68th National Conference on Weights and Measures 1983

The Near-Earth Objects Follow-up Program IV. CCD Photometry in 1996–1999

“…Lightcurves of this Apollo-type asteroid were obtained in 1984 by Tholen (1985), in 1989 by Wisniewski et al (1997), in the 1994/1995 apparition by Meech et al (1996), and in 1995 and 1997 by Pravec et al (1998). These observations revealed a synodic rotation period around 3.6 h, with amplitude ranging from 0.11 to 0.34 mag.…”