MCQ 11 Mark
The energy of the highest energy photon of Balmer series of hydrogen spectrum is close to
- A
$13.6 eV$
- ✓
$3.4 eV$
- C
$1.5 eV$
- D
$0.85 eV$
AnswerCorrect option: B. $3.4 eV$
$E=13.6\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right]$.
For highest energy in Balmer series $n_1=2$ and $n_2=\infty \Rightarrow E=13.6\left[\frac{1}{(2)^2}-\frac{1}{(\infty)^2}\right]=3.4 \mathrm{eV}$
View full question & answer→MCQ 21 Mark
In the spectrum of hydrogen atom, the ratio of the longest wavelength in Lyman series to the longest wavelength in the Balmer series is
- ✓
$5 / 27$
- B
$1 / 93$
- C
$4 / 9$
- D
$3 / 2$
AnswerCorrect option: A. $5 / 27$
In Lyman series $\lambda_{\max }=\frac{4}{3 R}$In Balmer series $\lambda_{\max }=\frac{36}{5 R}$.
So required ratio $=\frac{5}{27}$
View full question & answer→MCQ 31 Mark
The ratio of the wavelengths for $2 \rightarrow 1$ transition in $L i, H e$ and $H$ is
- A
$1: 2: 3$
- B
$1: 4: 9$
- ✓
$4: 9: 36$
- D
$3: 2: 1$
AnswerCorrect option: C. $4: 9: 36$
$ \frac{1}{\lambda}=R Z^2\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right) \Rightarrow \lambda \propto \frac{1}{Z^2}$
$ \lambda_{L^{++}}: \lambda_{H e^{+}}: \lambda_H=4: 9: 36$
View full question & answer→MCQ 41 Mark
In the following transitions, which one has higher frequency
Answer$3-1$ transition has higher energy so it has higher frequency$\left(v=\frac{E}{h}\right)$
View full question & answer→MCQ 51 Mark
Energy of an electron in an excited hydrogen atom is $-3.4 eV$. Its angular momentum will be: $h=6.626 \times 10^{-34} J -s$
- A
$1.11 \times 10^{34} J sec$
- B
$1.51 \times 10^{-31} J sec$
- ✓
$2.11 \times 10^{-34} J sec$
- D
$3.72 \times 10^{-34} J sec$
AnswerCorrect option: C. $2.11 \times 10^{-34} J sec$
The electron is in the second orbit $(n=2)$
Hence $L=\frac{n h}{2 \pi}=\frac{2 h}{2 \pi}=\frac{6.6 \times 10^{-34}}{\pi}=2.11 \times 10^{-34} \mathrm{~J}-\mathrm{sec}$
View full question & answer→MCQ 61 Mark
Which of the following statements are true regarding Bohr's model of hydrogen atom$(1)$ Orbiting speed of electron decreases as it shifts to discrete orbits away from the nucleus$(11)$ Radii of allowed orbits of electron are proportional to the principal quantum number$(111)$ Frequency with which electrons orbits around the nucleus in discrete orbits is inversely proportional to the principal quantum number $(IV)$ Binding force with which the electron is bound to the nucleus increases as it shifts to outer orbits Select correct answer using the codes given below Codes :
- ✓
$1$ and $111$
- B
$11$ and $1 V$
- C
$1, 11$ and $111$
- D
$11, 111$ and $1 V$
AnswerCorrect option: A. $1$ and $111$
Orbital speed varies inversely as the radius of the orbit. Energy increases with the increase in quantum number.
