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Among species H, Li^(2+), He^(+), Be^(3+...

Among species `H, Li^(2+), He^(+), Be^(3+) and AI^(3+)` Bohr's model was able to explain the spectra of

A

all of these

B

none of these

C

all other species except `Be^(3+)`

D

all other species except `AI^(3+)`

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The correct Answer is:
D

Except `Al^(3+)` all contain one electron and Bohr's model could explain the spectra for one electron system, Bohr's model was not able to explain the spectra of multielectron system.
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Bohr's Model(spectrum of H like species)

Bohr's theory can be applied to the hydrogen-like species (He^(+), Li^(2+),Be^(3+) , and so on). With the increase of Z (atomic number), the value of enegry becomes_____and that of radius becomes________.

Consider the following statements (I) Bohr's theory can also be used to explain the spectra of He^(+) ion (II) Energy of an electron in the first Bohr orbit of hydrogen atom is -13.6eV (III) Bohr's theory is only applicable to hydrogen atom and not to any other species (IV) The energy of an electron in a hydrogen atom is quantised The correct statements are

Bohr's model enables us to derive the energy of an electron revolving in nth orbit. For H-atom and hydrogen like species : E_n = (2 pi^2 m e^4 Z^2)/(n^2 h^2) or = - (13.6 Z^2)/(n^2) eV "atom"^(-1) = (21.8 xx 10^(-19) Z^2)/(n^2) J "atom"^(-1) This helps to calculate the radius of an orbit, r_n = (0.529 n^2)/(Z) Å Bohr's model also explains the occurrence of different spectral lines. The wavelengths of difference line can be given as : 1/lambda = barv ("in" cm^(-1)) = R (1/(n_1^2) - 1/(n_2^2)) R = 109678 cm^(-1) and n_2 > n_1 . What is the ratio of radius of 4th orbit of hydrogen and 3rd orbit of Li^(2+) ion ?

Bohr's model enables us to derive the energy of an electron revolving in nth orbit. For H-atom and hydrogen like species : E_n = (2 pi^2 m e^4 Z^2)/(n^2 h^2) or = - (13.6 Z^2)/(n^2) eV "atom"^(-1) = (21.8 xx 10^(-19) Z^2)/(n^2) J "atom"^(-1) This helps to calculate the radius of an orbit, r_n = (0.529 n^2)/(Z) Å Bohr's model also explains the occurrence of different spectral lines. The wavelengths of difference line can be given as : 1/lambda = barv ("in" cm^(-1)) = R (1/(n_1^2) - 1/(n_2^2)) R = 109678 cm^(-1) and n_2 > n_1 . Which series of hydrogen spectrum lies in the visible region ?

Bohr's model enables us to derive the energy of an electron revolving in nth orbit. For H-atom and hydrogen like species : E_n = (2 pi^2 m e^4 Z^2)/(n^2 h^2) or = - (13.6 Z^2)/(n^2) eV "atom"^(-1) = (21.8 xx 10^(-19) Z^2)/(n^2) J "atom"^(-1) This helps to calculate the radius of an orbit, r_n = (0.529 n^2)/(Z) Å Bohr's model also explains the occurrence of different spectral lines. The wavelengths of difference line can be given as : 1/lambda = barv ("in" cm^(-1)) = R (1/(n_1^2) - 1/(n_2^2)) R = 109678 cm^(-1) and n_2 > n_1 . Which transition between Bohr's orbits corresponds to third line in Lyman series?

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