# point (TeX) to parsec conversion

Conversion number between point (TeX) [pt] and parsec [pc] is 1.1390036524837 × 10-20. This means, that point (TeX) is smaller unit than parsec.

### Contents [show][hide] Switch to reverse conversion:
from parsec to point (TeX) conversion

### Enter the number in point (TeX):

Decimal Fraction Exponential Expression
 [pt]
eg.: 10.12345 or 1.123e5

Result in parsec

?
 precision 0 1 2 3 4 5 6 7 8 9 [info] Decimal: Exponential:

### Calculation process of conversion value

• 1 point (TeX) = ((254/722700)) / (3.085677581*10^16) = 1.1390036524837 × 10-20 parsec
• 1 parsec = (3.085677581*10^16) / ((254/722700)) = 8.7796031015303 × 10+19 point (TeX)
• ? point (TeX) × ((254/722700)  ("m"/"point (TeX)")) / (3.085677581*10^16  ("m"/"parsec")) = ? parsec

### High precision conversion

If conversion between point (TeX) to metre and metre to parsec is exactly definied, high precision conversion from point (TeX) to parsec is enabled. Since definition contain rounded number(s) too, there is no sense for high precision calculation, but if you want, you can enable it. Keep in mind, that converted number will be inaccurate due this rounding error!

### point (TeX) to parsec conversion chart

 Start value: [point (TeX)] Step size [point (TeX)] How many lines? (max 100)

visual:
point (TeX)parsec
00
101.1390036524837 × 10-19
202.2780073049673 × 10-19
303.417010957451 × 10-19
404.5560146099347 × 10-19
505.6950182624184 × 10-19
606.834021914902 × 10-19
707.9730255673857 × 10-19
809.1120292198694 × 10-19
901.0251032872353 × 10-18
1001.1390036524837 × 10-18
1101.252904017732 × 10-18
Copy to Excel

## Multiple conversion

Enter numbers in point (TeX) and click convert button.
One number per line.

Converted numbers in parsec:
Click to select all

## Details about point (TeX) and parsec units:

Convert Point (TeX) to other unit:

### point (TeX)

Definition of point (TeX) unit: ≡  1⁄72.27 in .

Convert Parsec to other unit:

### parsec

Definition of parsec unit: ≈ 3.085677581x1016. Distance of star with parallax shift of one arc second from a base of one astronomical unit 