5905 Johnson (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "5905 Johnson" in English language version.

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  • Central Bureau for Astronomical Telegrams – IAUC 8511
    Photometric observations obtained between 1 and 11 April 2005, reveal, that 5905 Johnson is a binary system with an orbital period of 21.78 hours. The primary rotates with a period of 3.783 hours. The lightcurve's amplitude of 0.11 magnitude suggests a nearly spheroidal shape. Mutual eclipse and occultation events between 0.15 and 0.18 magnitude, suggest a secondary-to-primary mean-diameter ratio of 0.4. The system's mean absolute R magnitude is 12.8±0.1.
    Reported by: Brian Warner (Palmer Divide Obs.) Petr Pravec and Peter Kušnirák (Ondřejov Obs., Czech Republic) Donald P. Pray (Carbuncle Hill Obs.); Adrián Galád and Štefan Gajdoš (Modra Obs., Slovakia) and P. Brown and Z. Krzeminski, Department of Physics and Astronomy, University of Western Ontario

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  • "JPL Small-Body Database Browser: 5905 Johnson (1989 CJ1)" (2018-01-26 last obs.). Jet Propulsion Laboratory. Retrieved 28 February 2018.

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