Rev 160 Titan monitoring, Recent change in Senkyo Options

[titanicrivers]

Rev 160 http://www.ciclops.org/view/7051/Rev160 view of Senkyo region appears to be showing less bright spot albedo change (yellow arrow) than 2 months ago. Image is from quite a distance however (3.2M km). Kraken in the north (red arrow) appears to have a brighter rim surrounding the darker sea, perhaps an artifact of my image processing. edit: sorry for the typo in the topic description! (fixed - Mod)

[ngunn]

I'm pretty sure the relatively bright 'halo' around Kraken Mare is real. Certainly it has been discussed before. I think Juramike had some ideas. I also think it's been mentioned in the literature. (Sorry I don't have references handy.) Anyhow it would be interesting to have people's latest thoughts on this.

[Jason W Barnes]

I'm pretty sure the relatively bright 'halo' around Kraken Mare is real. Certainly it has been discussed before. I think Juramike had some ideas. I also think it's been mentioned in the literature. (Sorry I don't have references handy.) Anyhow it would be interesting to have people's latest thoughts on this.

Ring around Kraken isn't in the literature yet. VIMS T67 attached. Its spectrum, location, and morphology are consistent with evaporite.

- Jason

Attached thumbnail(s)

 

[ngunn]

Very interesting! That great image clearly shows the bright halo is most prominent at the heads of the southern bays whereas the capes between are relatively halo-free. Oh for some radar coverage of those bays to confirm that their shores are indeed smoother and more gently shelving.

[titanicrivers]

Yes fascinating. Kraken and its evaporative ring (black arrow) have been relatively stable over the 2010-11 period at least in ISS images (see below). The ISS ring appears more uniform and continuous around Kraken. Are the very bright portions of the VIMS image evaporite or clouds hugging the shoreline???
That small Senkyo area affected by the arrow storm (red arrow) went from a dark patch to a bright spot over the Dec 2010 to Sept 2011 time period. I would presume this might be an evaporite as well. Jason, is there a post-arrow storm image VIMS image of Senkyo covering the same area as that neat April 2010 pre-storm image you have posted above ?

[Juramike]

(...keeping quiet until the LPSC abstracts publish on Friday...)

[Jason W Barnes]

I note that based on your arrow this change appears not occur within Senkyo, but rather within the newly named Yalaing Terra.

- Jason

[ngunn]

Is this the absract that relates to this discussion?
http://www.lpi.usra.edu/meetings/lpsc2012/pdf/2762.pdf

[titanicrivers]

"I note that based on your arrow this change appears not occur within Senkyo, but rather within the newly named Yalaing Terra."

- Jason

Thanks for the proper name! Yes Yalaing Terra is what I had been referring to as Senkyo or South of Senkyo or S Senkyo since noting the change in December of 2010. http://www.unmannedspaceflight.com/index.php?showtopic=6829 The center of this region became a dark albedo post arrow-storm that gradually brightened and persisted as bright throughout most of 2011 (now fading a bit towards its pre-arrow storm albedo). The grid I made last year matches the official IAU coordinates of Yalaing Terra. The link below shows the projected position of the ‘arrow-storm’ directly over this terra!
http://www.unmannedspaceflight.com/index.p...st&id=23524
The change over the last year has been interesting to follow:
http://www.unmannedspaceflight.com/index.p...st&id=26004
and now its interesting to read of the possible mechanisms of such changes in your LPSC abstract Nigel has highlighted above!

[Jason W Barnes]

Is this the absract that relates to this discussion?
http://www.lpi.usra.edu/meetings/lpsc2012/pdf/2762.pdf

Yup. I note that these days the IAU only likes to name areas that require names in order to be referred to in a peer-reviewed scientific paper.

- Jason