Uploaded August 2022 | Updated September 2026, 1 week ago
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It’s commonly thought that Albert Einstein won the 1922 Nobel Prize for his work on relativity. Not true. Einstein’s prize was for his earlier 1905 explanation of the photoelectric effect, a phenomenon later incorporated in devices such as electric eyes, light meters, and, before digital, readers of motion picture soundtracks. Today, the photoelectric effect is applied to photovoltaic electric cells on the roofs of buildings and in sprawling solar energy farms.
Ejected electrons
Quite simply, the photoelectric effect is the ejection of electrons from certain surfaces or from atoms below those surfaces when illluminated with light. Several investigators in the latter part of the 19th century noted the curious ability of light striking metal surfaces to create electric current. Figure 1 shows an arrangement for observing this “photoelectric effect.” Light shining on the negatively charged curved metal plate liberates electrons that are attracted to a small positive plate. This process produces a measurable electric current.
PHOTOELECTRIC EFFECT
The definition of the photoelectric effect states that it is a phenomenon in which light causes electrons to be expelled from a metallic surface when exposed to the light of an appropriate frequency.
The expelled electrons are called photoelectrons.
The law of conservation of energy is the basic principle of the photoelectric effect.
Albert Einstein was the first to successfully explain the laws of the photoelectric effect after years of research in this field.
He came to the conclusion that this effect was caused by light energy being transported in discrete quantized packets called photons.
A photoelectric effect diagram is given below.
THE PHOTOELECTRIC EFFECT EXPERIMENT
The photoelectric effect can be explained by the experiment wherein the electrons on the metal body absorb energy from the incident light and then use it to counteract the attractive forces that bind them to the metallic nuclei.
The photons( the 'particles' of light that make up the visible spectrum) that strike the metal's surface must have enough energy to overcome the attractive forces that bind the electrons to the nuclei in order for the photoelectric effect to occur.
The threshold energy for the photoelectric effect is the least quantity of electricity required to remove an electron from a metal.
The photoelectric effect experiment cannot be explained using the wave model of light.
However, the particle nature of light, which can be viewed as a stream of electromagnetic energy particles, can explain this behavior.
The photoelectric effect can be explained by Planck's equation E = h𝜈 = hc/λ.
SUMMARY
The photoelectric effect is a phenomenon that causes electrons to be expelled from a metallic surface when exposed to the light of an appropriate frequency.
The electrons at the surface of the metal absorb energy from the incident light and then use it to counteract the attractive forces that bind them to the metallic nuclei.
The photoelectric effect can be explained by Planck's equation:
E = h𝜈 = hc/λ.
Please don't hesitate to send an email for comments, advices, recommendation, even for support and classes. My email address is here
thephysicspartner@gmail.com
It’s commonly thought that Albert Einstein won the 1922 Nobel Prize for his work on relativity. Not true. Einstein’s prize was for his earlier 1905 explanation of the photoelectric effect, a phenomenon later incorporated in devices such as electric eyes, light meters, and, before digital, readers of motion picture soundtracks. Today, the photoelectric effect is applied to photovoltaic electric cells on the roofs of buildings and in sprawling solar energy farms.
Ejected electrons
Quite simply, the photoelectric effect is the ejection of electrons from certain surfaces or from atoms below those surfaces when illluminated with light. Several investigators in the latter part of the 19th century noted the curious ability of light striking metal surfaces to create electric current. Figure 1 shows an arrangement for observing this “photoelectric effect.” Light shining on the negatively charged curved metal plate liberates electrons that are attracted to a small positive plate. This process produces a measurable electric current.
PHOTOELECTRIC EFFECT
The definition of the photoelectric effect states that it is a phenomenon in which light causes electrons to be expelled from a metallic surface when exposed to the light of an appropriate frequency.
The expelled electrons are called photoelectrons.
The law of conservation of energy is the basic principle of the photoelectric effect.
Albert Einstein was the first to successfully explain the laws of the photoelectric effect after years of research in this field.
He came to the conclusion that this effect was caused by light energy being transported in discrete quantized packets called photons.
A photoelectric effect diagram is given below.
THE PHOTOELECTRIC EFFECT EXPERIMENT
The photoelectric effect can be explained by the experiment wherein the electrons on the metal body absorb energy from the incident light and then use it to counteract the attractive forces that bind them to the metallic nuclei.
The photons( the 'particles' of light that make up the visible spectrum) that strike the metal's surface must have enough energy to overcome the attractive forces that bind the electrons to the nuclei in order for the photoelectric effect to occur.
The threshold energy for the photoelectric effect is the least quantity of electricity required to remove an electron from a metal.
The photoelectric effect experiment cannot be explained using the wave model of light.
