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Perihelion, Aphelion and the Solstices

The Earth is closest to the Sun – at its Perihelion – about 2 weeks after the December Solstice and farthest from the Sun – at its Aphelion – about 2 weeks after the June Solstice.

Illustration image

Earth's orbit around the Sun changes.

Earth is farthest from the Sun on its orbit when it is summer in the Northern Hemisphere

Changing Elliptical Orbit

Earth orbits the Sun in an elliptical path, which means that there is 1 point of the path when the Sun is at its closest to the Earth and 1 point when it is furthest away.

Orbit Changes Shape

The shape of this path varies due to gravitational influences of other planetary objects, particularly the Moon.

Approximately every 100,000 years, Earth's orbital path changes from being nearly circular to elliptical. The difference of the Earth’s orbital shape from a perfect circle is known as its eccentricity. An eccentricity value of 0 is a circular orbit, while values between 0 and 1 describe an elliptical orbit.

Perihelion in Fullerton, California, USA is on
Saturday, January 4, 2020 at 11:47 pm PST (Change city)

Distance from the Sun's center to Earth's center will be 147,091,144 km (91,398,199 mi)

YearPerihelionDistanceAphelionDistance
2019January 2, 2019 9:19 pm91,403,554 miJuly 4, 2019 3:10 pm94,513,221 mi
2020January 4, 2020 11:47 pm91,398,199 miJuly 4, 2020 4:34 am94,507,635 mi
2021January 2, 2021 5:50 am91,399,454 miJuly 5, 2021 3:27 pm94,510,886 mi
2022January 3, 2022 10:52 pm91,406,842 miJuly 4, 2022 12:10 am94,509,598 mi
2023January 4, 2023 8:17 am91,403,034 miJuly 6, 2023 1:06 pm94,506,364 mi
* All aphelion/perihelion times are in local Fullerton time.

Earth's Perihelion and Aphelion

The Earth is closest to the Sun, or at the perihelion, about 2 weeks after the December Solstice, when it is winter in the Northern Hemisphere. Conversely, the Earth is farthest away from the Sun, at the aphelion point, 2 weeks after the June Solstice, when the Northern Hemisphere is enjoying warm summer months.

Is the Timing a Coincidence?

The dates when Earth reaches the extreme points on its orbit are not fixed because of the variations in its eccentricity. In 1246, the December Solstice was on the same day as the Earth reached its Perihelion. Since then, the Perihelion and Aphelion dates have drifted by a day every 58 years. In the short-term, the dates can vary up to 2 days from one year to another.

Mathematicians and astronomers estimate that in the year 6430, over 4000 years from now, the timing of the Perihelion and the March Equinox will coincide.

Perigee and Apogee

Like the Earth's orbit around the Sun, the Moon's path around the Earth is elliptical. The point in the Moon's orbit that is closest to the Earth is called the Perigee and the point farthest from the Earth is known as the Apogee. The terms are also sometimes used interchangeably with the Earth's Perihelion and Aphelion.

Did You Know...

...that the words Perihelion and Aphelion come from ancient Greek, where peri means close, apo means far, and helios means the Sun? They are used in astronomy to refer to the closest and farthest points of the orbits of any object revolving around the Sun. Together, they are called apsides - the points of least or greatest distance of a celestial object in orbit around another astronomical body.

Topics: Astronomy, Solstice, Sun, Equinox


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