Earth
Earth's orbit
Once round the Sun every 365.3 days, on an ellipse drawn here from the ephemeris rather than from a formula.
- Orbital period
- 365.3
- days for one lap
- Eccentricity
- 0.0167
- 0 would be a circle
- Semi-major axis
- 1.000
- AU · the orbit's average radius
- Speed now
- 29.84
- km/s, from the ephemeris
What is worth knowing about it
Earth is closest to the Sun in early January and furthest in early July — the opposite of what most northern-hemisphere readers expect. Seasons come from axial tilt, not from this three per cent swing in distance.
The shape of it
Earth does not travel a circle. It comes as close as 0.983 AU (0.147 billion km) and goes as far as 1.017 AU (0.152 billion km) — aphelion is 1.03 times further out than perihelion, a swing of 4,996,217 km. At 0.0167 its orbit is very nearly a circle — draw it to scale and the difference from one would be thinner than the line.
Because the Sun sits at a focus rather than the centre, Earth does not move at a constant speed either. It runs fastest when it is closest and slowest when it is furthest, sweeping equal areas in equal times — which is Kepler's second law, and is visible in the diagram above as the uneven spacing of a constant time step.
Where it is now
Today Earth is 0.999 AU from the Sun, 46% of the way from perihelion to aphelion, travelling at 29.84 km/s. It reaches perihelion on 3 January 2027 at 0.983 AU.
Common questions
- How long is Earth's orbit?
- Earth takes 365.3 days to go once round the Sun. It is travelling at 29.84 km/s at the moment — a speed that changes through the orbit, fastest at perihelion and slowest at aphelion.
- What shape is Earth's orbit?
- An ellipse with the Sun at one focus, not at the centre. Its eccentricity is 0.0167, derived here from the perihelion and aphelion distances rather than quoted: 0.983 AU at closest and 1.017 AU at furthest, a difference of 4,996,217 km.
- Where is Earth in its orbit now?
- 0.999 AU from the Sun — 0.149 billion km — which is 46% of the way from its closest point to its furthest. It next reaches perihelion on 3 January 2027.
Positions from VSOP87 via Astronomy Engine, accurate to within one arcminute. The orbit above is traced by sampling a full period rather than drawn from elements, so the tilt and the off-centre Sun are the real ones. See Earth’s distance from the Sun, Earth right now, or watch the whole system move in the live simulation.