Celestial Sphere, Poles and Equator
Celestial Sphere, Poles and Equator
The Celestial Sphere
- The Celestial Sphere is an imaginary sphere with the observer at the centre.
- All objects in the observer’s sky can be thought of as located on the inside surface of the celestial sphere.
- The celestial sphere is a useful tool for observing celestial objects, despite it not being a representation of the actual scale of the universe.
Celestial Poles and Equator
- The North Celestial Pole and the South Celestial Pole are the points in the sky directly above Earth’s North and South Poles, respectively.
- The celestial poles are the projection of Earth’s axis of rotation onto the celestial sphere.
- The Celestial Equator is an imaginary line above the Earth’s equator. It divides the celestial sphere into the northern and southern hemispheres.
- The celestial equator is perpendicular to the celestial poles.
Movement of Celestial Objects
- Celestial objects appear to move across the sky because of the Earth’s rotation, which is from west to east.
- The paths of celestial objects depend on the observer’s latitude.
- For an observer at the poles, celestial objects move horizontally, parallel to the horizon.
- For an observer at the equator, celestial objects rise perpendicularly from the horizon and set straight down.
Ecliptic and Zodiac
- The Ecliptic is the apparent path the Sun follows across the celestial sphere over the course of a year.
- The ecliptic is tilted at an angle of about 23.5° to the celestial equator due to the tilt of Earth’s axis of rotation.
- The zodiac is a belt of the celestial sphere extending about 8° either side of the ecliptic that includes the apparent paths of the Sun, Moon, and the planets excluding Pluto.
- The zodiac is divided into twelve equal parts, each named after the constellation that once appeared in its section.
Declination and Right Ascension
- Declination and Right Ascension are the celestial equivalent of latitude and longitude on Earth.
- Declination is measured in degrees, from +90° (north celestial pole) to -90° (south celestial pole).
- Right ascension is measured in time (hours, minutes, and seconds), from 0h to 24h. One hour of right ascension corresponds to 15°.
- The zero point of right ascension is the position of the Sun at the vernal equinox, also known as the First Point of Aries.