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With thermal infrared observations detected by the NEOWISE project, we havemeasured diameters for 1742 minor planets that were also observed by theInfrared Astronomical Satellite (IRAS). We have compared the diameters andalbedo derived by applying a spherical thermal model to the objects detected byNEOWISE and find that they are in generally good agreement with the IRASvalues. We have shown that diameters computed from NEOWISE data are often lesssystematically biased than those found with IRAS. This demonstrates that theNEOWISE dataset can provide accurate physical parameters for the >157,000 minorplanets that were detected by NEOWISE.

Thermal Model Calibration for Minor Planets Observed with WISE/NEOWISE: Comparison with IRAS