Convert Furlong (fur) to Earth's Polar Radius (R⊕ (p)) instantly.
Furlong to Earth's Polar Radius conversion
1 Furlong (fur) = 0.000031646226 Earth's Polar Radius (R⊕ (p)). To convert Furlong to Earth's Polar Radius, multiply the value by 0.000031646226.
| Furlong (fur) | Earth's Polar Radius (R⊕ (p)) |
|---|---|
| 1 | 0.000031646226 |
| 2 | 0.000063292452 |
| 5 | 0.00015823113 |
| 10 | 0.00031646226 |
| 25 | 0.00079115564 |
| 50 | 0.0015823113 |
| 100 | 0.0031646226 |
| 1000 | 0.031646226 |
Frequently asked questions
How many Earth's Polar Radius are in one Furlong?
One Furlong (fur) equals 0.000031646226 Earth's Polar Radius (R⊕ (p)).
How do I convert Furlong to Earth's Polar Radius?
To convert Furlong to Earth's Polar Radius, multiply the value by 0.000031646226.
What is 10 Furlong in Earth's Polar Radius?
10 Furlong = 0.00031646226 Earth's Polar Radius.
About these units
Furlong (fur)
A furlong, equal to 10 chains or 660 feet, originated as the distance a team of oxen could plow before needing rest. Its name derives from "furrow-long," indicating the length of a typical plowed furrow in medieval agriculture. This agricultural basis linked the furlong to the acre: a rectangle one furlong long and one chain wide equaled one acre in area. Today, the furlong is most notably used in horse racing, where race distances are often measured in furlongs rather than miles. This tradition reflects both the unit's historical importance and its suitability for describing moderate distances. While archaic in most contexts, the furlong remains a culturally iconic measure that connects modern sports to medieval agricultural practices.
Earth's Polar Radius (R⊕ (p))
The Earth's polar radius is approximately 6,356.8 km, slightly shorter than the equatorial radius due to the Earth's flattening at the poles. This measurement is critical in modeling Earth's shape, gravity field, and rotation. It impacts satellite orbits, geodetic surveys, and global positioning systems (GPS). The difference between the equatorial and polar radii also explains phenomena such as centrifugal force variations, equatorial bulges, and sea level differences across latitudes. Understanding R⊕ (p) is essential for precision navigation, Earth science, and astronomy.