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astro300_f17:boardwork_questions [2017/08/01 04:41] – created ccheng | astro300_f17:boardwork_questions [2017/08/01 04:41] (current) – ccheng | ||
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+ | =====Board Work Questions===== | ||
+ | * Why is this statement true? “If we were to measure Doppler shifts in spectra of Saturn' | ||
+ | * Why is this statement false? “It is easier to use parallax to measure distances to stars in distant galaxies.” | ||
+ | * Why again is Venus' | ||
+ | * This homework question asks us to estimate how long it would take for us to lose sight of Jupiter (at 4 AU) if the Sun were to suddenly shut off (i.e., stop shining). The problem says we can assume the Sun-Earth-Jupiter system are all aligned, for simplicity. | ||
+ | * What does the professor mean by the “dark side of the Moon”? I said that part of the Moon never receives sunlight and got the question wrong. | ||
+ | * Why do atoms only accept photons of particular wavelengths? | ||
+ | * I have to compare the luminosity of two stars. One of them is twice as massive as the other and I know that L goes as the fourth power of M. There aren't enough numbers here for me to calculate the answer. | ||
+ | * Can you go over the homework problem: Two stars at the same distance from us are the same temperature, | ||
+ | * The Sun appears slightly bigger in the sky in January than it does in July. Given this information, | ||
+ | * It doesn' | ||
+ | * Why is Orion considered a Winter constellation? | ||
+ | * Why do we need to build some telescopes in space? | ||
+ | * I don't understand how Olber' | ||
+ | * How is the Milky Way's rotation curve different than that of our Solar System' | ||
+ | * I don't understand how if I'm standing at the equator I can see all the stars. | ||
+ | * [lab] How do I find a star's position in my data? Can I take the maximum pixel value? | ||
+ | * [lab] Why do we need darks and flats when observing? | ||
+ | * [lab] How do I know what wavelength each pixel in my data corresponds to? |