ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2013 MAY-JUNE.
作者： Brian D. Warner
DOI:
关键词: Geology 、 Asteroid 、 Rotation period 、 Solar System 、 Primary (astronomy) 、 Amplitude 、 Orbital period 、 Astronomy 、 Rotation
摘要: Lightcurves for eleven asteroids were obtained at the Center Solar System Studies-Palmer Divide Station (CS3-PDS) in 2013 May and June. The a mostly mix of Hungaria Phocaea members along with some outer main-belt asteroids. New data failed to remove existing rotation period ambiguity asteroid 1355 Magoeba, although number possibilities may have been reduced. A new is proposed 4436 Ortizmoreno, 8.24 h (or 16.48 h), superseding one reported by Birlan et al. (1996). member 26074 Carlwirtz be binary primary P1 = 2.5493 ± 0.0003 satellite orbital Porb 16.11 0.02 h. (125742) 2001 XT117 shows signs low amplitude precision period, i.e., it possibly non-principal axis (NPAR).
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