Answer any 8 of the following 10 questions. Each is worth 12 points.
1) Even though most stars have very similar abundances of Hydrogen, the absorption line strengths of Hydrogen can differ from star to star depending upon the surface temperature.
2) Star A and star B have identical surface temperatures and compositions, and neither star has a significant rotation speed. The absorption lines from star A, however, are much broader than the absorption lines from star B.
3) Two interstellar clouds (X and Y) are located at identical distances from us, but we know from emission line spectra that cloud X is much warmer than cloud Y. Assume for this question that stars are distributed uniformly across the sky.
4) Below are the light curves for two eclipsing binary systems:
5) In a face-on binary system, we can easily measure the angular separation between the binary pair. From parallax measurements, we also know the distance from the Earth to the system. Assuming the companion star orbit is circular...
6) We estimate the main-sequence lifetime of the star Alpha Centauri to be about 12 billion years. The star Procyon has a mass of about twice the mass of Alpha Centauri. The lifetime of a star depends inversely on its mass squared.
7) Imagine a spherical volume of space with a radius of about 200 parsecs (the maximum distance out to which we can make reliable parallax-based distance estimates) centered on the Sun. Explain why this volume of space will contain more low mass stars (masses < 1 solar mass) than high mass stars (masses > 1 solar mass).
8) The nucleus of Hydrogen consists of simply one proton. An isotope of Hydrogen called "Deuterium" has a nucleus containing one proton and one neutron (so the nucleus has the same charge as Hydrogen but twice the mass).
Suppose you want to try to fuse Deuterium, but you want to maintain the same density as the gas in which Hydrogen fusion has successfully occured. Explain how and why (just one reason) the temperature in the Deuterium gas will need to be different in order for fusion to occur.
9) At the end of the Hydrogen burning phase (the main sequence) part of a solar-mass star's lifetime, several changes occur in the star.
10) We know that the absolute luminosity of a star can be written as follows:
Our own Sun has a temperature of 6000 K.