Thanks Trent, that does help.  We default to the triaxial ellipsoid in our 
definitions and I'll ask our astrodynamics team how they'd like to proceed.

From: Hare, Trent M <th...@usgs.gov>
Sent: Monday, December 23, 2024 3:23 PM
To: Reynolds, Scott <sc...@agi.com>
Cc: Newcomb, Doug <doug_newc...@fws.gov>; gdal-dev@lists.osgeo.org
Subject: EXTERNAL: Re: [EXTERNAL] [gdal-dev] Shape update/addition for Ceres

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Scott,
   That spherical value of 470 km, as defined in ESRI's projection, was 
intended. We are still working with the IAU to update these rules, but when 
that projection was defined, we used this rule:
If the IAU defined a "mean" radius for a body (see Table 6.0 page 
33<https://astropedia.astrogeology.usgs.gov/download/Docs/WGCCRE/WGCCRE2015reprint.pdf#page=33>
 of the report), we default to that value as a sphere.

This value was provided to the IAU by Thomas Roatsch (DLR) from the Dawn Team.

The Dawn team, which produced the control mosaic for Ceres, also used 470 km as 
a sphere for the final mosaic and digital terrain model ( 
DTM<https://astrogeology.usgs.gov/search/map/ceres_dawn_fc2_hamo_global_dtm_137m>):

reference: https://doi.org/10.1016/j.pss.2016.05.011
quote, "Ceres' shape model was then used for the calculation of the ray 
intersection points, while the map projection itself was placed onto a 
reference sphere of Ceres with a mean radius of 470 km."
image mosaic: 
https://astrogeology.usgs.gov/search/map/ceres_dawn_fc_global_mosaic_140m

While it might seem strange to use a sphere, this is common for irregular 
shaped bodies. This is mostly true for bodies defined as a triaxial since 
mapping applications do not commonly support triaxial map projections. The IAU 
defines these mean radii to help support interoperability across applications. 
We are working with the IAU and could update some of these rules. For example, 
I will say it is odd to see that Ceres is NOT defined as a triaxial, but the 
Dawn Team and the IAU promote a "mean" radius. I'm sure we will revisit this in 
the future.

BTW, it doesn't mean you can't define your own projection for Ceres if you need 
to. But I would recommend matching the current best-of image mosaic and DTM.
I hope that helps,
Trent



________________________________
From: Newcomb, Doug <doug_newc...@fws.gov<mailto:doug_newc...@fws.gov>>
Sent: Sunday, December 22, 2024 8:12 PM
To: Reynolds, Scott <sc...@agi.com<mailto:sc...@agi.com>>
Cc: Hare, Trent M <th...@usgs.gov<mailto:th...@usgs.gov>>
Subject: Re: [EXTERNAL] [gdal-dev] Shape update/addition for Ceres

check with Trent Hare at USGS
________________________________
From: gdal-dev 
<gdal-dev-boun...@lists.osgeo.org<mailto:gdal-dev-boun...@lists.osgeo.org>> on 
behalf of Reynolds, Scott via gdal-dev 
<gdal-dev@lists.osgeo.org<mailto:gdal-dev@lists.osgeo.org>>
Sent: Saturday, December 21, 2024 9:17 AM
To: gdal-dev@lists.osgeo.org<mailto:gdal-dev@lists.osgeo.org> 
<gdal-dev@lists.osgeo.org<mailto:gdal-dev@lists.osgeo.org>>
Subject: [EXTERNAL] [gdal-dev] Shape update/addition for Ceres




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As a user of GDAL in some of our products I'm trying to find a contact, 
probably/possibly at Esri, that could add a new entry for Ceres that uses the 
oblate parameters defined 
here<https://astropedia.astrogeology.usgs.gov/download/Docs/WGCCRE/WGCCRE2015reprint.pdf>
 (487.3km, 446km). ESRI:104972 exists for the spherical definition (470 km).



Thanks,

Scott
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