DataTable 1 |
|
Focal length, f |
1.76 |
2f |
3.52 |
Height of object, ho |
4.0 |
Data Table 2 |
|||||
General Description |
Object Dist. (cm) |
Image Dist. (cm) |
Object Size (cm) |
Image Size (cm) |
Other Observations (real, virtual or no image?) (Upright or inverted image?) |
Object about 5 f |
10 |
74.04 |
4 |
-29.62 |
Real, inverted |
Object about 2.5f |
10 |
7.87 |
4 |
-3.15 |
Real, inverted |
Object 2f |
10 |
5.44 |
4 |
-2.18 |
Real, inverted |
More than f and less than 2f |
10 |
4.29 |
4 |
-1.71 |
Real, inverted |
Object at f. |
10 |
2.14 |
4 |
-0.86 |
Real, inverted |
Object less than f. |
10 |
1.11 |
4 |
-0.44 |
Real, inverted |
Data Table 3 |
||
Trial 1= 2f |
Trial 2= f |
|
f (cm) |
-3.53 |
-1.76 |
do (cm) |
10 |
10 |
di (cm) |
-2.61 |
-1.5 |
ho (cm) |
4 |
4 |
hi (cm) |
1.09 |
0.6 |
Type of image: real, virtual, none |
Virtual |
Virtual |
Direction of image: inverted or upright |
upright |
upright |
The key to understanding a telescope is to remember that the purpose is to gather light from distant objects. The image from the primary lens is magnified by a second lens to increase its size. Why should you use a longer focal length lens as the primary lens and then add other lenses as eyepieces.
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