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Mauna Kea, Hawaii – August 12, 2009:
While far from a tropical rain forest, the equatorial region of Saturn’s largest moon, Titan,
has recently displayed tantalizing evidence that the parched, dry,
ultra-frigid desert can support large-scale storms.
The research, published in the August 13, 2009 issue of the journal
announces the discovery of significant cloud formation (about three million square kilometers)
within the moon’s tropical zone near its equator. Prior to this event (in April 2008)
it was not known whether significant cloud formation was possible in Titan’s tropical regions.
This activity in Titan’s tropics and mid-latitudes also seems to have triggered
subsequent cloud development at the moon’s south pole
where it was considered improbable due to the Sun’s seasonal angle relative to Titan.
The evidence comes from a team of US astronomers using the Gemini North telescope and NASA’s Infrared Telescope Facility (IRTF) both on Hawaii’s Mauna Kea. “We obtain frequent observations with IRTF giving us a ‘weather report’ of sorts for Titan. When the IRTF observations indicate that cloud activity has increased, we are able to trigger the next night on the Gemini telescope to determine where on Titan the clouds are located,” said team member Emily Schaller of the University of Hawai‘i (when this work was conducted). In fact, in the past eight years of monitoring at Gemini no significant clouds over Titan’s tropical regions were spotted.
This image of the clouds on Titan (bright area, lower right)
was taken with the Gemini North telescope adaptive optics system on April 15, 2008.
Image: Gemini Observatory / AURA;
E. Schaller et al.
Titan, the solar system’s second largest moon,
has received considerable attention by scientists since
NASA’s Cassini mission deployed the Huygens probe
that descended through the moon’s atmosphere in January 2005.
During its descent, the probe’s cameras
revealed small-scale channels and what appear to be stream beds
in the equatorial regions that seemed to contradict atmospheric models
predicting extremely dry desert-like conditions near the equator.
Until now these erosional (fluvial) features have been explained
by the possibility of liquid methane seeping out of the ground.
"In April 2008 we observed what was a global event that shows how storm activity in one region can trigger clouds,
and probably rainfall, over arid regions, such as the tropics where Huygens landed,"
said team member Henry Roe from
"Of course these rain showers are not liquid water like here on Earth,
but are instead made of liquid methane.
Just like the streambeds and channels that are carved by liquid water on Earth,
we see features on Titan that have been created by flowing liquid methane."
Unlike the Earth, on Titan, where the temperature is some −178°C, methane (or natural gas) is a liquid and it is the dominant driver of the moon’s weather and surface erosion. Any water on Titan is frozen on or below the moon’s frigid surface and resemble rocks or boulders on Titan's surface.
Mid-latitude and polar cloud formations have been observed for many years (by this team and others)
but the combination of extensive monitoring at the
with rapid follow-up using
allowed the team to capture the process as it unfolded near the equator.
The team monitored Titan on 138 nights over 2.2 years
and during that time cloud cover was well under one percent.
Then, mid-April of 2008, just after team member and
Ph.D. candidate Schaller had handed in her doctoral dissertation focusing on
Titan’s minimal cloud cover she noticed the dramatic increase in cloud cover.
During this three-week episode clouds forming at about 30 degrees south latitude were observed, followed several days later by clouds closer to the equator and at the moon’s south pole. The apparent connection between the cloud formations leads to the possibility that cloud formation in one area of the moon can instigate clouds in other areas by a process known as atmospheric teleconnections. This same phenomena occurs in the Earth’s atmosphere and is caused by what are called planetary Rossby waves which are well understood.
The high-resolution Gemini images of Titan were all obtained with adaptive optics technology which uses a deformable mirror to remove distortions to light caused by the Earth’s atmosphere and produce images showing remarkable detail in the tiny disk of the moon. “Without this technology this discovery would be impossible from the surface of the Earth,” said Schaller.
Currently the Cassini spacecraft is orbiting Saturn but only flies by Titan once every 6 weeks or so. This makes continuous ground-based monitoring important for studying features like these with shorter periods on the order of 3-weeks – like this storm.
E.L. Schaller, H.G. Roe, T. Schneider and M.E. Brown,
"Storms in the tropics of Titan," Nature 460, 873–875 (2009)
Methane Clouds Discovered at South Pole of Saturn's Moon Titan, Dec 2002.
New Clouds Add to Titan's Mystery, Dec 2004.
Ground-Based AO Observations Of Titan Back Up Huygens Probe Landing, Feb 2005.
Methane Drizzle On Saturn's Moon Titan, Oct 2007.
Full Press Release:
U. of Hawaii
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