updated with improved Mercury map from imaging as collected and reprojected by Steve Albers
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README
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README
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@ -326,18 +326,18 @@ Texture maps
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# Fridger Schrempp
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'Available data' Pluto and Charon textures using maps created by Marc Buie at
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Lowell Observatory. Buie's maps were generated from photometric data
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'Available data' Pluto and Charon textures using maps created by Marc Buie
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at Lowell Observatory. Buie's maps were generated from photometric data
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gathered during six years of mutual occultations of Pluto and Charon.
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Titan's cloud texture in natural colors and its surface map at near-infrared
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wavelength. They are based on resources available from the imaging site
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(Ciclops) of the Cassini mission,
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http://ciclops.lpl.arizona.edu/index.php
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(Ciclops) of the Cassini mission
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(http://ciclops.lpl.arizona.edu/index.php)
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The Phoebe base texture was created from the cylindrical map published by the
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Cassini imaging team,
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http://photojournal.jpl.nasa.gov/catalog/PIA07775
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The Phoebe base texture was created from the cylindrical map published by
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the Cassini imaging team
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(http://photojournal.jpl.nasa.gov/catalog/PIA07775)
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The Tethys textures are based on the Oct 2008 Ciclops map
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(http://photojournal.jpl.nasa.gov/catalog/PIA11116)
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@ -345,11 +345,16 @@ Texture maps
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The Iapetus texture was created from the Oct 2008 Ciclops map
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(http://photojournal.jpl.nasa.gov/catalog/PIA11116)
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The Lunar topography and bump maps, using Clementine laser altimeter data,
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merged in the polar regions with topographic data from Clementine 750 nm
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oblique and nadir images,
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ftp://ftpflag.wr.usgs.gov/dist/pigpen/moon/usgs/topo/global/
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The Lunar topography and bump maps, using Clementine laser altimeter data,
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merged in the polar regions with topographic data from Clementine 750 nm
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oblique and nadir images
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(ftp://ftpflag.wr.usgs.gov/dist/pigpen/moon/usgs/topo/global/)
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The Mercury map was created from a combination of Mariner 10 imaging
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with recent MESSENGER WAC images from the first two flybys, as collected
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and reprojected by Steve Albers:
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See http://laps.noaa.gov/albers/sos/sos.html.
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# Phil Stooke
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Proteus, Janus, Prometheus and Epimetheus maps are from Phil Stooke.
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@ -357,7 +362,7 @@ oblique and nadir images,
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The Ida and Gaspra photomosaic maps are by Phil Stooke.
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# Venus's clouds and the textures for Ganymede, Callisto and Saturn are from
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Björn Jónsson. His site at http://www.mmedia.is/~bjj/ is an excellent
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Bj<EFBFBD>rn J<>nsson. His site at http://www.mmedia.is/~bjj/ is an excellent
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resource for solar system rendering.
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# Venus's surface is a copyright-free NASA image, prepared from Magellan radar
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@ -372,10 +377,6 @@ oblique and nadir images,
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The Io and Europa maps are by Steve Albers. His planetary maps are at:
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http://laps.noaa.gov/albers/sos/sos.html
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The Mercury map was created from Mariner 10 images and MESSENGER WAC images
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from the first two flybys. The partial color information was removed by
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Chris Laurel in a global conversion to grayscale.
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# The textures for the Uranian satellites were created by Ivan Rivera from JPL
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data. His Celestia page is: http://bruckner.homelinux.net/celestia.html
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