IRTF observations of Io from 1983 to 1993

    These images show Jupiter's moon Io obtained at different infrared wavelengths with the W. M. Keck Observatory's 10-meter Keck II telescope on Aug. 15, 2013 (a and c), and the Gemini North telescope on Aug. 29, 2013 (d).Image Credit: NSF/NASA/JPL-Caltech//UC Berkeley/Gemini Observatory/W. M. Keck Observatory

    IRTF observations of Io from 1983 to 1993

    NASA's Infrared Telescope Facility (IRTF) data were collected at 4.8 μ (M band), 8.7 μ,10 μ (N band),and 20 μ (Q band).These data were published in 1994 by Veeder, G. J., et al. Io's heat flow from infrared radiometry: 1983-1993, J. Geophys. Research, 99, 17095-17162. An electronically accessible form is provided here.

    PDS4 Bundle

    Data Description

    Data (Tables 2, 3, 4 and 5 are 4.8, 8.7, 10 and 20 µ, respectively)

    Tables 1, A1 an A2 are ancillary data

    Citing Data Sets for Publications

    A. G. Davies, G.J. Veeder (2020), Io IRTF Photometry 1983-1993, NASA Planetary Data System, https://doi.org/10.17189/1518953.