Are Galaxies Mostly Stars? Mass and Luminosity Determination of Spiral Galaxies and Stellar Groups
In order to determine what spiral galaxies are composed of, we have to find their mass and their luminosity to produce a mass/luminosity ratio. This will help us determine what spiral galaxies are composed of because we can compare their mass/luminosity ratios to known stellar mass/luminosity ratios. By comparing these two different mass/luminosity ratios, we can determine if galaxies are composed mostly of stellar material. In this report, I will be analyzing 26 different spiral galaxies by finding their mass, their luminosity, and their mass/luminosity ratio. By using these techniques, I will show that only \(10\%\) of the total galactic mass is made of stellar material and that \(90\%\) of a galaxy is composed of non luminous “dark matter.”
A very important question in astronomy is if spiral galaxies are composed entirely of stellar material - stars. This question has puzzled astronomers for years and in this report, I will explain how to find the answer to this question. I will be finding the mass and luminosity of 26 different galaxies in order to find their mass/luminosity ratio. I will be using the Inital Mass Function to find the mass/luminosity ratio of stars and I will compare the two mass/luminosity values in order to find the percent of stellar mass in a galaxy. I will be using data from an astronomy Java program for the galaxy data and Guy Worthey’s Interpolation Medel (an Initial Mass Function program) for the stellar data.
This paper will be outlined as follows: Section 1: How to find the mass/luminosity relationship for Galaxies, Section 2: How to Determine a mass/luminosity relationship for Stars using the IMF, Section 3: Comparing the two different mass/luminosity relationships and what that means for Spiral Galaxies, and finally, Conclusions.
The Java applet used for galaxy data provides the flux of the galaxy in \(Watt/ m^2\), the velocity of the galaxy in \(km/s\), and the X and Y position of the velocity data in arc seconds ("
It is important to understand that the only reason we can measure a doppler shift (and therefore a radial velocity) is because the galaxy has an inclination toward or away from Eath. The only reason doppler shifts happen is because the star are moving toward or away from Earth in their respective galactic orbit. For example, an inclination of 90 degrees is edge on, and an inclination of 0 degrees is face on, and any angle in between will describe the tilt from Earth. If the galaxy is face on, we can not measure a doppler shift,