Astronomy class 2012
Friday, May 18, 2012
Monday, May 7, 2012
Module 6
State the B-v, the absolute and apparent magnitudes and the distance in parsecs and light years for each of your 3 stars.
Thursday, May 3, 2012
Module 5
Give the 3 names of your stars. For each star state the temperature, the class, the balmer lines and any other absorption lines that you used to determine your classification. Then go to the simbad website and find the B and V magnitudes for each star.
Monday, April 23, 2012
Thursday, March 29, 2012
Module 1, assignment 1
Describe the light sources and spectra that you have projected in detail as well as any experimental difficulties you encountered in the process. How do the different light sources compare with each other?
Thursday, January 5, 2012
Introduction
Please use the comment box to introduce your self to the astroBITS group. The course material can be found at http://www.noao.edu/education/astrobits/course-outline.php. Also check azastro.pbworks.com
Module 1, Assignment 2
What is the largest value you can find within the image of the sun? Let’s call these “Data Numbers” or DN value.Comment on what you estimate is your measurement accuracy. How many significant figures are meaningful? (In other words, can you measure the diameter to an accuracy of one pixel? One tenth of a pixel? One hundredth of a pixel? None of these?)How much fainter in DN units is the sunspot than its surroundings?Repeat your measurement of the Sun’s diameter several times and post your average value of the diameter in kilometers on the Blog. Include a comment about sig figs.
Describe the general nature of the sun's surface around the location of this sunspot.
Describe the general nature of the sun's surface around the location of this sunspot.
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