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92 5855 Yukitsuna. Our data are consistent with the period of 19.2 h found by Behrend (2008). Acknowledgement Construction of the Oakley Southern Sky Observatory was funded by a grant from the Oakley Foundation and by a generous donation made by Niles Noblitt. This research was partially supported by a grant from NASA administered by the American Astronomical Society. References Alvarez-Candal, A., Duffard, R., Angeli, C.A., Lazzaro, D., and Fernandez, S. (2004). “Rotational lightcurves of asteroids belonging to families.” Icarus 172, 388-401. Behrend, R. (2008). Observatoire de Geneve web site, http://obswww.unige.ch/~behrend/page_cou.html Binzel, R.P. (1987). “A photoelectric survey of 130 asteroids.” Icarus 72, 135-208. Warner, B.D. (2006). “Asteroid lightcurve analysis at the Palmer Divide Observatory: March –June 2006.” Minor Planet Bul. 33, 85-88. Minor Planet Bulletin 36 (2009)
Minor Planet Bulletin 36 (2009) 93
Page 1 and 2: THE MINOR PLANET BULLETIN BULLETIN
Page 3 and 4: 79 OBSERVER & OBSERVING NO. PLANET
Page 9 and 10: 85 turn enabled determination of th
Page 11 and 12: 87 LIGHTCURVES OF 494 VIRTUS, 556 P
Page 13 and 14: 89 5905 JOHNSON: A HUNGARIA BINARY
Page 15: 91 ASTEROID LIGHTCURVE ANALYSIS AT
Page 19 and 20: 95 contaminated our results. We the
Page 21 and 22: 97 were chosen by comparing well-pl
Page 23 and 24: 99 Figure 1 shows the predicted ori
Page 25 and 26: 101 angles and those on alternate n
Page 27 and 28: 103 more data were acquired, we wer
Page 29 and 30: 105 magnitude scale. Acknowledgemen
Page 31 and 32: Minor Planet Bulletin 36 (2009) 107
Page 33 and 34: 109 ASTEROID LIGHTCURVE ANALYSIS AT
Page 35 and 36: 111 (87343) 2000 QH25. This lightcu
Page 41 and 42: 117 result for the rotation period,
Page 43 and 44: 119 LIGHTCURVES FOR SHAPE MODELING
Page 45 and 46: 121 PHOTOMETRIC OBSERVATIONS AND LI
Page 49 and 50: 125 ASTEROIDS OBSERVED FROM GMARS A
Page 53 and 54: asteroids/goldstone_asteroid_schedu
Page 55 and 56: 131 DATE RA(2000) DC(2000) E.D. S.D

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