The Sun's Yearly Motion

Project 6

 

Project Goal: To observe the changing altitude and azimuth of the Sun throughout the year.

 

What You Need for This Project

To do this project you will have to be able to view the movie clip included with this project.  All Macs come with a version of QuickTime and computers running Windows have a movie viewer called Media PlayerThe movie clip should play using either type of computer or player.

If your computer does not have QuickTime movie viewer installed you can download the Macintosh or Windows version from the internet by clicking on QuickTime.  Also, an installable version of QuickTime is included on the StarryNight CD program disk.

Start the movie and watch as Sirius rises and sets.  Drag the horizontal scroll box to the left to rewind to the first frame of the movie.  Clicking once to the right of the scroll box will advance to the next time frame.  Alternately, if you are using a QuickTime viewer, you can click the right arrow at the end of the scroll bar.   Each click advances one time frame forward.  The left arrow allows you to step backward in time.  

 

What You Need to Know for This Project

In the upper left hand corner of the movie screen you will see the date (March 21, 2000) and time (12 noon), as well as the altitude, azimuth, right ascension, and declination of the Sun.  This data updates every 2 days for one year as the movie runs.

Record the date and corresponding altitude, azimuth, right ascension, and declination of the Sun. begining March 21, 2000 A.D. and ending March 22, 2001.A.D,

The Sun's noon (upper transit) altitude = 90deg  -  Latitude  + The Sun's declination.

For a discussion of relavent information see Voyage 2, Voyage 4, Voyage 6.

To begin your observations click The Sun's Yearly Motion

 

Print or copy the Project Results Form on which to record you answers and hand it in to your instructor.

 

Project 6

Results Form

 

Name____________________ Student Number__________ Class ______________

Date ____________________

 

Task 1: Observing the Sun"s yearly motion.

 

Time of Observations___________________

Latitude_____________    Longitude________________

 

Date                                                Altitude                      Azimuth                  Right Ascension                 Declination

March 21, 2000 _____________________________________________________________________________

__________________________________________________________________________________________

__________________________________________________________________________________________

__________________________________________________________________________________________

June 21, 2000_______________________________________________________________________________

__________________________________________________________________________________________

__________________________________________________________________________________________

__________________________________________________________________________________________

September 21 2000__________________________________________________________________________

__________________________________________________________________________________________

__________________________________________________________________________________________

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March 21, 2001_____________________________________________________________________________

 

Task 2: Plot the Sun's altitude on the vertical axis of a graph and azimuth on the horizontal axis.

Hint: Because the Sun"s azimuth remains around 180 degrees, the best units for the azimuth axis might possibly be in minutes of arc.  There are 60 minutes of arc in 1 degree.

 

Based on your observations:

 

1. Describe how the Sun's altitude varies throughout the year.

 

 

2. On what date is the Sun's altitude largest?___________________.

 

 

3. On what date is the Sun's altitude smallest?___________________

 

 

4. The Sun's noon altitude on March 21, 2000 A.D. was__________________.  Is this value what you would predict using the relationship,

The Sun's noon (upper transit) altitude = 90deg  -  Latitude  + The Sun's declination.

Predicted value:_____________________.

 

5. Compare the Sun's noon altitude on December 21, 2000 A.D. with the predicted value.

Observed Value______________________

Predicted value:_____________________.

 

6. Complete the following table based on your observations,

 

                                   Sun"s Noon  

                                                          Right Ascension     Declination    Altitude     Azimuth

        Vernal Ewuinox (March 21)         __________________________________________________

        Summer Solstice (June 21)       __________________________________________________

        Autumnal Equinox (Sept 21)       __________________________________________________

        Winter Solstice (December 21)  __________________________________________________