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Convert link (US survey) to Kiloparsecs

link (US survey)




Kiloparsecs


How to use this link (US survey) to Kiloparsecs Converter 🤔

Follow these steps to convert given link (US survey) value from link (US survey) units to Kiloparsecs units.

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

Formula

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

Kiloparsecs = link (US survey) / 153387785859797880000

Calculation

Calculation will be done after you enter a valid input.

link (US survey) to Kiloparsecs Conversion Table

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

link (US survey) (li)Kiloparsecs (kpc)
0 li0 kpc
1 li0 kpc
2 li0 kpc
3 li0 kpc
4 li0 kpc
5 li0 kpc
6 li0 kpc
7 li0 kpc
8 li0 kpc
9 li0 kpc
10 li0 kpc
20 li0 kpc
50 li0 kpc
100 li0 kpc
1000 li0 kpc
10000 li0 kpc
100000 li0 kpc

link (US survey)

A link (US survey) is a unit of length used primarily in land surveying in the United States. One US survey link is equivalent to exactly 0.66 feet or approximately 0.201168 meters.

The US survey link is defined as one-hundredth of a US survey chain, where one US survey chain is 66 feet long. This unit provides precision for finer measurements in land surveying and mapping.

Links (US survey) are used in land surveying to measure shorter distances and ensure accuracy in property measurement and mapping activities in the United States.

Kiloparsecs

A kiloparsec (kpc) is a unit of length used in astronomy to measure astronomical distances. One kiloparsec is equivalent to 3,262 light-years or approximately 3.086 × 10^16 meters.

The kiloparsec is defined as one thousand parsecs, where one parsec is the distance at which one astronomical unit subtends an angle of one arcsecond.

Kiloparsecs are used to measure large distances between celestial objects, such as the size of galaxies or the distance between galactic structures. They provide a convenient scale for expressing vast distances in the universe.