3309 Brorfelde (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "3309 Brorfelde" in English language version.

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arxiv.org

doi.org

harvard.edu

adsabs.harvard.edu

ui.adsabs.harvard.edu

cbat.eps.harvard.edu

  • Electronic Telegram No. 279, (3309) Brorfelde, 7 November 2005[5]
    Photometric observations obtained from 25 October to 3 November 2005, revealed that 3309 Brorfelde is a binary system with an orbital period of 18.48±0.01 hours. The primary rotates with a period of 2.5041±0.0002 hours, and its light-curve has a brightness variation of 0.13 magnitude, indicating a nearly spheroidal shape. Mutual eclipse/occultation events with an amplitude of 0.07-0.15 magnitude suggest a ratio of 0.26±0.02 for its secondary-to-primary mean-diameter. Assuming G = 0.15, the calibrated data gives an absolute magnitude of 13.4±0.2.
    B. D. Warner, Palmer Divide Observatory, Colorado Springs; P. Pravec and P. Kusnirak, Ondrejov Observatory; W. Cooney, J. Gross, and D. Terrell, Sonoita Research Observatory, Sonoita, AZ; and S. Nudds, Elginfield Observatory, University of Western Ontario Central Bureau for Astronomical Telegrams No.279

minorplanet.info

minorplanetcenter.net

nasa.gov

ssd.jpl.nasa.gov

  • "JPL Small-Body Database Browser: 3309 Brorfelde (1982 BH)" (2017-05-02 last obs.). Jet Propulsion Laboratory. Retrieved 3 July 2017.

nih.gov

pubmed.ncbi.nlm.nih.gov

obsunige.ch

planetarysciences.org

  • Lightcure plots of (3309) Brorfelde at the Center for Solar System Studies (CS3) in 2014

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