The study, published in the journal Science Advances, builds on the initial discovery in 2009 of water and a related molecule - hydroxyl, which consists of one atom each of hydrogen and oxygen - in the lunar soil.
Scientists from Brown University in the US used a new calibration of data taken from NASA's Moon Mineralogy Mapper, which flew aboard Chandrayaan-1 spacecraft, to quantify how much water is present on a global scale.
"The amount of water increases toward the poles and does not show significant difference among distinct compositional terrains," said Li, who is now a postdoctoral researcher at the University of Hawaii.
The water concentration reaches a maximum average of around 500 to 750 parts per million in the higher latitudes. That is less than what is found in the sands of Earth's driest deserts, researchers said.
More From This Section
"This is a roadmap to where water exists on the surface of the Moon," said Ralph Milliken, an associate professor at Brown.
The researchers said that the way the water is distributed across the Moon gives clues about its source.
The distribution is largely uniform rather than splotchy, with concentrations gradually decreasing toward the equator.
That pattern is consistent with implantation via solar wind - the constant bombardment of protons from the Sun, which can form hydroxyl and molecular water once emplaced.
For example, the researchers found higher-than-average concentrations of water in lunar volcanic deposits near the Moon's equator, where background water in the soil is scarce.
Rather than coming from solar wind, the water in those localised deposits likely comes from deep within the Moon's mantle and erupted to the surface in lunar magma.
The study also found that the concentration of water changes over the course of the lunar day at latitudes lower than 60 degrees, going from wetter in the early morning and evening to nearly bone dry around lunar noon. The fluctuation can be as much as 200 parts per million.