This image shows the distribution of surface ice at the moon’s south pole (left) and north pole (right), as detected by NASA’s Moon Mineralogy Mapper instrument, which flew aboard India’s Chandrayaan-1 spacecraft. Blue represents ice locations, and the gray scale corresponds to surface temperature, with darker gray representing colder areas and lighter shades indicating warmer ones.

It's official: There's water ice on the surface of the moon.

Researchers have confirmed the presence of the frozen stuff on the ground around the lunar north and south poles, a new study reports. That's good news for anyone eager to see humanity return to the moon for more than just a flag-planting mission.

"With enough ice sitting at the surface — within the top few millimeters — water would possibly be accessible as a resource for future expeditions to explore and even stay on the moon, and potentially easier to access than the water detected beneath the moon's surface," NASA officials wrote in a statement Monday (Aug. 20). [The Search for Water on the Moon in Pictures]

As that statement indicates, scientists already knew that the lunar underground isn't bone-dry. For example, in 2009, an impactor released by NASA's Lunar Crater Observation and Sensing Satellite (LCROSS) blasted a bunch of water into space after slamming into a permanently shadowed region of Cabeus Crater, which lies near the moon's south pole.

But it wasn't clear from the LCROSS data where, exactly, that excavated ice originally lay — how much gray dirt once sat atop it. And, while several instruments have spotted tantalizing hints of exposed lunar ice over the years, these detections had remained unconfirmed until now.

"Previous observations indirectly found possible signs of surface ice at the lunar south pole, but these could have been explained by other phenomena, such as unusually reflective lunar soil," NASA officials wrote in the same statement.

Some of those observations were made by NASA's Moon Mineralogy Mapper (M3) instrument, which flew aboard India's Chandrayaan-1 spacecraft. The pioneering Chandrayaan-1 — India's first moon probe, and the first spacecraft to return compelling evidence of lunar water — studied Earth's nearest neighbor from orbit from November 2008 through August 2009.

In the new study, a team led by Shuai Li of the University of Hawaii and Brown University took a fresh look at M3 data. They spotted a distinctive signature of water ice in the reflectance spectra gathered by the instrument. [Moon Base Visions: How to Build a Lunar Colony (Images)]

This signature is present at many of the coldest and darkest spots on the lunar surface, within 20 degrees of both poles. There are differences from hemisphere to hemisphere, however. Ice is more abundant in the south, where it's found principally at the bottoms of permanently shadowed craters; in the north, the stuff is more widely, and thinly, dispersed.

Several factors might be responsible for this relative paucity of ice. For one thing, the moon's axis of rotation may have shifted more frequently over the eons than those of Mercury and Ceres, potentially exposing polar crater floors to sunlight more often, the researchers said. And it's possible that meteorite impacts have disrupted the moon's supplies of surface and near-surface ice more dramatically.

The new study was published online Monday in the journal Proceedings of the National Academy of Sciences.

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