Mars Proton Aurora

  • Released Monday, July 23rd, 2018
  • Updated Thursday, November 9th, 2023 at 12:29PM
View full credits

On Earth, the northern and southern lights occur when the solar wind (electrically charged particles from the Sun) follow our planet's geomagnetic field lines to the poles and collide with the upper atmosphere. Mars lacks a global magnetic field, so instead the solar wind piles up in front of Mars in a bow shock, which blocks charged particles from reaching the bulk of the atmosphere. However, in a process first observed by the MAVEN mission, some solar wind protons can slip past the bow shock by first bonding with electrons from the Mars upper atmosphere to form hydrogen atoms. Because these hydrogen atoms are electrically neutral, they can pass through the bow shock and go on to create an ultraviolet proton aurora on the dayside of Mars.

Learn more about MAVEN's observation of a proton aurora at Mars.

ANIMATED GIF - Mars proton aurora with data from the MAVEN Imaging Ultraviolet Spectrograph (IUVS) at bottom. Credit: NASA/MAVEN/University of Colorado/LASP/Anil Rao

ANIMATED GIF - Mars proton aurora with data from the MAVEN Imaging Ultraviolet Spectrograph (IUVS) at bottom. Credit: NASA/MAVEN/University of Colorado/LASP/Anil Rao

GRAPHIC - Protons from the solar wind approach the Martian upper atmosphere.

GRAPHIC - Protons from the solar wind approach the Martian upper atmosphere.

GRAPHIC - Solar wind protons undergo a series of charge exchanges to slip past the bow shock, causing a proton aurora.

GRAPHIC - Solar wind protons undergo a series of charge exchanges to slip past the bow shock, causing a proton aurora.

For More Information



Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center


Missions

This visualization is related to the following missions:

Series

This visualization can be found in the following series: