PIA03791: Dust Devil Tracks


Dust Devil Tracks

Caption:


(Released 8 May 2002)

The Science
This image, centered near 50.0 S and 17.7 W displays dust devil tracks on the surface. Most of the lighter portions of the image likely have a thin veneer of dust settled on the surface. As a dust devil passes over the surface, it acts as a vacuum and picks up the dust, leaving the darker substrate exposed. In this image there is a general trend of many of the tracks running from east to west or west to east, indicating the general wind direction. There is often no general trend present in dust devil tracks seen in other images. The track patterns are quite ephemeral and can completely change or even disappear over the course of a few months. Dust devils are one of the mechanisms that Mars uses to constantly pump dust into the ubiquitously dusty atmosphere. This atmospheric dust is one of the main driving forces of the present Martian climate.

The Story
Vrrrrooooooooom. Think of a tornado, the cartoon Tasmanian devil, or any number of vacuum commercials that powerfully suck up swirls of dust and dirt. That's pretty much what it's like on the surface of Mars a lot of the time. Whirlpools of wind called "dust devils" whip up dust that has settled all over the surface.

In this image, the dust is a bright blanket of material. As the dust devils pass over the surface, they pick up this light dust and take it with them, exposing the darker surface below. It may look like a "clean up" effort on the ground, but it's the atmosphere that suffers. Dust devils may vacuum the surface, but they sure churn up a dusty atmosphere that is the main driving force in current climate change on the red planet. That's why these devilish winds on this hostile planet are so important to understand.

Take a look at the faint tracings of dust devil tracks. Can you tell which way the wind usually blows in this area? While there's some variation, the wind typically seems to move east to west . . . or is it west to east?! Regardless, this pattern is pretty regular . . . and that's actually ODD. Dust devil tracks in other Martian areas are much more crazy and erratic in their path, and can completely change or disappear over the course of a few months.

Cataloging Keywords:

Name Value Additional Values
Target Mars
System
Target Type Planet
Mission 2001 Mars Odyssey
Instrument Host Mars Odyssey
Host Type Orbiter
Instrument Thermal Emission Imaging System (THEMIS)
Detector
Extra Keywords Atmosphere, Dust, Grayscale
Acquisition Date
Release Date 2002-05-24
Date in Caption 2002-05-08
Image Credit NASA/JPL/Arizona State University
Source photojournal.jpl.nasa.gov/catalog/PIA03791
Identifier PIA03791