IPB
X   Site Message
(Message will auto close in 2 seconds)

Welcome Guest ( Log In | Register )

T8 Radar Releases
volcanopele
post Nov 1 2005, 06:34 PM
Post #101


Senior Member
****

Group: Moderator
Posts: 3242
Joined: 11-February 04
From: Tucson, AZ
Member No.: 23



The RADAR team today released portions of the SAR swath acquired during the T8 encounter Friday morning. For reference, a map of their coverage is available at :

http://pirlwww.lpl.arizona.edu/~perry/T8_RADAR_coverage.jpg

I will be updating this map to include boxes showing the locations of the sections released.

Tectonic Features
http://photojournal.jpl.nasa.gov/catalog/PIA03566
This image shows feature in the central part of Adiri. For comparison, check out the Huygens landing site map using VIMS data released in January. The areas covered in cat scratches in this RADAR view are the dark features seen in the middle of Adiri near center left in the VIMS mosaic. The somewhat lighter band running from top to bottom in the RADAR view just left of center is the bright north-stripe in the middle of the dark patch in the VIMS view. Other cat scratchless areas in the RADAR view correspond to bright albedo features in VIMS and ISS.

Note here chains of ridges and hills within Adiri, suggesting tectonic activity. The ring of material at far left may be a degraded crater but that hasn't been confirmed.

Dunes Galore
http://photojournal.jpl.nasa.gov/catalog/PIA03567
This image shows cat scratches, thought to be longitudinal dunes, in southeastern Senkyo. Again, in the equatorial regions of Titan, we see these dunes covering much of the landscape. You can see stream line forms assocated with aeolian erosion (not caused by liquid methane flow, these dunes are WAY too big for that).

Diverse Geology
http://photojournal.jpl.nasa.gov/catalog/PIA03568
This image covers several large islands in the divide between Senyko and Belet. Note the dark, stubby channel terminator in good sized smooth region without cat scratches. So there is at least some evidence for fluid flow in the equatorial regions.

Pinpointing Huygens Landing Site
http://photojournal.jpl.nasa.gov/catalog/PIA03569
This composite shows the Huygens landing site region. Note that the position may shift slightly over time, probably slightly to the north east, as I think the island to the north of the current position is the large island seen in Huygens images. The two cat scratches seen in the RADAR swath north of the landing site maybe the two dark lines seen in Rene's mosaic. Definitely will need confirmation of this. Note once again the prevalence of dunes north of the landing site, forming stream-lined forms (once again let me stress that the fluid is the atmosphere).


--------------------
&@^^!% Jim! I'm a geologist, not a physicist!
The Gish Bar Times - A Blog all about Jupiter's Moon Io
Go to the top of the page
 
+Quote Post

Posts in this topic
- volcanopele   T8 Radar Releases   Nov 1 2005, 06:34 PM
2 Pages V  < 1 2


Reply to this topicStart new topic

 



RSS Lo-Fi Version Time is now: 15th December 2024 - 10:47 PM
RULES AND GUIDELINES
Please read the Forum Rules and Guidelines before posting.

IMAGE COPYRIGHT
Images posted on UnmannedSpaceflight.com may be copyrighted. Do not reproduce without permission. Read here for further information on space images and copyright.

OPINIONS AND MODERATION
Opinions expressed on UnmannedSpaceflight.com are those of the individual posters and do not necessarily reflect the opinions of UnmannedSpaceflight.com or The Planetary Society. The all-volunteer UnmannedSpaceflight.com moderation team is wholly independent of The Planetary Society. The Planetary Society has no influence over decisions made by the UnmannedSpaceflight.com moderators.
SUPPORT THE FORUM
Unmannedspaceflight.com is funded by the Planetary Society. Please consider supporting our work and many other projects by donating to the Society or becoming a member.