Magikarpmaster629 wrote:Hmm...I'm having trouble figuring out what math I need to know, besides the usual Kepler's Laws, light-related equations (Wien's Law, doppler shift, etc.), distance equations (parallax, distance modulus). I think I've seen age of a cluster from an HR diagram, but that's pretty simple. Last year we had all this stuff related to detecting exoplanets, like an equation to find the radius of a transiting exoplanet or the mass of an exoplanet from its radial velocity. I guess those both can be done with binary stars as well, but is there anything else I should know how to calculate? Specifically related to SN Ia, white dwarfs, or accretion disks?
Last year they had some really cool stuff with gas clouds and SEDs too!!!!!!!!! In addition to what you said, maybe some Hubble's Law stuff, but that stuff is pretty straightforward. I think you won't see much math in isolation, but rather, embedded within harder, more complex questions that test tough concepts. There, the math itself won't be hard, but figuring out the concepts behind it will be
Also, pretty random, but what was the first white dwarf to be discovered? It won't really help on a test in scioly, since it's just trivia; I'm just curious. I've seen a variety of sources say it's 40 Eridani B, while other sources say it's Sirius B. 40 Eridani B was discovered in 1783 and astronomers figured out it was a white dwarf in 1910. Sirius B was discovered in 1844 through calculations and astronomers figured out it was a white dwarf in 1915 (all this information is straight off Wikipedia). However, a lot of websites (such as
http://whitedwarf.org/education/ask/index.html#3) say it's Sirius B. What would cause the discrepancy?