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Earn 100

The degeneracy of hydrogen atom that has energy equal to (where RH is Rydberg constant) is
(a)4
(b)6
(c)9
(d)12

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Important Questions on Atomic Structure
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An electron in an orbital of high angular momentum stays away from the nucleus than an electron in the orbital of lower angular momentum.
For a given value of the principal quantum number, the size of the orbit is inversely proportional to the azimuthal quantum number.
According to wave mechanics, the ground state angular momentum is equal to .
The plot of Vs for various azimuthal quantum numbers, shows peak shifting towards higher value.

HARD
Column – 1 | Column – 2 | Column – 3 |
(I) orbital | (i) |
(P) |
(II) orbital | (ii) One radial node | (Q) Probability density at nucleus |
(III) orbital | (iii) | (R) Probability density is maximum at nucleus |
(IV) orbital | (iv) -plane is a nodal plane | (S) Energy needed to excite an electron from state to state is times the energy needed to excite electron from state to state. |

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The number of given orbitals which have electron density along the axis is

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Column 1 | Column 2 | Column 3 |
(I) orbital | (i) |
(P) |
(II) orbital | (ii) One radial node | (Q) Probability density at the nucleus . |
(III) orbital | (iii) | (R) Probability density is maximum at the nucleus. |
(IV) orbital | (iv) -plane is a nodal plane | (S) Energy needed to excite an electron from state to state is times the energy needed to excite are electron from state to state. |

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Column 1 | Column 2 | Column 3 |
(I) orbital | (i) |
(P) |
(II) orbital | (ii) One radial node | (Q) Probability density at the nucleus . |
(III) orbital | (iii) | (R) Probability density is maximum at the nucleus. |
(IV) orbital | (iv) -plane is a nodal plane | (S) Energy needed to excite an electron from state to state is times the energy needed to excite are electron from state to state. |

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The correct order of their increasing energies will be:

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Consider the following pairs of electrons:
(A) (a)
(b)
(B) (a)
(b)
(C) (a)
(b)
The pairs of electrons present in degenerate orbitals is/are:

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