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 The electron in the hydrogen atom undergoes transition from higher orbitals to orbital of radius 211.6 pm.  This transition is associated with :
Option: 1  Lyman series
Option: 2  Balmer series
Option: 3  Paschen series
Option: 4  Brackett series  
 

For hydrogen atom, the radius of n??????th orbit, r??????n = 52.9 pm ×n2

211.6 pm = 52.9 pm×n2

n??????2=4

n=2

Hence, the transition is from a higher orbit to the second orbit.
This corresponds to the Balmer series.

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Posted by

vishal kumar

For the Balmer series in the spectrum of H atom, \bar{v}=\mathrm{R}_{\mathrm{H}}\left\{\frac{1}{\mathrm{n}_{1}^{2}}-\frac{1}{\mathrm{n}_{2}^{2}}\right\} the correct statements among (I) to (IV) are: (1) As wavelength decreases, the lines in the series converge
(II) The integer n1 is equal to 2
(III) The lines of longest wavelength corresponds to n2 = 3
(IV) The ionization energy of hydrogen can be calculated from wavenumber of these lines
 
Option: 1 (II),(III),(IV)
Option: 2 (I),(III),(IV)
Option: 3 (I),(II),(III)
Option: 4 (I),(II),(IV)
 

Line Spectrum of Hydrogen-like atoms

\frac{1}{\lambda }= RZ^{2}\left ( \frac{1}{n_{1}^{2}}-\frac{1}{n_{2}^{2}} \right )

Where R is called Rydberg constant, R = 1.097 X 107,  Z is the atomic number

n1= 1, 2, 3….

n2= n1+1, n1+2 ……

Lyman Series spectrum:

Where

n1= 1 and  n2= 2, 3, 4....

This lies in the Ultraviolet region.

Balmer Series Spectrum:

Where n1= 2 and  n2= 3, 4, 5, 6....

It lies in the visible region.

Paschen, Bracket and Pfund Series spectrums:

these lies in Infrared Region.

-

Since, \mathrm{\Delta E\: \propto\:\frac{1}{\lambda} } so for wavelength to be longest or maximum the energy gap should be minimum. For the Balmer series, the transition for the longest wavelength is from n = 3 to n = 2. Thus clearly, n1 value for the Balmer series is 2. Further, as wavelength decreases, the lines in the series converge.

Therefore, Option(3) is correct.

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vishal kumar

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The number of orbitals associated with quantum numbers n = 5, m_s = +1/2
is:
Option: 1 25
Option: 2 11
Option: 3 15
Option: 4 50
 

We have:

n = 5, ms = +1/2

Thus, the values of l are from 0 to (n-1)

l = 0 to 4

Thus, values of l are 5s, 5p, 5d, 5f, and 5g

Now, the total number of orbitals = n^2 = 5^2 = 25

Therefore, Option(1) is correct.

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Posted by

Kuldeep Maurya

The radius of the second Bohr orbit, in terms of the Bohr radius, a_{0}, in Li^{2+} is : 
Option: 1 \frac{2a_{0}}{3}

Option: 2 \frac{4a_{0}}{3}

Option: 3 \frac{4a_{0}}{9}

Option: 4 \frac{2a_{0}}{9}
 

As we have learnt,

 

Radius, velocity and the energy of nth Bohr orbital -

 

Bohr radius of nth orbit:

r_{n}= 0.529 \frac{n^{2}}{z}A^{0}

where Z is the atomic number

Velocity of electron in nth orbit:

v_{n}= (2.165\times 10^{6})\frac{z}{n}\: m/s

where z is atomic number

Total energy of electron in nth orbit:

E_{n}= -13.6\: \frac{z^{2}}{n^{2}}eV

Where z is atomic number

-

 

r=\frac{n^2a_o}{Z}.

\mathrm{For\ Li^{2+}\ r=\frac{2^2a_o}{3}=\frac{4a_o}{3}}

Therefore, Option(2) is correct.

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vishal kumar

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In the sixth period, the orbitals that are filled are :
Option: 1 6s, 4f, 5d, 6p
Option: 2 6s, 5d, 5f, 6p
Option: 3 6s, 5f, 6d, 6p
Option: 4 6s, 6p, 6d, 6f

Energy order of orbital’s according to Aufbau principle-

The order of orbitals filling is 6s, 4f, 5d, 6p.

Therefore, the correct option is (1).

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Posted by

Kuldeep Maurya

The difference between the radii of 3rd and 4th orbits of Li^{2+} is \Delta R_{1}. The difference between the radii of 3rd and 4th orbits of He^{+} is \Delta R_{2}. Ratio \Delta R_{1}:\Delta R_{2}  is  :
Option: 1 8 : 3
Option: 2 3 : 8
Option: 3 2 : 3
Option: 4 3 : 2

We know the formula,

The radius of nth Bohr's Orbit

\mathrm{r = 0.529\times\frac{n^2}{Z}}\mathrm{\ A^{\circ}}

Where
n = principal quantum number of orbit.
Z = Atomic number

Now, 

The difference between the radii of 3rd and 4th orbits of Li^{2+} is \Delta R_{1}. 

\mathrm{\left(R_{4}-R_{3}\right)_{L i^{+2}}=\frac{0.529}{3}\left\{4^{2}-3^{2}\right\}=\Delta R_{1}}

 

The difference between the radii of 3rd and 4th orbits of He^{+} is \Delta R_{2}. 

