What is the angular size of the moon as viewed from Earth's surface?

In summary: For part b, you need to consider the telescope's magnifying power. Remember, the telescope works by making the object seem larger, so you have to adjust your equation accordingly. In summary, to find the angular size of the moon as viewed from Earth's surface, you need to use the equation theta=s/r, where s is the physical size of the moon and r is the distance from Earth. For the second part of the question, you need to use the equation M=-L/fo x N/Fe, where M is the magnifying power, L is the focal length of the telescope, and fo and Fe are the focal lengths of the objective and eyepiece, respectively.
  • #1
monke
21
0

Homework Statement



a) what is the angular size of the moon as viewed from the Earth's surface?
b) The objective and eyepiece of a refracting telescope have focal lenghts 80cm and 2.0cm. What is the angular size of the moon as viewed though this telescope?

mean radius of the moon- 1.737x10^6m
mean distance from earth- 3.854x10^8m

Homework Equations



Im not sure what equations to use or why the answer from the book is in radians


The Attempt at a Solution



i tried using the equation m=near point/ object distace, with the near point being 25cm and object distace being the distance from the earth. HOwever the anwer from the book is in radians.


Thanks in advanced!
 
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  • #2
monke said:
Im not sure what equations to use or why the answer from the book is in radians

Of course the answer is in radians. It's asking you for the angular size. The angular size is defined as the angle subtended (spanned) by the object as seen by the observer. In other words, how big does it look? How much of your field of view does it take up?

What is the equation for an angle in terms of of the radius and the arc length (which you can equate to physical size)?
 
  • #3
would that be theata= h (size of object)/N ( near point =25cm)?
 
  • #4
No, I was just talking about the equation that gives you the definition of an angle (in the radian system)
 
  • #5
i think i found it
theata = 2(radius)/disatance from the sun?
 
  • #6
angle in terms of radians is
theta= s/r
(size of arc)/ radius
 
  • #7
how should i have applied that to this particular question?
 
  • #8
for the second part of the question, if a refracting telescope functions like a compound microscope does that mean that you would use the same angular equation?

M= -L/foX N/Fe
 
  • #9
monke said:
angle in terms of radians is
theta= s/r
(size of arc)/ radius

monke said:
how should i have applied that to this particular question?

Well, how big is the object? How far away is it? Therefore, what angle does it span? This is its angular (or apparent) size. That will get you the answer to part a.
 

1. What is angular size and how does it relate to telescopes?

Angular size is a measure of an object's apparent size as viewed from a specific distance. For telescopes, it is the field of view that the telescope is able to capture. The larger the angular size, the more detail can be seen through the telescope.

2. How is angular size measured?

Angular size is measured in degrees, arcminutes, and arcseconds. One degree is divided into 60 arcminutes, and one arcminute is divided into 60 arcseconds. These units are commonly used in astronomy to measure the apparent size of objects in the sky.

3. How does the size of a telescope affect its angular size?

The size of a telescope's objective lens or mirror determines its ability to gather light and resolve finer details. The larger the objective, the larger the angular size of the objects that can be seen through the telescope.

4. How does the distance between the observer and the object affect its angular size?

The closer the observer is to an object, the larger its angular size will appear. This is because the object takes up more of the observer's field of view. Conversely, the farther away the object is, the smaller its angular size will appear.

5. Can different telescopes have the same angular size?

Yes, different telescopes can have the same angular size if they have the same objective size and are positioned at the same distance from the observed object. However, they may have different levels of magnification, which can affect the perceived size of the object when viewed through the telescope.

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