Polar Radius of Neptune
| Value | 24,341,000 m |
| Status | Measured: ± 30,000 m (0.0012 relative) |
| Source | NASA NSSDC Planetary Fact Sheet, Neptune (polar radius at 1 bar) |
| Categories | Astronomicalsolar-systemplanets |
| Planck length | 1.5060124e+42 lP |
| femtometer | 2.4341000e+22 fm |
| picometer | 2.4341000e+19 pm |
| bohr radius | 4.5997824e+17 a0 |
| angstrom | 2.4341000e+17 Å |
| nanometer | 2.4341000e+16 nm |
| micrometer | 24,341,000,000,000 μm |
| thou | 958,307,090,000 thou |
| point | 68,998,110,000 pt |
| millimeter | 24,341,000,000 mm |
| pica | 5,749,842,500 pc |
| centimeter | 2,434,100,000 cm |
| inch | 958,307,090 in |
| decimeter | 243,410,000 dm |
| hand | 239,576,770 hh |
| link | 120,998,370 li |
| foot | 79,858,924 ft |
| US survey foot | 79,858,764 ftUS |
| yard | 26,619,641 yd |
| meter | 24,341,000 m |
| fathom | 13,309,821 ftm |
| rod | 4,839,934.8 rd |
| chain | 1,209,983.7 ch |
| cable length | 131,430.89 cb |
| furlong | 120,998.37 fur |
| kilometer | 24,341 km |
| mile | 15,124.796 mi |
| nautical mile | 13,143.089 nmi |
| league | 5,041.5987 lea |
| megameter | 24.341 Mm |
| Earth radius | 3.8205933 REarth |
| light-second | 0.081192836 ls |
| lunar distance | 0.063322225 LD |
| solar radius | 0.034987782 Rsun |
| light-minute | 0.0013532139 lmin |
| astronomical unit | 0.00016270954 AU |
| light-year | 2.5728457e-09 ly |
| parsec | 7.8883809e-10 pc |
| kiloparsec | 7.8883809e-13 kpc |
| megaparsec | 7.8883809e-16 Mpc |
| gigaparsec | 7.8883809e-19 Gpc |
Learning zone
Neptune's poles sit 423 km below its equator — a flattening of 1.7 per cent, the smallest of any giant planet, the combined result of the highest density among the four and a moderate 16.11-hour rotation. The value derives from Voyager 2's occultation profiles joined to stellar occultations observed from Earth, and its quoted uncertainty is the largest of the giant-planet radii: one flyby, one geometry, 1989.
Even a modest oblateness works hard at 30 au. The J₂ harmonic it generates precesses the orbits of the inner moons and the narrow, clumpy rings — the "arcs" of the Adams ring, whose stubborn persistence against spreading is still being explained, are confined partly by resonances that depend on exactly this figure. When the arcs were first detected by occultation in 1984, before Voyager arrived, the flattening was among the unknowns that made the data so hard to read.