Short Answer: These four lines are utterly specific for Hydrogen, just like a fingerprint.
1: 2, 3, 4 2: 3, 4 3: 4
There are an infinite number of transitions, but only 4 of these transitions emit energy in the visible region of the spectrum. That's what our teacher told us。
Each energy level corresponds to an exact amount of energy needed by the electron to orbit the nucleus. Transitions from a higher energy level to a lower energy level correspond to the difference in the energy needed for an electron to occupy those two energy levels. This difference creates the emission spectrum.
atom give line spectrum because it is sharukh khan and molecule is salman khan that is why it give continiuos spectrum
This would consist of several series of lines corresponding to the energies of electron transitions. They are bright lines for an emission spectrum and dark for absorbtion.
Seven
There are an infinite number of transitions, but only 4 of these transitions emit energy in the visible region of the spectrum. That's what our teacher told us。
Each energy level corresponds to an exact amount of energy needed by the electron to orbit the nucleus. Transitions from a higher energy level to a lower energy level correspond to the difference in the energy needed for an electron to occupy those two energy levels. This difference creates the emission spectrum.
Because the spectra of elements is determined by the energy of transitions of electrons between two allowed quantum states. Since these energy differences can have only certain specified values, the spectrum consists of lines: The spectrum frequency values intermediate between the lines do not correspond to transitions between any two allowed quantum states and therefore do not appear in the spectrum
The precise energy levels of each orbital vary depending on the nuclear charge. Since the spectral lines correspond to transitions between orbitals, each element will have different energies for these transitions, and therefore will have a unique spectrum.
No. The emission and absorption spectrum covers everything from UHF radio to X-rays. (There are no energy level transitions that correspond to the low energy HF or VHF radio bands and below. The lowest-energy transition is the one at 1420 MHz/21 cm.)
The color in the flame is the representation of a specific line in the spectrum.
The spectrum of sunlight is continuous while for hydrogen is line spectrum (discontinuous)
atom give line spectrum because it is sharukh khan and molecule is salman khan that is why it give continiuos spectrum
It was discovered by finding lines in the spectrum of the Sun that corresponded to calculations for the electronic transitions in helium.
LBP Spectrum?
The series of lines in an emission spectrum caused by electrons falling from energy level 2 or higher (n=2 or more) back down to energy level 1 (n=1) is called the Lyman series. These emission lines are in the ultra-violet region of the spectrum.
This would consist of several series of lines corresponding to the energies of electron transitions. They are bright lines for an emission spectrum and dark for absorbtion.