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Helio and You: August 2026

Here on Earth, we're lucky to get total solar eclipses from time to time. But did you know that eclipses can happen on other worlds, too? Find out all about eclipses and what they're like on Earth and elsewhere.

NASA's Mars Global Surveyor shows the shadow of the martian moon, Phobos, as it was cast upon western Xanthe Terra on August 26, 1999.

Helio and You: Studying Eclipses Near and Far

What is an Eclipse?

Every so often, people on Earth get the chance to experience a total solar eclipse. Recent examples include the eclipses that swept across North America in 2017 and 2024 and the one that visited Spain and other parts of Europe and Canada in August 2026. These celestial events happen somewhere on the planet about every 18 months or so, and any given spot on Earth experiences a total solar eclipse only every few hundred years. For this reason, many people travel hundreds or even thousands of miles to see them in person.

An eclipse happens when the Moon passes directly between the Sun and Earth, blocking the Sun’s light for a short time. This allows those in the path of the Moon's fullest shadow (which is called totality) to experience unique lighting conditions that resemble 360-degree sunrise or sunset. Animals may also behave strangely during these eclipses, and scientists can study those responses.

The Moon is just the right size (about 400 times smaller than the Sun) and just the right distance away from the Earth (about 400 times closer than the Sun) to perfectly block the Sun when it comes between the Sun and Earth. With the bright photosphere (surface of the Sun) blocked by the Moon, observers are able to see the Sun’s wispy outer atmosphere (the corona). This is actually how the corona was discovered in the first place!

A processed image of the total solar eclipse from 2017 shows the moon completely covering the disk of the Sun. Encircling the moon, the solar corona can be seen in white light with well-defined structures.
A composite image taken during the August 2017 total solar eclipse shows the corona visible around the edges of the Moon as it comes directly between the Sun and Earth.
Credit: Miloslav Druckmüller, Peter Aniol, Shadia Habbal/NASA Goddard, Joy Ng

But Earth is not the only planet with eclipses. Any time a moon or planet goes between a star and an observer (called a transit), the object passing in front of the star eclipses part of that star’s light. Any planet with a moon large enough, round enough, and with the right distance to size ratio compared to the local star could have total solar eclipses like ours. So, what would the eclipses be like on these other planets?

Do Other Planets Get Eclipses, Too?

In our solar system, some planets (like Mercury and Venus) have no moons, so eclipses are impossible. Other planets (like Jupiter and Saturn) have lots of moons, but most of them aren’t big enough or at the right distance to fully block the Sun’s light. Mars’ two small, potato-shaped moons, Phobos and Deimos, are not large enough to do anything more than partially obscure the Sun when they do pass in front of it. These transits can make for interesting viewing for rovers down on the surface of Mars, but they are only seeing a partial solar eclipse.

Many of the moons of the gas giants are also too small or too distant (or both) for them to block anything more than a small part of the Sun’s light. Saturn and Uranus, for example, don’t have any moons big enough or close enough to cause total solar eclipses. But there are a few locations where the combination of moon size and distance would make it possible to have total solar eclipses like the ones here on Earth.

Jupiter Moon Transit, January 24, 2015 (07:10 UT) – Annotated
Three moons and their shadows parade across Jupiter near the end of a multi-moon eclipsing event on January 24, 2015. This image clearly shows how the four Galilean moons (Io, Europa, Ganymede, and Callisto) can each cast large shadows on Jupiter.
Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

Jupiter’s second largest moon, Callisto, is just the right size and the right distance away from Jupiter to cause total solar eclipse like the ones here on Earth. Callisto would also cause eclipses at Jupiter about every 16 days for three years at a time (although there would then be a three-year period with none). While Jupiter’s other large moons (Io, Europa, and Ganymede) are too close for the corona to be visible when they eclipse the sun, future visitors to Jupiter might experience a double or even rarer triple total solar eclipse when the moons align.

But perhaps the best eclipses beyond Earth would take place on Saturn. While many of Saturn’s moons (including Titan) aren’t right or distance for total solar eclipses, the moons Janus, Pandora, Prometheus, and Epimetheus are all the right size and distance from Saturn to block sunlight like our Moon does here. Thanks to their relative closeness, size, and irregular shape, they could also cause partial and annular (ring of fire) eclipses, too.

There could be eclipses in other star systems, too. As our catalogue of known exoplanets grows (that’s worlds orbiting stars other than the Sun), we find more and more systems with multiple planets orbiting a single star. In the small, tightly packed systems which exist round red dwarf stars like TRAPPIST-1, where seven terrestrial planets all orbit in an orbital radius smaller than that of Mercury, it might even be possible for multiple of the planets in one star system to eclipse their star in each other’s skies.