View full question & answer→MCQ 71 Mark
Who discovered spin quantum number
View full question & answer→MCQ 81 Mark
What will be the angular momentum of a electron, if energy of this electron in $H$-atom is $1.5 eV$ (in $/$-sec) $\quad$
- A
$1.05 \times 10^{-34}$
- B
$2.1 \times 10^{-34}$
- ✓
$3.15 \times 10^{-34}$
- D
$-2.1 \times 10^{-34}$
AnswerCorrect option: C. $3.15 \times 10^{-34}$
Energy of electron in $H$ atom $E_n=\frac{-13.6}{n^2} \mathrm{eV}$
$\Rightarrow-1.5=\frac{-13.6}{n^2} \Rightarrow n^2=\frac{13.6}{1.5}=3$
Now angular momentum$p=n \frac{h}{2 \pi}=\frac{3 \times 6.6 \times 10^{-34}}{2 \times 3.14}=3.15 \times 10^{-34} \mathrm{~J} \times \mathrm{sec}$
View full question & answer→MCQ 91 Mark
If $\lambda_{\text {max }}$ is $6563 \mathring A$, then wave length of second line for Balmer series will be
- ✓
$\lambda=\frac{16}{3 R}$
- B
$\lambda=\frac{36}{5 R}$
- C
$\lambda=\frac{4}{3 R}$
- D
AnswerCorrect option: A. $\lambda=\frac{16}{3 R}$
For Balmer series $\frac{1}{\lambda}=R\left(\frac{1}{2^2}-\frac{1}{n^2}\right)$ where $n=3,4,5$
For second line $n=4$
So $\frac{1}{\lambda}=R\left(\frac{1}{2^2}-\frac{1}{4^2}\right)=\frac{3}{16} R \Rightarrow \lambda=\frac{16}{3 R}$
View full question & answer→MCQ 101 Mark
If scattering particles are $56$ for $90^{\circ}$ angle then this will be at $60^{\circ}$ angle
AnswerAccording to scattering formula
$ N \propto \frac{1}{\sin ^4(\theta / 2)} \Rightarrow \frac{N_2}{N_1}=\left[\frac{\sin \left(\theta_1 / 2\right)}{\sin \left(\theta_2 / 2\right)}\right]^4$
$\Rightarrow \frac{N_2}{N_1}=\left[\frac{\sin \frac{90^{\circ}}{2}}{\sin \frac{60^{\circ}}{2}}\right]^4=\left[\frac{\sin 45^{\circ}}{\sin 30^{\circ}}\right]^4 $
$\Rightarrow N_2=(\sqrt{2})^4 \times N_1=4 \times 56=224$
View full question & answer→MCQ 111 Mark
Which one of the series of hydrogen spectrum is in the visible region
AnswerBalmer series lies in the visible region.
View full question & answer→MCQ 121 Mark
lonization energy of hydrogen is $13.6\ eV$. If $h=6.6 \times 10^{-34} J - sec$, the value of $R$ will be of the order of
- A
$10^{10} m ^{-1}$
- ✓
$10^7 m ^{-1}$
- C
$10^4 m ^{-1}$
- D
$10^{-7} m ^{-1}$
AnswerCorrect option: B. $10^7 m ^{-1}$
$ E=-R c h \Rightarrow R=-\frac{E}{c h}=-\frac{13.6 \times 1.6 \times 10^{-19}}{3 \times 10^8 \times 6.6 \times 10^{-34}} $
$ =1.098 \times 10^7 \text { per } m$
View full question & answer→MCQ 131 Mark
The first line of Balmer series has wavelength $6563 \mathring A$. What will be the wavelength of the first member of Lyman series
- ✓
$1215.4 \mathring A$
- B
$2500 \mathring A$
- C
$7500 \mathring A$
- D
$600 \mathring A$
AnswerCorrect option: A. $1215.4 \mathring A$
$ \frac{1}{\lambda_{\text {Balmer }}}=R\left[\frac{1}{2^2}-\frac{1}{3^2}\right]=\frac{5 R}{36}, \frac{1}{\lambda_{\text {Lyman }}}=R\left[\frac{1}{1^2}-\frac{1}{2^2}\right]=\frac{3 R}{4} $
$ \therefore \lambda_{\text {Lyman }}=\lambda_{\text {Balmer }} \times \frac{5}{27}=1215.4 \mathring A$
View full question & answer→MCQ 141 Mark
With the increase in principle quantum number, the energy difference between the two successive energy levels
- A
- ✓
- C
- D
Sometimes increases and sometimes decreases
View full question & answer→MCQ 151 Mark
When the wave of hydrogen atom comes from infinity into the first orbit then the value of wave number is
- ✓
$109700 cm$
- B
$1097 cm$
- C
$109 cm$
- D
AnswerCorrect option: A. $109700 cm$
$ \text { Wave number } \bar{v}=\frac{1}{\lambda}=R\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right] ; n_2=\infty \quad \text { and } n_1=1 $
$ \Rightarrow \bar{v}=R=1.097 \times 10^7 \mathrm{~m}^{-1}=109700 \mathrm{~cm}^{-1}$
View full question & answer→MCQ 161 Mark
Which of the following is true for number of spectral lines in going form Layman series to Pfund series
- A
- ✓
- C
- D
May decreases or increases
AnswerMaximum number of spectral lines are observed in Lymen series.
