Enceladus in eclipse |
Enceladus in eclipse |
Sep 20 2007, 12:18 PM
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#1
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Senior Member Group: Members Posts: 3648 Joined: 1-October 05 From: Croatia Member No.: 523 |
Some weird looking raws of Enceladus of what appears to be the moon entering Saturn's shadow. Solar System Simulator confirms this:
Before - During When exactly did Enceladus' eclipse season start? -------------------- |
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Sep 20 2007, 03:49 PM
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#2
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Administrator Group: Admin Posts: 5172 Joined: 4-August 05 From: Pasadena, CA, USA, Earth Member No.: 454 |
Nice catch, ugordan!
--Emily -------------------- My website - My Patreon - @elakdawalla on Twitter - Please support unmannedspaceflight.com by donating here.
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Sep 21 2007, 12:19 PM
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#3
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Interplanetary Dumpster Diver Group: Admin Posts: 4404 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
We are approaching the ring plane crossing of 2009, so things like this should become more common.
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Sep 22 2007, 08:53 AM
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#4
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Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
Random note: At the moment of solar ring plane crossing (which given the presence of ring-warp, and the 3 arc-min solar diameter, is a somewhat extended moment), illumination of ring topography and "atmospheres" (dust, whatever) will be very faint except at the directly illuminated ring edge. Saturn light on the rings will largely swamp ultra-oblique solar illumination. The best place for grazing incidence illumination studies of the rings is where the rings enter and exit Saturn-shadow. Ringlight on the planet's nightside, will be very low at that time.
An inclined orbit is called for to make those observations. What other tradeoffs on other observations and their preferred orbits will be, I don't know. |
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Sep 26 2007, 04:28 PM
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#5
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Junior Member Group: Members Posts: 76 Joined: 19-October 05 Member No.: 532 |
Random note: At the moment of solar ring plane crossing (which given the presence of ring-warp, and the 3 arc-min solar diameter, is a somewhat extended moment), illumination of ring topography and "atmospheres" (dust, whatever) will be very faint except at the directly illuminated ring edge. Saturn light on the rings will largely swamp ultra-oblique solar illumination. The best place for grazing incidence illumination studies of the rings is where the rings enter and exit Saturn-shadow. Ringlight on the planet's nightside, will be very low at that time. An inclined orbit is called for to make those observations. What other tradeoffs on other observations and their preferred orbits will be, I don't know. The extended mission tour has already been chosen, with the usual uncertainties we know where the spacecraft is going to be until July 2010. this sort of this was considerd and decided on in January (I think) |
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Sep 27 2007, 07:55 AM
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#6
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Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
"The extended mission tour has already been chosen, with the usual uncertainties we know where the spacecraft is going to be until July 2010. .."
I know. I just don't recall much discussion, certainly no detailed discussion, of the sorts of observations planned at the time of solar ring-plane crossing, or what orbit the spacecraft will be in at that time. Most discussion centered on the Titan and Enceladus flybys, and dropping 1 Enceladus flyby to get some really good data on the other inner sats. |
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