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Mauna Kea, Hawaii – December 15, 2004:
Using adaptive optics on the
telescopes on Mauna Kea, Hawai'i,
a U.S. team has discovered a new phenomenon in the atmosphere of Saturn's largest moon Titan.
Unlike previous observations showing storms at the south pole,
these new images reveal atmospheric disturbances at Titan's temperate mid latitudes –
about halfway between the equator and the poles.
Explaining the unexpected activity has proven difficult,
and the team speculates that the storms could be driven by
anything from short-term surface events to shifts in global wind patterns.
"We were fortunate to catch these new mid-latitude clouds when they first appeared in early 2004," said team leader Henry Roe (California Institute of Technology). "We are not yet certain how their formation is triggered. Continued observations over the next few years will show us whether these clouds are the result of a seasonal change in weather patterns or a surface-related phenomenon."
The causes of these storms might include activities that disturb the atmosphere from the surface. It's
possible that geysers of methane "slush" are brewing from below,
or a warm spot on Titan's surface is heating the atmosphere.
Cryovolcanism – volcanic activity that spews an icy mix of chemicals –
has also been suggested as one mechanism that would cause disturbances.
It's also possible that the storms are driven by
seasonal shifts in the global winds that circulate in the upper atmosphere.
Hints about what is happening on this frigid world could be
obtained as the Huygens probe from the
Cassini mission drops through Titan's atmosphere in mid-January, 2005.
Astronomers using Gemini North telescope and the Keck II observatory
observed these mid-latitude features at Saturn's largest moon,
and the solar system's second largest moon, Titan.
All images are from NIRI/Altair on
except December 2003 and September 2004,
which are from Keck II.
Sub-observer longitude and latitude are given. All images are scaled to show Titan at the same size, although its angular diameter ranged between 0.73–0.88 arcseconds.
In the stratospheric probing images only the limb-brightened stratospheric haze is visible, with a seasonal north-south asymmetry. In the tropospheric probing images the stratospheric hazes appear limb-brightened, with a general brightening in the south due to the tropopause cirrus, the distinct south polar clouds (see especially 9 April, although a cloud is near the south pole in every one of these images), and the new ~40 degrees south clouds, which are especially apparent on 8–9 April, 4 May, and 2 September. The new temperate-latitude clouds are indicated with white arrows. In the surface-probing images Titan's 22.5 degree-per-day rotation rate is apparent and the tropospheric clouds are also evident.
Image: Gemini Observatory
The Gemini-Keck II observations were the result of good timing and telescope availability.
scientist Chad Trujillo, Titan's weather patterns can be stable for many months,
with only occasional bursts of unusual activity like these recently discovered atmospheric features.
The chances of catching such occurrences depend largely on the
availability of flexible scheduling like that used at
"This flexible scheduling is absolutely critical to Titan meteorology studies," he said.
"Imagine how hard it would be to understand the
Earth's diverse meteorological phenomena if you only saw a weather report a few nights every year."
Like Earth, Titan is surrounded by a thick atmosphere of mostly nitrogen. Conditions on Earth allow water to exist in liquid, solid, or vapor states, depending on localized temperatures and pressures. The phase changes of water between these states are an important factor in the formation of weather in our atmosphere. Titan's atmosphere is so cold that any water is frozen solid, but conditions are such that methane can move between liquid, solid, and gaseous states. This leads to a methane meteorological cycle on Titan in analogy to the water-based weather cycle on Earth.
As it does on Earth, seasonal solar heating can drive atmospheric activity on Titan, and this could be the mechanism behind the previously observed south polar clouds. However, the new temperate-latitude cloud formations cannot be explained by the same solar heating process If a seasonal circulation shift is causing the newly discovered features, the team theorizes that they will drift northward over the next few years as Titan's year progresses through the southern summer and into autumn. If it is being caused by geological changes, such as methane geysers or a geologic "warm" spot on the surface, the feature should stay at the observed 40-degree latitude as the surface activity spurs changes in atmospheric convection and methane cloud formation. Continued storm formations will be easily distinguishable in future ground-based observations using Gemini, Keck and other adaptive-optics enabled telescopes.
"Using adaptive optics from the Earth allows us to see things that just a few years ago would have been invisible," said Keck Scientist Antonin Bouchez. "These observations show that ground-based telescopes are a perfect complement to space missions like Cassini."
Art Poster Metal Framed Print
Starfire Adaptive Optics Telescope
Poster Size: 16 x 20 in
(Unframed), (Wood Framed)
H.G. Roe, A.H. Bouchez, C.A. Trujillo, E.L. Schaller and M.E. Brown,
"Discovery of Temperate Latitude Clouds on Titan," Ap. J. Lett. 618, L49–L52 (2005)
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