Final answer:
To find the distance at which a coin can be resolved by a telescope, we can use the formula θ = 1.22 × (λ / D). By substituting the values into the formula and solving, we find that the coin can be resolved at a distance of approximately 0.0398 miles from the telescope mirror.
Step-by-step explanation:
To calculate the minimum distance from the telescope mirror to resolve an object, we can use the formula:
θ = 1.22 × (λ / D)
Where θ is the angular scale, λ is the wavelength of light, and D is the diameter of the telescope mirror.
- Convert the diameter of the coin from cm to m: 3.0 cm ÷ 100 = 0.03 m
- Convert the wavelength of light from nm to m: 389 nm ÷ 10^9 = 3.89 × 10^-7 m
- Convert the diameter of the telescope mirror from cm to m: 102 cm ÷ 100 = 1.02 m
- Substitute the values into the formula: θ = 1.22 × (3.89 × 10^-7 m / 1.02 m) = 4.67 × 10^-7 radians
- Convert the radians to degrees: 4.67 × 10^-7 radians × (180 ÷ π) = 0.027 degrees
- Now we can find the distance using the formula:
d = diameter of the object / tan(θ)
- Substitute the values into the formula: d = 0.03 m / tan(0.027 degrees)
- Calculate the tangent of the angle in degrees: tan(0.027 degrees) = 0.000469
- Calculate the distance: d = 0.03 m / 0.000469 = 64.02 m
- Convert the distance to miles: 64.02 m ÷ 1609 = 0.0398 miles
Therefore, you can place a coin of diameter 3.0 cm at a distance of approximately 0.0398 miles from a 102 cm telescope mirror and still resolve the coin using light of wavelength 389 nm.