An **azimuth** (/ˈæzɪməθ/) (from Arabic "السَّمْت" *as-sumūt*, meaning "the directions") is an angular measurement in a spherical coordinate system. The vector from an observer (origin) to a point of interest is projected perpendicularly onto a reference plane; the angle between the projected vector and a reference vector on the reference plane is called the azimuth.

## Contents

- Navigation
- Cartographical azimuth
- Calculating coordinates
- Calculating azimuth
- Mapping
- Astronomy
- Right ascension
- Horizontal coordinate
- Polar coordinate
- Other uses of the word
- Etymology of the word
- References

An example is the position of a star in the sky. The star is the point of interest, the reference plane is the horizon or the surface of the sea, and the reference vector points north. The azimuth is the angle between the north vector and the perpendicular projection of the star down onto the horizon.

Azimuth is usually measured in degrees (°). The concept is used in navigation, astronomy, engineering, mapping, mining and artillery.

## Navigation

In land navigation, azimuth is usually denoted alpha, *α*, and defined as a horizontal angle measured clockwise from a north base line or *meridian*. *Azimuth* has also been more generally defined as a horizontal angle measured clockwise from any fixed reference plane or easily established base direction line.

Today, the reference plane for an azimuth is typically true north, measured as a 0° azimuth, though other angular units (grad, mil) can be used. Moving clockwise on a 360 degree circle, east has azimuth 90°, south 180°, and west 270°. There are exceptions: some navigation systems use south as the reference vector. Any direction can be the reference vector, as long as it is clearly defined.

Quite commonly, azimuths or compass bearings are stated in a system in which either north or south can be the zero, and the angle may be measured clockwise or anticlockwise from the zero. For example, a bearing might be described as "(from) south, (turn) thirty degrees (toward the) east" (the words in brackets are usually omitted), abbreviated "S30°E", which is the bearing 30 degrees in the eastward direction from south, i.e. the bearing 150 degrees clockwise from north. The reference direction, stated first, is always north or south, and the turning direction, stated last, is east or west. The directions are chosen so that the angle, stated between them, is positive, between zero and 90 degrees. If the bearing happens to be exactly in the direction of one of the cardinal points, a different notation, e.g. "due east", is used instead.

## Cartographical azimuth

The cartographical azimuth (in decimal degrees) can be calculated when the coordinates of 2 points are known in a flat plane (cartographical coordinates):

Remark that the reference axes are swapped relative to the (counterclockwise) mathematical polar coordinate system and that the azimuth is clockwise relative to the north. This is the reason why the X and Y axis in the above formula are swapped. If the azimuth becomes negative, one can always add 360°.

The formula in radians would be slightly easier:

## Calculating coordinates

When the coordinates (*X*_{1}, *Y*_{1}) of one point, the distance *L*, and the azimuth *α* to another point (*X*_{2}, *Y*_{2}) are known, one can calculate its coordinates:

This is typically used in triangulation.

## Calculating azimuth

We are standing at latitude *φ*_{1}, longitude zero; we want to find the azimuth from our viewpoint to Point 2 at latitude *φ*_{2}, longitude *L* (positive eastward). We can get a fair approximation by assuming the Earth is a sphere, in which case the azimuth *α* is given by

A better approximation assumes the Earth is a slightly-squashed sphere (an *oblate spheroid*); *azimuth* then has at least two very slightly different meanings. *Normal-section azimuth* is the angle measured at our viewpoint by a theodolite whose axis is perpendicular to the surface of the spheroid; *geodetic azimuth* is the angle between north and the *geodesic*; that is, the shortest path on the surface of the spheroid from our viewpoint to Point 2. The difference is usually immeasurably small; if Point 2 is not more than 100 km away, the difference will not exceed 0.03 arc second.

Various websites will calculate geodetic azimuth; e.g., GeoScience Australia site. Formulas for calculating geodetic azimuth are linked in the distance article.

Normal-section azimuth is simpler to calculate; Bomford says Cunningham's formula is exact for any distance. If *f* is the flattening for the chosen spheroid (e.g., ^{1}⁄_{7002298257223563000♠298.257223563} for WGS84) then

If *φ*_{1} = 0 then

To calculate the azimuth of the sun or a star given its declination and hour angle at our location, we modify the formula for a spherical earth. Replace *φ*_{2} with declination and longitude difference with hour angle, and change the sign (since the hour angle is positive westward instead of east).

## Mapping

There is a wide variety of azimuthal map projections. They all have the property that directions (the azimuths) from a central point are preserved. Some navigation systems use south as the reference plane. However, any direction can serve as the plane of reference, as long as it is clearly defined for everyone using that system.

## Astronomy

Used in celestial navigation, an *azimuth* is the direction of a celestial body from the observer. In astronomy, an *azimuth* is sometimes referred to as a bearing. In modern astronomy azimuth is nearly always measured from the north. (The article on coordinate systems, for example, uses a convention measuring from the south.) In former times, it was common to refer to azimuth from the south, as it was then zero at the same time that the hour angle of a star was zero. This assumes, however, that the star (upper) culminates in the south, which is only true if the star's declination is less than (i.e. further south than) the observer's latitude.

## Right ascension

If, instead of measuring from and along the horizon, the angles are measured from and along the celestial equator, the angles are called right ascension if referenced to the Vernal Equinox, or hour angle if referenced to the celestial meridian.

## Horizontal coordinate

In the horizontal coordinate system, used in celestial navigation and satellite dish installation, azimuth is one of the two coordinates. The other is altitude, sometimes called elevation above the horizon. See also: Sat finder.

## Polar coordinate

In mathematics, the azimuth angle of a point in cylindrical coordinates or spherical coordinates is the anticlockwise angle between the positive *x*-axis and the projection of the vector onto the *xy*-plane. The angle is the same as an angle in polar coordinates of the component of the vector in the *xy*-plane and is normally measured in radians rather than degrees. As well as measuring the angle differently, in mathematical applications theta, *θ*, is very often used to represent the azimuth rather than the representation of symbol phi *φ*.

## Other uses of the word

For magnetic tape drives, *azimuth* refers to the angle between the tape head(s) and tape.

In sound localization experiments and literature, the *azimuth* refers to the angle the sound source makes compared to the imaginary straight line that is drawn from within the head through the area between the eyes.

An azimuth thruster in shipbuilding is a propeller that can be rotated horizontally.

## Etymology of the word

The word azimuth is in all European languages today. It originates from medieval Arabic *al-sumūt*, pronounced *as-sumūt* in Arabic, meaning "the directions" (plural of Arabic *al-samt* = "the direction"). The Arabic word entered late medieval Latin in an astronomy context and in particular in the use of the Arabic version of the Astrolabe astronomy instrument. The word's first record in English is in the 1390s in *Treatise on the Astrolabe* by Geoffrey Chaucer. The first known record in any Western language is in Spanish in the 1270s in an astronomy book that was largely derived from Arabic sources, the *Libros del saber de astronomía* commissioned by King Alfonso X of Castile.