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Titan Has Liquid Lakes, Scientists Report in Nature

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Titan Has Liquid Lakes, Scientists Report in Nature baalke 01-03-2007
Posted by baalke on January 3, 2007, 6:58 pm
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http://www.jpl.nasa.gov/news/features.cfm?feature=1258

Titan Has Liquid Lakes, Scientists Report in Nature
January 03, 2007

Scientists report definitive evidence of the presence of lakes filled
with liquid methane on Saturn's moon Titan in this week's journal
Nature
cover story.

Radar imaging data from a July 22, 2006, flyby provide convincing
evidence for large bodies of liquid on Titan today. A new false-color
radar view gives a taste of what Cassini saw. Some highlights of the
article follow below.

Lake Characteristics:

-Radar-dark patches are interpreted as lakes based on their very low
radar reflectivity and morphological similarities to lakes, including
associated channels and location in topographic depressions.

-Radar-dark surfaces are smooth and most likely liquid, rock, ice or
organics. More than 75 radar-dark patches or lakes were seen, ranging
from 3 kilometers (1.8 miles) to more than 70 kilometers (43 miles)
across.

-Some lakes appear partly dry, while others seem liquid-filled. Some of
the partly filled lakes may never have filled fully, or may have partly
evaporated at some point in the past. The dry lakes have margins or
rims
and a radar brightness similar to the rest of the surrounding terrain,
making them appear devoid of liquid.

-The varying states of how full the lakes are suggest that lakes in
this
region of Titan might be temporary on some unknown timescale.

-Approximately 15 of the dark patches seem filled and show no clear
evidence of erosion. These dark patches resemble terrestrial lakes
confined within impact basins (for example, Clearwater Lakes in Canada)
or within volcanic calderas (for example, Crater Lake, Oregon). The
nest-like nature of these lakes and their limited range of sizes make
it
unlikely that they originated from an impact. A volcanic origin for the
depressions is possible, given their appearance.

-Some lakes have steep margins and very distinct edges, suggesting a
topographic rim. These lakes are consistent with seepage or groundwater
drainage lakes.

-Other lakes have diffuse, more scalloped edges, with a gradual
decrease
in radar brightness towards the center of the lake. These lakes are
more
likely to be associated with channels, and may be either drainage lakes
or groundwater drainage lakes.

-Yet other lakes have curvy channel-like extensions, similar in
appearance to terrestrial flooded river valleys (for example Lake
Powell).

-Bright patches near the lake edges could be small islands peeking
through the surface. Floating icebergs are unlikely because most
materials would not float in liquid hydrocarbons.

Other Observations:

-Based on the lake characteristics, Cassini scientists think they are
observing liquid-filled lakes on Titan today. Another possibility is
that these depressions and channels formed in the past and have now
been
filled by a low-density deposit that is darker than any observed
elsewhere on Titan. However, the absence of wind-blown features in this
area makes the low-density hypothesis unlikely.

-These northern hemisphere lakes are the strongest evidence yet that
Titan's surface and atmosphere have an active hydrological cycle,
though
with a condensable liquid other than water. In this cycle, lakes are
filled through methane rainfall or intersect with a subsurface layer
saturated with liquid methane.

-As Titan's seasons progress over the 29-year cycle of Saturn's orbit
around the sun, lakes in the winter hemisphere should expand by steady
methane rain, while summer hemisphere lakes shrink or dry up entirely.

To read more about the radar imaging data from the July 2006 flyby, go
to Cassini Finds Lakes on Titan's Arctic Region
<http://www.jpl.nasa.gov/news/news.cfm?release=2006-097> .

-------------------------------------------------------------

Media contact: Carolina Martinez/JPL
818-354-9382


Posted by Chris on January 5, 2007, 7:13 am
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Carbon + energy = biology, is there any biology on Titan?


