Revolution of electron and that of the planets

In summary: Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?Electrons do not orbit the nucleus due to the presence of the strong nuclear force.
  • #1
AakashPandita
157
0
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?
 
Physics news on Phys.org
  • #2
Hi Aakash! :smile:
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?

The problem is that an accelerating charge emits electromagnetic radiation (and therefore loses energy).

(this is easy to prove, and has nothing to do with quantum theory).

So a planet with a net charge would lose energy. :wink:
 
  • #3
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?
Electrons also do not orbit the nucleus. This is Rutherford's antiquated view of the atom that has since been replaced by the understanding that electrons exist in "clouds" determined by their wavefunctions.
 
  • #4
thank you
 
  • #5
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?

In fact a planet orbiting a star does lose energy, albeit extremely slowly, to gravitational radiation. This is very closely analogous to the way an orbiting charge loses energy to electromagnetic radiation. But gravity is a very weak force, so energy losses due to gravitational radiation are unmeasurably small except in special cases.

In both cases, the point is that while centripetal and centrifugal forces do balance out, there is another force acting on the orbiting body. The radiation it emits "pushes back" on it, so there is a drag force that slows the body down and causes it to spiral inward.

To explain why this doesn't happen to electrons in atoms we need quantum mechanics.
 
  • #6
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force.


Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion. Then come the centripetal and centrifugal forces.



Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?


Your example is a very bad analogy, but i'd say they don't lose energy because they are not really in motion. Lots of stuff at the micro scale is motion-like, real-like, spinning-like, etc. -like(but not quite so in reality).
 
  • #7
In GR, frame dragging induces orbital instability.
 
  • #8
Maui said:
Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion. Then come the centripetal and centrifugal forces.

http://en.wikipedia.org/wiki/Abraham-Lorentz_force
 
  • #9
Maui said:
Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion.
One problem with that: Newton's laws are not (exactly) correct. They are instead approximately correct in a limited regime velocities that are very, very low compared to the speed of light, distances that are very, very large compared to the Schwarzschild radius.

The_Duck in post #5 was referring to one of the predicted effects of general relativity. Gravitational radiation is immeasurably small in the case of the planets orbits about the Sun. The effect is not so small in the case of two very massive object orbiting very close to one another. It has in fact been observed. The observations eventually led to the discoverers receiving the 1993 Nobel Prize in physics.
 

1. What is the revolution of an electron?

The revolution of an electron refers to the movement of an electron around the nucleus of an atom. This movement is known as an orbit and is governed by the laws of quantum mechanics.

2. How does the revolution of an electron differ from that of a planet?

The revolution of an electron is vastly different from that of a planet. While an electron's orbit is confined to a specific energy level, a planet's orbit is influenced by the gravitational pull of other objects in its solar system.

3. What factors affect the revolution of an electron?

The revolution of an electron is primarily affected by the electric charge of the nucleus and the energy level of the electron. Other factors such as external magnetic fields and collisions with other particles can also impact an electron's orbit.

4. Can the revolution of an electron be observed?

No, the revolution of an electron cannot be directly observed due to its small size and the limitations of current technology. However, scientists can infer the orbit of an electron through indirect measurements and experiments.

5. How does the revolution of an electron contribute to chemical reactions?

The revolution of an electron is crucial in determining the chemical properties of an element. The arrangement and behavior of electrons in an atom's orbit determine how it will react with other atoms, forming chemical bonds and creating compounds.

Similar threads

Replies
21
Views
984
  • Quantum Physics
Replies
6
Views
2K
  • Quantum Physics
2
Replies
36
Views
1K
  • Quantum Physics
Replies
11
Views
894
  • Quantum Physics
Replies
13
Views
2K
Replies
2
Views
967
Replies
7
Views
1K
Replies
10
Views
1K
  • Quantum Physics
Replies
15
Views
2K
Back
Top