Solar flares: Be glad you're on Earth, not Mars (+video)
The recent solar flares provide a dramatic backdrop for a study that shows Mars gets far more of its atmosphere stripped away by solar storms than does Earth. Thank you, magnetosphere.
When solar storms strike Earth, as they have this week, the planet's magnetic field is a first line of defense against fast-moving clouds of charged particles hurtling from the sun.
A new study hints at how important that line of defense is in fostering a livable planet.
During a bout of turbulence in the solar wind in 2008, researchers found that Mars lost oxygen atoms in its atmosphere 10 times faster than did Earth – an observation the team attributes at least in part to the relative strength of each planet's magnetic field.
It marks the first time researchers have measured the effects of the solar wind on two planets at the same time and under the same windy conditions, and there is hope that the study can be extended to Venus, which has no magnetic field at all.
On one level, the results aren't surprising, the researchers acknowledge. Scientists have long thought that the presence of a natural, magnetic deflector shield would help a planet retain an atmosphere. This is seen as one reason Mars, with a magnetic field one-tenth as strong as Earth's, has such a comparatively tenuous atmosphere.
Yet during the past few years, discoveries involving the Earth's relatively expansive magnetosphere – the region of space around the planet that falls under the influence of its magnetic field – have cast some doubt on details of this generally accepted idea, the researchers say.
Some studies have suggested that the Earth's magnetosphere may be more efficient at transferring energy from the solar wind to the upper atmosphere than on smaller planets with weaker, smaller magnetospheres. This would render Earth's field a less-effective windbreak than previously thought.
By measuring the effect of the same solar-wind conditions on two planets at the same time, researchers can better quantify the shielding effect, as well as make comparisons to see how shield efficiency might change with the size of the magnetosphere.