the sun/radiation (sorta)/ fusion/(yea pretty much the sun)
Answer:
the last one
Explanation:
it looked similar to the question i had on A P E X but if it's not right can you put the right answer in the ch.at for others with the same question.
We can use the formula for orbital time period:
T² = (4π²/GM)a³; where T is in Earth years, a is distance from sun in AU, M is the solar mass (1 for the sun), G is the gravitational constant.
In the given units, 4π²/G = 1
T² = 0.66³
T = 0.536 Earth years = 195.71 Earth days
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Answer:
Hi! It's C. Moving to a new state.
Explanation:
A, B, and D are about things that happen temporarily. Moving to a new state is long term.