Astronomy Essentials

Ecliptic is the sun’s path in our sky

Ecliptic depicted by a blue ball orbiting a yellow sun. An arrow points out from the orbit to a flat red oval against the stars.
Animated depiction of Earth (the blue ball) orbiting the sun (the yellow ball), showing the projection of Earth-sun plane – the ecliptic – onto the background stars. Image via Tfr000/ Wikimedia Commons.

Ecliptic aka sun’s path

Maybe you’ve noticed that the moon and planets follow the sun’s path across your sky? Unless you live in the high Arctic or Antarctic, you see the sun arc across your sky each day from east to west. The moon follows the sun’s path. And so do the major planets in our solar system. This imaginary track across our sky is called the ecliptic. Technically speaking, it’s a projection of the plane of Earth’s orbit around the sun, traced onto our sky. Practically speaking, the ecliptic forms a great circle around the sky and is a useful tool for stargazers.

Why do the moon and planets follow the sun’s path? It’s mainly because, long ago – before there was a solar system as we know it today – there was a vast cloud of gas and dust in space. This cloud was spinning, and, as it spun, it flattened out. Our sun formed in the center of this cloud. The major planets, including Earth, and most other solar system objects formed in the flat disk surrounding the sun. The ecliptic is this flat disk of planets in our sun’s family – our solar system – translated onto our sky.

Planets follow the ecliptic

So the major planets – and many of the minor planets, aka asteroids – orbit the sun in more or less the same plane. We can speak of this plane as defined by Earth’s orbit around the sun: the ecliptic.

If we could watch the solar system from far above the Earth’s north pole, we’d see the planets, moons, asteroids, and some of the comets (but not all of them) rushing around the sun counterclockwise in this plane, like marbles rolling around a flat dish. Actually, the major planets are more within the dish than on it. They’re within the plane of the ecliptic, more or less.

They retain the outline of the original cloud in space from which they were born, and their movement around the sun is an echo of the original spin of the cloud.

Flat plane of the solar system, with Mercury, Venus and Earth orbits.
The ecliptic is defined by the plane of Earth’s orbit around the sun. The major planets in our solar system and their moons, and some asteroids, orbit more or less in this same plane.
Saturn, Mars, Moon in line seen from Earth.
View larger. | Moon and planets on October 12, 2016, by Karthik Easvur in Hyderabad, India. The moon and planets trace out a line across our sky because they all orbit the sun, more or less, in a single plane. And – as seen from Earth – we look edgewise into that flat plane of the solar system.

Ecliptic defines the zodiac

Far beyond the cold edges of our solar system, we see the stars of our Milky Way galaxy. And the stars are moving, too, in great orbits around the galaxy’s center. But they’re so far away that they don’t seem to move over the course of a human lifespan. That’s why we speak of the “fixed” stars. Fixed stars on the ecliptic – or sun’s path – seemed special to the early stargazers. They identified constellations made of these stars, and used the word zodiac for the wider pathway traveled by these constellations. And so we find the sun, moon and our major planets within the constellations of the zodiac.

Now about that phrase we keep using, the phrase more or less

The other planets don’t orbit exactly in the Earth-sun plane. Each major planet’s orbit is inclined a little bit to this plane. Some of the asteroids have orbits that are more inclined. And comets tend to have the most inclined orbits of all. See a chart at Wikipedia with the inclinations of the major planets’ orbits.

The moon and the ecliptic

Interestingly, Earth’s moon isn’t exactly on the ecliptic, either. Its orbit around Earth is tilted by about 5.15 degrees relative to the ecliptic. This means the moon spends most of its time above or below the ecliptic. It crosses it twice each orbit: once going upward and once downward from our point of view. Therefore, we usually see the moon close to, but not exactly alongside the other solar system objects.

On the other hand, the moon sometimes passes right in front of other solar system objects, in an event called an occultation.

So there are little variations. But – for all practical purposes of skywatching – you can think of the ecliptic as a line across our sky. You can think of the sun, moon and major planets of the solar system as moving along that line. One thing to remember, though. The sun’s path is high in summer and low in winter. So the location of the ecliptic in your sky shifts a bit, seasonally.

High bright arc of sun's path across daytime sky, and another low arc.
The ecliptic in June and December. Image from Stellarium.

Ecliptic, eclipse

If the word ecliptic sounds familiar, you’re right. It’s from the same root as the word eclipse, from the Latin and Greek meaning to “fail to appear” or “to be hidden” because the moon hides the sun during an eclipse. The ecliptic got its name because the ancients saw that solar eclipses happen when the moon crosses the ecliptic during the new moon phase.

Later, astronomers gave the name node to the places where the moon crosses the ecliptic. If the moon traveled exactly on the ecliptic, and the other planets did, too, the moon would occult, or block out, all the planets and the sun every orbit. We’d have lunar and solar eclipses every month. Ho hum.

Watch the sky

If you’re able, keep an eye on the sun, the moon and the planets for a while. Watch for a few days, a few weeks, months, years, even. You’ll begin to get a feel for the ecliptic in your sky. You’ll notice the planets, sun and moon are always on or near the ecliptic, and you can use this line across your sky to help you find your way around, making your way between the constellations and stars. You’ll notice the sun’s path – the ecliptic – higher in the sky during the summer months and lower during the winter.

Eventually, you’ll be able to imagine the sun’s path in your sky, long after the sun has set.

When that happens, you’ll be able to pick out a planet from a star very quickly and easily, which is a great party trick. Mars is the red one; Saturn the yellow one; Venus the bright white one that never gets too far from the sun; Mercury the seldom-seen one; and Jupiter the very bright one (but never as bright as Venus) that often gets far from the sun.

Welcome to stargazing, friend!

Array of many square photos showing planets lined up.
View larger. | The cameras of the Voyager 1 spacecraft acquired the images to create this mosaic on February 14, 1990, as it journeyed out of the solar system. It pointed back toward the sun and took this series of pictures of our sun and several major planets, making the first-ever “portrait” of our solar system as seen from the outside. The mosaic consists of a total of 60 frames. Voyager 1 was at a distance of approximately 4 billion miles (over 6 billion km) and about 32 degrees above the ecliptic plane. Read more about this image via NASA PhotoJournal.

Bottom Line: The ecliptic is the path the sun takes across our sky. It’s the Earth-sun plane. And, more or less, it’s the plane of the orbits of the major planets and their moons, and some asteroids, our solar system. Stargazing tip: Learn the whereabouts of the ecliptic in your sky. You’ll always find the sun, moon and planets on or near it.

July 25, 2021
Astronomy Essentials

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