Telescopes: Difference between revisions

Latest revision as of 19:41, 6 December 2015

Telescopes are tools used to study the night sky. The key to any telescope is getting as much information from the night sky as possible. This is done by taking advantage of the physical properties of light.

The Main Idea

Telescopes utilize systems of Mirrors and Lenses (sometimes very complicated) to take as much information from light as possible. Most telescopes used today are reflecting telescopes. The two major types of visible light telescopes are reflecting and refracting. Reflecting telescopes tend to be more compact and easier to maintain. The Quantum Properties of Light allow scientists to model light as both a particle and a wave as it bounces off mirrors and refracts through transparent mediums.

Parts of a Telescope

The two major parts of a telescope are the objective lens and the eye piece. The most complicated structures come from reflecting lens.

Important Equations

Magnification is equal to the focal length of the objective lens divided by the focal length of the eyepiece.

[math]\displaystyle{ \mathbf{M} = \frac{F} {f} }[/math]

The light gathering ability of a telescope is equal to the area of its objective lens.

[math]\displaystyle{ \mathbf{LGA} = (pi)*R^2 }[/math]

R=Radius of objective lens

The resolution of an image is dependent on the wavelength of the light being observed. Resolution of the image (in arc-seconds) is equal to a constant multiplied by the wavelength divided by the diameter of the telescope.

[math]\displaystyle{ \mathbf{α} = \frac{2.5e5*λ}{D} }[/math]

Refracting Telescopes

Refracting telescopes use a lens to gather and concentrate a beam of light. The lens can be thought of as a series of prisms combined in such a way that all the light waves arrive parallel to the axis (which is the line through the center of the lens). Refraction is the bending of light as it passes through a transparent medium.

Reflecting Telescopes

Reflecting telescopes use a curved mirror instead of a lens to focus the incoming light. The focal length of a reflecting telescope is equal to the total distance the light travels in-between reflection from mirror to mirror.

Different Models of Reflecting Telescopes

Connectedness

As an aerospace engineering major, I found this topic to be very related to my major. Aerospace vehicles are often used to place telescopes in better locations for observation.

History

The earliest telescopes were refracting telescopes. Galileo Galilei was one of the first notable people to use a telescope to observe the night sky. Galileo's telescope was a simple refracting and was the best at its time. He used it to observe many celestial objects including Mars and even 4 of Jupiters moons.

References

"Telescope - Google Search." Telescope - Google Search. N.p., n.d. Web. 05 Dec. 2015.
Chaisson, Eric, and Steve McMillan. "Astronomy Today." Astronomy Today. Pearson, n.d. Web. 05 Dec. 2015.
http://www.astronomy.gatech.edu/Courses/Phys2021/

@@ Line 1: / Line 1: @@
 Telescopes are tools used to study the night sky.  The key to any telescope is getting as much information from the night sky as possible.  This is done by taking advantage of the physical properties of light.
 ==The Main Idea==
+Telescopes utilize systems of [[Mirrors]] and [[Lenses]] (sometimes very complicated) to take as much information from light as possible.  Most telescopes used today are reflecting telescopes.  The two major types of visible light telescopes are reflecting and refracting.  Reflecting telescopes tend to be more compact and easier to maintain.   The  [[Quantum Properties of Light]] allow scientists to model light as both a particle and a wave as it bounces off mirrors and refracts through transparent mediums.
-Telescopes take utilizes complicated systems of [[Mirrors]] and [[Lenses]]
+===Parts of a Telescope===
-===Types of Telescopes===
+The two major parts of a telescope are the objective lens and the eye piece.  The most complicated structures come from reflecting lens.
+[[File:31mSg3OkZ0L.jpg|500px|]]
-What are the mathematical equations that allow us to model this topic.  For example <math>{\frac{d\vec{p}}{dt}}_{system} = \vec{F}_{net}</math> where '''p''' is the momentum of the system and '''F''' is the net force from the surroundings.
+===Important Equations===
-===Refracting Telescopes===
+Magnification is equal to the focal length of the objective lens divided by the focal length of the eyepiece.
+<math> \mathbf{M} = \frac{F} {f} </math>
+The light gathering ability of a telescope is equal to the area of its objective lens.
-===Reflecting Telescopes===
+<math> \mathbf{LGA} = (pi)*R^2 </math>
-===Different Models of Reflecting Telescopes===
+R=Radius of objective lens
-How do we visualize or predict using this topic. Consider embedding some vpython code here [https://trinket.io/glowscript/31d0f9ad9e Teach hands-on with GlowScript]
-====
+The resolution of an image is dependent on the wavelength of the light being observed.  Resolution of the image (in arc-seconds) is equal to a constant multiplied by the wavelength divided by the diameter of the telescope.
-Be sure to show all steps in your solution and include diagrams whenever possible
+<math> \mathbf{α} = \frac{2.5e5*λ}{D} </math>
-==Connectedness==
+===Refracting Telescopes===
-#As an aerospace engineering major, I found this topic to be very related to my major.  Aerospace vehicles are often used to place telescopes in better locations for observation.
+Refracting telescopes use a lens to gather and concentrate a beam of light.  The lens can be thought of as a series of prisms combined in such a way that all the light waves arrive parallel to the axis (which is the line through the center of the lens).  [[Refraction]] is the bending of light as it passes through a transparent medium.
-==History==
+[[File:IMG 3035.JPG|300px|]]
-Put this idea in historical context. Give the reader the Who, What, When, Where, and Why.
+===Reflecting Telescopes===
+Reflecting telescopes use a curved mirror instead of a lens to focus the incoming light. The focal length of a reflecting telescope is equal to the total distance the light travels in-between reflection from mirror to mirror.
-== See also ==
+[[File:IMG 3036.JPG|300px|]]     [[File:IMG 3038.JPG|300px|]]
-Are there related topics or categories in this wiki resource for the curious reader to explore?  How does this topic fit into that context?
-===Further reading===
+===Different Models of Reflecting Telescopes===
-Books, Articles or other print media on this topic
+[[File:IMG 3037.JPG|300px|]]
-===External links===
+==Connectedness==
-[http://www.scientificamerican.com/article/bring-science-home-reaction-time/]
+As an aerospace engineering major, I found this topic to be very related to my major.  Aerospace vehicles are often used to place telescopes in better locations for observation.
+==History==
+The earliest telescopes were refracting telescopes.  [[Galileo Galilei]] was one of the first notable people to use a telescope to observe the night sky.  Galileo's telescope was a simple refracting and was the best at its time.  He used it to observe many celestial objects including Mars and even 4 of Jupiters moons.
 ==References==
-Chaisson, Eric, and Steve McMillan. "Astronomy Today." Astronomy Today. Pearson, n.d. Web. 05 Dec. 2015.
+#"Telescope - Google Search." Telescope - Google Search. N.p., n.d. Web. 05 Dec. 2015.
+#Chaisson, Eric, and Steve McMillan. "Astronomy Today." Astronomy Today. Pearson, n.d. Web. 05 Dec. 2015.
+#http://www.astronomy.gatech.edu/Courses/Phys2021/