Decimeters to Parsecs (dm to pc)

Metric Conversions.

Parsecs to Decimeters (Swap units)

1dm = 0pc

Note: You can increase or decrease the accuracy of this answer by selecting the number of significant figures required from the options above the result.

Decimeters to Parsecs conversion formula

Parsecs = Decimeters / 3.0856769049426E+17

Decimeters to Parsecs calculation

Parsecs = Decimeters / 3.0856769049426E+17

Parsecs = 1 / 3.0856769049426E+17

Parsecs = 0

What is a decimeter?

A decimeter is a unit of length in the metric system, specifically in the International System of Units (SI). It is equal to one-tenth of a meter or 10 centimeters. The prefix "deci" indicates a factor of 10^-1, which means that a decimeter is 10 times smaller than a meter.

The decimeter is commonly used in various fields, including science, engineering, and everyday measurements. It provides a convenient unit for measuring small distances, especially when centimeters are too small and meters are too large. For example, a decimeter can be used to measure the length of small objects such as pencils, books, or the width of a hand.

In comparison to the imperial system, a decimeter is equivalent to approximately 3.937 inches. This conversion factor allows for easy conversion between the metric and imperial systems. The decimeter is part of a larger range of metric units, which provide a consistent and decimal-based system for measuring length, mass, volume, and other quantities.

What is a Parsec?

A parsec is a unit of length used in astronomy to measure vast distances between celestial objects. The term "parsec" is derived from the words "parallax" and "second," which refer to the method used to calculate this unit. Specifically, a parsec is defined as the distance at which an object would have a parallax angle of one arcsecond when observed from opposite ends of Earth's orbit around the Sun.

To understand the concept of a parsec, it is important to grasp the idea of parallax. Parallax is the apparent shift in the position of an object when viewed from different vantage points. In the case of astronomy, scientists use the Earth's orbit as a baseline to measure the parallax of distant stars. By observing a star from opposite ends of Earth's orbit, astronomers can calculate the angle of parallax and subsequently determine the star's distance.

 

Decimeters to Parsecs table

Starting value
Increment
Accuracy
Decimeters
Parsecs
0dm
0.00000pc
1dm
0.00000pc
2dm
0.00000pc
3dm
0.00000pc
4dm
0.00000pc
5dm
0.00000pc
6dm
0.00000pc
7dm
0.00000pc
8dm
0.00000pc
9dm
0.00000pc
10dm
0.00000pc
11dm
0.00000pc
12dm
0.00000pc
13dm
0.00000pc
14dm
0.00000pc
15dm
0.00000pc
16dm
0.00000pc
17dm
0.00000pc
18dm
0.00000pc
19dm
0.00000pc
20dm
0.00000pc
21dm
0.00000pc
22dm
0.00000pc
23dm
0.00000pc
24dm
0.00000pc
25dm
0.00000pc
26dm
0.00000pc
27dm
0.00000pc
28dm
0.00000pc
29dm
0.00000pc
30dm
0.00000pc
31dm
0.00000pc
32dm
0.00000pc
33dm
0.00000pc
34dm
0.00000pc
35dm
0.00000pc
36dm
0.00000pc
37dm
0.00000pc
38dm
0.00000pc
39dm
0.00000pc
40dm
0.00000pc
41dm
0.00000pc
42dm
0.00000pc
43dm
0.00000pc
44dm
0.00000pc
45dm
0.00000pc
46dm
0.00000pc
47dm
0.00000pc
48dm
0.00000pc
49dm
0.00000pc
50dm
0.00000pc
51dm
0.00000pc
52dm
0.00000pc
53dm
0.00000pc
54dm
0.00000pc
55dm
0.00000pc
56dm
0.00000pc
57dm
0.00000pc
58dm
0.00000pc
59dm
0.00000pc
60dm
0.00000pc
61dm
0.00000pc
62dm
0.00000pc
63dm
0.00000pc
64dm
0.00000pc
65dm
0.00000pc
66dm
0.00000pc
67dm
0.00000pc
68dm
0.00000pc
69dm
0.00000pc
70dm
0.00000pc
71dm
0.00000pc
72dm
0.00000pc
73dm
0.00000pc
74dm
0.00000pc
75dm
0.00000pc
76dm
0.00000pc
77dm
0.00000pc
78dm
0.00000pc
79dm
0.00000pc
;