In today's episode we’re going to space.
Specifically, Mars. You didn’t really think that earth science is really
limited to the earth, did you? Our topic today will be the Valles Marineris.
The Valles Marineris is a long
series of canyons east of Olympus Mons, the largest mountain in the solar
system. These canyons are about 4,000 km long, 200 km wide and up to 7 km
(23,000 ft) deep. On terrestrial scales, the Valles Marineris is as long as the
distance from New York to Los Angeles. That’s about the same as Beijing to Hong
Kong or Madrid to Copenhagen for our international listeners. They are as wide
as central Florida, central Italy, or the middle of the Korean peninsula. Two
and a half times deeper than Death Valley, though only about 60 percent of the
depth of the Marianas Trench, the lowest point on earth.
Not to be outdone, our planet, Earth,
has even bigger valleys. These occur at the oceanic ridges, where plate
spreading takes place. The longest rift valley on earth lies in the middle of
the Mid-Atlantic Ridge, and it is more than double the length of the Valles
Marineris. But let’s not belittle Mars. After all, while we have a pretty good
idea for how oceanic rifts form on earth, there is quite a bit of debate about
how Mars’ great valley formed.
The most popular theory suggests
that the Valles Marineris are an analog to our oceanic rifts, and formed by the
same process. As the volcanoes of the nearby Tharsis region developed, the
Martian crust bowed down toward the center of the planet due to the weight of
the new volcanic rocks. In time, the crust began to crack. This crack is what we
see in the Valles Marineris. Unlike on Earth, this rift valley did not continue
expanding, but shut down as the Tharsis Region, and Mars as a whole, cooled.
Remembe