Radius of Proxima Centauri

RProx=107,280,000 mR_{\mathrm{Prox}} = 107,280,000\ \text{m}
Value107,280,000 m
StatusMeasured: ± 3,100,000 m (0.029 relative)
SourceRibas et al. (2017), 0.1542 ± 0.0045 R⊙
CategoriesAstronomicalstellar
Radius of Proxima Centauri in every length unit
Planck length6.6375665e+42 lP
femtometer1.0728000e+23 fm
picometer1.0728000e+20 pm
bohr radius2.0272982e+18 a0
angstrom1.0728000e+18 Å
nanometer1.0728000e+17 nm
micrometer107,280,000,000,000 μm
thou4,223,622,000,000 thou
point304,100,790,000 pt
millimeter107,280,000,000 mm
pica25,341,732,000 pc
centimeter10,728,000,000 cm
inch4,223,622,000 in
decimeter1,072,800,000 dm
hand1,055,905,500 hh
link533,285,610 li
foot351,968,500 ft
US survey foot351,967,800 ftUS
yard117,322,830 yd
meter107,280,000 m
fathom58,661,417 ftm
rod21,331,424 rd
chain5,332,856.1 ch
cable length579,265.66 cb
furlong533,285.61 fur
kilometer107,280 km
mile66,660.702 mi
nautical mile57,926.566 nmi
league22,220.234 lea
megameter107.28 Mm
Earth radius16.838801 REarth
light-second0.35784756 ls
lunar distance0.27908501 LD
solar radius0.1542044 Rsun
light-minute0.005964126 lmin
astronomical unit0.00071712251 AU
light-year1.1339505e-08 ly
parsec3.4767080e-09 pc
kiloparsec3.4767080e-12 kpc
megaparsec3.4767080e-15 Mpc
gigaparsec3.4767080e-18 Gpc

Learning zone

Proxima is startlingly small: 0.154 of the Sun's radius makes it only about 1.5 Jupiters across, though 130 times Jupiter's mass — matter at the bottom of the main sequence is crushed to enormous density, and Proxima's mean density is some forty times the Sun's. Feed this radius and its 3000 K effective temperature into the Stefan–Boltzmann law and the luminosity comes out near 0.0016 L⊙: if Proxima replaced the Sun, Earth would receive less light than a heat lamp across a room, and its habitable zone huddles twenty times closer than Mercury.

The radius is not imaged but inferred — from the measured luminosity and temperature, cross-checked by interferometry at the VLT that just resolves a disc about one milliarcsecond across, the angular size of a coin at four thousand kilometres. That such a measurement is possible at all for so small a star is itself a fact worth knowing about modern optics.