Structure of Atom Practice
Take 5 chapter-wise practice tests of 25 questions each on Structure of Atom for NEET with +4/-1 scoring, answer review, and concise explanations.
Take 5 chapter-wise practice tests of 25 questions each on Structure of Atom for NEET with +4/-1 scoring, answer review, and concise explanations.
5 original practice tests, 25 questions each, NEET 4/-1 marking, and answer review after submission.
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1. The particle carrying a positive charge in the atom is:
Explanation: Protons are positively charged and present in the nucleus.
2. Atomic number represents the number of:
Explanation: Atomic number uniquely identifies the element.
3. Mass number is equal to:
Explanation: It counts total nucleons in the nucleus.
4. In a neutral atom, number of electrons equals:
Explanation: Neutrality requires total positive and negative charges to match.
5. Cathode rays are streams of:
Explanation: J.J. Thomson established the electron through cathode ray experiments.
6. Canal rays mainly helped in the discovery of:
Explanation: Positive rays pointed to positively charged subatomic particles.
7. In Thomson's atomic model, electrons were embedded in a sphere of:
Explanation: It is the 'plum pudding' model.
8. Most alpha particles passed undeviated through gold foil because atoms are mostly:
Explanation: Rutherford concluded most atomic volume is empty.
9. The dense central core of the atom was called:
Explanation: Rutherford proposed a small dense positively charged nucleus.
10. Rutherford's model could not explain:
Explanation: Classical electrodynamics predicted orbiting electrons would lose energy.
11. Speed of electromagnetic radiation in vacuum is:
Explanation: That is the speed of light in vacuum.
12. The relation between wavelength and frequency is:
Explanation: Wave speed equals wavelength times frequency.
13. Energy of a photon is:
Explanation: Planck related energy to frequency using Planck constant.
14. Photoelectric effect supports the particle nature of light because it shows:
Explanation: Emission occurs only when photons have sufficient threshold energy.
15. Bohr proposed that electrons revolve only in:
Explanation: Only selected orbits were allowed without energy loss.
16. Angular momentum of electron in Bohr orbit is quantized as:
Explanation: This is Bohr's quantization condition.
17. Bohr model successfully explained the spectrum of:
Explanation: It worked best for one-electron species.
18. Which is a one-electron species?
Explanation: Singly ionised helium has only one electron.
19. Bohr model is applicable to:
Explanation: Any one-electron species can be treated similarly.
20. The main limitation of Rutherford model was that it did not address:
Explanation: The model lacked a stability mechanism.
21. Line spectra arise because atomic energies are:
Explanation: Only specific transitions are allowed.
22. Higher frequency radiation has:
Explanation: $E=h\nu$, so energy increases with frequency.
23. Shorter wavelength corresponds to:
Explanation: Since $c$ is constant, smaller wavelength means larger frequency.
24. The nucleus occupies only a very small fraction of atomic volume, so the atom is considered:
Explanation: That was the key Rutherford conclusion.
25. The historical sequence best supported by experiments is:
Explanation: Atomic models evolved with new experimental evidence.
26. The radius of the first Bohr orbit of hydrogen is denoted by:
Explanation: $a_0$ is the Bohr radius.
27. Radius of nth orbit in hydrogen-like species varies as:
Explanation: Bohr radius formula scales this way.
28. Energy of nth orbit in hydrogen is proportional to:
Explanation: Bohr energies become less negative with increasing n.
29. Ground state of hydrogen corresponds to:
Explanation: The lowest allowed orbit is the ground state.
30. Any state with n greater than 1 is called:
Explanation: Its energy is higher than the ground state.
31. When an electron jumps from higher to lower orbit, it:
Explanation: Downward transition releases a photon.
32. When an electron jumps from lower to higher orbit, it:
Explanation: Energy must be supplied for excitation.
33. Ionisation energy of hydrogen from ground state is:
Explanation: Removing the electron from n = 1 to n = infinity needs 13.6 eV.
34. Energy required to excite hydrogen from n = 1 to n = 2 is:
Explanation: Difference between -13.6 eV and -3.4 eV is 10.2 eV.
35. The Lyman series lies in the:
Explanation: These transitions end at n = 1.
36. The Balmer series lies in the:
Explanation: Balmer lines correspond to transitions ending at n = 2.
