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Convert Furlongs (US survey) to Parsecs

Furlongs (US survey)




Parsecs


How to use this Furlongs (US survey) to Parsecs Converter 🤔

Follow these steps to convert given Furlongs (US survey) value from Furlongs (US survey) units to Parsecs units.

  1. Enter the input Furlongs (US survey) value in the text field.
  2. The given Furlongs (US survey) is converted to Parsecs in realtime ⌚ using the formula, and displayed under the Parsecs label.
  3. You may copy the resulting Parsecs value using the Copy button.

Formula

To convert given length from Furlongs (US survey) to Parsecs, use the following formula.

Parsecs = Furlongs (US survey) / 153387785983224.97

Calculation

Calculation will be done after you enter a valid input.

Furlongs (US survey) to Parsecs Conversion Table

The following table gives some of the most used conversions from Furlongs (US survey) to Parsecs.

Furlongs (US survey) (fur)Parsecs (pc)
0 fur0 pc
1 fur0 pc
2 fur0 pc
3 fur0 pc
4 fur0 pc
5 fur0 pc
6 fur0 pc
7 fur0 pc
8 fur0 pc
9 fur0 pc
10 fur0 pc
20 fur0 pc
50 fur0 pc
100 fur0 pc
1000 fur1e-11 pc
10000 fur7e-11 pc
100000 fur6.5e-10 pc

Furlongs (US survey)

A furlong (US survey) is a unit of length used primarily in land surveying and agriculture in the United States. One US survey furlong is equivalent to exactly 660 feet or approximately 201.168 meters.

The US survey furlong is defined as one-eighth of a US survey mile, providing a convenient measurement for distances used in surveying and land measurement.

Furlongs (US survey) are utilized in contexts such as land surveys, property measurement, and horse racing in the United States. The unit ensures consistency and accuracy in measuring shorter distances in these fields.

Parsecs

A parsec (symbol: pc) is a unit of length used in astronomy. One parsec is approximately 3.26 light-years or 3.086 × 10¹³ kilometers.

The term parsec comes from "parallax of one arcsecond." It is the distance at which one astronomical unit subtends an angle of one arcsecond.

Parsecs are commonly used to measure large distances between astronomical objects outside our solar system, such as between stars or galaxies.