This is more guesswork:
Assume that the whole energy directed towards the Moon (so gamma and x-rays together with fast atoms and bomb fragments) gets absorbed uniformly in the first 10cm of the surface. To get the best light output per energy, heating the surface to ~6000K is good. With half of the 2PJ, how large can the area be?
It
looks like lunar regolith can be approximated by SiO2 but with a
lower density of 1660kg/m^3.
How much energy do we need to break the bonds of SiO2? Afterwards, we have 3/2 R at 20 g/mol -> 0.6J/g. I'll use this as lower limit for the energy we need to heat the material.
Therefore, we can heat 1PJ/(600J/(kg*K)*1660kg/m^3*10cm*6000K) = 1.7km^2. Let's assume that we manage to heat exactly this surface and nothing else. This will radiate with a power of 73MW/m^2 or 73TW/km^2 (
WA), 40% of this is visible light (
from here). 50TW... but how long does it last? Typical particle velocities of silicon atoms at this temperature are E
kin~kT => ~2km/s (oxygen is a bit faster). After 1/2 millisecond, the hot layer will have expanded by a factor of ~10 (order of magnitude), and cooled so much that its power is negligible. This would lead to ~25GJ of visible light. Using the eye light integration time from above (now it is useful :D), we get an effective power of 250GW.
1/6000 of a full moon.
10 units of apparent magnitude, which puts our nuclear explosion at -3. Close to the maximal brightness of Mars and Jupiter, so definitely visible (but not very spectacular, given the short time).
I think this is more like an upper estimate of the brightness. For an event so short, I guess an apparent magnitude of +4 is a reasonable limit for the visibility, so my estimate is a factor of 200 above that limit.
Hmm... could be possible.