> http://www.jpl.nasa.gov/news/features.cfm?feature=1258
>
> Titan Has Liquid Lakes, Scientists Report in Nature
> January 03, 2007
>
> Scientists report definitive evidence of the presence of lakes filled
> with liquid methane on Saturn's moon Titan in this week's journal
> Nature
> cover story.
>
> Radar imaging data from a July 22, 2006, flyby provide convincing
> evidence for large bodies of liquid on Titan today. A new false-color
> radar view gives a taste of what Cassini saw. Some highlights of the
> article follow below.
>
> Lake Characteristics:
>
> -Radar-dark patches are interpreted as lakes based on their very low
> radar reflectivity and morphological similarities to lakes, including
> associated channels and location in topographic depressions.
>
> -Radar-dark surfaces are smooth and most likely liquid, rock, ice or
> organics. More than 75 radar-dark patches or lakes were seen, ranging
> from 3 kilometers (1.8 miles) to more than 70 kilometers (43 miles)
> across.
>
> -Some lakes appear partly dry, while others seem liquid-filled. Some of
> the partly filled lakes may never have filled fully, or may have partly
> evaporated at some point in the past. The dry lakes have margins or
> rims
> and a radar brightness similar to the rest of the surrounding terrain,
> making them appear devoid of liquid.
>
> -The varying states of how full the lakes are suggest that lakes in
> this
> region of Titan might be temporary on some unknown timescale.
>
> -Approximately 15 of the dark patches seem filled and show no clear
> evidence of erosion. These dark patches resemble terrestrial lakes
> confined within impact basins (for example, Clearwater Lakes in Canada)
> or within volcanic calderas (for example, Crater Lake, Oregon). The
> nest-like nature of these lakes and their limited range of sizes make
> it
> unlikely that they originated from an impact. A volcanic origin for the
> depressions is possible, given their appearance.
>
> -Some lakes have steep margins and very distinct edges, suggesting a
> topographic rim. These lakes are consistent with seepage or groundwater
> drainage lakes.
>
> -Other lakes have diffuse, more scalloped edges, with a gradual
> decrease
> in radar brightness towards the center of the lake. These lakes are
> more
> likely to be associated with channels, and may be either drainage lakes
> or groundwater drainage lakes.
>
> -Yet other lakes have curvy channel-like extensions, similar in
> appearance to terrestrial flooded river valleys (for example Lake
> Powell).
>
> -Bright patches near the lake edges could be small islands peeking
> through the surface. Floating icebergs are unlikely because most
> materials would not float in liquid hydrocarbons.
>
> Other Observations:
>
> -Based on the lake characteristics, Cassini scientists think they are
> observing liquid-filled lakes on Titan today. Another possibility is
> that these depressions and channels formed in the past and have now
> been
> filled by a low-density deposit that is darker than any observed
> elsewhere on Titan. However, the absence of wind-blown features in this
> area makes the low-density hypothesis unlikely.
>
> -These northern hemisphere lakes are the strongest evidence yet that
> Titan's surface and atmosphere have an active hydrological cycle,
> though
> with a condensable liquid other than water. In this cycle, lakes are
> filled through methane rainfall or intersect with a subsurface layer
> saturated with liquid methane.
>
> -As Titan's seasons progress over the 29-year cycle of Saturn's orbit
> around the sun, lakes in the winter hemisphere should expand by steady
> methane rain, while summer hemisphere lakes shrink or dry up entirely.
>
> To read more about the radar imaging data from the July 2006 flyby, go
> to Cassini Finds Lakes on Titan's Arctic Region
> <http://www.jpl.nasa.gov/news/news.cfm?release=2006-097> .
>
> -------------------------------------------------------------
>
> Media contact: Carolina Martinez/JPL
> 818-354-9382
>



Posted by Sjouke Burry on January 5, 2007, 5:05 pm
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Chris wrote:
> Carbon + energy = biology, is there any biology on Titan?
>
temperature is a bit low, sunlight is rather weak,
I think any unicellular life there has frostbite.
Google says -187 degree celcius, so that should stop
pretty much most forms of chemical reactions.

Posted by Kevin on January 7, 2007, 3:37 am
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> Chris wrote:
>> Carbon + energy = biology, is there any biology on Titan?
>>
> temperature is a bit low, sunlight is rather weak,
> I think any unicellular life there has frostbite.
> Google says -187 degree celcius, so that should stop
> pretty much most forms of chemical reactions.

I certainly agree that the odds are pretty strongly against
life there, but I'm not prepared to rule it out. I can imagine
bacterial-grade organisms with slow metabolism, reproducing much
more slowly than terrestrial bacteria.


Kevin

Posted by Sean on January 7, 2007, 10:15 pm
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Kevin wrote:
>
>>Chris wrote:
>>
>>>Carbon + energy = biology, is there any biology on Titan?
>>>
>>
>>temperature is a bit low, sunlight is rather weak,
>>I think any unicellular life there has frostbite.
>>Google says -187 degree celcius, so that should stop
>>pretty much most forms of chemical reactions.
>
>
> I certainly agree that the odds are pretty strongly against
> life there, but I'm not prepared to rule it out. I can imagine
> bacterial-grade organisms with slow metabolism, reproducing much
> more slowly than terrestrial bacteria.
>
>
> Kevin

It's an interesting thought. Given the far slower reactions that would
occur under the circumstances, there may, repeat may, be protolife
similar to that found on earth at the dawn of life here. Whether such
molecular structures would have become self replicating is another
matter entirely. At those temperatures, it's hard to see how such
energy hungry reactions could occur.

Sean

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