P/Wirtanen is now the main target of the Rosetta mission. The orbit of
this Jupiter family comet is perturbed by frequent approaches to Jupi
ter. The last one occurred in 1984, and placed the comet on an orbit w
ith reduced perihelion distance. Since no observations with electronic
detectors are yet available, the visual lightcurves of the last perih
elion passages in 1986 and 1991 are studied. This yields a production
rate of 4 x 10(28) H2O melec s(-1) at perihelion acco to a simple corr
elation law between heliocetric magnitude and production rate. The mag
nitudes at recoveries on photographic plates indicate a nuclear absolu
te magnitude of about 16.5, corresponding to a nucleus of radius 1.8 k
m, assuming an albedo of 0.03. In order to reconcile the nuclear radiu
s with the gas production curve, it is found that the fraction of the
active area of P/Wirtanen should be as high 0.25. This appears to offe
r the best explanation to the large nongravitational acceleration suff
ered by this comet.