3.96 10-19 j
The transition energy corresponding to an absorption line at 460nm is about 2.7 electronvolts (eV). This energy is calculated using Planck's equation, E = hc/λ, where h is Planck's constant, c is the speed of light, and λ is the wavelength in meters.
4.32 x 10^-19 j
The second longest wavelength in the absorption spectrum of hydrogen corresponds to the transition from the n=2 to n=4 energy levels. This transition produces a spectral line known as the H-alpha line, which falls in the red part of the visible spectrum at a wavelength of 656.3 nm.
The wavelength of the hydrogen atom in the 2nd line of the Balmer series is approximately 486 nm. This corresponds to the transition of an electron from the third energy level to the second energy level in the hydrogen atom.
The spacing between the lines in the spectrum of an element are constant. This is called the emission spectrum of an element. Each element has a unique emission spectra that will be the same each time.
3.96 10-19 j
The transition energy corresponding to an absorption line at 460nm is about 2.7 electronvolts (eV). This energy is calculated using Planck's equation, E = hc/λ, where h is Planck's constant, c is the speed of light, and λ is the wavelength in meters.
4.32 x 10^-19 j
An absorption line is a line which corresponds to the absorption of electromagnetic radiation at a specific wavelength.
The second longest wavelength in the absorption spectrum of hydrogen corresponds to the transition from the n=2 to n=4 energy levels. This transition produces a spectral line known as the H-alpha line, which falls in the red part of the visible spectrum at a wavelength of 656.3 nm.
The transition energy corresponding to an absorption line at 502nm can be calculated using the formula E = hc/λ, where E is the energy, h is Planck's constant, c is the speed of light, and λ is the wavelength. Plugging in the values, we get E = (6.63 x 10^-34 J s * 3 x 10^8 m/s) / (502 x 10^-9 m) ≈ 3.96 x 10^-19 J.
Each colored line in hydrogen's emission spectrum corresponds to a specific transition of an electron between energy levels in the hydrogen atom. The wavelengths of these lines are unique to each transition, creating a distinct pattern that can be used to identify elements and their energy levels.
5.69 × 1014 Hz
6.52 1014 Hz
The lines in an atomic spectrum are caused by the emission or absorption of photons as electrons move between different energy levels within the atom. Each line corresponds to a specific energy transition, and the distinct set of lines is unique to each element, making them a fingerprint for identifying elements.
The corresponding frequency of absorption is 3.440 cm-1 * 2.99792 x 10^10 cm/s = 1.032 x 10^11 Hz. The two energy levels involved in this transition correspond to the rotational energy levels of the NO molecule.
The absorption spectrum of an element have lines in the same places as in its emission spectrum because each line in the emission spectrum corresponds to a specific transition of electrons between energy levels. When light is absorbed by the element, electrons move from lower energy levels to higher ones, creating the same lines in the absorption spectrum as the emission spectrum. The frequencies of light absorbed and emitted are the same for a specific element, resulting in matching lines.