The concept of hydrostatic equilibrium is critical to understanding how the Sun has remainedstable long enough for life to evolve here.
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Q2: We know the Sun rotates differentially by
Q3: A sunbather on the clear day is
Q4: The energy of the Sun starts as
Q5: The Sun's density is about the same
Q6: Sunspots are only about 2,000 K cooler
Q8: The photosphere is about 100 times the
Q9: The Sun is a fairly normal star.
Q10: The Sun's luminosity is greatest when there
Q11: Scientists suspect changes in the flow of
Q12: Solar activity cannot disrupt communications on Earth.
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