The features of hydrogen spectrum: discontinuous spectrum(line spectrum) the frequency of the visible line spectrum meets with the following empirical equation empirical equation: v=3289x105(29 red红(Ha) n=4 blueness青(HB) n=5 blue-purple蓝紫Hy) n=3,4,5,6, n=6 purple紫(H6) But what does 2,n,3.289X 1015 mean in the empirical equation?
• discontinuous spectrum (line spectrum) • the frequency of the visible line spectrum meets with the following empirical equation 1 22 15 s) 1 2 1 (10289.3 − −×= n v n= 3,4,5,6, … But what does 2 ， n ，3.289 ×1015 mean in the empirical equation? empirical equation ： The features of hydrogen spectrum ： n = 3 red 红（H α ） n = 4 blueness 青（H β ) n = 5 blue-purple 蓝紫 ( H γ ) n = 6 purple 紫（H δ )
3.Bohr's theory Three major assumptions of Bohr's theory DAn electron in an atom could be located only in certain orbits that have particular radii and energies; 2Usually,an electron would remain in the orbit which is the most close to the nucleus.The atom is said to be in its ground state under this condition,which corresponds to the most stable energy state;Energy absorbed by the atom causes the electron to move from the orbits close to the nucleus to those far from it,then the atom is said to be in an excited state
3.Bohr’s theory Three major assumptions of Bohr’s theory ： ①An electron in an atom could be located only in certain orbits that have particular radii and energies； ②Usually, an electron would remain in the orbit which is the most close to the nucleus. The atom is said to be in its ground state under this condition, which corresponds to the most stable energy state; Energy absorbed by the atom causes the electron to move from the orbits close to the nucleus to those far from it, then the atom is said to be in an excited state
3An electron originally in a higher energy orbit will fall back to a lower energy orbit.As a result,a photon with energy hy is given off hv=E2-E E:the energy of an orbit E2-E1 h:Planck's constant h The H spectra can be well explained with Bohr's theory
③An electron originally in a higher energy orbit will fall back to a lower energy orbit. As a result, a photon with energy hν is given off. h EE EEh 12 12 − = = − ν ν E：the energy of an orbit h：Planck’s constant The H spectra can be well explained with Bohr’s theory
The energy levels in the H atom and the various emission series 76 Brackett series Paschen series Balmer series v=3.289x10z·s Lyman n=3red红(Ha,n=4 blueness青(Hg) n=5blue-purple蓝紫(Hy),n=6 purple紫(Hs) series
The energy levels in the H atom and the various emission series Balmer series Lyman series Paschen series Brackett series n = 3 red 红(H α), n = 4 blueness 青(H β ) n = 5 blue-purple蓝紫(H γ), n = 6 purple 紫(H δ ) ν = 3.289 ×1015( - )s 1 -1 2 2 1 n 2
v=3.289×105( n2>n1 △E=hv =6.626×10-34J-s×3.289×105(1 =2.179×10-18 n 2 Ru:Rydberg constant, n 2.179×10-18J
1- 2 2 2 1 15 s) 11 (10289.3 nn v −×= 12 > nn Δ = hvE RH：Rydberg constant， 2.179×10-18J. ) 11 ( 2 2 2 1 H nn RE −=Δ J) 11 (102.179 2 2 2 1 18- nn −×= 1- 2 2 2 1 34 15 s) 11 (10289.3sJ10626.6 nn −××⋅×= −