From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Apr 01 2004 - 13:15:02 PST
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From: cunews_at_cornell.edu<mailto:cunews_at_cornell.edu>
To: CUNEWS-PHYSICAL_SCIENCE-L_at_cornell.edu<mailto:CUNEWS-PHYSICAL_SCIENCE-L_at_cornell.edu> ; CUNEWS-SCIENCE-L_at_cornell.edu<mailto:CUNEWS-SCIENCE-L_at_cornell.edu>
Sent: Thursday, April 01, 2004 4:02 PM
Subject: Cornell News: Cambell testifies about lunar base
Discovery of water would make proposed lunar base possible, but
recovery will be hard, Cornell astronomer tells House committee
FOR RELEASE: April 1, 2004
Contact: David Brand
Office: 607-255-3651
E-mail: deb27_at_cornell.edu<mailto:deb27_at_cornell.edu>
WASHINGTON, D.C. -- The discovery of accessible deposits of water on
the moon would "profoundly" affect the economics and viability of a
lunar base, Cornell University astronomer Donald Campbell told a
House of Representatives subcommittee today, April 1. Unfortunately,
he said, recovering water deposits will not be an easy task, since
they are likely to exist in the bottoms of very cold, permanently
dark craters at the moon's poles.
"For a permanent or reusable base, a local supply would be invaluable
both for human needs in the form of water and oxygen and for
production of rocket fuel," Campbell told the House subcommittee on
space at a hearing on "Lunar Science and Resources" in the Rayburn
House Office Building.
In January President George Bush announced a goal of returning humans
to the moon by the end of the next decade and using a lunar base as a
launch pad to Mars. The president said he would seek an additional $1
billion over the next five years to begin research on the program,
and he directed NASA to divert $11 billion from existing programs to
support development of technology needed to reach the moon and Mars.
Campbell is professor of astronomy at Cornell and associate director
of the National Astronomy and Ionosphere Center, based at Cornell,
which operates Arecibo Observatory, Puerto Rico, for the National
Science Foundation.
A viable lunar base, Campbell told the committee, would enable
further exploration of the moon and "has the potential to allow
exploitation of lunar resources." These resources, he said, include a
variety of minerals, such as oxides of iron and titanium, "and it is
possible that these minerals can be utilized to provide resources
such as oxygen to sustain an extended human presence on the moon."
Campbell spent much of his testimony discussing the possibility that
water is trapped below the lunar surface. Over the past decade, he
said, there has been evidence from instruments on lunar orbiting
spacecraft suggestive of the presence of water ice in the polar
regions.
Suggestions of lunar ice first came in 1996 when radio data from the
Clementine spacecraft gave some indications of the presence of ice on
the wall of a crater at the moon's south pole. Then, neutron
spectrometer data from the Lunar Prospector spacecraft, launched in
1998, indicated the presence of hydrogen, and by inference, water, at
a depth of about a meter at the lunar poles. But radar probes by the
12-cm-wavelength radar at Arecibo showed no evidence of thick ice at
depths of up to a meter.
However, Campbell told the committee, "While perhaps unlikely, the
possibility still exists that there are thick ice deposits in the
bottoms of some shaded impact craters at the lunar poles." There are
definitely higher concentrations of hydrogen at the lunar poles
compared with other areas of the moon, he said, "but both its origin
-- and its current form -- hydrogen, ice or hydrated minerals -- is a
topic of considerable discussion in the relevant scientific
community."
He warned that "before we spend too much time making plans for
exploiting water resources on the moon, we should determine whether
there are any recoverable deposits of water, in what form --
distributed at low concentrations in the lunar soil or in
concentrated deposits -- of what type -- ice or hydrated minerals --
and how accessible."
To do this, he said, it will be necessary to send one or more
missions with these specific objectives.
-30-
The web version of this release may be found at
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