A novel technique for the measurement of the excitation of molecular h
ydrogen formed on surfaces has been applied to the study of H-2 format
ion on carbon. The results show that on certain carbon surfaces H-2 ma
y form in vibrational levels as high as v = 7, and that at a surface t
emperature of 90 K between 2.6 and 7% of the molecules can be found in
the v = 1 level. This supports the proposal that a significant contri
bution to the population of vibrationally excited hydrogen in the inte
rstellar medium comes from the formation of molecular hydrogen on carb
onaceous interstellar grains.