 Viewed from an object with a perfectly circular orbit and no axial tilt, the Sun would always appear at the same point in the sky at the same time of day throughout the year and the analemma would be a dot.For an object with a circular orbit but significant axial tilt, the analemma would be a figure of eight with northern and southern lobes equal in size.For an object with an eccentric orbit but no axial tilt, the analemma would be a straight east–west line along the celestial equator.