Messier 14 (also known as M14 or NGC 6402) is a globular cluster of stars in the constellation Ophiuchus. It was discovered by Charles Messier in 1764.
Taking his cue from the observed capability of quasars to eject enormously concentrated beams of matter from their interiors in a controlled, non-concentric version of the “Big—bang” he envisages a similar process occurring in the generation of the universe( see Exhibit 4, next page).