Little notes from Monday at DPS 2010: Iapetus, Kiviuq, LHB, Steins, Cherry Gary, and more
Posted by Emily Lakdawalla
2010/10/06 11:24 CDT
Here's a post with some random facts and notes from Monday at Division of Planetary Sciences meeting that didn't fit in any other writeup.
Iapetus has a much larger opposition surge than any other Saturnian moon (or Uranian moon, for that matter). If you're taking notes, Iapetus' is 1.8; next highest is Ariel, at 1.2. But binary Kuiper belt objects have much higher opposition surges at 2.1. Thomson Fisher et al. interpret this as evidence for the movement of ice around Iapetus' surface, which is redeposited as lacy frost that generates this opposition surge.
James Bauer, speaking about WISE's views of comets, said they detected 93 and discovered 19, including 3 cases of activity on known bodies. He referred to comet 67P/Churyumov-Gerasimenko, the eventual target of Rosetta, as "Cherry Gary." He said they got 18 frames on Deep Impact's target, Hartley 2, in mid-May. Here's one of those.Tilmann Denk gave two papers in one about small moon rotation rates. First he reported some Earth-based observations of Jupiter's moon Himalia's rotation rate, which he determined to be 7.78 hours. This is quite a bit shorter than the previously reported rate, and he showed how an error in combining two nights of observations resulted in the erroneously long previous measurement. Then he went on to talk about Cassini's observations of Saturn's outer irregular moons. Siarnaq's rotation rate is 6.69 hours. Albiorix' is 13.32 hours. Ymir's is 7.3 hours but this is tentative because the two measured peaks in the light curve, which was measured over about 8 hours, differ in intensity by 10% (it should not do this). Kiviuq was shown to have an unusually long rotation rate of more than 21 hours, so they negotiated for Cassini to record its rotation for about 22 hours, a record-breaking observation. They successfully measured 102% of one day, therefore determining its rotation rate to be 21.82 hours with reasonably high confidence. All these spin rates and their diameters fall in to the normal range of asteroid sizes and rotation rates.
Roger Clark showed some really remarkably good model fits to "squiggly lines" (spectra) measured for Saturn's icy moons using only three components: water ice, hydrated hematite, and nanophase iron. Bill McKinnon asked him "where did the carbon go?" Clark answered that it's probably present, just not optically abundant. I think the crowd was really surprised at just these three components being able to match the spectral shapes so amazingly well.
Matija Cuk argued that the impact spike in the lunar cratering record observed at 3.9 billion years ago -- the Late Heavy Bombardment -- could be explained from the tidal disruption of a Vesta-sized, Mars-crossing rocky asteroid, the parent of the "mesosiderite" meteorites.
Rita Schultz, summarizing Rosetta's Steins encounter, said that YORP effects are causing material to slide toward Steins' equator, erasing smaller craters. She tried not to reveal too much about the Lutetia encounter. She did say that Lutetia had an 800-meter-thick regolith over a more solid interior -- like the Moon. And she wouldn't cite a number for the density but she said "the density is such that it could be differentiated." A poster I saw on Tuesday said the density was 3.1 grams per cubic centimeter, which is about the density of a pretty dense rock like basalt; considering it's a small asteroid and likely has at least some void space, I assume that implies a rock and metal mixture.
Ray Arvidson's presentation on current Mars science duplicated a lot of the stuff I saw him present just the week previously at the Curiosity landing site selection meeting. He did say that "we think Spirit is alive, scrounging every photon to keep its battery alive," and that he expects the rover to wake up "in October."
That's when I left Day 1. At this rate it'll be the end of October before I get all my notes down in the blog!
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