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The mysterious 3rd magnitude long period eclipsing binary star system epsilonAurigae is predicted to be starting its 2 year eclipse in the late summer of2009. While this is when the real excitement starts, much is to be learnedbefore first contact. This paper discusses current observational results thathave accumulated thus far, using photometric monitoring, H-alpha spectroscopyand with other data sources. Key among the findings are that (1) the lowamplitude light variation quasi-period has decreased significantly over thepast 20 years, and (2) that the duration of egress, eclipse-to-eclipse has beendecreasing, while the duration of total eclipse has been increasing. Thewebsite for the observing campaign is: www.du.edu/~rstencel/epsaur.htm .

Gearing Up for Epsilon Aurigae's First Eclipse of the Millennium