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Solvated electrons. The electrons "dissolve" from the metal. It's blue because electrons have a different absorption spectra.
Different atoms have a different number of electrons. This is why they show different spectra.
The Bohr model fails to accurately predict an atom's spectra when dealing with more complex atoms that have multiple electrons. This is because the model assumes that electrons move in circular orbits around the nucleus, whereas in reality, electrons occupy regions of space called orbitals. Additionally, the model only accounts for the behavior of electrons in the ground state and does not consider excited states where electrons can transition between different energy levels.
That electrons can orbit their nucleus in only certain discrete orbits at certain specific levels of energy
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Spectra
The lines are at the same frequencies
the arrangment of electrons
Michael Edward O'Byrne has written: 'Combination frequencies and infra-red absorption spectra of certain alkaloids' -- subject(s): Absorption spectra, Alkaloids, Infrared spectra, Spectrum analysis, Tables
A single, extremely tiny unit of light known as a photon is produced when one electron in an atom undergoes a quantum drop in energy level. There are many such energy changes that electrons in the atoms of a single element can undergo, and they are all different. Furthermore, the energy changes for one element differ from the energy changes for all other elements. Now for why this is important: The amount of energy in a photon is directly proportional to the frequency of the light or other electromagnetic radiation of that photon. Therefore, each atom produces a set of electromagnetic frequencies that represents the possible downward changes in energy levels of its electrons.
Aside from determining how many electrons the atom has, the nucleus does not affect the spectra of that atom in any way.
Solvated electrons. The electrons "dissolve" from the metal. It's blue because electrons have a different absorption spectra.
An atom doesn't have a frequency. It can vibrate with many different frequencies. It can absorb radiation of different frequencies under different circumstances. For instance, electrons moving between various energy levels absorb and release characteristic frequencies of visible and ultra-violet light, and in a magnetic field radio frequency energy can be absorbed as the nucleus moves from one spin state to another. Bonds between hydrogen and other atoms absorb energies in the infra red. All these things give spectra of various frequencies, not an individual frequency.
Different atoms have a different number of electrons. This is why they show different spectra.
Different chemical elements emit (or absorb) certain specific frequencies of light. When the light from a star is split in to it's rainbow spectrum of light, certain parts of the spectrum will be black (in absorption spectra) or brighter (in emission spectra). By comparing these lines to the known emission and absorption spectra of elements, the composition of a stars atmosphere can be determined.
The Bohr model fails to accurately predict an atom's spectra when dealing with more complex atoms that have multiple electrons. This is because the model assumes that electrons move in circular orbits around the nucleus, whereas in reality, electrons occupy regions of space called orbitals. Additionally, the model only accounts for the behavior of electrons in the ground state and does not consider excited states where electrons can transition between different energy levels.