- #1
ciaranciaran1
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so the title speaks for itself i hope. my problem is i don't know how to work the formula. what are the ns about??
lamba^-1 = R(n1^-2 - n2^-2)
lamba^-1 = R(n1^-2 - n2^-2)
The visible emission spectrum for hydrogen is a series of colored lines that appear when hydrogen gas is excited by an electric current or other energy source. These lines represent the specific wavelengths of light that are emitted when the hydrogen atoms return to their ground state from an excited state.
The visible emission spectrum for hydrogen is calculated using the Rydberg formula, which is based on the energy levels of the hydrogen atom and the wavelengths of light that are emitted when an electron transitions from a higher energy level to a lower energy level. This formula can be used to determine the specific wavelengths of light that will be present in the visible emission spectrum for hydrogen.
The visible emission spectrum for hydrogen is significant because it provides evidence for the quantization of energy levels in atoms. It also allows scientists to study the structure of the hydrogen atom and gain a better understanding of the behavior of matter at a microscopic level.
The visible emission spectrum for hydrogen is unique in that it only consists of a few distinct lines in the visible range, while other elements may have more complex and varied spectra. This is due to the simplicity of the hydrogen atom and its single electron.
The visible emission spectrum for hydrogen has many practical applications in fields such as astronomy, chemistry, and physics. It is used to identify the presence of hydrogen gas in stars and other astronomical objects, as well as in chemical analysis and the development of new technologies such as hydrogen fuel cells.