The first half of the nineteenth century found the nebular

hypothesis accepted almost without question, but a tearing-down
process began in the second half of the century, and at present
not much of the original structure remains standing
The first half of the nineteenth century found the nebular
hypothesis accepted almost without question, but a tearing-down
process began in the second half of the century, and at present
not much of the original structure remains standing. This is
due in small part to discoveries since Laplace"s time, but
chiefly to a more careful consideration of the fundamental
principles involved. We have space to present only a few of the
more salient objections.


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