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Possible Crater at Zal Montes |
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When looking at images of Zal Patera and Zal Montes, I noticed a bowl shaped depression in the southern part of the Zal Montes "Plateau." Based on these images the crater is 7 km across and 1-2 km deep. The crater appears to be a simple bowl crater. This is the same as similar sized craters on the moon. It now appears to be a sinkhole formed after an explosive sapping event at the cliff that borders the north part of the crater. Here are some of my comments on it from my posts on Jupiter_List: From May 17, 2000 "Near the eastern end of this cliff appears to be the only obvious impact crater yet found on Io. It is 5-10 km across? and appears to have a bowl shape with a flat bottom. I hope to get more size constraints later, but it is definitely larger than the 1.5 km I reported earlier. " From May 9, 2000 "First off, none of the craters I have found are very
large; the largest being 1.5-2 km across. Secondly, they all occur on
From May 17, 2000 "I have a better size constraint for the crater at Zal. It appears to be 4-6 km across, but since I have nothing to compare it too in that mosaic, it could be as large as 14 km wide." From May 30, 2000 "Based on new info I received
last night, I am beginning to doubt the identification of the bowl structure
on the Zal Montes Plateau as an impact crater. A few weeks ago when
I announced my discovery of the crater, I also mentioned another possible
cause of the crater. I said since the crater was near a cliff, and
other cliffs on the same mountain have features that indicate sapping
has occured, I said it was possible that the crater was caused by sapping
at the cliff. This new info confirms to me that craters do form
when sapping occurs rapidly. This "explosive sapping"
leaves a cavity where the SO2 once was and a sink hole forms to fill the
cavity. This forms a crater. However, there are few problems that
still bother me about this crater being caused by sapping. Even
though other cliffs on the Zal Montes Plateau have undergone sapping,
the cliff that the crater is near does not show any other signs of sapping.
The cliff is straight and has none of the tailtell bright SO2 frosts that
often are associated with sapping cliffs on Io. Also, no other crater
like this has been found From June 6, 2000: "I was messing with the Solar System Collisions website, http://janus.astro.umd.edu/astro/impact.html , and based on what I have figured there, I believe I have determinged the size of the comet that struck Zal Montes "plateau." Assuming an impact speed of 35 km/sec. and that the impactor is a comet, the size of hte comet would be 370 meters in diameter. A bit smaller than I thought. I now have a definitive size for the crater. Drumroll please...the crater on Zal Montes "plateau" is 7 km across. This is based on "counting pixels" form the two images of the crater from I25. I then averaged the two figures and multiplied the resulting number by 260 m/pixel. The precise figure is 7020 meters. This size is the same as En-zu on Ganymede." From June 9, 2000: As most of you know, I have been harping for the past few
weeks on this list about a possible impact crater on Zal Montes "plateau."
Well, I got a message back from Dr. Paul Geissler today. This was
the message he sent me: From September 24, 2000: Here is a message I sent to the Outer Planets Mailing List that was directed to a newly joined member of the list, Jeffery Moore of the Ames Research Center: "A few months ago, there was a discussion on this list
about N. Zal Montes and I would like to ask what your opinion on this
is. In the southern part of the plateau, there is what appears to be a
crater- like feature. It appears to border a cliff and a trench. Now we
came up with two explainations for it. One is that it is the only crater
found on Io. It appears to be oblong but still would still be a simple
bowl crater, consistent with a crater its size (~7 km). The other is that
this is some kind of sinkhole formed after an explosive sapping event
at the cliff north of the pit. These are replies to this request for information on the Zal Montes pit. This is from Alex Blackwell, a planetary geologist at the University of Hawaii: "FWIW, I do not think it is an impact feature. There is a plateau formation that abuts the depression and that is topographically controlled by it. IOW, the depression appears to postdate the plateau. Although our knowledge of the surface properties of Io is very limited, it seems logical that an impactor that produces a 7 km excavation would probably have produced much more extensive modification of the surrounding terrain or obliterated the plateau." This is from Jeffery Moore, a planetary geologist at NASA's Ames Research Center: "We have asked ourselves that question but came up with no definitive answer. If it is an impact crater, then subsequent flows have covered its ejecta facies. Sinkholes and explosion craters are equally viable and equivocal." I have three images of the Crater at Zal: Last updated November 11, 2000 by Jason Perry volcanopele@netzero.net. |