\left(\mathrm{R}_{4}-\mathrm{R}_{3}\right)_{\mathrm{He}^{+2}}=\frac{0.529}{2}\left\{4^{2}-3^{2}\right\}=\Delta \mathrm{R}_{2}

Ratio \Delta R_{1}:\Delta R_{2}  is  

\frac{\Delta \mathrm{R}_{1}}{\Delta \mathrm{R}_{2}}=\frac{\left(\mathrm{R}_{4}-\mathrm{R}_{3}\right)_{\textup{Li}^{2+}}}{\left(\mathrm{R}_{4}-\mathrm{R}_{3}\right)_{\mathrm{He}^{+}}}=\frac{\frac{4^{2}}{3}-\frac{3^{2}}{3}}{\frac{4^{2}}{2}-\frac{3^{2}}{2}}=\frac{7 / 3}{7 / 2}=\frac{2}{3}

Therefore, the correct option is (3).

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Kuldeep Maurya

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The correct statement about parobability density (except at a distance from nucleus) is :-
Option: 1 it can be zero for 1s orbital
Option: 2 It can never be zero for 2s orbital
Option: 3 It can be negative for 2p orbital
Option: 4 it can be zero for 3p orbital

Probability density can be zero for 3p orbital.

Therefore, Option(4) is correct.

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Posted by

Kuldeep Maurya

The region in the electromagnetic spectrum where the Balmer series lines appear is:
Option: 1 Visible
Option: 2 Microwave
Option: 3 Infrared
Option: 4 Ultraviolet

Balmer series give visible lines for H-atom.

As lines of Balamer series belongs to both UV as well visible region of EM spectrum. However most appropriate should be visible region.

Therefore, the correct option is (1).

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Kuldeep Maurya

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The shortest wavelength of H atom in the Lyman series is \lambda_{1}. The longest wavelength in the Balmer series He+ is:
Option: 1 \frac{36 \lambda _{1}}{5}
Option: 2 \frac{5\lambda _{1}}{9}
Option: 3 \frac{9 \lambda _{1}}{5}
Option: 4 \frac{27 \lambda _{1}}{5}

We know,

\Delta \mathrm{E}=\frac{\mathrm{hc}}{\lambda}

So,\lambda=\frac{h c}{\Delta E} for  \lambda minimum(Shortest)

\mathrm{\Delta \mathrm{E}= maximum}

for f H atoms in the Lyman series n = 1 & for \mathrm{\Delta \mathrm{E}_{maximum}}Transition must be form n = \infty to n = 1,

Z = 1 

\text { So } \frac{1}{\lambda}=R_{H} Z^{2}\left(\frac{1}{n_{1}^{2}}-\frac{1}{n_{2}^{2}}\right)

\frac{1}{\lambda_1}=\mathrm{R}_{\mathrm{H}} \mathrm{(1)}^{2}(1-0)

\frac{1}{\lambda_1}=\mathrm{R_H} \times(1)^{2} \Rightarrow \lambda_{1}=\frac{1}{\mathrm{R_H}}

For longest wavelength \mathrm{\Delta \mathrm{E}_{minimum}} for Balmer series n = 3 to n = 2 will have \mathrm{\Delta \mathrm{E}_{minimum}} for He+ , Z = 2

\text { So } \frac{1}{\lambda_{2}}=R_{H} \times Z^{2}\left(\frac{1}{n_{1}^{2}}-\frac{1}{n_{2}^{2}}\right)

\frac{1}{\lambda_{2}}=\mathrm{R}_{\mathrm{H}} \times (2)^2\left(\frac{1}{4}-\frac{1}{9}\right)

\frac{1}{\lambda_{2}}=\mathrm{R}_{\mathrm{H}} \times \frac{5}{9}

\lambda_{2}=\frac{1}{R_H} \times \frac{9}{5}

\lambda_{2}=\lambda_{1} \times \frac{9}{5}

Therefore, the correct option is (3).

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Posted by

Kuldeep Maurya

Consider the hypothetical situation where the azimuthal quantum number, l, takes values 0,1,2,.....n+1, where n is the principal quantum number. Then, the element with atomic number :
Option: 1 9 is the first alkali metal
Option: 2 13 has a half-filled valence subshell
Option: 3 8 is the first noble gas
Option: 4 6 has a 2p-valence subshell

GIven l= 0 to (n + 1)

Now for n = 1,
l = 0, 1, 2

Orbitals :

1s  , l =0 

1p , l = 1

1d , l = 2

 

And for

n = 2

l = 0, 1, 2, 3

\mathrm{Orbitals} : 2s,2p,2d,2f

 

And for

n = 3

l = 0, 1, 2, 3,4

\mathrm{Orbitals} : 3s,3p,3d,3f,3g

Now, in order to wire electronic configuration, we need to apply (n + l) rule.

Energy order : 1s < 1p < 2s < 1 d < 2p < 3s < 2d ...

1) 9 : 1s2 1p6 2s1 is the first alkali metal because after losing one electron, it will achieve the first noble gas configuration

2) 13 : 1s2 1p6 2s2 1d3 is not half filled. (Showing incorrect statement)

3) 8 : 1s2 1p6 is the first noble gas.

4) 6 : 1s2 1p4 has 1p valence subshell.

 

Therefore, Option 2 is correct.

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Kuldeep Maurya

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