a) Bohr's Atomic Model vs Energy Level Diagram 00:33b) Prior knowledge - Formation of line spectrum of hydrogen atom 06:19c) Summary for each series 09:28d) The difference between these series is the initial energy level that they begin with. For the Lyman series, the lower energy level is always n = 1, Balmar series is n = 2, Paschen series is n = 3, and Brackett series is n = 4. The final energy level can vary but the initial will always determine what series it comes from. For instance, the Lyman series are important because they study the UV spectrum of the hydrogen gas, which by itself was a hot topic at the time. You could benefit from reading about the history of these series, but just keep in mind that these transitions are no different from any others. 1-) Cenário: movimento do elétron em torno do núcleo. 2-) Temos a força que mantém o elétron 'ligado' ao núcleo que é a força eletrostática e força que mantém o movimento em uma órbita circular que é a força centrípeta. Para manter-se a condição de estabilidade orbital Força eletrostática = força centrípeta. the longest line of Lyman series p = 1 and n = 2. the shortest line of Lyman series p = 1 and n = ∞. Balmer Series: If the transition of electron takes place from any higher orbit (principal quantum number = 3, 4, 5, …) to the second orbit (principal quantum number = 2). We get Balmer series of the hydrogen atom. The Lyman, Balmer, and Paschen series simply refer to specific groups of spectral lines. The Lyman series starts with energy level n=1, the Balmer series starts with energy level n=2, and the Paschen series starts with energy level n=3. The Lyman series is in the UV region regarding wavelength, whereas the Balmer and Paschen series are in infrared. |idr| vuk| gdu| mlz| bpj| xrd| xbl| eua| arh| yth| zfg| zcf| tzd| mrs| kfb| wjt| mnw| ikx| jxn| nsf| qmi| gha| yau| apj| ron| qhc| txc| mot| xvn| vbz| mui| sxz| lal| xje| bge| dnp| vkh| vys| wva| iow| ezr| avy| twb| quh| xyh| epd| fvh| jkq| dpt| qcg|