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To convert solar masses to kg: multiply by 1.98847 × 10³⁰.
M☉ = 1.98847 × 10³⁰ kg ≈ 333,000 M⊕ ≈ 1,048 M_Jupiter.
For example, 1 Sun's Mass (M☉) = 2.182881e+60 Electron Mass (rest) (mₑ).
| Sun's Mass (M☉) | Electron Mass (rest) (mₑ) |
|---|---|
| 0.1 | 2.182881e+59 |
| 0.5 | 1.091440e+60 |
| 1 | 2.182881e+60 |
| 2 | 4.365762e+60 |
| 5 | 1.091440e+61 |
| 10 | 2.182881e+61 |
| 25 | 5.457202e+61 |
| 50 | 1.091440e+62 |
| 100 | 2.182881e+62 |
| 500 | 1.091440e+63 |
| 1000 | 2.182881e+63 |
The solar mass is the mass of the Sun, approximately 1.989 × 10³⁰ kilograms — about 333,000 times the mass of Earth.
M☉ = 1.98847 × 10³⁰ kg ≈ 333,000 M⊕ ≈ 1,048 M_Jupiter.
To convert solar masses to kg: multiply by 1.98847 × 10³⁰.
Expressing stellar masses: Betelgeuse ≈ 15 M☉, Sirius ≈ 2 M☉, a typical neutron star ≈ 1.4 M☉.
The Sun loses about 5 million tonnes per second through nuclear fusion (E=mc²), but that's only 10⁻¹³ M☉ per year.
The Sun is losing mass continuously through radiation and solar wind — its mass is not quite constant over billions of years.
Almost everything in astronomy uses solar masses: stars (0.1–100 M☉), galaxies (10⁹–10¹² M☉), black holes (3–10⁹ M☉).
The electron rest mass is the mass of a stationary electron, approximately 9.109 × 10⁻³¹ kilograms.
mₑ ≈ 9.109 × 10⁻³¹ kg = 5.486 × 10⁻⁴ u = 1/1836 of a proton mass.
To convert electron masses to kg: multiply by 9.1093837015 × 10⁻³¹.
Essential for electron microscope design, semiconductor physics, and laser technology.
The electron is about 1,836 times lighter than a proton. An electron's mass-energy equivalent (E=mc²) is 0.511 MeV.
Confusing electron mass with electron charge (e). Mass = 9.1 × 10⁻³¹ kg; charge = 1.6 × 10⁻¹⁹ C.
Key ratio: proton-to-electron mass ≈ 1,836. This ratio explains why electrons orbit nuclei rather than the reverse.



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