1 fingerprints in sunlight understanding spectroscopy deborah scherrer stanford university
TRANSCRIPT
![Page 1: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/1.jpg)
11
Fingerprints in Fingerprints in SunlightSunlight
Understanding SpectroscopyUnderstanding Spectroscopy
Deborah ScherrerDeborah ScherrerStanford University Stanford University
![Page 2: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/2.jpg)
22
What is What is light?light?
![Page 3: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/3.jpg)
Light is a form of energy, Light is a form of energy, the electromagnetic the electromagnetic
spectrum.spectrum.
33
![Page 4: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/4.jpg)
44
How can we can study the How can we can study the stars?stars?
Only/primary way of learning about distant objects Only/primary way of learning about distant objects is through their light (electromagnetic spectrum)is through their light (electromagnetic spectrum)
Light has Light has ‘‘fingerprintsfingerprints”” which provide information which provide information about itabout it
How can we How can we ““readread”” these fingerprints and what do these fingerprints and what do they tell us about the star?they tell us about the star?
No matter how good your No matter how good your telescope, a star is only a telescope, a star is only a point of lightpoint of light
We can’t get there from We can’t get there from herehere
![Page 5: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/5.jpg)
55
What is the What is the spectrum of spectrum of light?light?
Anything hotter than absolute zero Anything hotter than absolute zero radiates/emits energy, i.e. lightradiates/emits energy, i.e. light Sun & stars emit a continuous spectrum Sun & stars emit a continuous spectrum
(meaning all the colors of visible light). (meaning all the colors of visible light). They also emit radio, microwaves, They also emit radio, microwaves, infrared light, ultraviolet light, X-rays, infrared light, ultraviolet light, X-rays, and/or gamma raysand/or gamma rays
Our eyes see Our eyes see ““whitewhite”” light, which is light, which is made of the spectrum of colors visible made of the spectrum of colors visible in a rainbowin a rainbow
Spectrum = Spectrum = the “colors” of light emitted by the “colors” of light emitted by an objectan object
![Page 6: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/6.jpg)
66
What is a What is a spectrograph?spectrograph?
A relatively simple-to-A relatively simple-to-understand scientific understand scientific instrument to look at instrument to look at a spectruma spectrum
Like a prism – breaks Like a prism – breaks light into its colorslight into its colors
Thin, rectangular slit Thin, rectangular slit produces a rectangle produces a rectangle of lightof light
Example output from a
spectrograph
![Page 7: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/7.jpg)
77
Most astronomy is Most astronomy is done with done with spectrographs!spectrographs!
Your spectrograph Stanford Solar Center Home-made
spectrograph attached to telescope
NASA‘s Solar Dynamics Observatory (SDO) NASA’s IRIS mission
Student spectrograph & gas
lamp
![Page 8: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/8.jpg)
88
Our Simple Our Simple SpectrographSpectrograph
Diffraction gratingDiffraction grating
(similar effect to prism(similar effect to prism
or CD)or CD) Slit & light sourceSlit & light source Scale (optional)Scale (optional) Eye or instrument Eye or instrument
for viewingfor viewing
![Page 9: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/9.jpg)
99
What can we learn with What can we learn with a spectrograph?a spectrograph?
Sometimes there are extra bright Sometimes there are extra bright colorscolors
Sometimes there are missing Sometimes there are missing colorscolors
To infraredTo ultraviolet
![Page 10: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/10.jpg)
1010
Fingerprints in LightFingerprints in Light The extra or missing colors indicate certain The extra or missing colors indicate certain
chemical elements (e.g. hydrogen, helium, chemical elements (e.g. hydrogen, helium, gold, etc.) have affected the lightgold, etc.) have affected the light
Each chemical element changes the spectrum Each chemical element changes the spectrum either by making certain colors brighter or either by making certain colors brighter or removing certain colorsremoving certain colors
Each chemical element has a different and Each chemical element has a different and unique pattern of colors, hence the unique pattern of colors, hence the ““fingerprintfingerprintss””
![Page 11: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/11.jpg)
1111
Example fingerprintsExample fingerprints
HydrogenHydrogen
HeliumHelium
SodiumSodium
![Page 12: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/12.jpg)
12121212
Absorption vs. Absorption vs. Emission?Emission?
Absorption lines – appear dark and are Absorption lines – appear dark and are produced when a chemical element has produced when a chemical element has absorbed energy absorbed energy
Emission lines – appear extra bright and are Emission lines – appear extra bright and are produced when a chemical element has emitted produced when a chemical element has emitted energyenergy Whether something
produces an absorption or emission spectrum depends upon its temperature, the temperature of any gas between it and the observer, and the observer’s line of site.
![Page 13: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/13.jpg)
1313
Some Elements on the Some Elements on the SunSun Hydrogen (H)Hydrogen (H)
Helium (He)Helium (He)
Sodium (Na)Sodium (Na)
Oxygen (OOxygen (O2)2)
Iron (Fe)Iron (Fe)
![Page 14: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/14.jpg)
Different types of stars Different types of stars have different spectrahave different spectra
1414
![Page 15: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/15.jpg)
Want to build your Want to build your own spectrograph?own spectrograph?
1515
http://solar-center.stanford.edu/activities/cots.html
Your teachers can order class sets for free (just pay shipping)
![Page 16: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/16.jpg)
1616
What secrets do What secrets do spectra tell us?spectra tell us?
Chemical Chemical CompositionComposition
TemperatureTemperature MovementMovement Magnetic fieldsMagnetic fields
![Page 17: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/17.jpg)
17171717
Spectra tell us about Spectra tell us about compositioncomposition Am emission or absorption line Am emission or absorption line
means a specific chemical means a specific chemical element has been involved with element has been involved with the light you are seeingthe light you are seeing
Careful, though. The element Careful, though. The element could be from the source, or from could be from the source, or from an intervening plasma or gas an intervening plasma or gas cloudcloud
![Page 18: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/18.jpg)
18181818
Spectra tell us Spectra tell us temperaturestemperatures
If you look at the strongest colors or If you look at the strongest colors or wavelength of light emitted by a star, then you wavelength of light emitted by a star, then you can calculate its temperaturecan calculate its temperature
Specific spectral lines are only produced at Specific spectral lines are only produced at certain temperatures, so if you see them you certain temperatures, so if you see them you know what temperature you are looking atknow what temperature you are looking at
![Page 19: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/19.jpg)
19191919
How do spectra tell us How do spectra tell us about movement?about movement? A Doppler shift happens when an object is moving A Doppler shift happens when an object is moving
towards or away from us, as in a siren coming towards towards or away from us, as in a siren coming towards usus
Wavelength is influenced by the movementWavelength is influenced by the movement It works with sound, with light, with any waveIt works with sound, with light, with any wave
![Page 20: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/20.jpg)
20202020
Doppler, continuedDoppler, continued
Motion away Motion away from us from us results in a results in a ““red shiftred shift””
Motion Motion towards us towards us results in a results in a ““blue shiftblue shift
Why don’t they call it a violet shift?
![Page 21: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/21.jpg)
21212121
Spectra tell us about Spectra tell us about magnetismmagnetism
Sunspots are magnetic
storms on the Sun Magnetic fields
cause spectral lines to split into
thirds
![Page 22: 1 Fingerprints in Sunlight Understanding Spectroscopy Deborah Scherrer Stanford University](https://reader030.vdocument.in/reader030/viewer/2022032517/56649cbb5503460f949835b8/html5/thumbnails/22.jpg)
2222
What are your What are your questions?questions?
Thank you!Thank you!Sun Dragon Art image © by Henry Roll. Used with permission.