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Convert Feet (US survey) to Parsecs

Feet (US survey)




Parsecs


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

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

  1. Enter the input Feet (US survey) value in the text field.
  2. The given Feet (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 Feet (US survey) to Parsecs, use the following formula.

Parsecs = Feet (US survey) / 101235938665615180

Calculation

Calculation will be done after you enter a valid input.

Feet (US survey) to Parsecs Conversion Table

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

Feet (US survey) (ft)Parsecs (pc)
0 ft0 pc
1 ft0 pc
2 ft0 pc
3 ft0 pc
4 ft0 pc
5 ft0 pc
6 ft0 pc
7 ft0 pc
8 ft0 pc
9 ft0 pc
10 ft0 pc
20 ft0 pc
50 ft0 pc
100 ft0 pc
1000 ft0 pc
10000 ft0 pc
100000 ft0 pc

Feet (US survey)

A foot (US survey) is a unit of length used in land surveying and mapping in the United States. One foot (US survey) is defined as exactly 1200/3937 meters, which is approximately 0.3048006096 meters or about 0.3048 meters.

The US survey foot is slightly different from the international foot, which is defined as exactly 0.3048 meters. The difference is due to historical measurement standards and is used in specific contexts such as land surveying and engineering in the United States.

US survey feet are used primarily in the United States for property measurement, land surveying, and mapping, ensuring consistency in measurements within 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.