Written by Elizabeth Zubritsky
NASA Goddard Space Flight Center
Greenbelt, MD – Just weeks before the historic encounter of comet C/2013 A1 (Siding Spring) with Mars in October 2014, NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft entered orbit around the Red Planet.
To protect sensitive equipment aboard MAVEN from possible harm, some instruments were turned off during the flyby; the same was done for other Mars orbiters. But a few instruments, including MAVEN’s magnetometer, remained on, conducting observations from a front-row seat during the comet’s remarkably close flyby.The one-of-a-kind opportunity gave scientists an intimate view of the havoc that the comet’s passing wreaked on the magnetic environment, or magnetosphere, around Mars. The effect was temporary but profound.
“Comet Siding Spring plunged the magnetic field around Mars into chaos,” said Jared Espley, a MAVEN science team member at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We think the encounter blew away part of Mars’ upper atmosphere, much like a strong solar storm would.”
Unlike Earth, Mars isn’t shielded by a strong magnetosphere generated within the planet. The atmosphere of Mars offers some protection, however, by redirecting the solar wind around the planet, like a rock diverting the flow of water in a creek.
This happens because at very high altitudes Mars’ atmosphere is made up of plasma — a layer of electrically charged particles and gas molecules. Charged particles in the solar wind interact with this plasma, and the mingling and moving around of all these charges produces currents. Just like currents in simple electrical circuits, these moving charges induce a magnetic field, which, in Mars’ case, is quite weak.
Comet Siding Spring is also surrounded by a magnetic field. This results from the solar wind interacting with the plasma generated in the coma – the envelope of gas flowing from a comet’s nucleus as it is heated by the sun.
› NASA’s newest Mars orbiter, MAVEN, arrived just in time for a comet’s close flyby of Mars in 2014.
› The powerful magnetic field around the comet temporarily merged with — and overwhelmed — Mars’ weak magnetic field.
Comet Siding Spring’s nucleus — a nugget of ice and rock measuring no more than about one-third mile (half a kilometer) — is small, but the coma is expansive, stretching out more than 600,000 miles (a million kilometers) in every direction. The densest part of the coma — the inner region near the nucleus — is the part of a comet that’s visible to telescopes and cameras as a big fuzzy ball.
When comet Siding Spring passed Mars, the two bodies came within about 87,000 miles (roughly 140,000 kilometers) of each other. The comet’s coma washed over the planet for several hours, with the dense inner coma reaching, or nearly reaching, the surface. Mars was flooded with an invisible tide of charged particles from the coma, and the powerful magnetic field around the comet temporarily merged with — and overwhelmed — the planet’s own weak one.
“The main action took place during the comet’s closest approach,” said Espley, “but the planet’s magnetosphere began to feel some effects as soon as it entered the outer edge of the comet’s coma.”
By the time of closest approach — when the plasma from the comet was densest — Mars’ magnetic field was in complete chaos. Even hours after the comet’s departure, some disruption continued to be measured.
Espley and colleagues think the effects of the plasma tide were similar to those of a strong but short-lived solar storm. And like a solar storm, the comet’s close passage likely fueled a temporary surge in the amount of gas escaping from Mars’ upper atmosphere. Over time, those storms took their toll on the atmosphere.
“With MAVEN, we’re trying to understand how the sun and solar wind interact with Mars,” said Bruce Jakosky, MAVEN’s principal investigator from the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder. “By looking at how the magnetospheres of the comet and of Mars interact with each other, we’re getting a better understanding of the detailed processes that control each one.”
This research was published in Geophysical Research Letters.
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