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Astronomy Says Olympus Mons on Mars Is About Two and a Half Times Taller Than Mount Everest

Astronomy Says Olympus Mons on Mars Is About Two and a Half Times Taller Than Mount Everest

Read all the way to the end – we save the one detail most people never think about for last.

Picture standing on a plain so wide that the ground curves away beneath you, and you still can’t see the top of the mountain you’re climbing. That’s roughly the problem with Olympus Mons, the giant volcano on Mars. It’s so large that its scale is hard to take in, even when you have the numbers in front of you.

The comparison to Mount Everest gets repeated a lot, and for good reason. Yet the figures behind it hold a few surprises, and a couple of caveats too. Here’s what astronomers and planetary scientists actually know about the red planet’s tallest peak.

What the Height Comparison Really Means

What the Height Comparison Really Means (Olympus Mons and the Northeast US #2, CC BY 2.0)
What the Height Comparison Really Means (Olympus Mons and the Northeast US #2, CC BY 2.0)
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Olympus Mons rises about 21 to 22 kilometers above the Martian datum, the reference level used for Mars, since the planet has no sea level. Everest stands about 8.8 kilometers above sea level on Earth. Divide one by the other and you land at roughly two and a half times taller.

That ratio is the headline, though it comes with a catch. Everest’s height is measured from sea level, not from its base, so the two numbers aren’t perfectly like for like. Measured from base to summit, Earth’s tallest mountain from the seafloor, Mauna Kea, is taller than Everest, but Olympus Mons still dwarfs it.

A Volcano Built Like a Shield

A Volcano Built Like a Shield (D-Stanley, Flickr, CC BY 2.0)
A Volcano Built Like a Shield (D-Stanley, Flickr, CC BY 2.0)
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Olympus Mons is a shield volcano, the same broad, gently sloping type as Hawaii’s Mauna Loa. These form when very fluid lava flows pour out again and again over long stretches of time, layering outward rather than piling steeply upward. The result looks less like a classic cone and more like a vast, shallow dome.

That shape matters for how it would feel to visit. The average slope is gentle, only a few degrees, so a hiker wouldn’t face a sheer wall. You’d simply walk uphill for a very long time.

Wider Than You Might Imagine

Wider Than You Might Imagine (Edited version of File:Olympus Mons.jpg originally from http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-mars.html#features., Public domain)
Wider Than You Might Imagine (Edited version of File:Olympus Mons.jpg originally from http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-mars.html#features., Public domain)
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Height is only part of the story. The volcano’s base spans roughly 600 kilometers across, comparable to the size of a large country or the state of Arizona. Its footprint is so enormous that it’s often described as being about the size of France in coverage.

Around its edge, a cliff known as the escarpment drops several kilometers in places. Because the mountain is so wide, a person standing on its flank would not see the whole thing at once, since the planet’s curvature hides the summit and the base from each other.

Why Mars Can Grow Such Giants

Why Mars Can Grow Such Giants (Image Credits: Pexels)
Why Mars Can Grow Such Giants (Image Credits: Pexels)
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Scientists point to a few reasons Mars supports volcanoes this large. Earth’s crust is split into moving tectonic plates, so a volcanic hotspot tends to drift away from its magma source and build a chain of islands. Mars lacks that kind of plate motion, so lava can keep building in the same place for an extremely long time.

Lower gravity also helps. Mars has roughly a third of Earth’s surface gravity, so the crust can support a much taller structure before it sags under its own weight. Together, those conditions let Olympus Mons grow far beyond anything on our planet.

Is It Still Active?

Is It Still Active? (Andrea Luck, Flickr, CC BY 2.0)
Is It Still Active? (Andrea Luck, Flickr, CC BY 2.0)
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Olympus Mons is generally considered dormant or extinct, not erupting today. Studies of its lava flows suggest that some surface areas are geologically young by planetary standards, with ages estimated in the range of millions of years. That hints that activity may have continued relatively recently in Martian history.

Still, whether it could ever wake up again is uncertain. Scientists don’t have a firm answer, and the evidence we have comes mostly from orbital imaging and crater counting rather than direct measurement on the ground.

Final Thoughts

Final Thoughts (Image Credits: Pexels)
Final Thoughts (Image Credits: Pexels)
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I find the Everest comparison a bit unfair to Everest, honestly. It’s a stunning mountain, but it plays on a different field. Olympus Mons reminds us that a planet’s rules, its gravity, its crust and its lack of moving plates, decide what kind of landscapes are even possible.

My view is that the number is a good hook, but the real lesson is the why. A mountain two and a half times Everest isn’t just trivia, it’s evidence of how differently a world can build itself when it’s left alone for billions of years.