View full question & answer→MCQ 171 Mark
Orbital acceleration of electron is
- ✓
$\frac{n^2 h^2}{4 \pi^2 m^2 r^3}$
- B
$\frac{n^2 h^2}{2 n^2 r^3}$
- C
$\frac{4 n^2 h^2}{\pi^2 m^2 r^3}$
- D
$\frac{4 n^2 h^2}{4 \pi^2 m^2 r^3}$
AnswerCorrect option: A. $\frac{n^2 h^2}{4 \pi^2 m^2 r^3}$
$m v r=\frac{n h}{2 \pi} \Rightarrow v=\frac{n h}{2 \pi m r} \Rightarrow \frac{v^2}{r}=\frac{n^2 h^2}{4 \pi^2 m^2 r^3}$.
View full question & answer→MCQ 181 Mark
Energy of electron in a orbit of $H-$atom is
Answer$E_n=-\frac{13.6}{n^2} \mathrm{eV}$
View full question & answer→MCQ 191 Mark
The energy of electron in first excited state of $H-$atom is $-3.4 eV$ its kinetic energy is
- A
$-3.4 eV$
- ✓
$+3.4 eV$
- C
$-6.8 eV$
- D
$6.8 eV$
AnswerCorrect option: B. $+3.4 eV$
Kinetic energy $=\mid$ Total energy $\mid$
View full question & answer→MCQ 201 Mark
For electron moving in $n$ orbit of $H$-atom the angular velocity is proportional to
- A
$n/1$
- B
$1 / n$
- C
$n$
- ✓
$1 / n$
AnswerCorrect option: D. $1 / n$
View full question & answer→MCQ 211 Mark
The third line of Balmer series of an ion equivalent to hydrogen atom has wavelength of $108.5 nm$. The ground state energy of an electron of this ion will be
- A
$3.4 eV$
- B
$13.6 eV$
- ✓
$54.4 eV$
- D
$122.4 eV$
AnswerCorrect option: C. $54.4 eV$
For third line of Balmer series $n_1=2, n_2=5$
$\therefore \frac{1}{\lambda}=R Z^2\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right]$ gives $Z^2=\frac{n_1^2 n_2^2}{\left(n_2^2-n_1^2\right) \lambda R}$
On putting values $Z=2$From $E=-\frac{13.6 Z^2}{n^2}=\frac{-13.6(2)^2}{(1)^2}=-54.4 \mathrm{eV}$
View full question & answer→MCQ 221 Mark
The extreme wavelengths of Paschen series are
- A
$0.365 \mu m$ and $0.565 \mu m$
- ✓
$0.818 \mu m$ and $1.89 \mu m$
- C
$1.45 \mu m$ and $4.04 \mu m$
- D
$2.27 \mu m$ and $7.43 \mu m$
AnswerCorrect option: B. $0.818 \mu m$ and $1.89 \mu m$
Similarly $\lambda_{\min }=\frac{9}{R}=\frac{9}{1.1 \times 10^7}=0.818 \mu \mathrm{m}$
$ \text { In Paschen series } \frac{1}{\lambda_{\max }}=R\left[\frac{1}{(3)^2}-\frac{1}{(4)^2}\right]$
$ \Rightarrow \lambda_{\max }=\frac{144}{7 R}=\frac{144}{7 \times 1.1 \times 10^7}=1.89 \times 10^{-6} \mathrm{~m}=1.89 \mu \mathrm{m}$
View full question & answer→MCQ 231 Mark
An ionic atom equivalent to hydrogen atom has wavelength equal to $1 / 4$ of the wavelengths of hydrogen lines. The ion will be
- ✓
$He ^{+}$
- B
$Li ^{++}$
- C
$Ne e^{9+}$
- D
$Na a^{10+}$
AnswerCorrect option: A. $He ^{+}$
$\bar{v} \propto \frac{1}{\lambda} \propto Z^2 \Rightarrow \lambda Z^2=$ constant $\Rightarrow \lambda=\frac{\lambda}{4} Z^2 \Rightarrow Z=2$
View full question & answer→MCQ 241 Mark
Which of the following spectral series in hydrogen atom give spectral line of $4860 \mathring A$
View full question & answer→MCQ 251 Mark
The ratio of the kinetic energy to the total energy of an electron in a Bohr orbit is
