In celestial coordinates, the angular distance north or south of the celestial equator is called the ______.

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Multiple Choice

In celestial coordinates, the angular distance north or south of the celestial equator is called the ______.

Explanation:
Declination is the angular distance north or south of the celestial equator in the celestial coordinate system. It mirrors latitude on the sky, measured in degrees with 0° at the celestial equator, +90° at the north celestial pole, and -90° at the south celestial pole. The celestial equator is the projection of Earth’s equator onto the celestial sphere. Altitude is the height above the horizon (observer-dependent), and longitude (in celestial terms) corresponds to right ascension along the equatorial plane, not north–south position. So the term for this north-south distance is declination.

Declination is the angular distance north or south of the celestial equator in the celestial coordinate system. It mirrors latitude on the sky, measured in degrees with 0° at the celestial equator, +90° at the north celestial pole, and -90° at the south celestial pole. The celestial equator is the projection of Earth’s equator onto the celestial sphere. Altitude is the height above the horizon (observer-dependent), and longitude (in celestial terms) corresponds to right ascension along the equatorial plane, not north–south position. So the term for this north-south distance is declination.

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