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NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 JUNE-OCTOBER - PubMed

. 2015 Jan-Mar;42(1):41-53.

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NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 JUNE-OCTOBER

Brian D Warner. Minor Planet Bull. 2015 Jan-Mar.

Abstract

Lightcurves for 45 near-Earth asteroids (NEAs) were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2014 June through October. Periods and lightcurve amplitudes were determined for 44 of the objects. No period or amplitude could be found for 2014 SZ144.

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References

    1. Benishek V (2014). “Rotation Periods and Lightcurves for Six Near-Earth Asteroids.” Minor Planet Bul 41, 257–260. - PubMed
    1. Behrend R (2008) Observatoire de Geneve web site. http://obswww.unige.ch/~behrend/page_cou.html
    1. Galád A, Pravec P, Kusnirák P, Gajdos S, Kornos L, and Világi J (2005). “Joint Lightcurve Observations of 10 Near-Earth Asteroids from Modra and Ondrejov.” Earth, Moon, and Planets 97, 147–163.
    1. Harris AW, Young JW, Bowell E, Martin LJ, Millis RL, Poutanen M, Scaltriti F, Zappala V, Schober HJ, Debehogne H, and Zeigler KW (1989). “Photoelectric Observations of Asteroids 3, 24, 60, 261, and 863.” Icarus 77, 171–186.
    1. Harris AW, Pravec P, Galad A, Skiff BA, Warner BD, Vilagi J, Gajdos S, Carbognani A, Hornoch K, Kusnirak P, Cooney WR, Gross J, Terrell D, Higgins D, Bowell E, and Koehn BW (2014). “On the maximum amplitude of harmonics on an asteroid lightcurve.” Icarus 235, 55–59.

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