Earth at Perihelion

StarDate: January 4, 2012

You are missing some Flash content that should appear here! Perhaps your browser cannot display it, or maybe it did not initialize correctly.

You are missing some Flash content that should appear here! Perhaps your browser cannot display it, or maybe it did not initialize correctly.



Break out the umbrellas, the swimsuits, and the sunscreen — Sun and Earth are closest for the entire year today, so we’re getting a little extra warmth from our favorite star.

Earth is at a point in its orbit called perihelion — a word that means “closest to the Sun.” We’re about a million-and-a-half miles closer to the Sun than average.

And as you might expect, we get a little extra solar energy — about three percent more than we average over the course of a year.

At this time of year, though, the Sun’s rays are falling most directly on the southern hemisphere, so it gets the bulk of the solar energy. But the oceans and atmosphere absorb that extra heat and transport it around the globe, keeping the planet’s overall climate in balance.

The distance to the Sun changes because Earth’s orbit is an ellipse — like a slightly stretched-out circle. In fact, all the planets follow elliptical orbits, but the “stretching” varies from planet to planet.

Venus has the most nearly circular orbit, so Venus’s distance from the Sun varies by less than one percent. Mercury, on the other hand, has the most lopsided orbit — its distance from the Sun varies by a fifth. So daytime temperatures on the airless planet vary by hundreds of degrees — all thanks to the changing distance to the Sun.

Here on Earth, the distance to the Sun will be increasing for months — until we reach our farthest point in early July.

 

Script by Damond Benningfield, Copyright 2011

 

For more skywatching tips, astronomy news, and much more, read StarDate magazine.

The one constant in the Universe: StarDate magazine

FacebookTwitterYouTube

©2014 The University of Texas McDonald Observatory