What is the resolving power of a 25-cm (10-in.) telescope at a wavelength of 550 nm (in the middle of the visual band)?
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Q: 7. As seen from Earth, the two stars known as Krueger 60 have an angular separation of 2.5 arc…
A: Given- λ=550 nm=550×10-9 m
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Q: How much better light-gathering-power does a professional telescope with a diameter of 6 meters have…
A: Diameter of professional telescope is D = 6 mt Diameter of roof telescope is d = 20 cm = 0.2 cm
Q: The figures are to scale. Which telescope has the biggest diameter?
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Q: Astronauts observing from a space station need a telescope with a resolving power of 0.9 arc seconds…
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Q: Compared to a 0.2 m diameter telescope, a 0.4 m diameter telescope has how much more light gathering…
A: The diameter of telescope 1: d1 = 0.2 m The diameter of telescope 2: d2 = 0.4 m
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A: Answer ------- X-rays do not penetrate Earth's atmosphere. Because
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A: Charged Coupled Devices or CCDs are light detectors used in telescopes. They are highly sensitive…
Q: How many telescopes does Kitt Peak National Observatory have?
A: Kitt peak national observatory have THREE major telescope.
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A: The property of a telescope that enables it to capture small details of an object is called its…
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Q: If Telescope A has one-fourth the light-gathering power of Telescope B, how does the diameter of…
A: Given : LGPA = 1/4 LGPB
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Q: The main characteristics of a telescope that defines how much light they can gather is the size of…
A: Given Data : Telescope To Find : Fill the characteristics of telescope in the blanks.
Q: Astronauts observing from a space station need a telescope with a resolving power of 0.9 arc seconds…
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Q: How many more times can a Keck telescope 10m diameter gather rather than armature telescope .25 m in…
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Q: Why would radio astronomers build identical radio telescopes in many different places around the…
A: Concept: Astronomers use radio telescopes to investigate areas of space. In astrophysics,…
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A: Introduction: From Galileo to Newton, now telescopes are made larger to study even far away objects.…
Q: Blue light has a wavelength of about 400 nm. Red light has a wavelength of about 700 nm. If both…
A: Given that: The wavelength of blue light is λBlue=400 nm The wavelength of red light is λRed=700 nm…
Q: Why must most infrared telescopes operate at very high altitudes or in space?
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Q: (diameter LGP = Area = t 2
A: The Light Gathering Power is calculated as : LGP = Area = π (diameter/2)2
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A: we can compare the different sized apertures for their Light gathering power . Light gathering power…
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Q: What is the approximate diffraction limit in arc second, of a 99 meter diameter radio telescope…
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Q: What is the resolving power of an 8-inch telescope (if necessary, you may assume λ=550 nm)? By the…
A: Given: The wavelength of light is 550 nm. The diameter of the aperture of the telescope is 8 in. The…
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A: Given: Diameter of the light gathering power 1,D1=300mDiameter of the light gathering power…
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A: Electromagnetic radiation is made of packets of energy called photons. They are differentiated by…
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A: The angular resolution (θ) of a telescope is given by the equation: θ = 1.22 × L / D where L is the…
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A: Light gathering power of a telescope is directly proportional to the diameter of the aperture P∝D…
Q: two reflecting telescopes have the same angular resolution, but one of them uses visible light and…
A: The formula for angular resolution is, θ=1.22λD (1) Where λ and D are the wavelength of light and…
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- Astronauts observing from a space station need a telescope with a resolving power of 0.6 arc second at a wavelength of 530 nm and a magnifying power of 220. Design a telescope to meet their needs. (State the necessary primary diameter of the telescope, in m, and the ratio of the focal lengths below.) What will its light-gathering power be, compared with a dark-adapted human eye? (Assume that the pupil of your eye can open to a diameter of about 0.8 cm in dark conditions.)Plz show full and simple easy to follow explanation and working. ThanksHow does human vision's peak in color sensitivity relate to the Sun? Why can't long-wavelength radio observations be made from Earth's surface?
- Why are x-ray telescopes all in space, rather than on the Earth?Astronauts observing from a space station need a telescope with a resolving power of 0.5 arc second at a wavelength of 570 nm and a magnifying power of 280. Design a telescope to meet their needs. (State the necessary primary diameter of the telescope, in m, and the ratio of the focal lengths below.)Astronauts observing from a space station need a telescope with a resolving power of 0.4 arc second at a wavelength of 530 nm and a magnifying power of 300. Design a telescope to meet their needs. (State the necessary primary diameter of the telescope, in m, and the ratio of the focal lengths below.) Dtelescope= m Feyepiece Fprimary = What will its light-gathering power be, compared with a dark-adapted human eye? (Assume that the pupil of your eye can open to a diameter of about 0.8 cm in dark conditions.) LGPtelescope LGPeye =
- The light-gathering power of a telescope is directly related to the area of the telescope's primary mirror. A mirror with four times the diameter of another mirror collects how many times more light as the smaller mirror does in the same amount of time? (Numerical answer only, please.)Compare the light-gathering power of one of the 10-m Keck telescopes with that of a 0.5-m telescope.Astronauts observing from a space station need a telescope with a resolving power of 0.6 arc second at a wavelength of 530 nm and a magnifying power of 220. Design a telescope to meet their needs.What will its light-gathering power be, compared with a dark-adapted human eye? (Assume that the pupil of your eye can open to a diameter of about 0.8 cm in dark conditions.)(State the necessary primary diameter of the telescope, in m, and the ratio of the focal lengths below.)
- Theoretically (that is, if seeing were not an issue), the resolution of a telescope is inversely proportional to its diameter. How much better is the resolution of the ALMA when operating at its longest baseline than the resolution of the Arecibo telescope?Suppose you want a telescope that would allow you to see distinguishing features as small as 6.5 km on the Moon some 384,000 km away. Assume an average wavelength of 550 nm for the light received. What is the minimum diameter of the mirror (in centimeters) that you could use in the telescope?These images show one of the large `VLT’ telescopes at the European Southern Observatory’s facility at Cerro Paranal, Chile. The place where the laser beam comes out (seen in the inset photo) is just out of sight off of the top edge of the large photo. Also note that if you look down the telescope tube (in the main photo), you can see the tube’s front-end structure. Imagine that this telescope had a flaw similar to the Hubble Space Telescope’s - its light-gathering element was shaped wrong. What problem would this cause for the telescope? Group of answer choices It would not be able to bring rays of light from a distant object to a focus. The imperfect shape would mean that it could focus rays of visible light, but not rays of light of any other wavelength. It wouldn’t be able to gather much light compared to the pupil of a human eye. It would mean that the telescope could only work if placed above the Earth’s atmosphere, like the Hubble telescope.