The Nature of Light Flashcards
(81 cards)
Who Proposed that light was a form of Electromagnetic radiation (EMR)
Maxwell
How does the Electromagnetc wave work
He proposed that if a changing elecric field is produced, it will also produce a magnetic field at right angles to the electric field. The changing magnetic field would then in turn produce a changing electric field and the cycle be repeated. In effect this would produce two mutually propagating fields oscillating at the same frequency.
what is the formula for the speed of light
c = f x h
c is the speed of light (ms^-1)
f is the frequency of the wave (HZ)
h is the wavelength of the wave (m)
How did Heinrich Hertz support Maxwell’s theory
in the 1880s Heinrich Hertzs performed experiments that demonstrated the existence of ‘invisible’ electromgantetic waves (radiow waves).
His basic experiment design involved a high voltage source to produce a spark and a detector formed from a loop of a copper wire with a small gap. Radio waves produced by the spark were detected when a tiny spark was induced across the gap in the detector. He found that the invisible waves behind like visibile light, and the speed of the waves was the same as the speed of the light.
How siginificant were Maxwell’s theory of light was
He provided an explantation of the nature of light, but also a strong theoretical basis for the wave model of light as he brought together several formerly distinct areas of study to form his theory
how did Hippolyte Fizeau experiment calculate the speed of light
Fizeau shone a bright light through a toothed cogwheel. As the wheel turned, sometimes light would be blocked by the cogs. Fizeau set up a mirror 8km away from the cog in order to measure the time-of-flight for light to travel the 16km path. As the pulse of the light needed to pass again through the teeth on the way back for it to be observered, knowing the speed of the rotation of the wheel, and knowing the distance between the cogwheel and the mirror, Fizeau was able to calculate the speed of light to be approximately 315 000kms^-1
how did Leon Foucault calulate the speed of light
Leon Foucalt refined Fizeau’s method by using a rotating mirror to block the light’s path and by 1862 he deteremined a result of 298 000 kms^-1 which is just over the 0.5% off the modern estimate.
What is the electromagnetic spectrum
the range of all types of radiation that has both electric and magnetic fields that travel in waves.
what are the different waves in the electromagnetic spectrum
AM radio wave: 100m wavelenght and 3 x 10^ 6 Hz frequency
FM radio or TV wave: 3m wavelength and 1 x 10^8 Hz frequency
Microwaves: 0.03 m wavelength and 1 x 10^10 Hz frequency
infared: 10^-5m wavelength and 3 x 10^13 Hz frequency
Visible light: 10^-7m wavelength and 3 x 10^15 Hz frequency
Ultraviolet: 10^-8m wavelength and 3 x 10^16 Hz frequency
X-ray: 10^-10m wavelength and 3 x 10^18
Gamma ray: 10^-15 m wavelength and 3 x 10^23
what type of waves are Electromagnetic waves
Transverse waves
What is spectroscopy
The brance of science investigating the spectra produced when matter interacts with or emits electromagnetic radiation is reffered to as spectroscopy.
What is spectroscopy used for
it is widely used in chemistry to detect and characterise atoms and molecules, as well as in astronomy and sensing technologies.
What are the types of spectra
Absorption
Emission
Black body radiation/continuous spectra
What is the absorption spectra
It is where light passing through an object has dark/missing lines from the spectrum. The dark/missing lines represent absorbed wavelengths or frequencies by certain elements of the object. By comparing the absorbed lines to elements, scientist can determine which elements are present in the object.
What is Emmision Spectra
When elements are heated to high temperature, or have an electrical current passed through them, they produce light. The Atoms in the material absorb energy and become ‘excited’ which makes the atom unstable and eventual return to the ‘unexcited’/ground state. The colour of light that becomes excited are the missing/darklines from the Absorption Spectra.
where is the visible spectrum around in wavelength
400nm and 750nm
What is an Incandescent light bulb
it is a lightbulb that produces light by heating a metal filament to a very high temperature, this produces electromagnetic radiation at a range of wavelengths; that is, the light from the incandescent globe is a continuous spectrum.
What are Discharge tubes
Discharge tube contains low-pressure gas through which a current is passed. The light emitted by the gas is in the ultraviolet range. The inside of the glass is coated with a material called a phospher, the ultraviolet light excites the phoser which then emits light over the entire visible spectrum. They emit less energy in the infrared range so more effciently convert the electrical energy into light energy and remain cool to touch, however they are much more expensive to manufacture incandescent globe but it has much lower running costs. Fluroesecnt lights are a type of discharge tube.
Do Planets and moons emit light?
no, they reflect light from a nearby luminous body like a star.
How can we determine what elements are in a star
by matching the missing bands in the absorbption spectra to the absobring substance.
What are the types of astronomies
Radio astronomy studies emission from cold objects such as interstellar gas and the cosmic microwave backgroudn radiation residual from the big bang
Submillimetre astronomy is used to look at molecular clouds and galaxy formation
infared astronomy is used to study star clusters, proto-stars and planets
Optical(visible) astronomy is the oldest form and reveals the chemical composition and temperature of stars.
Ultraviolet astronomy is used to study hotter objects such as young stars or stars approaching nova
X-ray astronomy studies very hot objects at temperatures of millions of degrees
Gamma-ray astronomy studies nuclear processes like supernova explosions and matter-antimatter interaction
what is the formula for Wien’s law
h = b/T
h is the peak wavelength (m)
T is the temperature in kelvins (K)
b is the Wien’s constant (mK)
Is the peakwavelength of an emitted light inversely proportional to the temperature of the object
yes
What is Redshifting
it is when the absorbption lines in the spectra are slightly longer (moved to the right) and it indicates that the planet/object is moving away from