Howdy Stan, I wouldn't so readily dismiss the idea of eta Car (not the nebula) brighten in a short period of time. What you have described is reasonably correct so as long as the brightening involves its nebula as well as the central light source. For an LBV eruption, it's conceivable that the star's diameter expands out (as it cools and becomes redder) while the total luminosity increase (as its surface area increases). In the case of a brightening by 0.5 astronomical magnitude, the star needs to increase its flux by 1.6 times or so. That implies, if purely based on apparent stellar size, the increase in diameter by 25% or so in one day. Yeah I agree that's pushing the limit; but I wouldn't know for sure if it's improbable either (BTW I think it is probable). Of course, if the brightening were real, I'd expected the surrouding nebula to be affected by the time scale that Stan was describing. So maybe someone wants to monitor eta Car with a moderately high-spatial imaging cameras. Finally I second Stan on the issue of how difficult to observe eta Car with naked eyes. I will never be able to do it (nor would I trust myself for it), but many of you seem to manage that. And that's pretty impressive to me. Regards, Bish PS. Sorry about the loss of your friend. -- "Bish" K. Ishibashi, Ph.D. Massachusetts Institute of Technology Center for Space Research e bish@space.mit.edu 77 Massachusetts Ave. NE80-6011 Cambridge, MA 02139