Earlier today, the Earth was at the point in its elliptical orbit closest to the Sun – the perihelion.
The featured image is the Sun at around the time of today’s perihelion as viewed by NASA’s Solar Dynamics Observatory.
The Earth’s orbit is only very slightly elliptical. Its semi-major axis (half the long axis of the ellipse) is 149.6 million kilometres, but as its eccentricity is only 0.01671123, the semi-minor axis is only about 21,000 km smaller. It’s very hard to spot that this is an ellipse rather than a perfect circle.
The Sun lies at one focus of this elliptical orbit, offset 2.5 million kilometres from the centre*. So, on one side of its orbit (at perihelion), the Earth is 5 million kilometres closer to the Sun than on the opposite side (aphelion).
I thought I’d try illustrating this with a properly scaled drawing.
* The separation of focus and centre is given by the product of the eccentricity and the semi-major axis.