bhavjain wrote:Do Type II Cepheids have a longer period than Type I?
I don't think they can, although this graph may not show everything.
bhavjain wrote:Do Type II Cepheids have a longer period than Type I?
How do you get the temperature of the x-coordinate? Sorry, new to AstroAdi1008 wrote:This is a plot of surface gravity (on the y axis) vs. temperature (on the x axis) of post AGB stars on their way to becoming the central star of a planetary nebula. The lines show different evolutionary tracks over time for post AGB stars of different masses.Unome wrote:Going to move my question to this thread: what is this?Adi1008 wrote:Here's my question:
(a) What do the colored lines represent?
(b) Rank A, B, C, and D in terms of mass
(c) What is the x-coordinate of the point labeled 2015, in Kelvin?
(...)
More massive stars are (in general) hotter, which is why the more massive stars are on the left, and vice versa
By knowing the surface gravity, it also gives us properties like the radius (size) and luminosity.
You might be wondering what the g/(cm/s^2) stuff is. Initially, it may look like grams/(cm/s^2), but the argument of a logarithm should be dimensionless - that is, the units should cancel out in order for the logarithm to make sense. When it says "g", they don't mean g for "gram", they mean "g" for surface gravity, like g = -9.8 m/s^2 for Earth. It's hard to know that they're talking about that type of "g" though, but you can still figure it out. Since the argument of the logarithm has to be dimensionless, you know that whatever "g" is must have the same dimensions as "cm/s^2", which is just acceleration. Personally, when I see "g" and the units for acceleration, it's clear as to what it's trying to say. Additionally, log(g) is a common term in astronomy (I think, at least; Wikipedia says surface gravity is often expressed as log(g): https://www.wikiwand.com/en/Surface_gravity). You'l notice that's why plots have things like log(T_effective/K); the K is to get rid of the unit on the temperature.
Magikarpmaster asked about this in the question marathon thread too; I'll post some more stuff there too
The x coordinate shows what log(T/K)* is equal to. For example, if the x coordinate is 10, then that means that log(T/K) = 10, so T = 10^10 Kelvin (that's really hot!).bhavjain wrote:How do you get the temperature of the x-coordinate? Sorry, new to Astro
It's derived here: https://somewhatoverwhelmed.wordpress.c ... e-modulus/bhavjain wrote:Is it possible to derive the distance modulus formula from the inverse square law and other laws?
Not really.gryphaea1635 wrote:Is there a good textbook to use for studying for this event?
Hello eris_joseph! And welcome to Astronomy! Hope you have fun with this event; I know I have! First, some sites I like to use for the Deep Sky Objects are the NASA Astronomy Picture of the Day, the Chandra Telescope website, and the Hubble website. On those websites, you can search up each DSO and find articles about them that'll tell you lots about what the objects are, their characteristics, and why they're important. In addition, you can get the pictures of the objects as well as find out in what wavelength they're taken in. Sometimes a question might ask you in what wavelength the picture was taken in and why that's important and those websites can help you out in that regard. In addition, I would recommend just practice practice practice! Use flashcards to make sure you understand the formulas and why they're important, including (and probably most importantly) in what situations you would use them. For instance, I might write a flashcard on the Stefan-Boltzmann Law, say that it's important for analyzing blackbody radiation and write down the formula so that I don't have to dig through my formula sheet the day of. (As much as that sheet's helpful, it can also be painful if you don't know what you're looking for!) In addition, I would recommend categorizing a lot of the material depending on what they're about, so for instance one category could be mathematical calculations on distances and binary orbits, one category could be about the deep sky objects, and one category could be about stellar evolution and its characteristics. Hope that helps and good luck with all your Astronomy endeavours! And if you need any more, I and a bunch of the other astro/physics people (syo, Alpha, Karp, foreverphysics, East, etc. I'm sure I'm missing some) would be glad to help; just give us a notice and we'll do our best to help!eris_joseph wrote:new to this event. if anyone has site recommendations or tips that would be great.