cepheidvariablesandthecosmicdistancescalelab - Cepheid...

Info iconThis preview shows pages 1–2. Sign up to view the full content.

View Full Document Right Arrow Icon
Cepheid Variables and the Cosmic Distance Scale I. Purpose : The purpose of the Cepheid Variables and Cosmic Distance scale lab is to determine the distances to distant stars. By knowing all of the stars in the Small Magnetic Cloud are the same distance from the sun, we learned that the brighter Cepheid’s are intrinsically more luminous. Basically, the period of a Cepheid is an indicator of intrinsic luminosity. II. Procedure : First, we used page 53 where we were given four Cepheid variables in the Small Magnetic Cloud, taken using yellow light by Halton C. Arp. We started by finding each stars maximum and minimum apparent magnitudes to the nearest 0.1 magnitude; we then took the average of the two. We then had to find the period in days for each, and we did this by taking the interval between peak to peak on the graph, also known as successive maxima. We then used the logarithm of the period. Next, using the graph paper provided we split the stars apparent magnitude as the ordinate against the logarithm of the period, to two decimal places. On the graph on page 56 we then
Background image of page 1

Info iconThis preview has intentionally blurred sections. Sign up to view the full version.

View Full DocumentRight Arrow Icon
Image of page 2
This is the end of the preview. Sign up to access the rest of the document.

This note was uploaded on 12/22/2010 for the course AST 8716 taught by Professor Reim during the Spring '10 term at University of Southern Maine.

Page1 / 3

cepheidvariablesandthecosmicdistancescalelab - Cepheid...

This preview shows document pages 1 - 2. Sign up to view the full document.

View Full Document Right Arrow Icon
Ask a homework question - tutors are online