Photo AI

Galileo is credited with inventing the first telescope in 1610 - Edexcel - A-Level Physics - Question 18 - 2023 - Paper 2

Question icon

Question 18

Galileo-is-credited-with-inventing-the-first-telescope-in-1610-Edexcel-A-Level Physics-Question 18-2023-Paper 2.png

Galileo is credited with inventing the first telescope in 1610. The picture shows an early demonstration of the telescope. A converging lens was positioned at one e... show full transcript

Worked Solution & Example Answer:Galileo is credited with inventing the first telescope in 1610 - Edexcel - A-Level Physics - Question 18 - 2023 - Paper 2

Step 1

a) Explain what can be concluded about the object being viewed.

96%

114 rated

Answer

In observing distant objects through a telescope, the rays must be parallel, indicating that the object is at a significant distance from the lens. Therefore, the image created will be clear and distinct, suggesting that the object itself is far away.

Step 2

b) State what is meant by virtual and upright.

99%

104 rated

Answer

Virtual: A virtual image is one that cannot be projected on a screen as the rays do not converge at the image location; they only appear to diverge from a point behind the lens.

Upright: An upright image maintains the same orientation as the original object, meaning that it is not inverted.

Step 3

c) Draw the ray diagram for the diverging lens.

96%

101 rated

Answer

To draw the ray diagram for the diverging lens, start with an incoming parallel ray toward the lens, which diverges after passing through it. Draw another ray passing through the center of the lens which will continue in a straight line. Extend the diverging rays backward to locate the virtual image.

Step 4

d) Calculate the focal lengths of each lens.

98%

120 rated

Answer

Given the magnification (M) of the telescope is 10 and the total distance (D) between the lenses is 90 cm:

Using the formula:

10 = \frac{f_c}{f_d}$$ Let focal length of the diverging lens be $f_d$, thus $f_c = 10 * f_d$. Since the total distance is given by: $$D = f_d + f_c = 90 \ (f_d + 10 f_d = 90) \ 11 f_d = 90 \ f_d = \frac{90}{11} \approx 8.18 ext{ cm} \ f_c = 10 * f_d \approx 81.82 ext{ cm}$$

Step 5

e) Calculate the mass of Jupiter.

97%

117 rated

Answer

To find the mass of Jupiter (M), use Kepler's third law:

T2=4π2GMa3T^2 = \frac{4\pi^2}{G M}a^3

Where:

  • T=171T = 171 hours converted to seconds (171×3600=614760 s171 \times 3600 = 614760\ s).
  • a=1.07×106 km=1.07×109 ma = 1.07 \times 10^6 \text{ km} = 1.07 \times 10^9 \text{ m}. Substituting the values: M=4π2a3GT2M = \frac{4 \pi^2 a^3}{G T^2} Using G=6.674×1011 N m2 kg2G = 6.674 \times 10^{-11} \text{ N m}^2\text{ kg}^{-2}, calculate: M=4π2(1.07×109)3(6.674×1011)(614760)21.9×1027 kgM = \frac{4 \pi^2 (1.07 \times 10^9)^3}{(6.674 \times 10^{-11})(614760)^2} \approx 1.9 \times 10^{27} \text{ kg}

Join the A-Level students using SimpleStudy...

97% of Students

Report Improved Results

98% of Students

Recommend to friends

100,000+

Students Supported

1 Million+

Questions answered

;