X-Ray
In Bohr's model of the hydrogen atom, hydrogen's emission spectrum is produced when electrons jump between different energy levels within the atom. When an electron moves from a higher energy level to a lower one, it releases energy in the form of light, which is observed as distinct spectral lines in the emission spectrum. The energy of the emitted light corresponds to the energy difference between the initial and final energy levels of the electron.
In the Bohr model of the hydrogen atom, electrons can transition between energy levels by emitting or absorbing photons. When an electron falls from a higher energy level to a lower one, it releases energy in the form of a photon, which corresponds to a specific wavelength. The emission spectrum of hydrogen is produced when electrons transition from higher to lower energy levels, resulting in the release of photons with distinct wavelengths that correspond to specific spectral lines.
Basically, energy is emitted when an electron falls from a higher energy level to a lower energy level. Such energy is emitted as electromagnetic waves, which in certain cases can be visible light.
Absorption spectrum is a gap in the overall spectrum. It happen when light makes an electron jump to a higher orbital and light energy is absorbed. Emission spectrum is light emitted at particular wavelengths (where the absorption spectrum gaps are). It happens when an electron falls from a higher orbital and emits light energy in doing so.
It doesn't. An absorbtion spectrum is produced when it absorbs energy. An emission spectrum is produced when it lets the energy go again. The energy changes are associated with the element's electrons going up to higher energy levels and then dropping down again.
When a sodium atom is heated and gives off a line spectrum, the outermost electron absorbs energy and gets excited to a higher energy level. As the electron returns to its original energy level, it releases this energy in the form of light, creating the characteristic line spectrum of sodium.
When an electron drops from a higher energy state to a lower energy state, it emits electromagnetic radiation in the form of a photon. This process is known as atomic emission, and the energy of the emitted photon corresponds to the energy difference between the two electron states.
When an electron in an atom jumps from a higher energy state to a lower one, it releases energy in the form of photons. Each electron transition corresponds to a specific energy difference, resulting in the emission of photons with distinct energies. This emission spectrum displays sharp peaks at wavelengths corresponding to these energy differences.
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.
That’s correct. Spectral lines are produced when electrons in atoms move between energy levels. When an electron drops to a lower energy level, it emits a photon of a specific energy corresponding to a specific wavelength of light, creating spectral lines in the emitted light spectrum.
A line spectrum is produced when electrons in an atom transition between discrete energy levels. When an electron absorbs energy, it can move to a higher energy level; when it falls back to a lower level, it emits energy in the form of light at specific wavelengths. This emission creates a series of distinct lines, each corresponding to a specific transition, resulting in a unique spectral fingerprint for each element. The line spectrum is characteristic of the element and can be used to identify it in various applications, such as spectroscopy.
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.