<p>For those that are interested in the subject, please read the last few entries on Emily Lakdawalla's TPS blog.</p><p>WOW!</p><p>
http://www.planetary.org/blog/</p><p> <strong>Oct. 14, 2008 | 15:58 PDT | 22:58 UTC</strong> </p><h2 class="sIFR-replaced"><span class="sIFR-alternate">
DPS meeting: Saturday: Enceladus -- it's cooler than we thought</span></h2><div class="small">Permalink:
http://www.planetary.org/blog/article/00001693/</div><p><br />I'll be writing quite a bit about the annual meeting of the Division of Planetary Sciences (DPS) of the American Astronomical Society this week; see
this post for an introduction. I got distracted by the fires yesterday, but things are looking less threatening this afternoon, so I'm back to work. <br /><br />John Spencer spoke on the results from the CIRS instrument of the March and August 2008 flybys of Enceladus. CIRS is an infrared sensor that can detect thermal emission from most surfaces in the Saturn system (though some of the surfaces are so cold that the thermal emission occurs at wavelengths longer than CIRS can "see.") How bright a surface appears at these thermal wavelengths correlates with its temperature; it takes some detailed modeling to figure out exactly how brightness correlates with temperature, especially for places like Enceladus where the field of view of CIRS may encompass materials with very different temperatures. In the past, CIRS has shown Enceladus' south pole to be anomalously hot, with some approximate correlation between the hottest areas and the locations of the "tiger stripes" (see
here for some background). <br /><br />John opened his talk with a very helpful summary of the eight close Enceladus flybys planned for the three years of 2008 to 2010. Since I can pause the playback of this session (thank you again to the IT magicians at Cornell) I can reproduce it fully here: <br /><br /><table border="0" class="info outline_all"><tbody><tr><th>Date</th><th>Orbit</th><th>Speed<br />(km/s)</th><th>Alt.<br />(km)</th><th>Orbit<br />inc.</th><th>Close approach science emphasis</th></tr><tr><td>March 12, 2008