Analysis and Assessment of Gateway Process § 34, ¶ 2

Messier 12 (Wikipedia) Messier 12 or M 12 (also designated NGC 6218) is a globular cluster in the constellation of Ophiuchus. It was discovered by the French astronomer Charles Messier on May 30, 1764, who described it as a “nebula without stars”. In dark conditions this cluster can be faintly seen with a pair of binoculars. Resolving the stellar components requires a telescope with an aperture of 8 in (20 cm) or greater. In a 10 in (25 cm) scope, the granular core shows a diameter of 3′ (arcminutes) surrounded by a 10′ halo of stars.

“The tangible world is movement, say the Masters, not a collection of moving objects, but movement itself. There are no objects “in movement,” it is the movement which constitutes the objects which appear to us: They are nothing but movement.

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