However, the particle nature of light, which can be viewed as a stream of electromagnetic energy particles, can explain this behavior.
The photoelectric effect can be explained by Planck's equation E = h𝜈 = hc/λ.
SUMMARY
The photoelectric effect is a phenomenon that causes electrons to be expelled from a metallic surface when exposed to the light of an appropriate frequency.
The electrons at the surface of the metal absorb energy from the incident light and then use it to counteract the attractive forces that bind them to the metallic nuclei.
The photoelectric effect can be explained by Planck's equation:
E = h𝜈 = hc/λ.







![Space Part 1 - Orbital Speed (IGCSE 0625/0972)
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The topic space is the newly injected topic in 0625/0972 IGCSE physics curriculum, exam will be conducted from 2023 onwards
Important Definition
Define Rotation of Earth: The circular movement of the Earth about its own axis is called as the rotation of the Earth.
Define Average orbital speed: It is defined using the equation: v = 2??r /T where r is the average radius of the orbit and T is the orbital period
Define Solar system: Solar system is a single term that includes eight planets and their moons in orbit round the sun. Also included in the solar system are the smaller bodies such as the comets., asteroids, and the meteoroids.
Define Orbital distance: Orbital distance is the term that tells us the time taken by one object to revolve around the other.
Define Orbital duration[ Orbital time}: Orbital duration is the time taken by one object to completely orbit around the other.
Define gravitational field strength: Gravitational field strength is a term that indicates the amount of gravitational force that is exerted per unit mass at a particular point. It has a symbol g
Define Interstellar clouds of gas and dust: It is a cloud comprising of dust, plasma and gases present in all the galaxies, including our own.
Define accretion disc: These are structures that surround the celestial objects such as the stars and the black holes. These structures are made of gas, plasma and dust
Define Planetary data: It refers to the data that gives us information on the different planets based on researches and explorations
6.2 Stars and the Universe
Define Stars: Stars are massive , self-luminous celestial objects, made of Hydrogen and Helium
Define Proto stars: A Protostar is a young star. .It is formed as a result of accretion in the nebula.
Define Stable stars: In every star, there is the gas pressure that exerts an outward force from the centre and at the same time , there is gravity that is pulling the atoms of Hydrogen and Helium inwards. When the outward pushing force balances the gravitational force, we call the star as a stable tar. Example of a stable star is the Sun.
Define Sun: The Sun is a very bright, luminous, celestial and a stable star, situated in the spiral arm of the Milky Way galaxy and at the centre of the Solar System.
Define Galaxy: The word galaxy encompasses billions of stars along with their solar systems, gas and dust held by their gravity. There are more than a hundred billion galaxies in the universe.
Define Milky way: Milky way is a spiral galaxy that includes our solar system. It has billions of stars, including our Sun.
Define Universe: Universe refers to the space, time and matter and all the laws that govern them.
Define Light-year: One light-year is the distance traveled in (the vacuum of) space by light in one year.
Define Red giants: These are massive , luminous stars with a very low surface temperature and a high volume , with a reddish-orange hue, in their final stage of stellar evolution and that have exhausted their supply of Hydrogen in their core. Examples: Aldebaran (Alpha Tauri) and Mira (Omicron Ceti).
Define Red supergiants: Red supergiants are aging giant stars with a minimum of 15 solar masses. [solar mass refers to the mass of the sun, when used as a unit of mass. One solar mass is equal to 1.989 x 1030 kg ]
Define Supernova: Supernova is a powerful and luminous stellar explosion, that happens when a star has reached the end of its life. Example: Keplers Supernova
Define Nebula: Nebula is a Latin word for fog or cloud. It consists of interstellar clouds consisting of Helium, Cosmic Dust, ionized gases, hydrogen as well as molecular clouds. [There are in all 5 different types of Nebulae, namely; emission nebulae, reflection nebulae, dark nebulae, planetary nebulae, and supernova remnants.
Define Black hole: A black hole is a region in the space, in which the effect of gravity is so strong, that it lets nothing escape out f it, not even light. The region appears to be black and circular.[ There are approximately 100 billion super massive black holes]
Define Redshift: Redshift is a phenomenon in which the spectrum of an astronomical object gets displaced towards the longer( red) wavelength.
Define Cosmic microwave background radiation (CMBR): Cosmic microwave background radiation (CMBR) is the leftover of the cosmic radiation after the big bang.
Define Hubble constant Ho: Hubble constant is the ratio of the speed at which the galaxy is moving away from the Earth to its distance from the Earth Space Part 1 - Orbital Speed (IGCSE 0625/0972)](https://i.ytimg.com/vi/xT_XJeoeuAw/mqdefault.jpg)


