Computer simulation of the interaction of the solar wind with electrically charged particles (ions) in Mars' upper atmosphere. The lines represent the paths of individual ions and the colors represent their energy, and show that the polar plume (red) contains the most-energetic ions.

Credits: X. Fang, University of Colorado, and the MAVEN science team

In light of its continued scientific success, the MAVEN mission was extended from November of this year through September of 2016. This will bring the MAVEN mission cycle in synch with the wider planetary mission review process, planned in 2016, that will determine future mission extensions. 

Atoms in the Martian upper atmosphere become electrically charged ions after being energized by solar and space radiation. Because they are electrically charged, these ions feel the magnetic and electric forces of the solar wind, a thin stream of electrically conducting gas blown from the surface of the Sun into space at about a million miles per hour. The solar wind and more violent solar activity, such as solar flares and Coronal Mass Ejections, have the ability to strip away ions from Mars' upper atmosphere through electric and magnetic forces generated by a variety of mechanisms, causing the atmosphere to become thinner over time. MAVEN's goal is to discover which mechanisms are most prominent for atmospheric loss, and to estimate the rate at which the Martian atmosphere is being eroded away.

"MAVEN is observing a polar plume of escaping atmospheric particles," said Bruce Jakosky of the University of Colorado, Principal Investigator for MAVEN. "The amount of material escaping by this route could make it a major player in the loss of gas to space." Preliminary MAVEN observations of this phenomenon were presented in March at the Lunar and Planetary Science Conference in Houston, Texas.

Theoretical models had predicted that the electric field generated by the incoming solar wind could drive ions in the direction of one pole or the other, creating a polar plume of escaping ions. "When tracing particle trajectories in the models, the plume looks a bit like a ‘Mohawk'," said David Brain of the University of Colorado, an interdisciplinary scientist working on the MAVEN mission.

MAVEN has also detected a long-lived layer in the electrically charged upper atmosphere (the ionosphere) of Mars made up of metal ions (iron and magnesium) that come from incoming solar-system debris, such as comet dust and meteorites.  The incoming material is heated up by the atmosphere as it enters, burns up and vaporizes, and even ionizes.

"MAVEN had previously detected the metal ion layer associated with dust from the close passage of Comet Siding Spring last October," said Jakosky.  "When MAVEN did its first 'deep dip' campaign in February, and lowered the closest point of the spacecraft's orbit to around 125 kilometers (almost 78 miles) altitude, we immediately detected metal ions that still resided in the upper atmosphere. As there was no comet encounter at around that time, this must be the long-lived layer that we expect to be present."

The spacecraft has also seen the Red Planet lighting up under the impact of violent solar activity. Coronal Mass Ejections (CMEs) blast billions of tons of solar material into space at millions of miles per hour. Because Mars is not protected by a global magnetic field like Earth, CME particles directly impact the Martian upper atmosphere, generating diffuse displays of light called aurora. The high-energy particles from the Sun hit the upper atmosphere, excite the atoms that are there, and the atoms give off energy as they "relax" to their ground state. On Earth, the effect of our magnetic field concentrates auroral displays near the Polar Regions, where they are known as the Northern and Southern lights. On Mars, the aurora seen by MAVEN is more diffuse, and the effects also could drive the escape of atmospheric gas into space.

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