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Cassini's Helene flyby
Posted by Emily Lakdawalla
2010/03/05 04:05 CST
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I was much anticipating Cassini's encounter with Helene on Wednesday. It looks like there was a problem with the pointing of the spacecraft, something that used to happen much more frequently on Cassini, but I don't see it much anymore, so that Helene falls off of the edges of many of the images. When I say "problem" I don't mean there's anything wrong with Cassini; I am sure Cassini pointed where it was told to, it's just either that there was some mistake in where it was told to point, or there is some mistake relating to the reference vector from which it measured where it was told to point, or (the most interesting possibility of all) that Helene is not quite exactly where the Cassini planners thought it was. The latter is a real possibility for Helene, whose orbit has it bobbing in a complicated fashion around a point 60 degrees ahead of the much more massive Dione. But I don't have any information as to why exactly Helene wasn't where Cassini evidently was told it should be.
In any case, some of the images did catch Helene, and they produced our best views of Helene to date. For reference, this is Cassini's previous best view of the moon, which is 36 by 32 by 30 kilometers in diameter:

NASA / JPL / SSI
Helene
Cassini passed within 36,000 kilometers of Helene to take this image on July 20, 2007. Helene is the leading co-orbital companion to Dione and is a small, irregular body measuring approximately 36 by 32 by 30 kilometers in size. This image has been enlarged by a factor of two.
NASA / JPL / SSI / montage by Emily Lakdawalla
Helene from Cassini's March 3, 2010 flyby
These four images of Helene, Dione's leading co-orbital satellite about 30 kilometers in diameter, were taken by Cassini during a close flyby on March 3, 2010. The top two images mostly show Helene's anti-Saturn hemisphere, while the bottom two mostly show Helene's sub-Saturn hemisphere, lit by Saturnshine. Two dark "donuts" on the bottom images are artifacts that result from dust within Cassini's optics.Blog Search
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