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Planetary Radio: Space Exploration, Astronomy and Science

Phil Christensen Explores Mars in the Infrared

Planetary Radio: Space Exploration, Astronomy and Science

The Planetary Society

Science, Technology

4.81.4K Ratings

🗓️ 26 May 2003

⏱️ 29 minutes

🧾️ Download transcript

Summary

Phil Christensen Explores Mars in the InfraredLearn more about your ad choices. Visit megaphone.fm/adchoices

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Transcript

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0:00.0

This is planetary radio. Matt Kaplan with another edition of our program about the final frontier, we're glad to have you with us this week.

0:24.0

Sometimes it's what you can't see with your own eyes that changes the world.

0:28.0

In this case, the world is Mars.

0:31.0

We'll talk with Phil Christensen, a planetary geologist who has devoted much

0:36.2

of his life to studying not just the red but the infrared planet. Later Bruce Betts will be here with What's Up and the new trivia contest.

0:46.0

First though, here's Emily trying not to get caught in a flash flood on Mars. years. Hi, I'm Emily Lochuwala with questions and answers.

1:10.0

A listener asked, given the planet's very low atmospheric pressure, how could enough water have existed on Mars to create a flood?

1:17.0

There are two major types of Martian channels, both of which were most likely formed by water.

1:23.0

There are two major types of Martian channels, both of which were most likely formed by water.

1:28.0

The most dramatic channels, called the outflow channels, have features similar to those found in catastrophic flood

1:34.9

channels on earth like the channeled scablands in Washington State.

1:38.7

The amount of water necessary to produce the Martian catastrophic floods is estimated at about 10 to 100 million cubic meters per second,

1:47.0

a flow about 100 times greater than the flow from Earth's largest river, the Amazon.

1:52.0

All of this water most likely came from Benjia. from Earth's largest river, the Amazon.

1:52.6

All of this water most likely came from beneath Mars's surface.

1:56.5

The temperature and pressure at the surface are too low

1:59.1

to allow liquid water to survive long before vaporizing. But conditions underground include higher

2:04.7

pressures and temperatures, probably warm enough for water to exist as a liquid. How could this

2:09.5

water come to the surface to start a flood? Stay tuned to planetary radio to find out. Dr Phil Christensen is the core professor of geologic sciences at Arizona State University.

2:31.3

That's also where he heads ASU's Mars Space Flight Facility.

2:36.6

And if you pick up a copy of the planetary report, the May-June issue of that magazine, which

2:41.7

is just about to appear.

...

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