See Explanation. Clicking on the picture will download the highest resolution version available.
This illustration provided by the European Southern Observatory (ESO) shows the potential for complex eclipses in small star systems like the one around TRAPPIST-1, a red dwarf star about 40 lightyears away from Earth. The seven planets in the TRAPPIST-1 system orbit within an orbital radius smaller than that of Mercury.
Credit: ESO / M. Kornmesser

What Can We Learn From Eclipses?

With all of this in mind, you might be asking yourself why scientists take such care to study eclipses in the first place. These celestial events allow us to study the Sun’s outer atmosphere, or corona, which is invisible to the naked eye when the main body of the Sun is not hidden behind the Moon. This is because sunlight from its surface (the photosphere) is simply too powerful for the corona to be visible during normal viewing conditions.

But during a total solar eclipse, the light of the photosphere is blocked by the Moon. It’s important to always remember that the only time it is safe to remove solar viewing glasses during an eclipse event is during totality, or when 100% of the Sun's light is blocked by the Moon. While scientists can use instruments called coronagraphs to block the Sun’s light and study the corona at any time, eclipses provide a unique opportunity for them to see the parts of the corona closest to the Sun, which cannot be seen with a coronagraph. Observations made during total solar eclipses offered some of the first insights into what the inner corona was really like.

A photograph shows several people in silhouette standing in a large field in front of the setting Sun, gathered around a large, round, white balloon floating just above their heads against a blue sky.
A student team from the University of Kentucky prepares to launch a balloon from Bloomington, Indiana, to take atmospheric measurements on April 8, 2024, during the 2024 Nationwide Eclipse Ballooning Project campaign. Studies like this gather data that advances our understanding of the Sun-Earth system.
Credit: Sean Bailey (University of Kentucky)

A total solar eclipse also helped prove Einstein’s theory of relativity. The May 29, 1919, total solar eclipse allowed scientists to see Einstein’s theory in action when they detected the gravitational lensing the theory predicted firsthand. In short, the Sun is so massive that its gravity pulls on the light of distant galaxies, warping that light so that galaxies “behind” the Sun are visible around its edges — but this is only possible during a total solar eclipse.

Eclipses also help us find out more about planets beyond our solar system. Based on data in NASA’s Exoplanet Archive, there were about 6,300 confirmed exoplanets in July 2026. Almost 4,700 of them (that's over 74 percent) were discovered using the transit method. This method of detection involves scanning other stars to perceive the slight dip in light intensity as an exoplanet crosses between us and the star — in other words, a transit. That means these distant eclipses are responsible for almost 74 percent of confirmed exoplanet detections.

In this animated artist's representation of how the transit method of exoplanetary detection works, we can see two different exoplanets (each of a different size) passing between Earth and their host star. In the grandest sense of the word, all of these transits are essentially eclipses.
Credit: NASA

Total solar eclipses can teach us about Earth, too. For one thing, a total solar eclipse changes the behavior of Earth’s atmosphere in the Moon’s shadow. Scientists can then study the Sun’s effects on the upper atmosphere (the ionosphere), which is home to many low-Earth orbit satellites as well as communications signals vital to us down on Earth. These studies are therefore useful for protecting our global communications network.

Could Our Eclipses End Someday?

As amazing as they are, we should understand that even the total solar eclipses we are used to enjoying on Earth will one day become a thing of the past. As the Moon orbits Earth, tidal forces (the same ones which cause tides in our oceans) caused by the Moon’s pull on Earth also pull on the Moon in an equal and opposite direction, as described in Newton's Laws. This exchange of tidal energy causes the Moon’s orbit to grow by about 4 centimeters per century. In other words, the Moon is getting farther away from Earth.

This means that a few billion years ago, the Moon orbited so close to Earth that total solar eclipses would have completely hidden the corona and caused total darkness more like nighttime. It also means that someday the Moon will be too far away for total solar eclipses to be possible. In another half a billion to a billion years, there will be a final total solar eclipse on Earth. So the next time you get the chance to experience an eclipse, remember how lucky we are that the conditions are right for us here on Earth to enjoy them at all.

But even though the circumstances on Earth are right for us to view total solar eclipses today, they are still a rare occurrence. After all, most of the planet is covered in water, and a good deal of what isn’t is not inhabited by humans. So if one happens to come through your backyard, or even your state, or even your county, take some time to check it out. They truly are a once in a solar system kind of opportunity.

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