Scorching-Hot Mercury Has a Surprisingly Icy North Pole

Mercury North Pole Craters
1. The pockmarked terrain of Mercury’s north pole harbors much more ice than scientists had expected. (Image credit: Head lab/ Brown University)

Mercury has much more ice scattered across its north pole than previously thought, new research suggests — both inside craters as well as in shadowed terrain between them. The small deposits add to a significant amount of previously unrecognized water ice, researchers said in a statement.

Mercury may seem like a surprising place to find ice: Although nights can get as cold as minus 275 degrees Fahrenheit (minus 170 degrees Celsius), temperatures can soar to 840 degrees F (450 degrees C) during the day. This is more than hot enough to boil away any water on the surface.

But Mercury's axis has very little tilt, so its polar regions don't receive much direct sunlight. This keeps the floor of some of its polar craters in perpetual shadow, researchers said in the statement. Mercury also has almost no atmosphere to hold in ambient heat, so the temperatures in these craters stay low enough for water to remain frozen. [Water Ice on Mercury: How It Stays Frozen (Infographic)]

The idea that Mercury may have water ice emerged in the 1990s when Earth-based telescopes first detected highly reflective regions at the planet's poles, researchers said in the statement. The hypothesis was verified in late 2012 by NASA's MESSENGER probe, which had entered Mercury's orbit in 2011. After a successful mission, the spacecraft deorbited in April 2015, crashing into the planet's surface. But the wealth of information it provided is still fueling research today.

In the new study, researchers from Brown University combed through old data from the MESSENGER spacecraft. They took advantage of readings from the orbiter's laser altimeter, which is generally used to determine map elevation, but also measures surface reflectivity, the researchers said in the statement.

They found evidence of ice in three large craters that had been measured at an oblique angle, rather than straight down. Ariel Deutsch, the study's lead author and a planetary scientist at Brown University, estimates that these deposits may account for an additional 1,313 square miles (3,400 square kilometers) of ice. That's a quarter larger than the state of Rhode Island.

The small-scale deposits scattered between the craters could add even more, though, the researchers said. Scientists believe the moon hosts similar ice deposits near its poles, and research models suggest that these deposits could roughly double the amount of lunar surface that could harbor ice.

"The assumption has been that surface ice on Mercury exists predominantly in large craters, but we show evidence for these smaller-scale deposits as well," Deutsch said in the statement. "Adding these small-scale deposits to the large deposits within craters adds significantly to the surface ice inventory on Mercury."

Scientists are still uncertain how water arrived on Mercury. According to the statement, their best hypothesis right now is that it was delivered by water-rich comet and asteroid impacts. Another idea is that hydrogen supplied by the solar wind combined with oxygen on the planet's surface to form water. These are some of the topics the researchers hope to investigate further.

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Harrison Tasoff
Former Contributing Writer

Harrison Tasoff is a science journalist originally from Los Angeles. He graduated from NYU’s Science, Health, and Environmental Reporting Program after earning his B.A. in mathematics at Swarthmore College. Harrison covers an array of subjects, but often finds himself drawn to physics, ecology, and earth science stories. In his spare time, he enjoys tidepooling, mineral collecting, and tending native plants.