Universities
Space Research Association, U.S. Naval Observatory, P.O. Box 1149, Flagstaff,
AZ 86002-1149
Presented
at the 91st Annual Meeting of the AAVSO, October 26, 2002; revised February 13,
2003
Abstract The peculiar nova V838 Mon has been
monitored since its initial outburst in January 2002. The light curve shows
several separate outbursts-a month-long hump in January, followed by a rapid
4-magnitude rise in February, two minor brightenings in March and April, and a
final decline in May. This paper will discuss the current state of the nova
itself, the remarkable light-echo around it, and offer some suggestions as to
how amateurs can continue to monitor the object over the coming seasons.