Scientists have hypothesized since the 1960s that the Sun is a source of ingredients that form water on the Moon. When a stream of charged particles known as the solar wind smashes into the lunar surface, the idea goes, it triggers a chemical reaction that could make water molecules.
Now, in the most realistic lab
simulation of this process yet, NASA-led researchers have confirmed this
prediction.
The finding, researchers wrote in a March 17 paper in JGR Planets, has implications for NASA’s Artemis astronaut operations at the Moon’s
South Pole. A critical resource for exploration, much of the water on the Moon
is thought to be frozen in permanently shadowed regions at the
poles.
“The exciting thing here is that with
only lunar soil and a basic ingredient from the Sun, which is always spitting
out hydrogen, there’s a possibility of creating water,” Li Hsia Yeo, a research scientist at NASA’s Goddard Space Flight Center in
Greenbelt, Maryland. “That’s incredible to think about,” said Yeo, who led the
study.
Solar wind flows constantly from the
Sun. It’s made largely of protons, which are nuclei of hydrogen atoms that have
lost their electrons. Traveling at more than one million miles per hour, the solar wind bathes the entire solar
system. We see evidence of it on Earth when it
lights up our sky in auroral light shows.
Computer-processed data of the solar wind from NASA’s
STEREO spacecraft. Download here: https://svs.gsfc.nasa.gov/20278/
NASA/SwRI/Craig DeForest
Most of the solar particles don’t reach the surface of Earth because our
planet has a magnetic shield and an atmosphere to deflect them. But the Moon
has no such protection. As computer models and lab experiments have shown, when
protons smash into the Moon’s surface, which is made of a dusty and rocky
material called regolith, they collide with electrons and recombine to form
hydrogen atoms.
Then, the hydrogen atoms can
migrate through the lunar surface and bond with the abundant oxygen atoms
already present in minerals like silica to form hydroxyl (OH) molecules, a
component of water, and water (H2O) molecules
themselves.
Scientists have found evidence of
both hydroxyl and water molecules in the Moon’s upper surface, just a few
millimeters deep. These molecules leave behind a kind of chemical fingerprint —
a noticeable dip in a wavy line on a graph that shows how light interacts with
the regolith. With the current tools available, though, it is difficult to tell
the difference between hydroxyl and water, so scientists use the term “water”
to refer to either one or a mix of both molecules.
Many researchers think the solar
wind is the main reason the molecules are there, though other sources like
micrometeorite impacts could also help by creating heat and triggering chemical
reactions.
In 2016, scientists discovered that water is released
from the Moon during meteor showers. When a speck of comet debris strikes the
moon, it vaporizes on impact, creating a shock wave in the lunar soil. With a
sufficiently large impactor, this shock wave can breach the soil’s dry upper
layer and release water molecules from a hydrated layer below. NASA’s LADEE
spacecraft detected these water molecules as they entered the tenuous lunar
atmosphere.
NASA's Goddard Space Flight Center Conceptual Image
Lab
Spacecraft measurements had already hinted that the solar wind is the
primary driver of water, or its components, at the lunar surface. One key clue,
confirmed by Yeo’s team’s experiment: the Moon’s water-related spectral signal
changes over the course of the day.
In some regions, it’s stronger in
the cooler morning and fades as the surface heats up, likely because water and
hydrogen molecules move around or escape to space. As the surface cools again
at night, the signal peaks again. This daily cycle points to an active source —
most likely the solar wind—replenishing tiny amounts of water on the Moon each
day.
To test whether this is true, Yeo
and her colleague, Jason McLain, a research scientist at NASA Goddard, built a custom apparatus to examine
Apollo lunar samples. In a first, the apparatus held all experiment components
inside: a solar particle beam device, an airless chamber that simulated the
Moon’s environment, and a molecule detector. Their invention allowed the
researchers to avoid ever taking the sample out of the chamber — as other
experiments did — and exposing it to contamination from the water in the
air.
“It took a long time and many
iterations to design the apparatus components and get them all to fit inside,”
said McLain, “but it was worth it, because once we eliminated all possible
sources of contamination, we learned that this decades-old idea about the solar wind turns out to be true.”
Using dust from two different
samples picked up on the Moon by NASA’s Apollo 17 astronauts in 1972, Yeo and
her colleagues first baked the samples to remove any possible water they could
have picked up between air-tight storage in NASA’s space-sample curation facility at NASA’s Johnson Space Center in Houston and
Goddard’s lab. Then, they used a tiny particle accelerator to bombard the dust
with mock solar wind for several days — the equivalent of 80,000 years on the
Moon, based on the high dose of the particles used.
They used a detector called a
spectrometer to measure how much light the dust molecules reflected, which
showed how the samples’ chemical makeup changed over time.
In the end, the team saw a drop in
the light signal that bounced to their detector precisely at the point in the
infrared region of the electromagnetic spectrum — near 3 microns — where water
typically absorbs energy, leaving a telltale signature.
While they can’t conclusively say
if their experiment made water molecules, the researchers reported in their
study that the shape and width of the dip in the wavy line on their graph
suggests that both hydroxyl and water were produced in the lunar samples.
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Source: Solar Wind and Moon's Water
No comments:
Post a Comment