KBO encounters |
KBO encounters |
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#1
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Newbie ![]() Group: Members Posts: 6 Joined: 1-August 08 Member No.: 4280 ![]() |
Hi,
I’m regular follower of NH and I’m also interested in the 2nd leg of the mission, i.e the 2016+ KBOs encounters. Does anyone know when operations about this leg (starting with searching objects of interest with HST or some other earth-based means, I suppose) are expected to begin ? |
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#2
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Member ![]() ![]() ![]() Group: Members Posts: 202 Joined: 9-September 08 Member No.: 4334 ![]() |
The first post in this thread says the search would start in 2010 - has it started yet, or will it be later this year?
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#3
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Member ![]() ![]() ![]() Group: Members Posts: 529 Joined: 19-February 05 Member No.: 173 ![]() |
The first post in this thread says the search would start in 2010 - has it started yet, or will it be later this year? Our best imager, LORRI, can resolve the size of an object from roughly 10^5 object diameters away. So for a 100 km object, for example, we have to be w/i 10^7 km just to resolved it; if you want crude shape information, cut that to 10^6 diameters, and if you want "geology," well, better come to approx 30,000 diameters or better. The point here is Crantor and other distant flybys don't yield much of use, so we have not expended effort on them. As to our KBO search, John Spencer is leading the organizational effort to recruit search teams; Andrew Steffl is helping John. Our plan is to conduct the search in 2011 and 2012, though Scott Shepard at least has already begun. -Alan |
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#4
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![]() Junior Member ![]() ![]() Group: Members Posts: 24 Joined: 29-May 08 From: Seattle, USA Member No.: 4162 ![]() |
Our best imager, LORRI, can resolve the size of an object from roughly 10^5 object diameters away. So for a 100 km object, for example, we have to be w/i 10^7 km just to resolved it; if you want crude shape information, cut that to 10^6 diameters, and if you want "geology," well, better come to approx 30,000 diameters or better. Alan, thanks for the info, but I'm a little confused... I assume that for crude shape information, you mean cut the maximum distance to 106 kilometers, since 106 diameters would be 108 kilometers. But which do you mean for the "geology" figure? 30,000 diameters would be 3 million kilometers for our theoretical 100 km object, which is tough enough, but 30,000 kilometers is more or less a bullseye: better targeting than even Apophis will manage ![]() |
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#5
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![]() Member ![]() ![]() ![]() Group: Members Posts: 259 Joined: 23-January 05 From: Seattle, WA Member No.: 156 ![]() |
The Tvashtar plume images were taken a lot closer to the sun than any KBO images will be. I imagine blurring due to longer exposure times would reduce resolution at comparable distances.
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#6
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![]() Member ![]() ![]() ![]() Group: Members Posts: 701 Joined: 3-December 04 From: Boulder, Colorado, USA Member No.: 117 ![]() |
I'll chip in here. Alan was talking about science at Centaurs that we might fly past on our way to Pluto- none of those will get close enough to be resolved. For the KBO target(s) beyond Pluto, we will deliberately target to get within a few tens of thousands of kilometers or closer- from 20,000 km, for instance, we would get 500 pixels across a 50 km KBO- sufficient to do some serious geology. LORRI can get well-exposed, unsmeared, images at Pluto's distance from the sun (it was designed to do that, of course), and while illumination conditions will be more challenging further out in the Kuiper Belt, there's enough performance margin that we expect to be able to do the same there.
At Crantor's distance, a LORRI pixel is 2000 km across, much bigger than Crantor itself. So there's no hope of getting any shape information. And to make sure no-one is still confused on this point, we will not be searching for KBOs with NH itself- huge ground-based telescopes with wide-field imagers can do that much better, even though they're stuck at 1 AU. John |
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