Astronomy beyond the visible
Beatriz García, Ricardo Moreno
International Astronomical Union
ITeDA and Universidad Tecnológica Nacional, Argentina
Colegio Retamar de Madrid, Spain
Goals
Presentation
Electromagnetic Spectrum
All wavelengths of electromagnetic radiation.
Blackbody Radiation
Any “black body” when heated emits light at many wavelengths.
There is λmax at which the intensity of radiation is maximum. This λmax depends on the temperatura T:
Wien’s Law
By studying the radiation of a distant object, we can measure its temperature without having to go there. This applies for the stars, which are almost black bodies
Solar radiaton
Windows for different energy regions
The Earth’s atmosphere is opaque to most wavelengths of radiation. We can detect the hight energies from space and low energies require special detectors.
When the solar electomagnetic energy goes through the atmosphere, the “black body” radiation change, but the λmax at which the irradiance is máximum remains almost without change
The night vision devices uses this λmáx.
We know that there is λmax at which the irradiance or emission is maximum depends on the temperature T, but it does not need to be in a visible region of the spectrum
For example, the human body has a temperature of T = 273+37 = 310 K.
Then, emits the maximun in λmáx = 9300 nm.
Activity 1: Building a spectrometer
Depending what you use, a DVD part or a CD one, you cut the matching portions the template.
Activity 1: Building a spectrometer
Remove the metal layer of the CD using tape or scratching it.
NB! The coating will not peel off white or commercial CDs.
Activity 1: Building a spectrometer
The black surface folded on the inside.
Compare the spectra from filament lamps, fluorescent lamps and streetlights.
Activity 1: Building a spectrometer
Activity 2: Decomposing sunlight with water drops
Children can split the sunlight and make a rainbow.
They need a hose with a fine spray. They must have their back to the Sun.
Other regions of the spectrum
The infrared radiaton
Activity 3: Herschel Experiment
Activity 3: Herschel Experiment
SPECTRUM THERMOMETERS
PRISM
PRISM
BOX
THERMOMETERS
In the spectrum
A little beyond the red
RED
YELLOW
BLUE
SUN
Activity 3: Herschel Experiment
Activity 3: Herschel Experiment
TABLE OF DATA COLLECTION | ||||
| Thermometer No. 1 in the blue | Thermometer No. 2 in the yellow | Thermometer No. 3 beyond the red | Thermometer No. 4 in the shadow |
After 1 minute | | | | |
After 2 minutes | | | | |
After 3 minutes | | | | |
After 4 minutes | | | | |
After 5 minutes | | | | |
Activity 4: IR detection with a phone
The power of the infrared
Activity 5: Detection of IR light of a bulb
Activity 6: Constellation with IR LEDs
Cassiopeia with IR LEDs.
Resistance between 100 and 500 Ω
Activity 7: Constellation with remote controls
Emission of radio waves
Activity 8: Producing radio waves
Ultraviolet radiation
Johann Ritter discovered ultraviolet radiation in 1801
Ultraviolet radiation
Ultraviolet light
Andromeda Galaxy in visible light (Hubble)
Andromeda Galaxy in UV light (Swift)
Activity 9: Black light (UV)
Activity 10: Filter UV radiation
Fluorescent material and glasses, illuminated with white light.
The same material and glasses but illuminated with UV light.
Shadow of the glasses on the material
Activity 10: Filter UV radiation
It is important to use special sunglasses to avoid retinal damage!
(with UV filter)
X-rays
X-rays
More energetic than UV
Gamma rays
Gamma rays
Fermi's Five-year View of the Gamma-ray Sky
Uses of EM radiation in Medicine
Use of X-rays
Use of Gamma-rays
Use of Radio Waves
MRI Normal knee
MRI Human heart
CAT Normal knee
X-ray
Thank you very much �for your attention! �