9260 Edwardolson (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "9260 Edwardolson" in English language version.

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  • Central Bureau for Astronomical Telegrams, No.270, 2 November 2005, for (9260) Edwardolson
    A photometric observations between 6 and 30 October 2005, show that 9260 Edwardolson is a binary system with an orbital period of 17.785±0.003 hours. The primary rotates with a period of 3.0852±0.0001 hours, and its lightcurve has a brightness variation of 0.11 magnitude, which is indicative of a nearly spheroidal shape. Mutual eclipse/occultation events, that are between 0.08 and 0.15 magnitude deep, indicate a secondary-to-primary mean-diameter ratio of 0.27±0.03.
    Reported by M. Jakubik and M. Husarik, Skalnate Pleso Observatory; J. Vilagi, S. Gajdos, and A. Galad, Modra Observatory; P. Pravec and P. Kusnirak, Ondrejov Observatory; W. Cooney, J. Gross and D. Terrell via Sonoita Research Observatory (Sonoita, AZ); D. Pray, Greene, RI; and R. Stephens, Yucca Valley, CA
    Central Bureau for Astronomical Telegrams

iau.org

  • "Edward C. Olson". IAU – International Astronomical Union. Retrieved 1 January 2016.

johnstonsarchive.net

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nasa.gov

ssd.jpl.nasa.gov

  • "JPL Small-Body Database Browser: 9260 Edwardolson (1953 TA1)" (2017-03-31 last obs.). Jet Propulsion Laboratory. Retrieved 5 July 2017.