radiation and spectra chapter 4. waveswaves l a stone dropped into a pool of water causes an...
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RADIATION AND SPECTRARADIATION AND SPECTRARADIATION AND SPECTRARADIATION AND SPECTRA
Chapter 4Chapter 4
WAVESWAVESWAVESWAVES
A stone dropped into a pool of water causes an A stone dropped into a pool of water causes an expanding disturbance called a expanding disturbance called a wavewave..
WAVESWAVESWAVESWAVES
Light and radio are Light and radio are waveswaves (called electromagnetic (called electromagnetic radiation) caused by charged particles (mostly radiation) caused by charged particles (mostly electrons) oscillating. electrons) oscillating.
A stone dropped into a pool of water causes an A stone dropped into a pool of water causes an expanding disturbance called a expanding disturbance called a wavewave..
Sound is a Sound is a wavewave caused by a pressure disturbance. caused by a pressure disturbance.
PROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATION
Speed = 3 x 10Speed = 3 x 1055 km/s in vacuum. km/s in vacuum. Radiation often behaves as a wave. Radiation often behaves as a wave. Wavelengths (1nm = 10Wavelengths (1nm = 10-9-9 m) m)
Radio = 1m (109 nm) Infrared = 10 m (104 nm) Visible = 0.5 m (500 nm) Ultraviolet = 10 nm X-ray = 0.1 nm-ray = 10-4 nm m = metre, = 10-6, n = 10-9
ELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATION
ELECTROMAGNETIC WAVESELECTROMAGNETIC WAVESELECTROMAGNETIC WAVESELECTROMAGNETIC WAVES
HUMAN SENSITIVITY to WAVESHUMAN SENSITIVITY to WAVESHUMAN SENSITIVITY to WAVESHUMAN SENSITIVITY to WAVES
Sound WavesSound Waves (wavelength) = pitchShort = high pitchLong = low pitch
Light WavesLight Waves (wavelength) = colourShort = bluerLong = redder
NANOMETERNANOMETERNANOMETERNANOMETER
Usual unit of Usual unit of for light is nm for light is nm(nano-meter = 10-9 metres)Blue light = 400 nmRed light = 700 nm
NANOMETERNANOMETERNANOMETERNANOMETER
Usual unit of Usual unit of for light is nm for light is nm(nano-meter = 10-9 metres)Blue light = 400 nmRed light = 700 nm
PROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATION Speed = 3 x 10Speed = 3 x 1055 km/s in vacuum. km/s in vacuum. Radiation often behaves as a wave. Radiation often behaves as a wave. Wavelengths (1nm = 10Wavelengths (1nm = 10-9-9 m) m)
Radio = 1m (109 nm) Infrared = 10 m (104 nm) Visible = 0.5 m (500 nm) Ultraviolet = 10 nm X-ray = 0.1 nm-ray m = metre, = 10-6, n = 10-9
Generally the hotter the source the shorter its emitted Generally the hotter the source the shorter its emitted wavelengthwavelength
ELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATIONELECTROMAGNETIC RADIATIONType of Type of
RadiationRadiationWavelength Wavelength Range (nm)Range (nm)
Radiated by Radiated by Objects at this Objects at this TemperatureTemperature
Typical SourcesTypical Sources
Gamma rays Less than 0.01
More than 108 K Few astronomical sources this hot. Some supernovae, pulsars, black holes and gamma ray quasars.
X rays 0.01 - 20 106 - 108 K Gas in clusters of galaxies; supernova remnants; solar corona
Ultraviolet 20-400 104 - 106 K Supernova remnants; very hot stars
Visible 400-700 103 - 104 K Stars
Infrared 103 - 106 10 - 103 K Cool clouds of dust and gas; planets; satellites
Radio More than 106 Less than 10K No astronomical objects this cold. Radio emission produced by electrons moving in magnetic fields (synchrotron radiation)
PROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATION
Speed = 3 x 10Speed = 3 x 1055 km/s in vacuum. km/s in vacuum. Radiation often behaves as a wave. Radiation often behaves as a wave. Wavelengths (1nm = 10Wavelengths (1nm = 10-9-9 m) m)
Radio = 1m (109 nm) Infrared = 10 m (104 nm) Visible = 0.5 m (500 nm) Ultraviolet = 10 nm X-ray = 0.1 nm-ray m = metre, = 10-6, n = 10-9
Propagation of radiationPropagation of radiation
PROPAGATION of RADIATIONPROPAGATION of RADIATIONPROPAGATION of RADIATIONPROPAGATION of RADIATION
INVERSE SQUARE LAW
PROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATIONPROPERTIES OF RADIATION Speed = 3 x 10Speed = 3 x 1055 km/s in vacuum. km/s in vacuum. Radiation often behaves as a wave. Radiation often behaves as a wave. Wavelengths (1nm = 10Wavelengths (1nm = 10-9-9 m) m)
Radio = 1m (109 nm) Infrared = 10 m (104 nm) Visible = 0.5 m (500 nm) Ultraviolet = 10 nm X-ray = 0.1 nm-ray m = metre, = 10-6, n = 10-9
Propagation of radiationPropagation of radiation Spectrum of radiation (blackbody)Spectrum of radiation (blackbody)
WHITE LIGHT SPECTRUMWHITE LIGHT SPECTRUMWHITE LIGHT SPECTRUMWHITE LIGHT SPECTRUM
BLACKBODY RADIATIONBLACKBODY RADIATIONBLACKBODY RADIATIONBLACKBODY RADIATION
Astronomical objects emit energy at different Astronomical objects emit energy at different wavelengthswavelengths
ORION CONSTELLATIONORION CONSTELLATIONORION CONSTELLATIONORION CONSTELLATION
Rigel
Betelgeuse
BLACKBODY RADIATIONBLACKBODY RADIATIONBLACKBODY RADIATIONBLACKBODY RADIATION
Astronomical objects emit energy at different Astronomical objects emit energy at different wavelengthswavelengths
Blackbody Blackbody
WHY?WHY? TemperatureTemperature
a source that absorbs all radiation hitting it.a source that absorbs all radiation hitting it. Energy is re-emitted at all wavelengths.Energy is re-emitted at all wavelengths. Spectrum emitted depends on the temperatureSpectrum emitted depends on the temperature At higher temperatures, more energy is emitted.At higher temperatures, more energy is emitted.
