Mars Wind Currents Reveal a Surprising Feature
By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below.
Credit: NASA/Goddard/MAVEN/CU Boulder/University of Michigan
Universal Production Music: “Glacial Shifts” by James Joshua Otto
Watch this video on the NASA Goddard YouTube channel.
Complete transcript available.
MAVEN is the first spacecraft specifically designed to study the Mars upper atmosphere, in order to better understand the evolution of its climate. Now, scientists have analyzed several years of data from MAVEN’s NGIMS instrument and produced the first map of wind currents in the Martian thermosphere (a layer of the upper atmosphere). This map led to an unexpected and surprising discovery – disturbances in high-altitude wind currents on Mars are caused by terrain features such as mountains and valleys on the planet’s surface.
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Credits
Please give credit for this item to:
NASA/Goddard/MAVEN/CU Boulder/University of Michigan
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Producer
- Dan Gallagher (USRA)
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Data visualizer
- Greg Shirah (NASA/GSFC)
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Animators
- Jonathan North (USRA)
- Michael Lentz (USRA)
- Walt Feimer (KBR Wyle Services, LLC)
- Chris Smith (USRA)
- John Blackwell (LPI)
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Visualizers
- Ernie Wright (USRA)
- Horace Mitchell (NASA/GSFC)
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Narrator
- Dan Gallagher (USRA)
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Art director
- Michael Lentz (USRA)
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Scientists
- Mehdi Benna (UMBC)
- Kali Roeten (University of Michigan)
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Support
- Paul Mahaffy (NASA/GSFC)
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Principal investigator
- Bruce Jakosky (LASP)
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Technical support
- Aaron E. Lepsch (ADNET Systems, Inc.)
Release date
This page was originally published on Thursday, December 12, 2019.
This page was last updated on Thursday, November 9, 2023 at 12:29 PM EST.