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Ariel at Voyager Closest Approach
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Alliance Member Comments
Dragon_of_Luck_Mah_Jonng1971 (Aug 14, 2009 at 5:30 PM):
(Of course 'features' , not 'featurs' .)
Dragon_of_Luck_Mah_Jonng1971 (Aug 14, 2009 at 5:13 PM):
Thank you for your observation, kheider.
Because of your observation I examined all Voyager 2 pictures of the 5 large Uranian satellites for this feature. I believe very much that they are image processing facts -- no real featurs -- because once this feature also is on a picture of Uranus. I found similar features on these pictures: PIA 00039 (Titania), PIA 00140 (Miranda), PIA 00032 (Uranus), PIA 00043 (Miranda) and PIA 01534 (Ariel). On PIA 00043 I found it four times and on PIA 01534 two times. On PIA 00032 only at the false-color picture of Uranus. At PIA 00140 it is cutting inside the limb and dark, so there its reversed. At PIA 00039 it's weaker. I believe so because there can't be cryovolcanic plumes at the edge of Uranus' atmosphere. But that doesn't mean for me that Ariel is not active in the present. I believe that in the past of these 5 satellites only Umbriel was not active. At the present I believe that Miranda, Ariel, Titania are active. If there were images of a new mission to Uranus or Uranus and Neptune of higher resolution then this would be easier to find out. At Oberon Voyager 2 images have only a low resolution so that I can't believe there something about activity. I believe that Oberon is active at the present because similar in size to Titania which is also active ( at least in the past ). kheider (Dec 29, 2008 at 10:18 AM):
Could that be a cryovolcanic plume at the 8 o'clock position?
-- Kevin Heider
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