Earth Orbital Eccentricity

e⊕=0.0167086 —e_\oplus = 0.0167086\ \text{—}
Value0.0167086 —
StatusConventional / typical value
SourceJPL Keplerian elements, epoch J2000 (secularly variable)
CategoriesAstronomical
Earth Orbital Eccentricity in every dimensionless unit
part per trillion16,708,600,000 ppt
part per billion16,708,600 ppb
part per million16,708.6 ppm
per cent mille1,670.86 pcm
basis point167.086 bp
per mille16.7086 per mille
percent1.67086 %
ratio0.0167086 —

Learning zone

Kepler needed Tycho Brahe's Mars observations, accurate to two arcminutes, to detect that orbits are ellipses at all; with Earth's eccentricity of only 0.0167, the orbit drawn to scale is indistinguishable from a circle by eye — the Sun simply sits 2.5 million km off centre. The consequence is not the seasons, which come from axial tilt, but a 6.8 per cent swing in incoming sunlight between January perihelion and July aphelion, currently mild for the northern hemisphere's summer.

Over long times the value is anything but constant. Jupiter's and Saturn's perturbations drive it between about 0.0034 and 0.058 on roughly 100 000- and 400 000-year cycles, and Milanković showed that this beat, combined with the tilt and precession cycles, paces the ice ages — a prediction confirmed in the 1970s by oxygen-isotope records in deep-sea cores.