Moonbase May Be Situated at Edge of Lunar Crater
Thursday, December 28, 2006
By Leonard David
NASA is on a flight path to replant astronauts on the Moon, looking
to sustain a human presence on that cratered, airless orb on a
"go-as-the nation-can-afford-to-pay" basis. That approach is seen
as letting people step back onto the lunar surface no later than
2020.
Space engineers have honed in on one possible site for a lunar
outpost: the Moon's south pole.
It's a tactical setting on the rim of Shackleton Crater, a feature
some 12 miles (19 kilometers) in diameter.
There's real estate here that basks in near-perpetual sunlight.
Also, it's a region that is a doorway into the depths of always
dark, Sun-deprived, territory.
What's possibly lurking there in that super-cold darkness is water
ice portrayed by some researchers as the gold standard for future
exploration on and from the Moon. Yet there is considerable debate
about this resource. If there, such a raw storehouse might be
processed into usable oxygen and hydrogen.
Experts have been chipping away at the water ice on the Moon issue
for years.
According to NASA Moon outpost thinkers, there are five key reasons
for building up an encampment near a lunar pole:
Polar sites have plenty of sunlight, which lessens concerns about
energy storage. It would be possible to operate a polar outpost on
solar power. While not highlighting it as such, NASA's go-solar
tactic also doubles as a non-nuclear, perhaps more politically
correct approach.
The environment at the poles of the Moon is relatively benign,
making it easier to design a habitat. Temperatures at the poles
vary no more than about 50 degrees Celsius all year round, while
temperatures at the equator can vary 250 degrees Celsius from day
to night.
At the Moon's south pole there is "ample evidence," NASA planners
point out, of enhanced hydrogen an important natural resource for
future development for energy generation, propellant production and
other potential uses.
The poles can teach robotic and human explorers volumes about the
Moon. This landscape is among the most complex of regions, yet very
little is known about them.
To land equipment and scientific payloads near the lunar south
pole, specifically, as opposed to another location, will require
less propellant and could be more cost effective.
Not in critical path
NASA's notional positioning of a base at the Moon's south pole was
not solely driven by the thought of driving over and diving into a
reservoir of potential water ice. On the other hand, if it's truly
there, so much the better.
There were many reasons for choosing the polar regions of the Moon
for the outpost location, said Jerry Sanders, In-Situ Resource
Utilization (ISRU) Project Manager at NASA's Johnson Space Center
in Houston, Texas.
One of them is the possibility of water/ice and other possible
cometary volatiles, said Sanders. He noted with interest that the
Stardust sample collection mission to comet Wild 2 found methyl and
ethylamines, which not only has hydrogen, but carbon and nitrogen
as well.
"The presence of large quantities of readily assessable water would
make long term settlement of the Moon much more attainable,"
Sanders explained to SPACE.com. "But for an initial outpost, oxygen
alone from the regolith [the Moon's topside layer of dust and rocky
debris] provides most of the benefits of early ISRU ... oxygen for
extravehicular activity and life support backup."
Sanders underscored a message that was made clear from an early
December space exploration meeting in Houston, Texas during which
NASA's lunar outpost proposal was rolled out in detail.
"Because ISRU has never been demonstrated, it cannot be in the
'critical path' of outpost success
be it water or oxygen from
regolith," Sanders said. "However, as ISRU capabilities and
processes come online and are shown to be valid, ISRU products will
help reduce the logistics required from Earth with the goal of use
in propulsion and surface exploration activities."
Hydrogen enhancement
Measurements taken by NASA's robotic Lunar Prospector that orbited
the Moon in 1998-1999 reported hydrogen enhancement over large
shadowed areas exciting some scientists about the prospect of
large quantities of water ice tucked away in always dark nooks and
crannies.
The projection is that billions of gallons of water could be locked
up in the form of water ice.
That finding seemed to back an earlier data point from the U.S.
Defense Department's Clementine Moon probe.
Scientists on that project reported that Clementine data suggested
the presence of ice at the bottom of a permanently shadowed crater
near the Moon's south pole.
Of late, the Advanced Moon Imaging Experiment on the European Space
Agency's (ESA) SMART-1 lunar orbiter searched for light, shadow and
ice at the Moon's south pole before it was purposely plowed into
the Moon in early September 2006.
The ESA craft made long repeated camera exposures to see inside the
shadowed areas, using imagery skills that could reveal patchy ice
surface layers inside the crater.
"We still do not know if this hydrogen is due to enhanced trapping
of solar wind, or to the water ice brought on the Moon by the
bombardment of comets and asteroids," said Bernard Foing, ESA's
SMART-1 project scientist. "We need to analyze all remote sensing
data sets consistently. Future lander and rover missions to the
Moon will help in the search and characterization of lunar polar
ice, both on the surface and below the subsurface," he
explained.
However, astronomers recently utilized Earth-based radio-telescopes
to scan the 1.3 mile (2 kilometer) wide inner edge of the
Shackleton crater ridge. The report is that they were not able to
identify a distinctive signature of ice deposits pigeon holed
within that south pole region.
Covering all your bases
Shackleton crater as the locale for a lunar outpost is not an X
marks the spot, done deal, said Ben Bussey, senior staff scientist
at the Johns Hopkins University Applied Physics Laboratory in
Laurel, Maryland.
"It might be the place ... but it might not," Bussey told
SPACE.com. "What you're doing is covering all your bases for
planning a lunar outpost."
Bussey said that there are places near the rim of Shackleton which
have a lot of illumination that is potentially constant. "And you
know you are close to areas of permanent shadow that we know have
enhanced hydrogen ... and may or may not have ice ... depending on
who you believe."
India's Chandrayaan-1 lunar orbiter, to be lofted in early 2008,
has a good shot at further identifying possible water ice-laden
spots with a U.S.-provided low-power imaging radar, Bussey advised
one of two U.S. experiments on the Indian Moon probe.
"The idea is that we find regions of interest with Chandrayaan-1
radar. We would investigate those using all the capabilities of the
radar on NASA's Lunar Reconnaissance Orbiter, Bussey added, a Moon
probe to be launched late in 2008.
Still, going to and touching the ice via robotic landers is key,
Bussey said. "From orbit, we're identifying what we hope is a
resource. But to characterize the absolute nature of the resource,
you have to touch it physically and do the sort of measurements you
can only do on the spot."
For Bussey, a verdict of ice would be a windfall if it's really
there.
"You don't have to have ice at the poles to make that a good place
for the initial lunar outpost. If you happen to have big resources
of ice
well, that's just icing on the cake so to speak. Pardon the
pun," Bussey concluded.
Copyright © 2006 Imaginova Corp. All Rights Reserved.
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