The Wide Field Camera 3 (WFC3) was installed in 2009 and is now the primary science
	instrument on HST. Under development since 1998, WFC3 expanded Hubble's ultraviolet and
	infrared imaging capabilities by factors of more than 20. WFC3 also provides an unparalleled capability
	for low resolution infrared spectroscopy of very faint sources. This talk will discuss the scientific
	goals for WFC3, its basic design and technological advances, the achieved in-flight performance,
	and our plans for future enhancement of its capabilities.