Ways of viewing the universe
Planets do not twinkle because they are closer and not a single point of light.
 
 
Because stars produce different kinds of energy, we want to  study all of them -  not just visible light!! Our eyes receive only a very small part of that energy!
We only see the visible range. But stars give off energy in all the wavelengths!
Optical telescopes - Using light to discover information about the universe. There are two kinds:
Uses lens to collect the light. Refracting
Two of Galileo's refracting scopes.
Today’s refracting telescopes!
Uses mirrors to collect light Reflecting scope Reflecting telescope
Newton's reflecting scope
Spotting scope - A small refractor to line up the big scope. Eyepiece for viewing Today’s reflector
Mount Palomar  Observatory Hale Telescope Inside Mt. Palomar Observatory Large telescopes are put in observatories to protect them.                                                                                    
Other scopes at Palomar Look across the mountain tops!                                                                                            
Where should we put our telescopes? 1.  Mountain tops above atmospheric haze.  Reduces the twinkle effect and distortion. 2.  Far from city lights ( light pollution). 3.  If  our atmosphere  blocks the wavelength needed to study, then the scope goes into orbit!
Notice which wavelengths are blocked!
The USA at night – notice the light pollution. Where would you put a telescope? Atlanta Notice the Great Lakes
Mauna Kea, Hawaii – elevation 13,796 ft High to “look through” less atmosphere
Multi-mirror reflector in Hawaii
Other scopes are studying all the  other wavelengths.
Infrared scope in Hawaii Infrared scopes “look for”  heat and  are best at locating  new stars  just forming.
COBE - An Infrared scope that  is in orbit. Cosmic Background Explorer It has located very important data about the formation of the universe. Infrared = heat
The constellation of Orion in visible light energy and infrared energy. These two views  see  very different things in the same area of the sky!
Radio Telescopes Records radio waves Sees to the edges of the universe
VLA New Mexico Very Large Array uses multiple radio telescopes.
VLA from above.  They work as a unit kind of like a fly’s eye.
Largest radio scope in the world in the top of an extinct volcano!  Puerto Rico
Ultraviolet telescopes Records UV radiation.  Astronomers use this wave length mostly to look at and track what the sun is doing.
Solar & Heliospheric Observatory   This spacecraft has an ultraviolet scope.
SOHO pictures The sun in different UV wavelengths.
X-ray telescopes Records x ray emissions from objects in “deep” space Best for “looking” for black holes, dying stars, and other strange objects. Must  be above the atmosphere!
Chandra X-Ray scope
X Rays from two Black holes in one Galaxy.
Gamma Rays These telescopes are looking for high energy events:  black holes, neutron stars and quasars. Due to their high energy content,  Gamma rays are able to cause  serious  damage  when absorbed by living cells.  Gamma rays are also able to penetrate dense materials.  Aren’t we glad our atmosphere blocks them!
The  Compton Gamma Ray Observatory   orbits the Earth, detecting high-energy photons –  GAMMA RAYS
The spectroscope Takes light from stars and analyzes it.
Light from a star or other source goes through the slit.
Every element has  a different set of  spectrum lines. Much like people  having different  fingerprints.
Krypton’s spectrum Neon’s  spectrum Emission  spectrum
Three kinds of spectra
So spectrum lines tell us what elements are in a star without going there!
Notice that emission and absorption are the same.
Any questions on how we view  and study the universe??

Telescopes & astronomy andie

  • 1.
    Ways of viewingthe universe
  • 2.
    Planets do nottwinkle because they are closer and not a single point of light.
  • 3.
  • 4.
  • 5.
    Because stars producedifferent kinds of energy, we want to study all of them - not just visible light!! Our eyes receive only a very small part of that energy!
  • 6.
    We only seethe visible range. But stars give off energy in all the wavelengths!
  • 7.
    Optical telescopes -Using light to discover information about the universe. There are two kinds:
  • 8.
    Uses lens tocollect the light. Refracting
  • 9.
    Two of Galileo'srefracting scopes.
  • 10.
  • 11.
    Uses mirrors tocollect light Reflecting scope Reflecting telescope
  • 12.
  • 13.
    Spotting scope -A small refractor to line up the big scope. Eyepiece for viewing Today’s reflector
  • 14.
    Mount Palomar Observatory Hale Telescope Inside Mt. Palomar Observatory Large telescopes are put in observatories to protect them.                                                                                    
  • 15.
    Other scopes atPalomar Look across the mountain tops!                                                                                            
  • 16.
    Where should weput our telescopes? 1. Mountain tops above atmospheric haze. Reduces the twinkle effect and distortion. 2. Far from city lights ( light pollution). 3. If our atmosphere blocks the wavelength needed to study, then the scope goes into orbit!
  • 17.
  • 18.
    The USA atnight – notice the light pollution. Where would you put a telescope? Atlanta Notice the Great Lakes
  • 19.
    Mauna Kea, Hawaii– elevation 13,796 ft High to “look through” less atmosphere
  • 20.
  • 21.
    Other scopes arestudying all the other wavelengths.
  • 22.
    Infrared scope inHawaii Infrared scopes “look for” heat and are best at locating new stars just forming.
  • 23.
    COBE - AnInfrared scope that is in orbit. Cosmic Background Explorer It has located very important data about the formation of the universe. Infrared = heat
  • 24.
    The constellation ofOrion in visible light energy and infrared energy. These two views see very different things in the same area of the sky!
  • 25.
    Radio Telescopes Recordsradio waves Sees to the edges of the universe
  • 26.
    VLA New MexicoVery Large Array uses multiple radio telescopes.
  • 27.
    VLA from above. They work as a unit kind of like a fly’s eye.
  • 28.
    Largest radio scopein the world in the top of an extinct volcano! Puerto Rico
  • 29.
    Ultraviolet telescopes RecordsUV radiation. Astronomers use this wave length mostly to look at and track what the sun is doing.
  • 30.
    Solar & HeliosphericObservatory This spacecraft has an ultraviolet scope.
  • 31.
    SOHO pictures Thesun in different UV wavelengths.
  • 32.
    X-ray telescopes Recordsx ray emissions from objects in “deep” space Best for “looking” for black holes, dying stars, and other strange objects. Must be above the atmosphere!
  • 33.
  • 34.
    X Rays fromtwo Black holes in one Galaxy.
  • 35.
    Gamma Rays Thesetelescopes are looking for high energy events: black holes, neutron stars and quasars. Due to their high energy content, Gamma rays are able to cause serious damage when absorbed by living cells. Gamma rays are also able to penetrate dense materials. Aren’t we glad our atmosphere blocks them!
  • 36.
    The ComptonGamma Ray Observatory orbits the Earth, detecting high-energy photons – GAMMA RAYS
  • 37.
    The spectroscope Takeslight from stars and analyzes it.
  • 38.
    Light from astar or other source goes through the slit.
  • 39.
    Every element has a different set of spectrum lines. Much like people having different fingerprints.
  • 40.
    Krypton’s spectrum Neon’s spectrum Emission spectrum
  • 41.
  • 42.
    So spectrum linestell us what elements are in a star without going there!
  • 43.
    Notice that emissionand absorption are the same.
  • 44.
    Any questions onhow we view and study the universe??