You want to create a telescope with a resolving power of 0.100 arc seconds at a wavelength of 550 nm. What diameter (in m) do you need? If you want to increase the light gathering power by a factor of 10, by what factor does the diameter need to increase? What would the new resolving power be (in arc seconds)? Part 1 of 5 The resolving power of a telescope is given by a = 2.06 x 105 D' where both A and D must have the same units. Part 2 of 5 We need to solve this expression for the diameter. You should express your values in meters. 0.00000055 5.50e-07 m D = 2.06 x 105| 0.100 arc seconds D = 1.133 1.13 m Part 3 of 5 The light gathering power of a telescope depends on the diameter squared. :-(Pnew LGP new = D. LGP old old Part 4 of 5 If we want to increase the light gathering power by a factor of 10, we need the new telescope to have 10 times the light-gathering power of the original. LGP new LGP old Rearranging the equation for light-gathering power to solve for Dnew LGP new Dold Dnew V ZGP old Plugging in for LGP, gives: ew Dnew = Dold And using the initial diameter, we can solve for the new diameter. Dnew m
You want to create a telescope with a resolving power of 0.100 arc seconds at a wavelength of 550 nm. What diameter (in m) do you need? If you want to increase the light gathering power by a factor of 10, by what factor does the diameter need to increase? What would the new resolving power be (in arc seconds)? Part 1 of 5 The resolving power of a telescope is given by a = 2.06 x 105 D' where both A and D must have the same units. Part 2 of 5 We need to solve this expression for the diameter. You should express your values in meters. 0.00000055 5.50e-07 m D = 2.06 x 105| 0.100 arc seconds D = 1.133 1.13 m Part 3 of 5 The light gathering power of a telescope depends on the diameter squared. :-(Pnew LGP new = D. LGP old old Part 4 of 5 If we want to increase the light gathering power by a factor of 10, we need the new telescope to have 10 times the light-gathering power of the original. LGP new LGP old Rearranging the equation for light-gathering power to solve for Dnew LGP new Dold Dnew V ZGP old Plugging in for LGP, gives: ew Dnew = Dold And using the initial diameter, we can solve for the new diameter. Dnew m
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
Related questions
Question
Assistance with part 4
![You want to create a telescope with a resolving power
of 0.100 arc seconds at a wavelength of 550 nm. What
diameter (in m) do you need?
If you want to increase the light gathering power by a
factor of 10, by what factor does the diameter need to
increase?
What would the new resolving power be (in arc
seconds)?
Part 1 of 5
The resolving power of a telescope is given by
a = 2.06 x 105
D'
where both A and D must have the same units.
Part 2 of 5
We need to solve this expression for the diameter. You
should express your values in meters.
0.00000055
5.50e-07 m
D = 2.06 x 105|
0.100 arc seconds
D =
1.133
1.13 m
Part 3 of 5
The light gathering power of a telescope depends on
the diameter squared.
:-(Pnew
LGP new =
D.
LGP
old
old
Part 4 of 5
If we want to increase the light gathering power by a
factor of 10, we need the new telescope to have 10
times the light-gathering power of the original.
LGP new
LGP old
Rearranging the equation for light-gathering power to
solve for
Dnew
LGP new Dold
Dnew
V ZGP
old
Plugging in for LGP,
gives:
ew
Dnew =
Dold
And using the initial diameter, we can solve for the new
diameter.
Dnew
m](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fda14446f-ef4d-47d5-9b14-b7a32b5fa1b1%2F69ed8e3b-e876-4a88-bb5a-7b4a82220221%2F5xzk57.jpeg&w=3840&q=75)
Transcribed Image Text:You want to create a telescope with a resolving power
of 0.100 arc seconds at a wavelength of 550 nm. What
diameter (in m) do you need?
If you want to increase the light gathering power by a
factor of 10, by what factor does the diameter need to
increase?
What would the new resolving power be (in arc
seconds)?
