An imaginary body which is assumed to travel around the equinoctial at a constant rate, completing one orbit in the same time that the earth takes to complete one orbit around the ecliptic. Because of the elliptical shape of the earth’s orbit, the apparent angular velocity of the sun we see is not constant; hence, the days as indicated by the apparent travel of the true or apparent sun are not of uniform length. To make the solar day of uniform length, astronomers have invented the mean sun, a fictitious body imagined to move at a uniform rate along the celestial equator, making a complete circuit from west to east in one year.