Although the "bulge" observing season is practically over, we would like to draw your attention to a very interesting microlensing event, OGLE-2000-BUL-43, currently in progress. Observations collected during the last few months at the Las Campanas Observatory indicate that that event is very interesting threefold: -- its time scale is very long: the Einstein radius crossing time, t_E, is about 180 days, -- point mass microlensing fit to the rising branch of the light curve indicates very high magnification at maximum light (the current, Nov 14.01 UT, magnification is A=5), -- the microlensed star is very bright. To our knowledge this is the brightest microlensing event which has been observed so far. At maximum the microlensed star might be well brighter than I=10 mag. Such bright events could likely be easily resolved into separate images with interferometric techniques in the near future, breaking the degeneracy of microlensing parameters and allowing straight and precise mass determination. Unfortunately, the predicted maximum time of OGLE-2000-BUL-43 occurs around Christmas, when the Galactic bulge is very close to the Sun on the sky. OGLE-2000-BUL-43 Field BUL_SC7 StarNo 20290 RA(J2000.0) 18:08:43.04 Dec(J2000.0) -32:24:39.5 Finding charts, light curve plots, photometric data (updated regularly) can be found in: http://vsnet.astrouw.edu.pl/~ogle/ogle2/ews/bul-43.html http://vsnet.astrouw.edu.pl/ogle/ogle2/ews/2000/bul-43.tar.gz This is probably the last alert issued by OGLE during the OGLE-II phase of the project. We hope to resume the service in 2001 when OGLE-III phase starts. regards, OGLE team.