If you double the amount of light shining on a metal, you will increase the number of photons hitting the metal surface. This can lead to more photoelectrons being ejected from the metal due to the increased energy provided by the additional photons.
The intensity of light is directly related to the number of photons present. Higher intensity light has more photons, while lower intensity light has fewer photons. Each photon detected carries a discrete amount of energy that contributes to the overall intensity of the light.
A source of blue light would need to emit more photons per second to produce the same amount of energy as a source of red light. This is because blue light has higher energy photons, so fewer photons are needed to achieve the same total energy output as red light, which has lower energy photons.
Each photon has a specific amount of energy.
Red light has a lower amount of energy than blue light. This is because red light has a longer wavelength, which corresponds to lower energy photons, while blue light has a shorter wavelength and higher energy photons.
A photoresistor (or light-dependent resistor) is an element whose resistance changes with the amount of light shining on it. When exposed to light, the resistance of a photoresistor decreases, and when in darkness, the resistance increases. This property makes photoresistors useful in light-sensing applications.
Photoelectrons do not have the same energy because each electron absorbs a different amount of energy from the incident photons based on the specific interaction between the photon and the electron. This is influenced by factors such as the photon energy, the binding energy of the electron in the material, and the angle of incidence. As a result, photoelectrons exhibit a range of energies rather than a single, uniform energy level.
The water molecules release energy in the form of infrared photons that are absorbed by the surrounding air.
The amount of energy and therefore the wavelength differs. X-rays are more energetic than the others you mentioned.
Nothing. The stars shine all the time; the amount of radiation that the Sun receives from distant stars is so insignificant that it won't noticeable affect the Sun.
Not exactly. The sun is always shining on parts of both the northern hemisphere and the southern hemisphere. As the Earth is tilted, there are times when it shines on more of one than the other. At the point it is shining on its maximum amount of one hemisphere, it is a solstice. It is still shining on the other hemisphere too, but just not as much as it is at other times. That happens in June, when it is mostly shining on the northern hemisphere, giving it longer days and shorter nights, and in December, when it is mostly shining on the southern hemisphere and it has the longer days and shorter nights.
The energy of the photons decreases as the wavelength increases
The amount of energy given off by excited electrons when they radiate energy is equal to the difference in energy level between the initial and final states. This emitted energy is typically in the form of photons.
The intensity of light is directly related to the number of photons present. Higher intensity light has more photons, while lower intensity light has fewer photons. Each photon detected carries a discrete amount of energy that contributes to the overall intensity of the light.
A source of blue light would need to emit more photons per second to produce the same amount of energy as a source of red light. This is because blue light has higher energy photons, so fewer photons are needed to achieve the same total energy output as red light, which has lower energy photons.
Each photon has a specific amount of energy.
Red light has a lower amount of energy than blue light. This is because red light has a longer wavelength, which corresponds to lower energy photons, while blue light has a shorter wavelength and higher energy photons.
Due nuclear reaction on sun which are uncontrolled chain reaction with huge amount of energy