Reality Check
Penultimate Amazing
DPS 2015: A little science from Rosetta, beyond perihelion
Since I wasn't able to attend the European Planetary Science Congress last month, the Division for Planetary Sciences meeting was my first opportunity to see science results from the Rosetta mission since comet Churyumov-Gerasimenko passed through perihelion on August 13. Here are my scattered notes from DPS sessions on Rosetta:
Martin Paetzold updated the basic physical properties of the comet. The mass -- about 10 billion tons (or a GM of 666.2 ± 0.2m3/s2) -- is the smallest ever determined through radio tracking. Now that sunlight has arrived to the previously winter-dark south pole of the comet, there are updated shape models, and the total volume of the comet has decreased by about 10% from what was reported in the first science papers. Mass and volume give you density: 0.533 ± 6 kg/m3. That's half the density of water ice, but we know that the comet contains at least some silicate material. With a bit of modeling, Paetzold concluded that the comet's porosity is a huge 72%. So then the next question is: are there gigantic caverns within the comet, or is the porosity an intrinsic property of cometary material? With several measurements of the gravity field complete, Paetzold concluded the latter: the comet seems to be homogeneously dense in its interior, and its ice and dust seem to be put together in a form that has lots and lots of open pores.


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