SIERRA COLLEGE OBSERVATIONAL ASTRONOMY

LABORATORY EXERCISE

NUMBER     II-Bb TITLE:   Field of View – Supplementary Exercise

DATE-                             PRINT NAME/S AND INITIAL EACH                GROUP

                                                               

DAY-                                      

                                                                               

LOCATION

 

 

OBJECTIVE:

·        Calculate the true Fields-of-View of several eyepiece-telescope combinations

·        By using TheSky, simulate to use of the drift method to calculate the field of view of a particular eyepiece-telescope combination

           

 

DESCRIPTION:

 

Celestial objects come in a variety of sizes and shapes.  When observing the moon, a planet, star cluster, or any celestial object, the size of the field of view (True Field) of a telescope will determine how much of the object will fit into the area of sky viewable through the eyepiece or camera.  This activity will provide the opportunity to predict and measure the area of sky accessible of a variety of telescope and eyepiece combinations.

 

PROCEDURES AND OBSERVATIONS:

I.  Magnification and FOV

 

1.      Calculate and record in Table D: Do and Fo of;

a.       A 8 in f/6.3 telescope.

b.      A 10 in f/10 telescope.

2.      Calculate and record in Table D:  the magnification and True FOV of

a.       A 8 in f/6.3 telescope with a 30 mm eyepiece

b.      A 10 in f/10 telescope with a 12 mm eyepiece?

 

 

 

 

 

 

TABLE D – TheSky Telescope True Fields of View

 

Telescope

Eyepiece

Do

 

Fo

 

M

 

TFo

10 in f/10

12 mm

 

 

 

 

8 in f/6.3

30 mm

 

 

 

 

Telrad

 

 

 

 

 

           inner

     xxxx

     xxxx

     xxxx

     xxxx

     0.5 O

mid

     xxxx

     xxxx

     xxxx

     xxxx

     2.0 O

outer

     xxxx

     xxxx

     xxxx

     xxxx

     4.0O

 

 

II.  Locating Objects in the Sky

 

  1. Set the time to 8 PM on today’s date.
  2. Go to View Menu, Select Status Bar, Select Field Width
  3. Go to View Menu, Select Field of View Indicators
  4. Select:
    1. Telrad
    2. 8 in f/6.3 30 mm eyepiece
    3. 10 in f/10 12 mm eyepiece
  5. Select the Pole Up icon on the menu bar or go to Orientation Menu, select Pole Up
  6. Find Betelgeuse – center on it
  7. Zoom in until FOV is between 8 – 9 degrees
  8. Using the up-down, left-right scroll bars and your SC001 chart to “star-hop”, slew your “Telrad View” of the sky until you locate M42  - attempt to center it
  9. Select M42 – The Great Orion Nebula, (right click on it) and center it (use the icon at the bottom left of the information box)
  10. Zoom in and determine what Telescope/eyepiece combination would give the best view of M42 (a view that shows most of the nebula in the eyepiece? Record the answers in your Bluebook
  11. What is the limitation when using the Telrad to locate objects in the eyepiece by “Starhopping”?

Put the answer in your Bluebook

 


III.   Large Star Clusters FOV

 

1.      Find and center M45

2.      Zoom in and determine what telescope/eyepiece combination or Telrad ring would be best for viewing the Pleiades

Put the answer in your Bluebook

 

IV.  Separating Double Stars

 

1.      Find and center on Albireo

2.      What telescope/eyepiece gives the best view of the two stars of the double star Albireo?

Put your answers in your Bluebook

 

V.  Moons of Jupiter

1.      Find and Center Jupiter

2.      What eyepiece gives the best view of Jupiter and all its moons?

                  Put your answer in your Bluebook

 

 

VI.  STAR DRIFT METHOD Using TheSky

      

1.      Go the View Menu, Select Field of View Indicators. Select:

a.      the Telrad,

b.      8 in f/6.3 telescope with 30 mm eyepiece and

c.      10 in f/10 telescope with 12 mm eyepiece and

d.      click OK

 

2.      Select the South (S) direction button on the toollbar

 

3.      Set the Time Interval to 0.1 second

 

4.      Use your SC001 chart and select a star near the Celestial Equator.  Center Star in FOV with the time advance stopped.

 

5.      Zoom in/out until the inner and middle Telrad FOV indicator rings, and the 8 in and 10 in telescope FOV indicator rings are within the screen.

 

6.      Use the clock on the front wall of the lab to measure time intervals

 

7.      Wait until the time reaches :00 seconds.  Note the time in minutes and  seconds, and immediately select the automatic time advance double arrow.


 

8.      When the center of the star reaches each of the following FOV rings the note the time to the second and record in Table E:

a.      10 in telescope ring

b.      Smallest of the three Telrad rings

c.      8 in telescope  ring

d.      Middle Telrad ring

 

9.       Complete Table E

 

10.  Which method of measuring FOV gave the best agreement with the actual values – The Direct Method or the Star Drift method

Record your answer in your Bluebook

 

 

 

 

 

 

TABLE E – Data for Star Drift Method

Telescope/

Eyepiece

Half-Times (sec)

Times “T” (sec)

TFo (EQ. #4)

10 in f/10

12 mm

                    x2=

 

 

8 in f/6.3

30 mm

                    X2=

 

 

 

                   

 

 

Telrad      Inner

 

      middle

     

                    X2=

 

 

                    X2=

 

 

 

 

 

                                                                 

TFo= T/240sec

 
This is a conversion from time to angle based on the Earth’s rotational speed of 15o per hour.                                 

                                                                         EQ. #4