Telescopes that observe nonvisible types of light work on the
same principles as visible telescopes, but they might require
different technologies. For instance, instead of lenses or mirrors,
a radio telescope (such as the one in the figure) uses technology
similar to the television satellite dish you might install on your
roof. As with visible light telescopes, bigger radio telescopes
yield greater light-gathering power and better angular
resolution.
However, the angular resolution (θ) of a telescope also
depends on the wavelength of light (λ) based on the
following equation, where D is the diameter of the
telescope, and the resolution is in units of arcseconds (when
D and λ have the same units).
θ=2.06×105(λD)
If there were two telescopes with the same diameter, but one is a
visible light telescope and the other a radio telescope, how would
the resolution of the images from each telescope compare? The
wavelength of visible light is several hundred nanometers (1
nanometer = 10–9 meters), and radio can be several
centimeters (1 cm = 10–2 meters) or several meters.
Select one:
a. There is not enough information to answer this question.
b. The radio telescope would have a much better angular resolution.
c. The radio telescope would have a much worse angular resolution.
d. The angular resolution of the two telescopes would be about the same.
Telescopes that observe nonvisible types of light work on the same principles as visible telescopes, but...
Part A How telescopes for invisible wavelengths differ from those for visible light? What other types of "cosmic messengers" can astronomers now observe? Drag the items on the left to the appropriate blanks on the right to complete the sentences. (Items can be used once or more than once.) Reset Help infrared Only the longest wavelengths act enough like the visible wavelengths that we can use neutrino the same sorts of telescopes with different detectors. At the shortest wavelengths, gamma-ray...
Consider the following 4 types of telescopes: 1. Visible light telescope 2. Infrared telescope 3. X-ray telescope 4. Radio wave telescope For each of these telescopes explain/discuss the following points: Give an example of what objects one would observe with this type of telescope. Discuss the location one would need to choose for this telescope. Consider the following options and explain what location is ideal for this telescope and why one would (or need to) choose one location over the...
Part A Listed following are the names and mirror diameters for six of the world’s greatest reflecting telescopes used to gather visible light. Rank the telescopes from left to right based on their light-collecting area from largest to smallest. For telescopes with more than one mirror, rank-based on the combined light-collecting area of the mirrors.Part B Shown following are the primary mirror arrangements and total light-collecting area of five different telescopes. Each mirror uses a different segmented arrangement, but assume that they...
The telescopes on some commercial surveillance satellites can resolve objects on the ground as small as 91 cm across (see Google Earth), and the telescopes on military surveillance satellites reportedly can resolve objects as small as 14 cm across. Assume first that object resolution is determined entirely by Rayleigh's criterion and is not degraded by turbulence in the atmosphere. Also assume that the satellites are at a typical altitude of 403 km and that the wavelength of visible light is...
Diffraction imposes a limit on the achievable resolution of an instrument. What is the smallest angular separation that two stars could have when viewed with a telescope with a diameter of 0.5 m. (A wavelength of 600 nm would be suitable as an estimation for visible light)
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1.) At what distance would a satellite orbiting the Earth be geosynchronous (orbiting the Earth once every 24 hours)? It would be geosynchronous at _________ × 104 m from the center of the Earth or __________× 104 m from the Earth's surface. 2.) Hydrogen also produces spectral lines at radio wavelengths, notably at 21.1 cm. If a galaxy is moving away from us at 9% of the speed of light, at what wavelength will we detect this line? Convert this...
Light of wavelength 589 nm is used to view an object under a microscope. The objective lens of the microscope is the lens that gathers light from the object being observed and focuses the light rays in order to form an image of the object. It acts as the aperture of the system, determining its resolution. In this case, the objective lens is circular, of diameter 0.95 cm. Assuming that the resolution of the microscope depends solely on the diffractive...
Part D What is the angular radius 0 of the first dark ring for a point source being imaged by this telescope? Use 550 nanometers for the wavelength,since this s near the average for visible light Express your answer in degrees, to three significant figures 197 ΑΣφ Request Answer Diftraction due to a circular aperture is important in astronomy Since a tolescopo has a circular aporture of finite size, stars are not imagod as points, but rathor as iftraction patterns....
Problem 7 (20 points): Each graph below shows the relative intensity versus 0 for a double slit experiment. The horizontal scale is the same for all graphs. The only possible differences among the cases are the values of the slit width (a) and distance between the centers of the slits (d). Case For each of the three cases, calculate the ratio- a) 0.5 b) Rank the cases according to distance between the centers Case 2 of the slits (d), from...