Early in its lifetime a 1-M ? protostar will have 100 times the Sun's luminosity. How is this possible?
A) The first nuclear reactions in a protostar are more energetic than the later hydrogen to helium fusion.
B) The initial temperature is low but the protostar's radius is large.
C) Although small, the protostar's initial temperature is high.
D) The Kelvin-Helmholtz contraction, the protostar's first energy generation mechanism, is more efficient than nuclear fusion.
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