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Imaging Space Imaging Space I believe that If we look I believe that If we look somewhere hard enough, we somewhere hard enough, we will find something… will find something… Presentation by Emily Bowers

Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

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Page 1: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Imaging SpaceImaging SpaceI believe that If we look I believe that If we look

somewhere hard enough, we will somewhere hard enough, we will find something…find something…

Presentation by Emily Bowers

Page 2: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

What is out there?What is out there?

The Electromagnetic SpectrumThe Electromagnetic Spectrum

““To start with you should know what a spectrum To start with you should know what a spectrum is: when white light is shone through a prism it is: when white light is shone through a prism it is separated out into all the colours of the is separated out into all the colours of the rainbow; this is the visible spectrum. So white rainbow; this is the visible spectrum. So white light is a mixture of all colours. Black is NOT a light is a mixture of all colours. Black is NOT a colour; it is what you get when all the light is colour; it is what you get when all the light is taken away.” –Purchon.comtaken away.” –Purchon.com

Page 3: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Spectrum of WavesSpectrum of Waves

Radio WavesRadio WavesMicrowavesMicrowaves Infra RedInfra RedVisible Light Visible Light

SpectrumSpectrumUltra VioletUltra VioletGamma RaysGamma RaysAnd X-RaysAnd X-Rays

Page 4: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Visible vs. Non-Visible WavesVisible vs. Non-Visible Waves

Visible wavesVisible wavesObjects that we can see with our own eyes in Objects that we can see with our own eyes in

the visible part of the wave spectrum, the visible part of the wave spectrum, otherwise known to us as normal light wavesotherwise known to us as normal light waves

Non-Visible wavesNon-Visible wavesOther types of waves within the spectrum that Other types of waves within the spectrum that

we as humans are unable to perceive with out we as humans are unable to perceive with out some kind of assistance, for instance; X-Rays.some kind of assistance, for instance; X-Rays.

Page 5: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Visible SpectrumVisible Spectrum

MoonbowMoonbow

Page 6: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Non-Visible SpectrumNon-Visible Spectrum

The Non-Visible Spectrum, Includes;The Non-Visible Spectrum, Includes;Radio WavesRadio WavesMicrowavesMicrowaves Infra RedInfra RedUltra VioletUltra VioletX-RaysX-RaysGamma RaysGamma Rays

Page 7: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Radio WavesRadio Waves

Scientist are able to pick up radio waves Scientist are able to pick up radio waves from different parts of space, these are the from different parts of space, these are the longest wave in the electromagnetic longest wave in the electromagnetic spectrum, and it as such, has the highest spectrum, and it as such, has the highest frequency.frequency.

Any amateur with a transceiver can also Any amateur with a transceiver can also point it into space and find some radio point it into space and find some radio waves to listen to; right from their own waves to listen to; right from their own backyard.backyard.

Page 8: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

MicrowavesMicrowaves

Microwaves are all around usMicrowaves are all around usYou use them every day with your;You use them every day with your;

cell phonecell phoneMicrowaveMicrowaveand any other wireless transmissionsand any other wireless transmissions

Microwaves are isotropic, what this means Microwaves are isotropic, what this means is that they are constant and surrounding is that they are constant and surrounding all of us all the time.all of us all the time.

Page 9: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Microwave BackgroundMicrowave Background

This is a WMAP Image of space“Wilkinson Microwave Anisotropy Probe”

Page 10: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Infra RedInfra Red

““These radio/light waves have a very short These radio/light waves have a very short wavelength; their wavelength is longer wavelength; their wavelength is longer than visible light. Infra-red can be detected than visible light. Infra-red can be detected by special infra-red film.” -Purchonby special infra-red film.” -Purchon

Page 11: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Infra Red Images from SpaceInfra Red Images from Space

Galaxy: Messier 81

These are multiple infrared photos of the

same galaxy, in the top right corner there is the visible light spectrum of

the same gallaxy.

