For a circular orbit, it's ##\sqrt{\frac{GM}{r}}## where ##G## is the gravitational constant, ##M## is the mass of the body being orbited (here: Moon), and ##r## is the distance from the centre of the body. The mass of the craft doesn't matter.
Find the values on Wikipedia and plug them in. Or, you can make it even easier, and take the escape velocity listed on Wikipedia's page about the Moon, and divide it by ##\sqrt{2}##. The result will be only marginally off.