Celestial angles terminology: the angle between the direction of a star and Earth’s rotation axis (i.e., the pole–star angular separation) is called what?

Introduction / Context:
Describing positions on the celestial sphere uses declination, right ascension, and related complements. Understanding the complement angles is key to interpreting star positions relative to the pole.

Given Data / Assumptions:

• Earth’s rotation axis defines the celestial poles.
• The angular separation between a star and the pole is sought.

Concept / Approach:
Declination (δ) is measured from the celestial equator. Its complement with respect to 90 degrees is the co-declination (90° − δ), which equals the angular distance of the star from the nearest pole (pole distance).

Step-by-Step Solution:
Define declination δ.Compute co-declination = 90° − δ.Interpret as the angle between star direction and Earth’s axis (pole distance).

Verification / Alternative check:
Star charts label pole distance as 90° − δ, confirming that co-declination is the required quantity.

Why Other Options Are Wrong:

• Co-latitude refers to 90° − φ (observer’s latitude), not a stellar coordinate.
• Declination itself is measured from the equator, not from the axis.
• Latitude pertains to Earth locations, not stellar angular distances.

Common Pitfalls:

• Confusing co-latitude with co-declination due to similar naming.

Final Answer:
co-declination