CCD photometric observations of eight asteroids were obtained from the Center for Solar System Studies from 2016 October to December.
CCD photometric observations of eight asteroids were obtained from the Center for Solar System Studies from 2016 October to December.
Lightcurves for 33 near-Earth asteroids (NEAs) obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2016 October through December were analyzed for rotation period and signs of satellites or tumbling.
Lightcurves for six Jovian Trojan asteroids were obtained at the Center for Solar System Studies (CS3) from 2016 October to December.
Lightcurves for 14 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2016 October through December.
CCD photometry observations made in 2016 October and November of the Hungaria asteroid (24465) 2000 SX155 showed it to be binary. The primary lightcurve has a period of 2.66087 ± 0.00005 h and an amplitude 0.08 ± 0.02 mag. The orbital period of the satellite is 9.252 ± 0.001 h, the shortest detected so far.
Lightcurves for 19 Hilda asteroids were obtained at the Center for Solar System Studies (CS3) from 2016 August through December.
Lightcurves for 46 near-Earth asteroids (NEAs) obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2016 July-September were analyzed for rotation period and signs of satellites or tumbling.
Lightcurves for 25 main-belt asteroids were obtained at the Center for Solar System Studies-Palmer Divide Station (CS3-PDS) from 2016 July to September.
Lightcurves for 16 Hilda asteroids were obtained at the Center for Solar System Studies (CS3) from 2016 June to September.
CCD photometric observations of twelve asteroids were obtained at the Center for Solar System Studies from 2016 July to September.