F = F = TT44
The higher the temperature, the shorter is the The higher the temperature, the shorter is the maximum wavelength.maximum wavelength.maxmax(nm) = 2.9 x 10(nm) = 2.9 x 1066 /T(ºK) /T(ºK) ºK = ºC + 273ºK = ºC + 273
BLACKBODY CURVESBLACKBODY CURVESBLACKBODY CURVESBLACKBODY CURVESE
MIT
TE
D E
NE
RG
Y
WAVELENGTH (nm)0 500 1000 1500 2000 2500 3000
| | | | | | |
3,000 K(960 nm)
4,000 K(725 nm)
5,000 K(580 nm)
WIEN’S LAW
x
max 2.9x106
T
T = Temp ºKmax in nanometers
7,000 K(400 nm)
ORION CONSTELLATIONORION CONSTELLATIONORION CONSTELLATIONORION CONSTELLATION
Rigel
Betelgeuse
FLASHCARDFLASHCARDFLASHCARDFLASHCARD
WHAT IS YOUR APPROXIMATE BODY WHAT IS YOUR APPROXIMATE BODY TEMPERATURE IN DEGREES K?TEMPERATURE IN DEGREES K?
A)A) 100 K100 K
B)B) 200 K 200 K
C)C) 300 K 300 K
D)D) 400 K 400 K
FLASHCARDFLASHCARDFLASHCARDFLASHCARD
AT WHAT WAVELENGTH DO YOU PUT OUT AT WHAT WAVELENGTH DO YOU PUT OUT MOST OF YOUR ENERGY?MOST OF YOUR ENERGY?
A)A) 100 nm (Ultra violet)100 nm (Ultra violet)
B)B) 1000 nm (deep red) 1000 nm (deep red)
C)C) 10,000 nm (infrared) 10,000 nm (infrared)
D)D) 1,000,000 nm (short radio) 1,000,000 nm (short radio)
DOPPLER SHIFTDOPPLER SHIFTDOPPLER SHIFTDOPPLER SHIFT
Doppler Shift FormulaDoppler Shift FormulaDoppler Shift FormulaDoppler Shift Formula
Change in wavelength = (original wavelength) times Change in wavelength = (original wavelength) times (v/c)(v/c) c = 300,000 km/sec c = 300,000 km/sec eg wavelength 400 nm from source moving ½ c away eg wavelength 400 nm from source moving ½ c away
from you.from you. change in wavelength = (wavelength) times (v/c) =
(400) times (½) = 200 nm wavelength thus observed at 600 nm – colour change
from blue to red
FLASHCARDFLASHCARDFLASHCARDFLASHCARD
IMAGINE THAT YOU ARE ON A SPACESHIP, IMAGINE THAT YOU ARE ON A SPACESHIP, SPEEDING TOWARDS MARS (THE RED SPEEDING TOWARDS MARS (THE RED PLANET). YOU GET CONFUSED AND PLANET). YOU GET CONFUSED AND MISIDENTIFY IT AS EARTH (THE BLUE PLANET). MISIDENTIFY IT AS EARTH (THE BLUE PLANET). HOW FAST WERE YOU GOING? HOW FAST WERE YOU GOING? (c = 3 x 10(c = 3 x 1055 km/s, blue light = 400 nm, red light = 700 nm) km/s, blue light = 400 nm, red light = 700 nm)
A)A) 2/7 c ( = 85,700 km/s)2/7 c ( = 85,700 km/s)
B)B) 3/7 c (= 128,570 km/s) 3/7 c (= 128,570 km/s)
C)C) 4/7 c (= 171,430 km/s) 4/7 c (= 171,430 km/s)
D)D) 5/7 c (= 214,290 km/s) 5/7 c (= 214,290 km/s)