Observations of Nereid with the 200-in. telescope on Palomar Mountain
over three contiguous nights in July 1995 show no evidence for the lar
ge photometric variations seen by earlier observers. Total brightness
variations within a single night are less than 10%. Our results sugges
t that Nereid may have a long rotational period, perhaps on the order
of weeks. Our observations were not obtained close enough to Nereid's
apoapsis to determine whether its rotation state is chaotic, as sugges
ted by Dobrovolskis (1993, Icarus 118, 181-198). (C) 1997 Academic Pre
ss.