Page 12: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Spitzer SatelliteSpitzer Satellite

Page 13: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

The Helix Nebula from Spitzer The Helix Nebula from Spitzer (Infra Red)(Infra Red)

Page 14: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Vs. The Helix Nebula from Hubble Vs. The Helix Nebula from Hubble & Blanco (Regular Light)& Blanco (Regular Light)

Page 15: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Visible Light SpectrumVisible Light Spectrum

Page 16: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Hubble Space TelescopeHubble Space Telescope

The Hubble Space Telescope produces the visible light photographs from space with out atmospheric interpherence.

Page 17: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Visible Light PhotosVisible Light Photoscaptured by the Hubble Telescopecaptured by the Hubble Telescope

Carina Nebula in visible light

Page 18: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Hubble takes first photo of a planet Hubble takes first photo of a planet circling another star:circling another star:

Page 19: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Ultra VioletUltra Violet These waves have very high energy and very These waves have very high energy and very

short wave lengths; shorter than visible light. -short wave lengths; shorter than visible light. -PerchonPerchon

Page 20: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Compare the ultra Violet of Compare the ultra Violet of Andromeda with the Visible LightAndromeda with the Visible Light

Page 21: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

X-RaysX-Rays

X-Rays of Galaxy NGC 4697 vs. the X-Rays of Galaxy NGC 4697 vs. the fuzzier optical imagefuzzier optical image

Page 22: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Gamma RaysGamma Rays

Compton Gamma-Ray Observatory

This is an image captured in Gamma Rays by Fermi.

Fermi is a Gamma Ray Detector.

Page 23: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

False Color ImagesFalse Color Images

Many images are created with Many images are created with false colorsfalse colors to emphasis a particular importance. to emphasis a particular importance.

“This is a visible light image of the planet Jupiter. It is in false color - the colors were chosen to emphasize the cloud structure on this banded planet - Jupiter would not look like this to your eyes”

Page 24: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

Milky WayMilky Way

Page 25: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

ConclusionConclusion

I have discovered many great things about I have discovered many great things about both visible and non-visible waves that we both visible and non-visible waves that we can see objects in space with, I hope that can see objects in space with, I hope that this has helped you to appreciate all that this has helped you to appreciate all that our growing technology has to offer us in our growing technology has to offer us in our quest to find more growth and activity our quest to find more growth and activity in the heavens.in the heavens.

Page 26: Imaging Space I believe that If we look somewhere hard enough, we will find something… Presentation by Emily Bowers

ReferencesReferences http://http://www.pa.uky.edu/~sciworks/light/preview/rainbo.htmwww.pa.uky.edu/~sciworks/light/preview/rainbo.htm http://www.gsfc.nasa.gov/scienceques2002/20030131.htmhttp://www.gsfc.nasa.gov/scienceques2002/20030131.htm http://www.purchon.com/physics/electromagnetic.htmhttp://www.purchon.com/physics/electromagnetic.htm http://map.gsfc.nasa.gov/media/080997/index.htmlhttp://map.gsfc.nasa.gov/media/080997/index.html Freedman, R. A., & Kaufmann, W. J. (2008). Freedman, R. A., & Kaufmann, W. J. (2008). Universe.Universe. New York: W. H. New York: W. H.

Freeman and Company.Freeman and Company. Microwaves: Universe 8th Ed. (pg. 700) Microwaves: Universe 8th Ed. (pg. 700) http://www.spitzer.caltech.edu/Media/releases/ssc2003-06/ssc2003-http://www.spitzer.caltech.edu/Media/releases/ssc2003-06/ssc2003-

06d.shtml06d.shtml http://gallery.spitzer.caltech.edu/Imagegallery/image.php?http://gallery.spitzer.caltech.edu/Imagegallery/image.php?

image_name=ssc2009-15aimage_name=ssc2009-15a http://science.hq.nasa.gov/kids/imagers/ems/visible.htmlhttp://science.hq.nasa.gov/kids/imagers/ems/visible.html http://imagine.gsfc.nasa.gov/docs/science/know_l2/emspectrum.htmlhttp://imagine.gsfc.nasa.gov/docs/science/know_l2/emspectrum.html http://asymptotia.com/2008/11/14/seeing-is-believing/http://asymptotia.com/2008/11/14/seeing-is-believing/ http://hubblesite.org/gallery/album/http://hubblesite.org/gallery/album/ http://outdoors.webshots.com/ http://outdoors.webshots.com/