M
MARSBOUND
EXPLORE THE RED PLANET

FAMOUS
LANDMARKS

Mars has some of the most extreme terrain in the solar system. Biggest volcano, deepest canyon, and craters that could swallow countries whole.

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VOLCANO
HEIGHT / DEPTH
21.9 km
SIZE
600 km wide

Olympus Mons

The biggest volcano in the solar system. It is so wide that if you stood at the base, you could not see the summit because Mars curves away first. About 3 times taller than Mount Everest. The caldera at the top is 80 km across.

FAST FACT: You can walk up the main slope without knowing you are climbing a volcano. The incline is only 5 degrees.
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CANYON SYSTEM
HEIGHT / DEPTH
7 km deep
SIZE
4,000 km long

Valles Marineris

A system of canyons that stretches across almost a quarter of Mars. By comparison, the Grand Canyon could fit inside one of its smaller side canyons. Scientists still debate whether it formed from tectonic activity or ancient volcanic collapse.

FAST FACT: The canyon is so long it would stretch across the entire United States.
IMPACT CRATER
HEIGHT / DEPTH
8 km deep
SIZE
2,300 km across

Hellas Planitia

One of the largest impact craters in the entire solar system. Hit by a massive asteroid billions of years ago. The bottom of Hellas has the highest atmospheric pressure on Mars, making it slightly less hostile than the rest of the planet.

FAST FACT: The air pressure at the bottom is twice as high as the Martian average. Still not breathable, but the best Mars has.
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VOLCANIC PLATEAU
HEIGHT / DEPTH
10 km above average
SIZE
5,000 km across

Tharsis Plateau

A massive raised plateau covered in ancient volcanoes. Home to Olympus Mons and three other enormous volcanoes: Ascraeus Mons, Pavonis Mons, and Arsia Mons. The sheer weight of this region actually tilts Mars slightly.

FAST FACT: The Tharsis bulge is so massive it changed the tilt of Mars over billions of years.
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ICE FORMATIONS
HEIGHT / DEPTH
3 km thick
SIZE
1,000 km across (north)

Polar Ice Caps

Mars has both north and south polar caps. They are made mostly of water ice with a seasonal layer of frozen carbon dioxide on top. In winter, they grow. In summer, the CO2 layer evaporates but the water ice stays. Our Grand Tour includes a polar cap visit.

FAST FACT: The north polar cap alone holds enough water ice that if it all melted, it could cover Mars in 5 meters of water.
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HISTORICAL SITE
HEIGHT / DEPTH
Gale Crater floor
SIZE
154 km wide crater

Curiosity Landing Site

Where NASA landed the Curiosity rover in 2012. Gale Crater contains Mount Sharp in the center, a 5 km tall mound built up from ancient sediment layers. The rover found evidence that this area had liquid water for millions of years.

FAST FACT: Curiosity is still rolling around this area. Guests on our extended tours have a chance to spot it from the air.
DAY-TO-DAY SIGHTS

OBSERVABLE FEATURES


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Dust Devils

Small rotating columns of dust up to 8 km tall. Visible daily from most locations. Harmless but interesting to watch from inside your habitat.

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Martian Sunsets

The sky turns blue around the sun at sunset due to how dust scatters light. Opposite of Earth. One of the most talked-about sights by returning travelers.

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Phobos and Deimos

Mars has two small moons. Phobos moves so fast it rises in the west and sets in the east. Deimos takes 30 hours to cross the sky.

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The Blue Dunes

Dark basalt sand forms blue-black dunes near the polar caps. They look striking against the red terrain.