Celestial latitude is an astronomical term used to define the north-south position of a celestial object in the night sky. It refers to the distance of an object from the celestial equator, which is equivalent to the Earth's equator projected into the sky. Some common synonyms for this term include ecliptic latitude, declination, and celestial coordinates. These terms are all used interchangeably to describe the celestial location of an object and help astronomers identify its position relative to other objects in the night sky. Understanding celestial latitude is essential for astronomers and stargazers alike, as it allows them to locate and track objects within the vast expanse of the cosmos.