Mars Upper Level Winds Observed by MAVEN - Visualizations

  • Released Thursday, December 12, 2019
View full credits

MAVEN is the first spacecraft specifically designed to study the Mars upper atmosphere, in order to better understand the evolution of its climate. These visualizations show MAVEN measuring the Martian upper level wind direction and magnitude over a series of thirty-three campaigns. In order for MAVEN to make these in-situ measurements, the spacecraft must be close to the upper atmosphere. The closest point of MAVEN's orbit to Mars (periapsis) dips into the tenuous upper reaches of the Martian thermosphere. The orbit also precesses over time to acquire measurements from different regions on the planet.

Now, scientists have used MAVEN data to map high-altitude wind currents on Mars for the first time. The data show that the Martian upper atmosphere is relatively independent of the daily rotation of Mars. On a day-to-day basis, high-altitude wind currents have a relatively fixed location with respect to the Sun, while Mars rotates underneath. Over the course of the Martian year, however, the currents follow the Sun north to south with the seasons.

MAVEN has also found that higher-elevation regions, such as the Tharsis plateau, cause small gravity waves that perturb the upper level winds and make them alter course. This means that certain topographic features on the Martian surface are detectable by MAVEN high above, as it skims the edge of space.

For More Information



Credits

Please give credit for this item to:
NASA/Goddard/SVS/MAVEN/CU Boulder/University of Michigan

Release date

This page was originally published on Thursday, December 12, 2019.
This page was last updated on Thursday, October 10, 2024 at 12:09 AM EDT.


Missions

This page is related to the following missions:

Datasets used

Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.