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DS-1 and Comet Borrelly
Phil Stooke
post Feb 21 2006, 03:59 AM
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These are two images of Comet Borrelly from Deep Space 1. I've been searching for the best images for mapping the nucleus.

I was disturbed to find that the raw images, in fact all the Borrelly data, were never properly archived and are difficult to track down. It seems the Deep Space 1 team were not very interested in collaborating with the PDS on archiving.

Anyway, these are specially processed composites of the versions I've been able to find. They show more detail along the terminator (bottom) than most images I have seen elsewhere. I have been working on a 3D shape model in my spare time. PDS has two shape models which are not suitable for conventional mapping.

Phil

Attached Image


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... because the Solar System ain't gonna map itself.

Also to be found posting similar content on https://mastodon.social/@PhilStooke
Maps for download (free PDF: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf
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Phil Stooke
post Feb 23 2006, 02:34 AM
Post #2


Solar System Cartographer
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Posts: 10265
Joined: 5-April 05
From: Canada
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Yes, but not properly documented, and the topo models are not in conventional mapping formats - they have to be projected into a planetocentric coordinate system to be converted to global maps.

Phil


--------------------
... because the Solar System ain't gonna map itself.

Also to be found posting similar content on https://mastodon.social/@PhilStooke
Maps for download (free PDF: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf
NOTE: everything created by me which I post on UMSF is considered to be in the public domain (NOT CC, public domain)
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tedstryk
post Jul 16 2008, 05:09 AM
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I have made two DS-1 compilations. The first contains one of each target it studied. The Jovian images were primarily for calibration, and the Mars images were to go along with much more valuable infrared spectra.

Attached Image


The second contains both of the Braille sets that did not miss. The first is a deconvoluted stack of the two CCD frames taken 15 minutes after the flyby. The second is from four frames obtained by the APS (Active Pixel Sensor) five minutes later. Thanks to spacecraft motion, it shows a very different angle on the lumpy asteroid. All frames are severely underexposed, which is why the quality is much poorer than the set from the CCD frames.

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