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There is more than one type of Nautical Mile

There are a few different types of Nautical Mile. On this site we have conversions for US Nautical miles, UK Nautical miles and International Nautical miles. Please either select the appropriate unit on the selection above of click the required unit in the links below:

US Nautical miles

UK Nautical miles

International Nautical miles

What is a nautical mile?

A nautical mile is a unit of measurement used in navigation and maritime travel. It is defined as one minute of latitude along any meridian, making it a unit of distance that varies slightly depending on the Earth's shape. The nautical mile is commonly used in aviation and shipping industries due to its convenience in measuring distances over water.

Historically, the nautical mile was derived from the circumference of the Earth, with one minute of latitude being divided into 60 equal parts to create the nautical mile. This unit of measurement is particularly useful for sailors and pilots as it allows for easy calculation of distances based on the Earth's coordinates. The nautical mile is also used in international treaties and agreements related to maritime boundaries and navigation regulations.

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.