Therefore, an electron in an orbit will emit radiation, the energy carried by radiation comes from electronic motion. According to the electromagnetic theory of Maxwell, charged particles when accelerated should emit electromagnetic radiation (This feature does not exist for planets since they are uncharged). So an electron in the nuclear model describing planet like orbits is under acceleration. Which of the following statements best describes how white light interacts with Rutherford's Classical Solar System Model in the simulation O the photons bounce off of the nucleus, none are absorbed O some photons are absorbed by the electron, only UV light is emitted O the electron orbits the nucleus and they eventually collide. However, when a body is moving in an orbit, it undergoes acceleration (even if the body is moving with a constant speed in an orbit, it must accelerate because of changing direction). The similarity between the solar system and nuclear model suggests that electrons should move around the nucleus in well defined orbits. Comment: What does this mean to our model It means that the electron must have its own 'ground-state' energy that resists/prevents the. Question 6: Briefly speculate why the electron loses energy and spirals into the nucleus. The theory can also calculate precisely the planetary orbits and these are in agreement with the experimental measurements. Use Rutherford's Classical Solar System Model: Switch to Rutherford's Model. When classical mechanics is applied to the solar system, it shows that the planets describe well-defined orbits around the sun. m 1m 2/r 2) where m 1 and m 2 are the masses, r is the distance of separation of the masses and G is the gravitational constant. Further, the coulomb force (kq 1q 2 /r 2) where q 1 and q 2 are the charges, r is the distance of separation of the charges and k is the proportionality constant) between electron and the nucleus is mathematically similar to the gravitational force (G. 22.Switch to theBohr model, click onShow electron energy level in the upper right hand corner, and set the speed. Using the Bohr model, determine the energy, in electron volts, of the photon produced when an electron in a hydrogen atom moves from the orbit with n 5 to the orbit with n 2. This was Rutherford’s model that assumes the atom is like our solar system.Describe what happens with the Solar System model. It is the amount of energy that an electron gains when subjected to a potential of 1 volt 1 eV 1.602 \ (×\) 10 19 J. Temperature is measured with a thermometer. 21.Just for fun, switch to theClassical Solar System model. Rutherford nuclear model of an atom is like a small scale solar system with the nucleus playing the role of the massive sun and the electrons being similar to the lighter planets. Temperature is a physical quantity that expresses quantitatively the attribute of hotness or coldness.
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