SUMMARY
The Lyman-α wavelength for hydrogen is located in the ultraviolet (UV) region of the electromagnetic spectrum, specifically at 121.6 nm. This wavelength corresponds to transitions between the ground state (n=1) and the first excited state (n=2) of the hydrogen atom. In contrast, the visible spectrum for hydrogen, known as the Balmer series, occurs between 400 and 800 nm, involving transitions from higher energy levels (n>2) to n=2. Understanding these distinctions is crucial for studying hydrogen's spectral lines.
PREREQUISITES
- Basic knowledge of atomic structure and energy levels
- Understanding of electromagnetic spectrum and wavelength measurement
- Familiarity with spectral lines and series, specifically the Balmer and Lyman series
- Ability to interpret scientific literature and diagrams related to atomic spectra
NEXT STEPS
- Research the Lyman series and its significance in astrophysics
- Study the Balmer series and its applications in spectroscopy
- Explore the concept of energy level transitions in hydrogen and other elements
- Learn about the applications of UV spectroscopy in various scientific fields
USEFUL FOR
Students of physics and chemistry, astrophysicists, and anyone interested in atomic spectroscopy and the behavior of hydrogen in different regions of the electromagnetic spectrum.