Electron Orbitals: Heat, Excitation and Radiation

In summary, electron spin and orbitals play a role in the emission of radiation when an electron transitions from a higher energy state to a lower energy state. This can happen through collisions or photon absorption, but there are also cases where the electron can remain in an excited state for a longer period of time. The term "spin" is often misused and refers to the intrinsic angular momentum of the electron, while orbitals contain the electron's motion.
  • #1
Biologik
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What do they have to do with heat? What exactly can cause and electron to become exited and what exactly does the particle it comes in contact with do that causes the electron to become ''exited''? The higher the orbitals and electron spins, the shorter the wavelengths of the radiation it emits correct? But WHY do they emit radiation when the move from a high orbital to a lower orbital?
 
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  • #2
What do they have to do with heat? More heat, more energy of the system, more energy for electrons.

What exactly can cause and electron to become exited and what exactly does the particle it comes in contact with do that causes the electron to become ''exited''? Typically "excited" is defined loosely as giving something, in this case electrons, more energy. Anything that gives energy to an electron allows it to become excited.

The higher the orbitals and electron spins, the shorter the wavelengths of the radiation it emits correct? Electrons only have two different ways they can carry spin, so it can't really increase in the sense to which you are referring. Also as you go up in energy levels, the longer the wavelength tends to get from one state to the next. For example going from n=2 to n=1 will be smaller than going from n=3 to n=2 in wavelength.

But WHY do they emit radiation when the move from a high orbital to a lower orbital? Energy has to go somewhere right? It's emitted as light (which carries energy).
 
  • #3
Biologik said:
What do they have to do with heat?

The electronic energy state is an energetic degree of freedom of an atom/molecule, just like its translation, vibrational and rotational energy states. Which are the components it's usually separated into. (Strictly speaking this separation is false; as these states are not independent of each other) In simplified descriptions heat is described as 'motion', i.e. only the latter three forms of energy. This isn't true in general, it's just that most molecules are completely in their electronic ground state except at very high temperatures, so they're not carrying any part of the thermal energy.
What exactly can cause and electron to become exited and what exactly does the particle it comes in contact with do that causes the electron to become ''exited''?

If it's a photon, its electrical field transfers energy to the electron through the electromagnetic force. If it's a collision between atoms or charged particles, then the electrical field of that charged particle.
The higher the orbitals and electron spins, the shorter the wavelengths of the radiation it emits correct?

No. First, if you mean spin by 'the higher the electron spins', then that doesn't necessarily correspond to a higher energy state. A higher spin state can correspond to a lower energy state. (E.g. the oxygen molecule, whose ground state is a triplet spin state) If you mean 'angular momentum', then higher angular momentum usually means higher energy, but only compared to a a state with the same principal quantum number. Second, the wavelength of the light emitted depends on which states its transitioning between. A high-energy state doesn't necessarily mean a high-energy transition.
But WHY do they emit radiation when the move from a high orbital to a lower orbital?

They don't have to; they can also transfer that energy 'non-radiatively', for instance when two atoms/molecules collide, or turn it into vibrational energy (vibronic coupling). A photon will only be emitted if the two states fulfill certain criteria (selection rules) which allow for photon creation; usually a change in the overall electrical or magnetic moment of the atom/molecule.

If an electron is in an excited state where selection rules stop it from decaying (a 'forbidden' transition, by which we really mean 'very improbable'), it can stay there for a very long time. Because then it has to wait for a collision, or utilize some other, more uncommon process. Such as creating two photons at once (which has quite different 'rules'), or wait for random vacuum fluctuations to induce an electric or magnetic moment that it can use to decay.
 
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  • #4
In several messages, you have been musing on "electron spin". I think you are misusing the term. "spin" normally refers to the intrinsic angular momentum of the particle, analogous to the Earth spinning on its axis. The electron's spin can point in different directions but never changes in total amount. It always must have exactly 1/2 unit.

Electron orbitals contain "motion" that is, to continue the analogy, like the Earth's movement around the sun. But as soon as you want details, the analogy breaks down since you don't have classical motion or position at that scale. Available orbitals have differing amounts of angular momentum, but also many orbitals in one "shell" have the same total angular momentum but arrange it differently.
 
  • #5


Electron orbitals are regions of space around an atom where an electron is likely to be found. Heat, excitation, and radiation are all related to the energy levels of electrons in these orbitals.

Heat is a form of energy that can cause electrons to become excited. When an atom is heated, its electrons absorb this energy and move to higher energy levels or orbitals. This is known as excitation.

There are several ways that an electron can become excited. One common way is through collisions with other particles, such as other atoms or photons (particles of light). When an electron collides with another particle, it can absorb energy and move to a higher energy level. Alternatively, an electron can also be excited by absorbing a photon of light, which has a specific amount of energy depending on its wavelength.

When an electron is in an excited state, it is unstable and will eventually return to its lower energy state or ground state. In order to do this, the electron must release the excess energy it gained when it was excited. This is where radiation comes in. The electron releases this excess energy in the form of a photon of light, which is emitted as radiation.

The wavelength of the radiation emitted by an electron depends on the energy difference between the two orbitals it transitions between. The higher the energy difference, the shorter the wavelength of the emitted radiation. This is known as the energy-level diagram.

So to answer your question, electrons emit radiation when they move from a higher orbital to a lower orbital because they are releasing excess energy gained during excitation. This excess energy is emitted as a photon of light, or radiation. The higher the energy difference between the two orbitals, the shorter the wavelength of the emitted radiation. This is why the higher the orbitals and electron spins, the shorter the wavelengths of the emitted radiation.

In summary, heat, excitation, and radiation are all related to the energy levels and movements of electrons in atom orbitals. Heat can cause electrons to become excited, which leads to the emission of radiation when they return to their ground state. Collisions with other particles or absorption of photons of light can also cause electrons to become excited. The wavelength of the emitted radiation depends on the energy difference between the two orbitals the electron transitions between.
 

Related to Electron Orbitals: Heat, Excitation and Radiation

1. What are electron orbitals?

Electron orbitals are regions of space around an atom's nucleus where electrons are most likely to be found. They are described by quantum mechanics and can have different shapes and energies.

2. How does heat affect electron orbitals?

Heat can cause electrons to absorb energy and jump to higher energy levels or orbitals. This is known as excitation, and when the electrons return to their original energy level, they release the excess energy as heat or light.

3. What is the difference between excitation and radiation?

Excitation is the process of electrons absorbing energy and moving to higher energy levels, while radiation is the release of this energy in the form of heat or light when the electrons return to their original energy level.

4. How do electron orbitals play a role in chemical reactions?

Chemical reactions involve the rearrangement of electrons between atoms. The electron orbitals determine the energy and stability of the atoms, which in turn affect the type and speed of the reaction.

5. Can electron orbitals be observed?

Electron orbitals cannot be directly observed, but their existence and properties can be inferred through experiments and mathematical models based on quantum mechanics principles.

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