The nucleus of comet C/1996 J1, whose duplicity was first detected in
early May 1997, similar to 4 months after perihelion, is found to have
split nontidally similar to 70 days before perihelion at 1.65 AU from
the Sun. The secondary nucleus, discovered when in outburst and subse
quently observed for 8-1/2 months, had separated from the primary nucl
eus at a rate of 1.7 m/s and drifted away from it with a radial nongra
vitational deceleration of similar to 31 x 10(-5) the Sun's attraction
, typical for the short-lived companions. At the time of splitting, th
is dynamically new comet was near conjunction with the Sun and therefo
re unobservable from Earth. In late 1997 and early 1998, when last see
n, the companion was greater than or similar to 100 times fainter rela
tive to the primary component than it had been when first reported.