The data sets listed in the table below are PDS3 legacy data sets. Once these data sets have been migrated to PDS4 they will be listed in the section above.
|Data Set Name||Data Set Description||Browse||Citation|
|Torino Polarimetry of 25143 Itokawa||This data set contains the polarimetry of asteroid 25143 Itokawa published in Cellino et al. (2005). The observations were made from June 26 through July 3, 2004 with the Torino photopolarimeter at the 2.15 m telescope of the El Leoncito Observatory in Argentina. The degree of linear polarization was measured in five filters (Johnson-Cousins UBVRI).||Browse|
"Cellino, A., Yoshida, F., Anderlucci, E., Bendjoya, P., DiMartino, M., Ishiguro, M., Nakamura, A.M., and Saito, J., Polarimetry of Asteroid Itokawa V1.0. EAR-A-I0066-3-ITOKAWAPOL-V1.0. NASA Planetary Data System, 2007."
|Stooke Small Bodies Maps||These maps of small solar system bodies have been prepared by Philip Stooke of the University of Western Ontario. This data set includes 270 map sheets of six asteroids, five planetary satellites, and three comets, all prepared from spacecraft images. This data set was updated in 2015 with the addition of 44 new map sheets.||Browse|
"Stooke. P., Stooke Small Bodies Maps V3.0. MULTI-SA-MULTI-6-STOOKEMAPS-V3.0. NASA Planetary Data System, 2015."
|Small Body Radar Shape Models||This data set contains radar-based shape models for small solar system bodies, generated by the method developed by Scott Hudson. The current version of this data set contains shape models for the following asteroids: 216 Kleopatra, 1620 Geographos, 2063 Bacchus, 4197 Toutatis (low and high resolution models), 4769 Castalia, 6489 Golevka, 1998 KY26, 52760 (1998 ML14), and 25143 Itokawa.||Browse|
"Neese, C., Ed. Small Body Radar Shape Models V2.0. EAR-A-5-DDR-RADARSHAPE-MODELS-V2.0, NASA Planetary Data System, 2004."
|Gaskell Itokawa Shape Model||The shape model of 25143 Itokawa derived by Robert Gaskell from Hayabusa AMICA images. The model is provided in the implicitly connected quadrilateral (ICQ) format in four levels of resolution. This version of the model was prepared on August 29, 2007. Vertex-facet versions of the models are also provided.||Browse|
"Gaskell, R., Saito, J., Ishiguro, M., Kubota, T., Hashimoto, T., Hirata, N., Abe, S., Barnouin-Jha, O., and Scheeres, D., Gaskell Itokawa Shape Model V1.0. HAY-A-AMICA-5-ITOKAWASHAPE-V1.0. NASA Planetary Data System, 2008."