View full question & answer→MCQ 261 Mark
The angular momentum of electron in $\pi$ orbit is given by
- A
$n h$
- B
$\frac{h}{2 \pi n}$
- ✓
$n \frac{h}{2 \pi}$
- D
$n^2 \frac{h}{2 \pi}$
AnswerCorrect option: C. $n \frac{h}{2 \pi}$
According to Bohr's second postulate.
View full question & answer→MCQ 271 Mark
Taking Rydberg's constant $R_H=1.097 \times 10^7 m$ first and second wavelength of Balmer series in hydrogen spectrum is
- A
$2000 \mathring A, 3000\mathring A$
- B
$1575 \mathring A, 2960 \mathring A$
- C
$6529 \mathring A, 4280 \mathring A$
- ✓
$6563 \mathring A, 4861 \mathring A$
AnswerCorrect option: D. $6563 \mathring A, 4861 \mathring A$
$\frac{1}{\lambda}=R\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right]$.
For first wavelength, $n_1=2, n_2=3$
$\Rightarrow \lambda_1=6563 \mathring A$.
For second wavelength, $n_1=2, n_2=4$
$\Rightarrow \lambda_2=4861 \mathring A$
View full question & answer→MCQ 281 Mark
The wavelength of light emitted from second orbit to first orbits in a hydrogen atom is
- ✓
$1.215 \times 10^{-7} m$
- B
$1.215 \times 10^{-5} m$
- C
$1.215 \times 10^{-4} m$
- D
$1.215 \times 10^{-3} m$
AnswerCorrect option: A. $1.215 \times 10^{-7} m$
Energy radiated $E=10.2 \mathrm{eV}=10.2 \times 1.6 \times 10^{-19} \mathrm{~J}$
$\Rightarrow E=\frac{h c}{\lambda} \Rightarrow \lambda=1.215 \times 10^{-7} \mathrm{~m}$
View full question & answer→MCQ 291 Mark
An electron jumps from $5^*$ orbit to $4^*$ orbit of hydrogen atom. Taking the Rydberg constant as $10^7$ per metre. What will be the frequency of radiation emitted
- A
$6.75 \times 10^{12} Hz$
- B
$6.75 \times 10^{14} Hz$
- ✓
$6.75 \times 10^{13} Hz$
- D
AnswerCorrect option: C. $6.75 \times 10^{13} Hz$
$ \text { By using } v=R C\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right]$
$ \Rightarrow v=10^7 \times\left(3 \times 10^8\right)\left[\frac{1}{4^2}-\frac{1}{5^2}\right]=6.75 \times 10^{13} \mathrm{Hz}$
View full question & answer→MCQ 301 Mark
In a hydrogen atom, the distance between the electron and proton is $2.5 \times 10^{-11} m$. The electrical force of attraction between them will be
- A
$2.8 \times 10^{-7} N$
- ✓
$3.7 \times 10^{-7} N$
- C
$6.2 \times 10^{-7} N$
- D
$9.1 \times 10^{-7} N$
AnswerCorrect option: B. $3.7 \times 10^{-7} N$
$F=\frac{9 \times 10^9 \times 1.6 \times 10^{-19} \times 1.6 \times 10^{-19}}{\left(2.5 \times 10^{-11}\right)^2}=3.7 \times 10^{-7} \mathrm{~N}$
View full question & answer→MCQ 311 Mark
The concept of stationary orbits was proposed by
View full question & answer→MCQ 321 Mark
The energy required to excite an electron from the ground state of hydrogen atom to the first excited state, is
- A
$1.602 \times 10^{-14} J$
- B
$1.619 \times 10^{-16} J$
- ✓
$1.632 \times 10^{-18} J$
- D
$1.656 \times 10^{-20} J$
