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Convert Fathoms (US survey) to Parsecs

Fathoms (US survey)




Parsecs


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

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

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

Parsecs = Fathoms (US survey) / 16872656445812036

Calculation

Calculation will be done after you enter a valid input.

Fathoms (US survey) to Parsecs Conversion Table

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

Fathoms (US survey) (fath)Parsecs (pc)
0 fath0 pc
1 fath0 pc
2 fath0 pc
3 fath0 pc
4 fath0 pc
5 fath0 pc
6 fath0 pc
7 fath0 pc
8 fath0 pc
9 fath0 pc
10 fath0 pc
20 fath0 pc
50 fath0 pc
100 fath0 pc
1000 fath0 pc
10000 fath0 pc
100000 fath1e-11 pc

Fathoms (US survey)

A fathom (US survey) is a unit of length used primarily in maritime contexts in the United States to measure water depth. One US survey fathom is equivalent to exactly 6 feet or approximately 1.8288 meters.

The US survey fathom is defined as 6 feet, consistent with historical maritime measurement practices and used for depth soundings and underwater measurements.

Fathoms (US survey) are utilized in navigation, fishing, and marine activities in the United States to describe water depth. The unit provides a practical measurement for underwater distances and ensures consistency in maritime practices.

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.