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Rev 134 - Jun 27-Jul 15, 2010 - Titan T71, Daphnis, Also "propellers"
jasedm
post Jun 27 2010, 08:01 PM
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Latest article available for the first revolution of the solstice mission here
A nice little squint at Daphnis (20-odd pixels in the NAC) accompanies a Titan flyby and 'propeller' studies amongst other things.

Thanks again Jason for the planned observation schedules.
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Astro0
post Jun 29 2010, 11:54 PM
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Very long sequence of images on the Cassini website showing thumbnails (256x256 pixels) that appear to be an aurora sequence.
It'll be interesting to see what the Cassini/Ciclops team get out of this observation set this time around.
Here's an enlarged and noise-reduced frame...
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brellis
post Jul 2 2010, 03:12 AM
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How's her fuel holding up?

from a 2009 sdc article:

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Cassini uses two types of fuel, hydrazine, which is used for small navigation maneuvers, and a standard bipropellant for larger maneuvers. While there is ample hydrazine to continue the mission through 2017, the Cassini navigation team has to be more conservative with its bipropellant. "We will design future tours knowing how much propellant is available for velocity change," Mitchell said.
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Stu
post Jul 6 2010, 06:06 PM
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Beautiful image of the rings... just beautiful...

http://saturn.jpl.nasa.gov/multimedia/imag...1/W00064671.jpg


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ugordan
post Jul 6 2010, 06:08 PM
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Very interesting specular-like brightening around the tiger stripes in these images. Brighter patches were visible before, but I don't think I've ever seen the effect as pronounced as here (right hand image is just an enhancement).
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If crystalline ice in the sulci is blue-green in the IR3/GRN/UV3 filter combo, what is white? Freshly fallen amorphous ice particles?


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nprev
post Jul 10 2010, 01:18 AM
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QUOTE (ugordan @ Jul 6 2010, 11:08 AM) *
If crystalline ice in the sulci is blue-green in the IR3/GRN/UV3 filter combo, what is white? Freshly fallen amorphous ice particles?


Possibly freshly condensed frost from vapor?

That's an interesting find, Gordan. I wonder if particle sizes can be determined in some way from the relfectance properties.


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remcook
post Jul 10 2010, 09:32 AM
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Large loose particles tend to be white/gray and highly scattering... In principle it is possible to determine particle size from wavelength-dependent scattering information, but for visible/uv wavelengths particles are quickly large compared to the wavelength (which is what counts), which makes it a lot harder with only visible images.
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Juramike
post Jul 10 2010, 01:26 PM
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QUOTE (nprev @ Jul 9 2010, 08:18 PM) *
I wonder if particle sizes can be determined in some way from the relfectance properties.


Definitely. Grain sizes can alter the detailed spectral shape. Water ice grains of different sizes have slightly different IR spectra.


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ugordan
post Jul 11 2010, 01:04 PM
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Saturn on July 9th. Tethys transiting and Enceladus' shadow:

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Hungry4info
post Jul 11 2010, 01:40 PM
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Nice! smile.gif


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ugordan
post Jul 17 2010, 08:44 PM
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Another one, July 15th:

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Don't know which moon that is, might be Rhea judging by the color.


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