AnswerCorrect option: C. $1.632 \times 10^{-18} J$
View full question & answer→MCQ 331 Mark
The energy of electron in the $n$th orbit of hydrogen atom is expressed as $E_n-\frac{e V}{n}$. The shortest and longest wavelength of Lyman series will be
- ✓
$910 \mathring A, 1213 \mathring A$
- B
$5463 \mathring A, 7858 \mathring A$
- C
$1315 \mathring A, 1530 \mathring A$
- D
AnswerCorrect option: A. $910 \mathring A, 1213 \mathring A$
$ \frac{1}{\lambda_{\max }}=R\left[\frac{1}{(1)^2}-\frac{1}{(2)^2}\right] \Rightarrow \lambda_{\max }=\frac{4}{3 R} \approx 1213 \mathring A $
$ \text { and } \frac{1}{\lambda_{\min }}=R\left[\frac{1}{(1)^2}-\frac{1}{\infty}\right] \Rightarrow \lambda_{\min }=\frac{1}{R} \approx 910 \mathring A$
View full question & answer→MCQ 341 Mark
The kinetic energy of electron in the first Bohr orbit of the hydrogen atom is
- A
$-6.5 eV$
- B
$-27.2 eV$
- ✓
$13.6 eV$
- D
$-13.6 eV$
AnswerCorrect option: C. $13.6 eV$
K.E. $=-($ Total energy $)=-(-13.6 \mathrm{eV})=+13.6 \mathrm{eV}$
View full question & answer→MCQ 351 Mark
The ionisation potential of hydrogen atom is $13.6$ volt. The energy required to remove an electron in the $n=2$ state of the hydrogen atom is
- A
$27.2 eV$
- B
$13.6 eV$
- C
$6.8 eV$
- ✓
$3.4 eV$
AnswerCorrect option: D. $3.4 eV$
Energy required to remove electron in the $n=2$ state $=+\frac{13.6}{(2)^2}=+3.4 \mathrm{eV}$
View full question & answer→MCQ 361 Mark
If $m$ is mass of electron, $v$ its velocity, $r$ the radius of stationary circular orbit around a nucleus with charge $Z e$, then from Bohr's first postulate, the kinetic energy $K=\frac{1}{2} m v^2$ of the electron in C.G.S. system is equal to
AnswerCorrect option: A. $\frac{1}{2} \frac{Z e^2}{r}$

in the revolution of electron, coulomb force provide the necessry centripetal force
$\Rightarrow \frac{z e^2}{r^2}=\frac{m v^2}{r} \Rightarrow m v^2=\frac{z e^2}{r}$
$\therefore \text { K.E. }=\frac{1}{2} m v^2=\frac{z e^2}{2 r}$ View full question & answer→MCQ 371 Mark
The wavelength of the first line of Balmer series is $6563 \mathring A$. The Rydberg constant for hydrogen is about
- ✓
(a) $1.09 \times 10^7$ per $m$
- B
(b) $1.09 \times 10^8$ per m
- C
(c) $1.09 \times 10^9$ per m
- D
(d) $1.09 \times 10^5$ per m
AnswerCorrect option: A. (a) $1.09 \times 10^7$ per $m$
$ \frac{1}{\lambda}=R\left[\frac{1}{4}-\frac{1}{9}\right]=\frac{5 R}{36} $
$ \therefore R=\frac{36}{5 \lambda}=\frac{36}{5 \times 6563 \times 10^{-10}}=1.09 \times 10^7 \mathrm{~m}^{-1}$
View full question & answer→MCQ 381 Mark
The Rydberg constant $R$ for hydrogen is
- A
$R=-\left(\frac{1}{4 \pi \varepsilon_0}\right) \cdot \frac{2 \pi^2 m e^2}{c h^2}$
- B
$R=\left(\frac{1}{4 \pi \varepsilon_0}\right) \cdot \frac{2 \pi^2 m e^4}{c h^2}$
- C
$R=\left(\frac{1}{4 \pi \varepsilon_0}\right)^2 \cdot \frac{2 \pi^2 m e^4}{c^2 h^2}$
- ✓
