[meteorite-list] Odd Spot on Titan Baffles Scientists

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Wed May 25 17:46:40 2005
Message-ID: <200505252146.j4PLk0G21042_at_zagami.jpl.nasa.gov>

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov

Carolina Martinez (818) 354-9382
Jet Propulsion Laboratory, Pasadena, Calif.

Lori Stiles (520) 626-4402
University of Arizona News Service, Tucson

Preston Dyches (720) 974-5859
Cassini Imaging Central Laboratory for Operations
Space Science Institute, Boulder, Colo.

News Release: 2005-086 May 25, 2005

Odd Spot on Titan Baffles Scientists

Saturn's moon Titan shows an unusual bright spot that
has scientists mystified. The spot, approximately the
size and shape of West Virginia, is just southeast of
the bright region called Xanadu and is visible to
multiple instruments on the Cassini spacecraft.

The 483-kilometer-wide (300-mile) region may be a "hot"
spot -- an area possibly warmed by a recent asteroid
impact or by a mixture of water ice and ammonia from a
warm interior, oozing out of an ice volcano onto colder
surrounding terrain. Other possibilities for the
unusual bright spot include landscape features holding
clouds in place or unusual materials on the surface.

"At first glance, I thought the feature looked strange,
almost out of place," said Dr. Robert H. Brown, team
leader of the Cassini visual and infrared mapping
spectrometer and professor at the Lunar and Planetary
Laboratory, University of Arizona, Tucson. "After
thinking a bit, I speculated that it was a hot spot. In
retrospect, that might not be the best hypothesis. But
the spot is no less intriguing."

The Cassini spacecraft flew by Titan on March 31 and
April 16. Its visual and infrared mapping spectrometer,
using the longest, reddest wavelengths that the
spectrometer sees, observed the spot, the brightest
area ever observed on Titan.

Cassini's imaging cameras saw a bright, 550-kilometer-wide
(345-mile) semi-circle at visible wavelengths at this same
location on Cassini's December 2004 and February 2005 Titan
flybys.

"It seems clear that both instruments are detecting the same
basic feature on or controlled by Titan's surface," said
Dr. Alfred S. McEwen, Cassini imaging team scientist, also
of the University of Arizona. "This bright patch may be due
to an impact event, landslide, cryovolcanism or atmospheric
processes. Its distinct color and brightness suggest that it
may have formed relatively recently."

Other bright spots have been seen on Titan, but all have been
transient features that move or disappear within hours, and
have different spectral (color) properties than this feature.
This spot is persistent in both its color and location. "It's
possible that the visual and infrared spectrometer is seeing a
cloud that is topographically controlled by something on the
surface, and that this weird, semi-circular feature is causing
this cloud," said Dr. Elizabeth Turtle, Cassini imaging
team associate, also from the Lunar and Planetary Laboratory.

"If the spot is a cloud, then its longevity and stability imply
that it is controlled by the surface. Such a cloud might result
from airflow across low mountains or outgassing caused by
geologic activity," said Jason Barnes, a postdoctoral researcher
working with the visual and infrared mapping spectrometer team
at the University of Arizona.

The spot could be reflected light from a patch of terrain made
up of some exotic surface material. "Titan's surface seems to be
mostly dirty ice. The bright spot might be a region with
different surface composition, or maybe a thin surface deposit
of non-icy material," Barnes added.

Scientists have also considered that the spot might be mountains.
If so, they'd have to be much higher than the 100-meter-high
(300-foot) hills Cassini's radar altimeter has seen so far.
Scientists doubt that Titan's crust could support such high
mountains.

The visual and infrared mapping spectrometer team will be able
to test the hot spot hypothesis on the July 2, 2006, Titan flyby,
when they take nighttime images of the same area. If the spot
glows at night, researchers will know it's hot.

For more information about the Cassini-Huygens mission visit
http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini .
For additional images visit the visual and infrared mapping
spectrometer page at http://wwwvims.lpl.arizona.edu and the
Cassini imaging team homepage
http://ciclops.org .

The Cassini-Huygens mission is a cooperative project of NASA,
the European Space Agency and the Italian Space Agency. The
Jet Propulsion Laboratory, a division of the California
Institute of Technology in Pasadena, manages the mission for
NASA's Science Mission Directorate, Washington, D.C. The Cassini
orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The visual and infrared mapping spectrometer
team is based at the University of Arizona. The imaging team is
based at the Space Science Institute in Boulder, Co.

- end -
Received on Wed 25 May 2005 05:46:00 PM PDT