Part 1 of 5
The resolving power of a telescope is given by
a = 2.06 x 105
D'
where both A and D must have the same units.
Part 2 of 5
We need to solve this expression for the diameter. You
should express your values in meters.
0.00000055
5.50e-07 m
D = 2.06 x 105|
0.100 arc seconds
D =
1.133
1.13 m
Part 3 of 5
The light gathering power of a telescope depends on
the diameter squared.
:-(Pnew
LGP new =
D.
LGP
old
old
Part 4 of 5
If we want to increase the light gathering power by a
factor of 10, we need the new telescope to have 10
times the light-gathering power of the original.
LGP new
LGP old
Rearranging the equation for light-gathering power to
solve for
Dnew
LGP new Dold
Dnew
V ZGP
old
Plugging in for LGP,
gives:
ew
Dnew =
Dold
And using the initial diameter, we can solve for the new
diameter.
Dnew
m
Expert Solution
![](/static/compass_v2/shared-icons/check-mark.png)
This question has been solved!
Explore an expertly crafted, step-by-step solution for a thorough understanding of key concepts.
This is a popular solution!
Trending now
This is a popular solution!
Step by step
Solved in 2 steps
![Blurred answer](/static/compass_v2/solution-images/blurred-answer.jpg)
Knowledge Booster
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Recommended textbooks for you
![College Physics](https://www.bartleby.com/isbn_cover_images/9781305952300/9781305952300_smallCoverImage.gif)
College Physics
Physics
ISBN:
9781305952300
Author:
Raymond A. Serway, Chris Vuille
Publisher:
Cengage Learning
![University Physics (14th Edition)](https://www.bartleby.com/isbn_cover_images/9780133969290/9780133969290_smallCoverImage.gif)
University Physics (14th Edition)
Physics
ISBN:
9780133969290
Author:
Hugh D. Young, Roger A. Freedman
Publisher:
PEARSON
![Introduction To Quantum Mechanics](https://www.bartleby.com/isbn_cover_images/9781107189638/9781107189638_smallCoverImage.jpg)
Introduction To Quantum Mechanics
Physics
ISBN:
9781107189638
Author:
Griffiths, David J., Schroeter, Darrell F.
Publisher:
Cambridge University Press
![College Physics](https://www.bartleby.com/isbn_cover_images/9781305952300/9781305952300_smallCoverImage.gif)
College Physics
Physics
ISBN:
9781305952300
Author:
Raymond A. Serway, Chris Vuille
Publisher:
Cengage Learning
![University Physics (14th Edition)](https://www.bartleby.com/isbn_cover_images/9780133969290/9780133969290_smallCoverImage.gif)
University Physics (14th Edition)
Physics
ISBN:
9780133969290
Author:
Hugh D. Young, Roger A. Freedman
Publisher:
PEARSON
![Introduction To Quantum Mechanics](https://www.bartleby.com/isbn_cover_images/9781107189638/9781107189638_smallCoverImage.jpg)
Introduction To Quantum Mechanics
Physics
ISBN:
9781107189638
Author:
Griffiths, David J., Schroeter, Darrell F.
Publisher:
Cambridge University Press
![Physics for Scientists and Engineers](https://www.bartleby.com/isbn_cover_images/9781337553278/9781337553278_smallCoverImage.gif)
Physics for Scientists and Engineers
Physics
ISBN:
9781337553278
Author:
Raymond A. Serway, John W. Jewett
Publisher:
Cengage Learning
![Lecture- Tutorials for Introductory Astronomy](https://www.bartleby.com/isbn_cover_images/9780321820464/9780321820464_smallCoverImage.gif)
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:
9780321820464
Author:
Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:
Addison-Wesley
![College Physics: A Strategic Approach (4th Editio…](https://www.bartleby.com/isbn_cover_images/9780134609034/9780134609034_smallCoverImage.gif)
College Physics: A Strategic Approach (4th Editio…
Physics
ISBN:
9780134609034
Author:
Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:
PEARSON