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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.
1 Newton in Earth gravity is the equivalent weight of 1/9.80665 kg on Earth. This is derived using Newton's second law f=ma and assuming Earth gravity of 9.80665 m/s2. 1 N (on Earth) = 0.101971621297793 kg.
In relation to the base unit of [mass weight] => (kilograms), 1 Sun Mass (M☉) is equal to 1.999999999E+30 kilograms, while 1 Newtons[Earth Gravity] (N) = 0.10197162129779 kilograms.| 9208000000000 Sun Mass | to common mass-weight units |
|---|---|
| 9208000000000 M☉ | = 1.8415999990792E+43 kilograms (kg) |
| 9208000000000 M☉ | = 1.8415999990792E+46 grams (g) |
| 9208000000000 M☉ | = 1.8415999990792E+49 milligrams (mg) |
| 9208000000000 M☉ | = 4.0600363301804E+43 pounds (lbs) |
| 9208000000000 M☉ | = 6.4960581282887E+44 ounces (oz) |
| 9208000000000 M☉ | = 9.207999995396E+46 carats (ct) |
| 9208000000000 M☉ | = 2.8420235514479E+47 grains (gr) |
| 9208000000000 M☉ | = 2.9000250367766E+42 stones (st) |
| 9208000000000 M☉ | = 1.4210115564283E+46 scruples (℈) |
| 9208000000000 M☉ | = 1.4500117922738E+42 quarters UK (1/4[UK]) |