A telescope has an objective lens of 10 cm diameter and is situated at...
The power of resolution of the telescope is given by:Δθ≈1.22 λ2awhere, a = radius of the lensetherefore,Δθ = 1.22 x5000x10−1010x10−2 (since the diameter is give in the question)Δθ = 6.1x10−6 radiansNow,Δθ = arc radius = minimum distance between the two points distance between the telescope and the location of two points 6.1x10−6 = minimum distance between the two points 103minimum distance between the two points = 6.1x10−3 m6.1x10−3 m is the minimum distance that the telescope will be able to resolve at that distance.The power of resolution of the telescope is given by:∆θ≈1.22 λ2awhere, a = radius of the lensetherefore,∆θ = 1.22 x5000x10-1010x10-2 (since the diameter is give in the question)∆θ = 6.1x10-6 radiansNow,∆θ = arc radius = minimum distance between the two points distance between the telescope and the location of two points 6.1x10-6 = minimum distance between the two points 103minimum distance between the two points = 6.1x10-3 m6.1x10-3 m is the minimum distance that the telescope will be able to resolve at that distance.
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A telescope has an objective lens of 10 cm diameter and is situated at...
Objective:
To calculate the minimum distance between two objects that can be resolved by a telescope with a given objective lens diameter and distance from the objects.
Given:
- Objective lens diameter: 10 cm
- Distance from the objects: 1 kilometer
- Mean wavelength of light: 5000 angstroms
Formula:
The minimum resolvable angle (θ) can be calculated using the formula:
θ = 1.22 * (λ / D)
Where:
- θ is the minimum resolvable angle in radians
- λ is the wavelength of light in meters
- D is the diameter of the objective lens in meters
Calculations:
1. Converting the objective lens diameter to meters:
10 cm = 0.1 meters
2. Converting the mean wavelength of light to meters:
5000 angstroms = 5000 * 10^(-10) meters = 5 * 10^(-7) meters
3. Substituting the values into the formula to calculate the minimum resolvable angle:
θ = 1.22 * (5 * 10^(-7) / 0.1)
4. Simplifying the equation:
θ = 1.22 * 5 * 10^(-6)
5. Calculating the minimum resolvable angle:
θ ≈ 6.1 * 10^(-6) radians
6. The minimum distance (Dmin) between two objects that can be resolved by the telescope can be calculated using the formula:
Dmin = R * θ
Where R is the distance from the objects to the telescope.
7. Substituting the values into the formula to calculate the minimum distance:
Dmin = 1000 * 6.1 * 10^(-6)
8. Simplifying the equation:
Dmin ≈ 6.1 meters
Answer:
The minimum distance between the two objects that can be resolved by the telescope is approximately 6.1 meters.
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