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New Theory Explains Ice on Mars

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New Theory Explains Ice on Mars baalke 09-14-2007
Posted by baalke on September 14, 2007, 8:17 pm
Please log in for more thread options
Embargoed until 1 p.m. Eastern Time (7 a.m. HST), September 12, 2007

Contacts:

Dr. Norbert Schorghofer
Institute for Astronomy
University of Hawaii at Manoa
Honolulu, Hawaii 96822
1-808-956-9086
norb1@ifa.hawaii.edu

Mrs. Karen Rehbock
Assistant to the Director
Institute for Astronomy
University of Hawaii at Manoa
1-808-956-6829
rehbock@ifa.hawaii.edu

Electronic version:
http://www.ifa.hawaii.edu/info/press-releases/Norbert-9-07/IceAgesOnMars.html

New Theory Explains Ice on Mars

Wobbles on Mars cause ice ages that are much more
dramatic than those on Earth, says astronomer
Norbert Schorghofer of the University of Hawaii.

Thanks to our large, stabilizing Moon, Earth's
rotation axis is always tilted by about 23
degrees. The tilt of Mars, however, can wobble by
as much as10 degrees from its current 25 degrees.
Wobbles cause big changes in the amount of
sunlight reaching different parts of Mars, so
vast amounts of ice shift between the poles and
the rest of the planet every 120,000 years.

Schorghofer's new theory appears in the September
13 issue of the journal Nature.

"We expect to see two types of ground ice when
the Phoenix Lander spacecraft arrives at Mars in
2008," says Schorghofer, "ice that formed on the
surface and was then buried, and ice hidden in
porous soil."

During the 19th century, scientists discovered
that Earth experienced ice ages. In the past few
years, spacecraft have discovered that ice ages
also occurred on Mars, but scientists have been
puzzled because more ice than expected has
survived far from the polar caps. What is left is
now thought to be a combination of old ice from
the last major glaciation and younger ice that
formed later and in a way entirely different from
the way ice formed on Earth.

The new theory sheds light on the history of vast
ice-rich areas, which once covered most of Mars.
Around 4 to 5 million years ago, ice accumulated
from extensive snowfall outside the martian polar
caps. The new theory describes what happened to
this ice as the rotation axis of Mars continued
to wobble over the last few million years.

Surface temperature and atmospheric humidity
changed because of varying sunlight. When the
climate was dry, the ice receded to a greater
depth or disappeared entirely except at the
highest latitudes. Dust contained in retreating
ice eventually covered the ice, making it no
longer visible on the surface.

So much of this subsurface ice has been detected
that its only plausible origin was thought to be
massive snowfall. However, Schorghofer's theory
suggests that a lot of that snowfall ice has
since been lost to the atmosphere. It has been
replaced by a new layer of ice, formed not from
snowfall, since the climate had meanwhile turned
less humid, but by diffusion of water vapor into
the soil. Atmospheric vapor can freeze inside the
soil and form "pore-ice," which is mainly soil
with some ice in pore spaces.

As the planet's tilt toward the sun went back and
forth, the climate kept changing between dry and
humid, causing many cycles of ice retreat and
formation. Today we are left with two kinds of
ground ice: the old massive ice sheet and very
recent pore-ice.

Schorghofer is part of the multidisciplinary UH
Astrobiology Institute, which is sponsored by
NASA and managed through the Institute for
Astronomy. Its research focuses on water as the
habitat of, and chemical enabler for, life.

Figure captions:

Figure 1. The two types of ice found on Mars, by
latitude. Dry soil covers both types of ice.

Figure 2. The history of subsurface ice layers on
Mars over the last few million years. The tilt of
the rotation axis changes with time, and the
planet periodically experiences dry and humid
climates.

The NASA Astrobiology Institute (NAI), founded in
1998, is a partnership between NASA, 16 major
U.S. teams, and five international consortia.
NAI's goal is to promote, conduct, and lead
integrated multidisciplinary astrobiology
research and to train a new generation of
astrobiology researchers. For more information,
see http://nai.nasa.gov/.

The Institute for Astronomy at the University of
Hawaii at Manoa conducts research into galaxies,
cosmology, stars, planets, and the sun. Its
faculty and staff are also involved in astronomy
education, deep space missions, and in the
development and management of the observatories
on Haleakala and Mauna Kea.

Established in 1907 and fully accredited by the
Western Association of Schools and Colleges, the
University of Hawaii is the state's sole public
system of higher education. The UH System
provides an array of undergraduate, graduate, and
professional degrees and community programs on 10
campuses and through educational, training, and
research centers across the state. UH enrolls
more than 50,000 students from Hawaii, the U.S.
mainland, and around the world.

