Solar mass

සූර්ය ස්කන්ධ (ඉංග්‍රීසි:  solar mass) (M_☉) යනු තාරකා විද්‍යාවේ සම්මත ඒකකයකි. එය ආසන්න වශයෙන් 2×10³⁰ kg පමණ වේ.

M_☉ = (1.98855±0.00025)×10³⁰ kg

Solar mass
The Sun contains more than 99% of the mass of the Solar System. Bodies lighter than Saturn are not visible at this scale.
General information
Unit system	astronomy
Unit of	mass
Symbol	M☉
In SI base units	(1.98847±0.00007)×1030 kg[1][2]

Size and mass of very large stars, from right to left: VY Canis Majoris (17 ± 8 M_☉), Betelgeuse (11.6 ± 5.0 M_☉), Rho Cassiopeiae (14-30 M_☉), and the blue Pistol Star (27.5 M_☉). The concentric ovals indicate the size of Neptune's (blue), Jupiter's (red) and the Earth's (grey) orbits. Properly scaled, the Sun (1 M_☉) only appears as a tiny dot in the center of the ovals (click for higher resolution to see Earth orbit and Sun).

ආශ්‍රිත=

• Chandrasekhar limit
• Gaussian gravitational constant
• Orders of magnitude (mass)
• Stellar mass
• Sun

මූලාශ්‍ර

1. "Astronomical Constants" (PDF). The Astronomical Almanac. 2014. p. 2. සම්ප්‍රවේශය 10 April 2019.
2. "Newtonian constant of gravitation". Physical Measurement Laboratory. සම්ප්‍රවේශය 10 April 2019.