Planck length
| Value | 1.616255e-35 m |
| Status | Measured: ± 1.80e-40 m (0.000011 relative) |
| Source | CODATA 2022 (derived from ħ, c and G; uncertainty inherited from G) |
| Categories | Universal & Atomicphysicsquantum |
| femtometer | 1.6162550e-20 fm |
| picometer | 1.6162550e-23 pm |
| nanometer | 1.6162550e-26 nm |
| micrometer | 1.6162550e-29 μm |
| millimeter | 1.6162550e-32 mm |
| centimeter | 1.6162550e-33 cm |
| decimeter | 1.6162550e-34 dm |
| meter | 1.6162550e-35 m |
| kilometer | 1.6162550e-38 km |
| inch | 6.3632087e-34 in |
| foot | 5.3026739e-35 ft |
| yard | 1.7675580e-35 yd |
| mile | 1.0042943e-38 mi |
| nautical mile | 8.7270788e-39 nmi |
| astronomical unit | 1.0803997e-46 AU |
| light-year | 1.7083829e-51 ly |
| parsec | 5.2379257e-52 pc |
Learning zone
Planck built his natural units in 1899, a year before he invented the quantum, by asking what lengths, masses and times can be assembled from G, c and h alone. The answer for length is 1.6 × 10⁻³⁵ m: twenty orders of magnitude smaller than a proton, and about 10⁻²⁰ times any distance the LHC can resolve. Probing it directly would need a collider of galactic proportions.
The physical claim is that at this scale the Schwarzschild radius of a particle and its Compton wavelength coincide, so you cannot localise anything more finely without making a black hole — spacetime itself presumably stops being smooth. String theory and loop quantum gravity both place their structure near here, and black-hole entropy counts Planck areas on the horizon. Resist the common overreach: nothing in established physics says space is pixellated at l_P; it is where our theories are known to fail, not a measured grain size.