$R=\left(\frac{1}{4 \pi \varepsilon_0}\right)^2 \cdot \frac{2 \pi^2 m e^4}{c h^3}$
AnswerCorrect option: D. $R=\left(\frac{1}{4 \pi \varepsilon_0}\right)^2 \cdot \frac{2 \pi^2 m e^4}{c h^3}$
$ R=\frac{2 \pi^2 k^2 e^4 m}{c h^3}=\left(\frac{1}{4 \pi \varepsilon_0}\right)^2 \frac{2 \pi^2 m e^4}{c h^3}$
View full question & answer→MCQ 391 Mark
The shortest wavelength in the Lyman series of hydrogen spectrum is $912 \mathring A$ corresponding to a photon energy of $13.6 eV$. The shortest wavelength in the Balmer series is about
- ✓
$3648 \mathring A$
- B
$8208 \mathring A$
- C
$1228 \mathring A$
- D
$6566 \mathring A$
AnswerCorrect option: A. $3648 \mathring A$
In Lyman series $\left(\lambda_{\min }\right)_L=\frac{1}{R}$ and $\left(\lambda_{\min }\right)_B=\frac{4}{R}$
$\Rightarrow\left(\lambda_{\min }\right)_B=4 \times\left(\lambda_{\min }\right)_L=4 \times 912=3648 \mathring A$
View full question & answer→MCQ 401 Mark
Which of the following is quantised according to Bohr's theory of hydrogen atom
- A
Linear momentum of electron
- ✓
Angular momentum of electron
- C
Linear velocity of electron
- D
Angular velocity of electron
AnswerCorrect option: B. Angular momentum of electron
View full question & answer→MCQ 411 Mark
An electron in the $n=1$ orbit of hydrogen atom is bound by $13.6 eV$ energy is required to ionize it is
- ✓
$13.6 eV$
- B
$6.53 eV$
- C
$5.4 eV$
- D
$1.51 eV$
AnswerCorrect option: A. $13.6 eV$
lonization energy $=$ Binding energy.
View full question & answer→MCQ 421 Mark
The possible quantum number for $3 d$ electron are
- A
$n=3, l=1, m_l=+1, m_s=-\frac{1}{2}$
- ✓
$n=3, l=2, m_l=+2, m_s=-\frac{1}{2}$
- C
$n=3, l=1, m_l=-1, m_s=+\frac{1}{2}$
- D
$n=3, l=0, m_l=+1, m_s=-\frac{1}{2}$
AnswerCorrect option: B. $n=3, l=2, m_l=+2, m_s=-\frac{1}{2}$
View full question & answer→MCQ 431 Mark
When the electron in the hydrogen atom jumps from $2^{-}$orbit to $1^{-}$ orbit, the wavelength of radiation emitted is $\lambda$. When the electrons jump from 3 orbit to 1 orbit, the wavelength of emitted radiation would be
- ✓
$\frac{27}{32} \lambda$
- B
$\frac{32}{27} \lambda$
- C
$\frac{2}{3} \lambda$
- D
$\frac{3}{2} \lambda$
AnswerCorrect option: A. $\frac{27}{32} \lambda$
$\frac{1}{\lambda}=R\left[\frac{1}{n_1^2}-\frac{1}{n_2^2}\right]$
First condition $\frac{1}{\lambda}=R\left[\frac{1}{1^2}-\frac{1}{2^2}\right] \Rightarrow R=\frac{4}{3 \lambda}$
Second condition $\frac{1}{\lambda^{\prime}}=R\left[\frac{1}{1^2}-\frac{1}{3^2}\right]$
$\Rightarrow \lambda^{\prime}=\frac{9}{8 R} \Rightarrow \lambda^{\prime}=\frac{9}{8 \times \frac{4}{3 \lambda}}=\frac{27 \lambda}{32}$
View full question & answer→MCQ 441 Mark
Four lowest energy levels of $H$-atom are shown in the figure. The number of possible emission lines would be
AnswerNumber of possible emission lines $=\frac{n(n-1)}{2}$
Where $n=4$; Number $=\frac{4(4-1)}{2}=6$.
