Jump to content

Navigational triangle

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by 27.252.229.190 (talk) at 03:00, 22 January 2022. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The navigational triangle or PZX triangle is a spherical triangle used in astronavigation to determine the observer's position in the world.[1] It is composed of three reference points on the celestial sphere:

  • P is the Celestial Pole (either North or South). It is a fixed point.
  • Z is the observer's zenith, or their position on the celestial sphere.
  • X is the position of a celestial body, such as the sun, moon, a planet, or a star.

The position of Z or X is described via its declination—the angular distance north or south of the equator (corresponding to its latitude)—and the hour angle—the angle between its meridian and the Greenwich meridian (corresponding to its longitude). If the observer knows the angles subtended by P, Z, and X, they can calculate their position in the world. By measuring the angle of the celestial body in the sky, the observer can get the local hour angle (LHA) of X, which is the angle subtended at P between Z and X (the angle between the Z and X's meridians) and calculate the longitude by subtracting from the Greenwich hour angle of the celestial body. Finding the latitude requires measuring the vertical angle (altitude) of X from the horizon using a sextant, the declination of X from a reference book, and a set of sight reduction Tables.

The sun, moon, and planets move relative to the celestial sphere, but the only the stars' hour angles change with the hypothetical rotation of the earth, completing a full 360 degrees every solar day.

References

  1. ^ Bowditch, Nathaniel (1802). The American Practical Navigator: An Epitome of Navigation (PDF) (1995 ed.). Bethesda Maryland: National Imagery and Mapping Agency. p. 256.