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As the motion of the gases increases, it causes and increase in the outward:
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
After the initial contraction, what happens to the temperature of this gaseous body?
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
When the core of a protostar reaches 10 million degrees Kelvin, the pressure is so great that the nuclear fusion of what gas begins?
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
A protostar is a developing star not yet hot enough to engage in the process of:
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
What does the forming star become when the outward pressure equals the inward force of gravity?
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
During the evolution of a star, what event takes at least a million years to occur?
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
The gaseous body that continues to form, now appears as a large red object called a:
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
After the initial contraction and when the temperature rises high enough, energy is radiated from the surface in the form of:
stable main-sequence star
initial contraction
rises
long-wavelength red light
gas pressure
hydrogen
nuclear fusion
protostar
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