View full question & answer→MCQ 451 Mark
The ratio of the speed of the electron in the first Bohr orbit of hydrogen and the speed of light is equal to (where $e, h$ and $c$ have their usual meanings)
- A
$2 \pi h c / e^2$
- B
$e^2 h / 2 \pi c$
- C
$e^2 c / 2 \pi h$
- ✓
$2 \pi e^2 / h c$
AnswerCorrect option: D. $2 \pi e^2 / h c$
Speed of electron in $n$ orbit (in CGS)$v_n=\frac{2 \pi Z e^2}{n h}(k=1)$
For first orbit $H_2 ; n=1$ and $Z=1$
So $v=\frac{2 \pi e^2}{h} \Rightarrow \frac{v}{c}=\frac{2 \pi e^2}{h c}$
View full question & answer→MCQ 461 Mark
The radius of the Bohr orbit in the ground state of hydrogen atom is $0.5 \mathring A$. The radius of the orbit of the electron in the third excited state of $He ^{+}$will be
- ✓
$8 \mathring A$
- B
$4 \mathring A$
- C
$0.5 \mathring A$
- D
$0.25 \mathring A$
AnswerCorrect option: A. $8 \mathring A$
$8 \mathring A$
View full question & answer→MCQ 471 Mark
If the ionisation potential of helium atom is $24.6$ volt, the energy required to ionise it will be
- ✓
$24.6\ eV$
- B
$24.6\ V$
- C
$13.6\ V$
- D
$13.6\ eV$
AnswerCorrect option: A. $24.6\ eV$
Energy required to ionise helium atom $=24.6\ \mathrm{eV}$
View full question & answer→MCQ 481 Mark
In terms of Rydberg's constant $R$, the wave number of the first Balmer line is
- A
$R$
- B
$3 R$
- ✓
$\frac{5 R}{36}$
- D
$\frac{8 R}{9}$
AnswerCorrect option: C. $\frac{5 R}{36}$
Wave number$=\frac{1}{\lambda}=R\left(\frac{1}{n_1^2}-\frac{1}{n_2^2}\right)$For first Balmer line $n=2, n=3$
$\therefore \text { Wave number }=R\left(\frac{1}{2^2}-\frac{1}{3^2}\right)=R\left(\frac{9-4}{9 \times 4}\right)=\frac{5 R}{36}$
View full question & answer→MCQ 491 Mark
Which of the following statements about the Bohr model of the hydrogen atom is false
- ✓
Acceleration of electron in $n=2$ orbit is less than that in $n=1$ orbit
- B
Angular momentum of electron in $n=2$ orbit is more than that in $n=1$ orbit
- C
Kinetic energy of electron in $n=2$ orbit is less than that in $n= 1$ orbit
- D
Potential energy of electron in $n=2$ orbit is less than that in $n$ $=1$ orbit
AnswerCorrect option: A. Acceleration of electron in $n=2$ orbit is less than that in $n=1$ orbit
Potential energy of electron in $n=2$ orbit is less than that in $n$ $=1$ orbit
View full question & answer→MCQ 501 Mark
An electron in the $n=1$ orbit of hydrogen atom is bound by $13.6 eV$. If a hydrogen atom is in the $n=3$ state, how much energy is required to ionize it
- A
$13.6\ eV$
- B
$4.53\ eV$
- C
$3.4\ eV$
- ✓
$1.51\ eV$
AnswerCorrect option: D. $1.51\ eV$
Required energy $E_3=\frac{+13.6}{3^2}=1.51 \mathrm{eV}$
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