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What Is Local Mean Time?

Local Mean Time (LMT) is a type of solar time, a timekeeping method using the Sun's movements across the sky. It is based on the average length of a solar day.

A sundial with the Sun casting a shadow.

Sundials show true solar time.

Sundials show True Solar Time. Because the Sun's movement across the sky is not constant, this method is not very exact. Mean Solar Time and LMT are based on the speed of a theoretical, average Sun.

©iStockphoto.com/mbastoni

In order to explain Local Mean Time, we first have to understand a few other terms:

  1. Apparent Solar Time / True Solar Time
    A sundial shows the true or apparent solar time. Because the Earth's rotation is not constant, solar days vary slightly in length. This means that the speed of true solar time is not constant.
  2. Mean Solar Time is based on the length of a mean or average solar day, which is 24 hours long. It moves at a constant speed.

Local Mean Time is the Mean Solar Time for a specific location on Earth. It is the same for all locations that share the same longitude.

Local Mean Time Today

While Local Mean Time does not directly determine civil time these days, it is still used to make sure our clocks follow the Sun as closely as possible. UT1, a version of Universal Time, is the Local Mean Time at the prime meridian in Greenwich, London. It is one of the components used to calculate Coordinated Universal Time (UTC), the time scale used to determine local times worldwide.

LMT is also used by astronomers around the world to time their observations.

LMT as International Time Standard

Until the 1960s, the Local Mean Time in Greenwich – Greenwich Mean Time (GMT) – was used as the world's time standard and the basis for civil time worldwide. It was replaced by UTC in 1967.

What is the difference between GMT and UTC today?

Different Time from City to City

Local Mean Time was officially used as civil time in many countries during the 19th century. Each city had a different local time defined by its longitude, the difference amounting to 4 minutes per degree longtitude. This equals a distance of 50 miles or 81 kilometers on New York's latitude.

As transport and communication methods evolved, this arrangement became increasingly impractical, so it was eventually replaced by standard time and time zones.

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Topics: Timekeeping, Astronomy, Sun, History

Coordinated Universal Time (UTC)

02:14:31

Thursday, October 24, 2019

UTC is the common time standard across the world

More about UTC
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