz) |
| 279000 M☉ | = 2.789999998605E+39 carats (ct) |
| 279000 M☉ | = 8.6112572855558E+39 grains (gr) |
| 279000 M☉ | = 8.7870002743339E+34 stones (st) |
| 279000 M☉ | = 4.3056279783178E+38 scruples (℈) |
| 279000 M☉ | = 4.393497937059E+34 quarters UK (1/4[UK]) |