Solar mass

The solar mass (M☉) is a standard unit of mass in astronomy, equal to approximately 1.99 × 1030 kilograms. It is used to indicate the masses of other stars, as well as clusters, nebulae and galaxies. It is equal to the mass of the Sun, about two nonillion kilograms: M☉ = (1.98855±0.00025)×1030 kg The above mass is about 332946 times the mass of Earth (M⊕), or 1048 times the mass of Jupiter (MJ).

Solar mass

The solar mass (M☉) is a standard unit of mass in astronomy, equal to approximately 1.99 × 1030 kilograms. It is used to indicate the masses of other stars, as well as clusters, nebulae and galaxies. It is equal to the mass of the Sun, about two nonillion kilograms: M☉ = (1.98855±0.00025)×1030 kg The above mass is about 332946 times the mass of Earth (M⊕), or 1048 times the mass of Jupiter (MJ).