ਪਰ੍ਸੇਕ ਰੂਪਾਂਤਰਣ ਲਈ ਫੀਟ

ਪਰ੍ਸੇਕ ਰੂਪਾਂਤਰਣ ਲਈ ਫੀਟ ਕਨਵਰਟਰ ਕੈਲਕੁਲੇਟਰ

ਫੀਟ ਨੂੰ ਪਰ੍ਸੇਕ (ਇਕਾਈਆਂ ਬਦਲੋ)

1ft = 0pc

ਨੋਟ: ਤੁਸੀਂ ਇਸ ਜਵਾਬ ਦੀ ਸਹੀਤਾ ਨੂੰ ਵਧਾ ਜਾਂ ਘਟਾ ਸਕਦੇ ਹੋ, ਜਦੋਂ ਤੁਸੀਂ ਨਤੀਜੇ ਤੋਂ ਉੱਪਰ ਵਾਲੇ ਚੋਣਾਂ ਤੋਂ ਮਹੱਤਵਪੂਰਨ ਅੰਕਾਂ ਦੀ ਗਿਣਤੀ ਕਰਦੇ ਹੋ।

ਫੀਟ ਤੋਂ ਪਰ੍ਸੇਕ ਕਨਵਰਟ ਸੂਤਰ

ਪਰ੍ਸੇਕ = ਫੀਟ / 1.0123612216812E+17

1 ਫੀਟ ਤੋਂ ਪਰ੍ਸੇਕ ਗਣਨਾ

ਪਰ੍ਸੇਕ = ਫੀਟ / 1.0123612216812E+17

ਪਰ੍ਸੇਕ = 1 / 1.0123612216812E+17

ਪਰ੍ਸੇਕ = 0

What is a foot?

A measurement foot, commonly referred to as a foot, is a unit of length in the imperial system of measurement. It is primarily used in the United States and a few other countries that have not adopted the metric system. The foot is defined as 12 inches, and it is a constituent of larger units such as yards, and miles.

The foot has a long history and has been used as a unit of measurement for thousands of years. It is believed to have originated from the length of a human foot, as it was a convenient and easily reproducible reference point. Over time, the foot has been standardized to ensure consistency in measurements.

In modern usage, the foot is commonly used to measure height, distance, and length in various applications. For example, it is used in construction and architecture to measure the dimensions of buildings and structures. It is also used in sports to measure the length of a field or track. While the metric system is widely used around the world, the foot remains an important unit of measurement in certain industries and regions.

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.

 

ਫੀਟ ਤੋਂ ਪਰ੍ਸੇਕ ਸਾਰਣੀ

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