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NASA’s Curiosity rover captures photos of Mars dust storm

However, the Curiosity rover, which has been studying Martian soil at Gale Crater, is expected to remain largely unaffected by the dust. While Opportunity is powered by sunlight, which is blotted out by dust at its current location, Curiosity has a nuclear-powered battery that runs day and night. The Martian dust storm has grown in size and is now officially a “planet-encircling” dust event. Though Curiosity is on the other side of Mars from Opportunity, dust has steadily increased over it, more than doubling over the weekend.

The atmospheric haze blocking sunlight, called “tau,” is now above 8.0 at Gale Crater – the highest tau the mission has ever recorded. Tau was last measured near 11 over Opportunity, thick enough that accurate measurements are no longer possible for Mars’ oldest active rover. For NASA’s human scientists watching from the ground, Curiosity offers an unprecedented window to answer some questions such as why some Martian dust storms last for months and grow massive, while others stay small and last only a week. Curiosity along with a fleet of spacecraft in the orbit of Mars, will allow scientists for the first time to collect a wealth of dust information both from the surface and from space.

The last storm of global magnitude that enveloped Mars was in 2007, five years before Curiosity landed there. Daily photos are being captured by the Curiosity rover’s Mast Camera, or Mastcam, show the sky getting hazier. This sun-obstructing wall of haze is about six to eight times thicker than normal for this time of season. Curiosity’s engineers at NASA’s Jet Propulsion Laboratory in Pasadena, California, have studied the potential for the growing dust storm to affect the rover’s instruments, and say it poses little risk.

The largest impact is to the rover’s cameras, which require extra exposure time due to the low lighting. The rover already routinely points its Mastcam down at the ground after each use to reduce the amount of dust blowing at its optics. Martian dust storms are common, especially during southern hemisphere spring and summer, when the planet is closest to the Sun. As the atmosphere warms, winds generated by larger contrasts in surface temperature at different locations mobilize dust particles the size of individual talcum powder grains. Carbon dioxide frozen on the winter polar cap evaporates, thickening the atmosphere and increasing the surface pressure. This enhances the process by helping suspend the dust particles in the air. In some cases, the dust clouds reach up to 60 kilometres or more in elevation. Though they are common, Martian dust storms typically stay contained to a local area. By contrast, the current storm, if it were happening on Earth, is bigger than North America and Russia combined, researchers said.

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