Instant · Precise · Universal
32 units available
6 categories total
To convert to meters: multiply by 2.8179403262 × 10⁻¹⁵.
re = e²/(4πε₀mec²) ≈ 2.8179 × 10⁻¹⁵ m, where e is electron charge and me is electron mass.
For example, 1 Electron Radius (Classical) (re) = 9.132256e-38 Megaparsec (Mpc).
| Electron Radius (Classical) (re) | Megaparsec (Mpc) |
|---|---|
| 0.1 | 9.132256e-39 |
| 0.5 | 4.566128e-38 |
| 1 | 9.132256e-38 |
| 2 | 1.826451e-37 |
| 5 | 4.566128e-37 |
| 10 | 9.132256e-37 |
| 25 | 2.283064e-36 |
| 50 | 4.566128e-36 |
| 100 | 9.132256e-36 |
| 500 | 4.566128e-35 |
| 1000 | 9.132256e-35 |
The classical electron radius is a theoretical length scale derived from the electron's charge and mass, approximately 2.818 × 10⁻¹⁵ meters.
re = e²/(4πε₀mec²) ≈ 2.8179 × 10⁻¹⁵ m, where e is electron charge and me is electron mass.
To convert to meters: multiply by 2.8179403262 × 10⁻¹⁵.
Used in calculating X-ray and gamma-ray scattering probabilities off electrons (Thomson and Compton scattering).
Despite its name, the electron is a point particle in quantum theory — the 'classical radius' is a theoretical construct, not the electron's actual size.
Assuming this is the actual physical size of the electron — quantum mechanics shows the electron has no measurable size.
Think of it as the scale at which classical electromagnetic self-energy equals the electron's mass-energy.
The megaparsec is equal to one million parsecs, approximately 3.26 million light-years, used for measuring distances between galaxies and in cosmology.
1 Mpc = 10⁶ pc = 3.0857 × 10²² m ≈ 3.262 × 10⁶ light-years.
To convert Mpc to light-years: multiply by 3.262 × 10⁶. To convert Mpc to meters: multiply by 3.0857 × 10²².
Measuring distances to galaxy clusters, Hubble flow calculations, and large-scale structure mapping.
The Andromeda Galaxy is about 0.78 Mpc away. The Virgo Cluster is about 16.5 Mpc distant.
Confusing Mpc with kpc — they differ by a factor of 1,000. kpc = within galaxies, Mpc = between galaxies.
Hubble's constant links distance (Mpc) to recession speed (km/s): the farther away a galaxy is, the faster it recedes.



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