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The Hubble Space Telescope has a mirror diameter of 2.4 m. Suppose the telescope is used to photograph stars near the center of our galaxy, 30,000 light years away, using red light with a wavelength of 650 nm.

a. What’s the distance (in km) between two stars that are marginally resolved? The resolution of a reflecting telescope is calculated exactly the same as for a refracting telescope.

b. For comparison, what is this distance as a multiple of the distance of Jupiter from the sun?

Short Answer

Expert verified

a. The distance between two stars that are marginally resolved is 3.30×10-7.

b. The distance as a multiple of the distance of Jupiter from the sun is 9.3777486×1010km.

Step by step solution

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01

Part(a) step 1: Given Information

We have given that:

Diameter of mirror D=2.4mand

the wavelength of red lightλ=650nm6.5x10-7m.

We need to find distance. between two stars that are marginally resolved.

02

Part (a) step 2: Calculation

By using the formula ,

Ar=1.22λD

Here, λis wavelength of red light and Dis the diameter of the mirror.

We get value for angular resolution Ar,

Ar=1.22λD

Substituting the values in equation,

localid="1650216005430" Ar=1.226.5x10-7m2.4m

Ar=3.30x10-7.

03

Part (b) step 1: Given Information

we need to find the distance as a multiple of the distance of Jupiter from the sun.

04

Part(b) step 2: simplification 

Now Distance x is:

χ=30000x(3.30x10-7)ly

χ=9.9x10-3lyχ=(9.9x10-3)x(9.4605295x1012)χ=9.3777486x1010km.

Here,Xis the distance.

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Most popular questions from this chapter

The resolution of a digital cameras is limited by two factors diffraction by the lens, a limit of any optical system, and the fact that the sensor is divided into discrete pixels. consirer a typical point-and--shoot camera that has a 20-mm-focal-lengthlens and a sensor with 2.5-μm-widepixels.

(a) . First, assume an ideal, diffractionless lens, at a distance of 100m,what is the smallest distance, in cmbetween two point sources of light that the camera can barely resolve? in answering this question, consider what has to happen on the sensor to show two image points rather than one you can use S1=fbecauses>>f.

(b) . You can achieve the pixel-limied resolution of part a only if the diffraction which of each image point no greater than the diffraction width of image point is no greater than 1pixel in diameter. for what lens diameter is the minimum spot size equal to the width of a pixel ? use 600nmfor the wavelength of light.

(c). what is the f-numberof the lens for the diameter you found in part b? your answer is a quite realistic value of the f-numberat which a camera transitions from being pixel limited to being diffraction limited for f-numbersmaller than this (larger-diameter apertures), the resolution is limited by the pixel size and does not change as you change the apertures. for f-numberlarger than this (smaller-diameter apertures). the resolution is limited by diffraction and it gets worse as you "stop down" to smaller apertures.

A 2.0-tall object is 20cmto the left of a lens with a focal length of 10cm. A second lens with a focal length of -5cm is 30cm to the right of the first lens.

a. Use ray tracing to find the position and height of the image. Do this accurately using a ruler or paper with a grid, then make measurements on your diagram.

b. Calculate the image position and height. Compare with your ray-tracing answers in part a.

You’ve been asked to build a telescope from a 2.0xmagnifying lens and a 5.0xmagnifying lens.

a. What is the maximum magnification you can achieve?

b. Which lens should be used as the objective? Explain.

c. What will be the length of your telescope?

A reflecting telescope is built with a 20cm-diameter mirror having an1.00m focal length. It is used with an10×eyepiece.

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A 1.0cm-tall object is 110cmfrom a screen. A diverging lens with focal length-20cmis 20cmin front of the object. What are the focal length and distance from the screen of a second lens that will produce a well-focused, 2.0cm-tall image on the screen?

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