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Granulation is the most obvious proof of solar convective energy transport.
Q1: What two energy transport mechanisms, in order
Q48: While none yet exist, in the very
Q51: Which molecule has not yet been detected
Q60: The region in the H-R Diagram where
Q73: Spectra of stars often show narrow absorption
Q80: Why are infrared observations useful when observing
Q80: The proton-proton chain requires a temperature of
Q94: Isolated main sequence stars as massive as
Q95: What feature of interstellar dust is inferred
Q106: How long does it take an M