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Since 1995, the detection of over 100 extrasolar planets has captured the attention of both astronomers and the public. The surprise of extrasolar planetary science, and the challenge to theorists, is the large number of Jupiter-class objects orbiting within 0.1 AU of sun-like stars. Did they form in place or migrate? Why did this not happen in our solar system? What happens when you heat Jupiter to 1400 K? The proximity of the parent star requires large telescopes and novel techniques to measure planets directly. Techniques that apply to planets that pass in front of or behind their stars are particularly attractive, and have begun to yield results. The primary-transit detections sodium and hydrogen in the atmosphere of HD 209458b, our significant non-detection of methane thermal emission in this object's secondary eclipse, and the declining central flash in the 18-day occultation by a probable protoplanet orbiting KH 15D are but the first liftings of the stellar veil. The talk will review developments in the field, focusing in particular on these two systems and giving an update on our recent observations at Palomar, IRTF, VLT, and Keck. |