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Astronomy
Seeing through different light…
Visible UV..
Visible IR
Visible Radio Xray
Venus -IR
Venus -UV
Venus -RADIO
Venus -VISIBLE
Types of Light
• Gamma rays• X-Rays• UV rays• Visible Rays• Infrared• Microwaves• Radio• Long Waves
Types of Light
• Gamma rays– Nuclear blast
• X-Rays– Go through skin and body, stopped by bone
• UV rays– Penetrates skin, causes damage
Types of Light
• Visible Rays– What we can see
• Infrared– Night vision goggles
• Microwaves– Excite water
• Radio• Long Waves
Optical Telescopes
• Why do astronomers use telescopes?– Magnification– Resolution – Brightness
Brightness
• Gathering light to make faint objects appear bright
• MOST important• Depends on the size of
the lens
Resolution
• How sharp an object looks
• Larger the lens, higher the resolution
• HDTV vs. normal tv
Magnification
• How many times larger an object looks
• LEAST IMPORTANT
Magnification calculations
• M = fo/fe• Fo = Focal length of the objective• Fe = Focal length of the eyepiece
How big is our universe?
• MONTE PYTHON VIDEO
Optical Telescopes
Relflectors and Refractors
Refractors
• Uses lenses to bend light
Refractor
• Objective lens • Eyepiece
• Focal Length • The distance from a lens to the focal point
• Focal Point
• The point where light rays converge to produce an in focus image
Two lenses are placed at their focal lengths apart
• Fo (focal length of objective)• +• Fe (focal length of eyepiece)• =• Length of telescope
• Fo = 1000mm• Fe= 20 mm• What is the length of the telescope?
• What is the magnification?
Activity
• Right Eye Focal Length:
• Left Focal length:
• Both eyes
II. Focal Length of a lens
Focal Length of Lens 1:
Focal Length of Lens 2:
III. Magnification
• Draw a small arrow• Measure it in cm
Reflector Telescopes
Newtonian and Cassegrain
Newtonian Reflector
• Uses a mirror to reflect light
Newtonian Reflector
Cassegrain Reflector
• Has eyepiece behind mirror
• Has a small hole drilled into the middle of the objective mirror so that they light can go through
Cassegrain
Refractors
PROS• Better resolution due to no
diagonal mirror blocking part of the objective
CONS• Chromatic Abberation
(colors smear)• Size limit on objective lens
- if glass lens is too big it will sag)
• - max size = 3 feet
Reflectorss
PROS• No size limit
– The objective mirror can be made up hundreds of smaller mirrors
• Easier to hook up a computer to
CONS• Slightly less resolution
Optical observatories
• Keck 1 and Keck II in Hawaii
• Hubble Space Telescope
• GEMINI in Chili
Places to Build optical observatories
• Away from cities• Away from light pollution
• Mountain tops or space• The more atmosphere a telescope looks through , the
blurrier the image
Atmospheric Window
• Transparent to: Visible and Radio• Semi-Transparent to: Infrared• Opaque to: UV, X-Ray, Gamma Ray
Radio Telescopes
• Parts– Dish: :Large dish that focuses the rays (does
not have the be smooth)– Receiver: Gathers the rays and send to a
computer to analyze
• FALSE COLOR IMAGE: – Bright Areas= high intensity– Dark Areas= low intensity
RESOLUTION:
- Since radio waves are very large, they have very low resolution
Interferometer Array
• A way to increase resolution
• Observe the same object with lots of different telescopes
• Send all data to computer to create a high resolution image
Length of telescope
• Distance the telescopes are separated
Where to place Radio Telescopes
• Valleys– Avoids radio interference (mountains block the
signal)
Examples of Radio Observatories
• Arecibo– Worlds largest single radio telescope– Puerto Rico
• VLA– Very large array– New Mexico– On Train Tracks
• VLBA– Very large Baseline Arrary– Array of the worlds largest telescopes– Size of earth
Infrared Telescopes
• Uses regular mirrors• Must be placed high in the atmosphere
Sophia
• Aircraft with a telescope built in it
Spitzer
• In space• Studies stars and
planet formation
Telescope Videos
http://hubblesite.org/hubble_discoveries/hubble_deep_field/
Argon’s spectra
• The colored lines on the spectrum come from Argon’s electrons relaxing back to the ground state and releasing photons
• Fingerprint/Bar code
• Each element/compound has unique spectra
Hydrogen
• Less lines = less energy levels/electrons
Helium
Where should we put telescopes?