Definition:North Polar Distance

Definition

Consider the celestial sphere $C$ with observer $O$.

Let $X$ be a point on $C$.

Let $X$ have declination of $\delta$.

The north polar distance of $X$, denoted $\operatorname {N.P.D.} x$, is defined as:

$\operatorname {N.P.D.} x = 90 \degrees - \delta$

That is, the north polar distance of $X$ length of the arc from the north celestial pole $P$ along the vertical circle through $X$.

Also known as

North polar distance is also known as codeclination.

Also see

• Definition:Declination

• Results about north polar distance can be found here.

Sources

• 1976: W.M. Smart: Textbook on Spherical Astronomy (6th ed.) ... (previous) ... (next): Chapter $\text {II}$. The Celestial Sphere: $19$. Declination and hour angle.
• 1998: David Nelson: The Penguin Dictionary of Mathematics (2nd ed.) ... (previous) ... (next): codeclination
• 1998: David Nelson: The Penguin Dictionary of Mathematics (2nd ed.) ... (previous) ... (next): declination (dec)
• 1998: David Nelson: The Penguin Dictionary of Mathematics (2nd ed.) ... (previous) ... (next): equatorial coordinate system
• 2008: David Nelson: The Penguin Dictionary of Mathematics (4th ed.) ... (previous) ... (next): codeclination
• 2008: David Nelson: The Penguin Dictionary of Mathematics (4th ed.) ... (previous) ... (next): declination (dec)
• 2008: David Nelson: The Penguin Dictionary of Mathematics (4th ed.) ... (previous) ... (next): equatorial coordinate system