###


Posted by BradGuth on September 16, 2007, 9:06 pm
Please log in for more thread options
On Sep 14, 5:17 pm, baa...@earthlink.net wrote:
> Embargoed until 1 p.m. Eastern Time (7 a.m. HST), September 12, 2007
>
> Contacts:
>
> Dr. Norbert Schorghofer
> Institute for Astronomy
> University of Hawaii at Manoa
> Honolulu, Hawaii 96822
> 1-808-956-9086
> no...@ifa.hawaii.edu
>
> Mrs. Karen Rehbock
> Assistant to the Director
> Institute for Astronomy
> University of Hawaii at Manoa
> 1-808-956-6829
> rehb...@ifa.hawaii.edu
>
> Electronic
version:http://www.ifa.hawaii.edu/info/press-releases/Norbert-9-07/IceAgesOnM...
>
> New Theory Explains Ice on Mars
>
> Wobbles on Mars cause ice ages that are much more
> dramatic than those on Earth, says astronomer
> Norbert Schorghofer of the University of Hawaii.
>
> Thanks to our large, stabilizing Moon, Earth's
> rotation axis is always tilted by about 23
> degrees. The tilt of Mars, however, can wobble by
> as much as10 degrees from its current 25 degrees.
> Wobbles cause big changes in the amount of
> sunlight reaching different parts of Mars, so
> vast amounts of ice shift between the poles and
> the rest of the planet every 120,000 years.
>
> Schorghofer's new theory appears in the September
> 13 issue of the journal Nature.
>
> "We expect to see two types of ground ice when
> the Phoenix Lander spacecraft arrives at Mars in
> 2008," says Schorghofer, "ice that formed on the
> surface and was then buried, and ice hidden in
> porous soil."
>
> During the 19th century, scientists discovered
> that Earth experienced ice ages. In the past few
> years, spacecraft have discovered that ice ages
> also occurred on Mars, but scientists have been
> puzzled because more ice than expected has
> survived far from the polar caps. What is left is
> now thought to be a combination of old ice from
> the last major glaciation and younger ice that
> formed later and in a way entirely different from
> the way ice formed on Earth.
>
> The new theory sheds light on the history of vast
> ice-rich areas, which once covered most of Mars.
> Around 4 to 5 million years ago, ice accumulated
> from extensive snowfall outside the martian polar
> caps. The new theory describes what happened to
> this ice as the rotation axis of Mars continued
> to wobble over the last few million years.
>
> Surface temperature and atmospheric humidity
> changed because of varying sunlight. When the
> climate was dry, the ice receded to a greater
> depth or disappeared entirely except at the
> highest latitudes. Dust contained in retreating
> ice eventually covered the ice, making it no
> longer visible on the surface.
>
> So much of this subsurface ice has been detected
> that its only plausible origin was thought to be
> massive snowfall. However, Schorghofer's theory
> suggests that a lot of that snowfall ice has
> since been lost to the atmosphere. It has been
> replaced by a new layer of ice, formed not from
> snowfall, since the climate had meanwhile turned
> less humid, but by diffusion of water vapor into
> the soil. Atmospheric vapor can freeze inside the
> soil and form "pore-ice," which is mainly soil
> with some ice in pore spaces.
>
> As the planet's tilt toward the sun went back and
> forth, the climate kept changing between dry and
> humid, causing many cycles of ice retreat and
> formation. Today we are left with two kinds of
> ground ice: the old massive ice sheet and very
> recent pore-ice.
>
> Schorghofer is part of the multidisciplinary UH
> Astrobiology Institute, which is sponsored by
> NASA and managed through the Institute for
> Astronomy. Its research focuses on water as the
> habitat of, and chemical enabler for, life.
>
> Figure captions:
>
> Figure 1. The two types of ice found on Mars, by
> latitude. Dry soil covers both types of ice.
>
> Figure 2. The history of subsurface ice layers on
> Mars over the last few million years. The tilt of
> the rotation axis changes with time, and the
> planet periodically experiences dry and humid
> climates.
>
> The NASA Astrobiology Institute (NAI), founded in
> 1998, is a partnership between NASA, 16 major
> U.S. teams, and five international consortia.
> NAI's goal is to promote, conduct, and lead
> integrated multidisciplinary astrobiology
> research and to train a new generation of
> astrobiology researchers. For more information,
> seehttp://nai.nasa.gov/.
>
> The Institute for Astronomy at the University of
> Hawaii at Manoa conducts research into galaxies,
> cosmology, stars, planets, and the sun. Its
> faculty and staff are also involved in astronomy
> education, deep space missions, and in the
> development and management of the observatories
> on Haleakala and Mauna Kea.
>
> Established in 1907 and fully accredited by the
> Western Association of Schools and Colleges, the
> University of Hawaii is the state's sole public
> system of higher education. The UH System
> provides an array of undergraduate, graduate, and
> professional degrees and community programs on 10
> campuses and through educational, training, and
> research centers across the state. UH enrolls
> more than 50,000 students from Hawaii, the U.S.
> mainland, and around the world.
>
> ###

A better theory; Mars no longer has any significant cache of fresh
water ice, and there's hardly any remains of salt. Go figure.
- Brad Guth -


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