**Sidereal Time. **Even though Sidereal Time is a more accurate measure of the Earth’s rotation, we normally use Solar Time for time-keeping because the Sidereal Day is not a practical unit for us to use. On the other hand, Sidereal Time is important because it enables us to find the hour angle of a star and is therefore essential if we wish to use stars for navigation.

**Solar Day. **A Solar Day is the time interval between two successive transits by the Sun across the meridian directly opposite that of the observer; that is the 24 hour interval from midnight to the following midnight at the observer’s meridian.

**Sidereal Day.** A Sidereal Day is the interval between two successive transits of a star across the observer’s meridian. A Sidereal Day is shorter that a Solar Day by approximately 4 minutes and is a true measure of the period of rotation of the Earth. For convenience, the First Point of Aries is used to mark the Sidereal Day instead of an actual star. The Sidereal Day is therefore defined as the interval between two successive transits of the First Point of Aries across the same meridian. The Sidereal Day begins when the First Point of Aries crosses the meridian.

**Local Sidereal Time** is equal to the Local Hour Angle of the First Point of Aries. This is abbreviated to **Local Sidereal Time = LHA of Aries. **

**First Point of Aries.** In astronomy, we need a celestial coordinate systems for fixing the positions of all celestial bodies in the celestial sphere. To this end, we express a celestial body’s position in the celestial sphere in relation to its angular distances from the Celestial Equator and the celestial meridian that passes through the ‘First Point of Aries’. This is similar to the way in which we use latitude and longitude to identify a position on the Earth’s surface in relation to its angular distances from the Equator and the Greenwich Meridian. The First Point of Aries is usually represented by the ‘ram’s horn’ symbol shown below:

Just as the Greenwich meridian has been arbitrarily chosen as the zero point for measuring longitude on the surface of the Earth, the first point of Aries has been chosen as the zero point in the celestial sphere. It is the point at which the Sun crosses the celestial equator moving from south to north (at the vernal Equinox in other words).

So the First Point of Aries is the starting point of the Solar Year and it is also the starting point of the Sidereal Day.

The confusing thing about the First Point of Aries is that, although it was in the constellation of Aries when it was chosen by the ancient astronomers, due to precession it now lies in Pisces.

**Hour angles explained:**

**Local Hour Angle (LHA). **In astro navigation, we need to know the position of a celestial body relative to our own position. In the diagram below:

LHA is the angle BNU on the Earth’s surface which corresponds to the angle ZPX in the Celestial sphere. In other words, it is the angle between the meridian of the observer and the meridian of the geographical position of the celestial body (GP).

Due to the Earth’s rotation, the Sun moves through 15^{o }of longitude in 1 hour and it moves through 15 minutes of arc in 1 minute of time. So the angle ZPX can be measured in terms of time and for this reason, it is known as the Local Hour Angle.

LHA is measured westwards from the observer’s meridian and can be expressed in terms of either angular distance or time. For example, at noon (GMT) the Sun’s GP will be on the Greenwich Meridian (0^{o}). If the time at an observer’s position is 2 hours and 3 minutes after noon, then the angular distance between the observer’s meridian of longitude and the Greenwich Meridian must be (2 x15^{o} ) + (3x 15’) = 30^{o} 45’. Because it is after noon at the observer’s position, the longitude of that position must be to the East of the Greenwich Meridian since the Earth rotates from West to East. Therefore the observer’s longitude must be 30^{o }45’ East and since LHA is measured westwards from the observer’s meridian, the LHA must also be 30^{o} 45’. However, it should be noted that as the Earth continues to rotate eastwards, the GP of the Sun will continue to move westwards so the LHA at the observer’s position will be continually changing.

**Greenwich Hour Angle (GHA**). As discussed above, the angle between two meridians of Longitude can be expressed as an hour angle. The hour angle between the Greenwich Meridian and the meridian of a celestial body is known as the Greenwich Hour Angle.

The Local Hour Angle between an observer’s position and the geographical position of a celestial body can be found by combining the observer’s longitude with the GHA.

**Sidereal Hour Angle (SHA**). SHA is the angle between the meridian running through the First Point of Aries and the meridian running through the celestial body measured westwards from Aries.** **The Nautical Almanac does not list the GHA of the stars; it lists their sidereal hour angle (SHA) instead. So, the GHA of a star has to be calculated from the GHA of Aries. Therefore, the SHA of the star must be added to the GHA of Aries in order to obtain the GHA of the star.

Relevant links:

Time Difference Between Meridians of Longitude

Find Your Longitude in a Survival Situation

A comprehensive exposition of this topic can be found in the book Astro Navigation Demystified.

www.astronavigationdemystified.com

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