37. Paschen series corresponds to transitions ending at:
Explanation: Paschen lines lie in the infrared region.
38. The Rydberg equation is used to calculate:
Explanation: It predicts hydrogen spectral wavelengths.
39. For $He^+$, the energy of first orbit is:
Explanation: Energy scales as $-13.6Z^2/n^2$ and here Z = 2.
40. Ionisation energy of $Li^{2+}$ from ground state is:
Explanation: For Z = 3, ionisation energy is 13.6 × 9.
41. Maximum wavelength in Balmer series corresponds to transition:
Explanation: Smallest energy gap in a series gives the longest wavelength.
42. Minimum wavelength in Lyman series corresponds to transition:
Explanation: Largest energy drop in the series gives shortest wavelength.
43. As n increases in hydrogen atom, orbit radius:
Explanation: Radius varies as $n^2$.
44. As n increases, electron energy becomes:
Explanation: The electron moves toward ionisation with increasing n.
45. Electron velocity in Bohr model varies with:
Explanation: Velocity decreases with higher n and increases with nuclear charge.
46. Emission spectrum is produced when electrons:
Explanation: These transitions emit photons of specific wavelengths.
47. Absorption lines arise when atoms:
Explanation: Only energies matching allowed gaps are absorbed.
48. Which series has the lowest-energy photons?
Explanation: Transitions ending at n = 3 involve smaller energy gaps than Lyman or Balmer.
49. In Bohr model, angular momentum is quantized, so allowed electron paths are:
Explanation: Only selected states satisfy the quantization condition.
50. The Bohr model's biggest success was explaining:
Explanation: It correctly predicted line energies for one-electron atoms.
51. de Broglie proposed that moving particles have associated:
Explanation: Matter waves were proposed for particles in motion.
52. The de Broglie wavelength is:
Explanation: Momentum and wavelength are inversely related.
53. A particle with larger momentum has:
Explanation: Since $\lambda=h/p$, wavelength decreases as momentum rises.
54. It is impossible to determine simultaneously the exact position and exact:
Explanation: This is Heisenberg's uncertainty principle.
55. Uncertainty principle mainly becomes important for:
Explanation: Quantum effects matter at very small scales.
56. Schrodinger's equation gives information about:
Explanation: It forms the basis of quantum mechanical model.
57. The square of wave function gives:
Explanation: $\psi^2$ gives the likelihood of finding the electron.
58. An orbital is a region in space where the probability of finding an electron is:
Explanation: It replaces the old fixed-orbit picture.
59. The principal quantum number is represented by:
Explanation: It largely decides size and energy level.
60. The azimuthal quantum number is represented by:
Explanation: It determines subshell and orbital shape.
61. The magnetic quantum number is represented by:
Explanation: It indicates orientation of orbital.
62. Spin quantum number can have values:
Explanation: Electron spin has two allowed orientations.
63. For n = 3, the allowed values of l are:
Explanation: l ranges from 0 to n - 1.
64. Number of orbitals in a subshell is:
Explanation: Each subshell contains these many orbitals.
65. Number of orbitals in p-subshell is:
Explanation: For p, l = 1, so 2l+1 = 3.
66. Number of orbitals in d-subshell is:
Explanation: For d, l = 2, so there are 5 orbitals.
67. Maximum number of electrons in an orbital is:
Explanation: Pauli exclusion principle allows at most two with opposite spins.
68. Maximum number of electrons in p-subshell is:
Explanation: Three p orbitals hold 6 electrons.
69. Maximum number of electrons in n = 3 shell is:
Explanation: Shell capacity is $2n^2$.
70. s-orbitals are generally:
Explanation: s-orbitals are spherically symmetric.
71. p-orbitals are generally:
Explanation: Each p orbital has two lobes.
72. Total number of nodes in an orbital is:
Explanation: Total nodes are sum of radial and angular nodes.
73. Number of angular nodes equals:
Explanation: Angular node count depends only on azimuthal quantum number.
74. Number of radial nodes equals:
Explanation: This is the standard formula.
75. Quantum mechanics replaced fixed Bohr orbits with:
Explanation: Electron location is treated probabilistically, not as a fixed path.
76. Electrons fill orbitals in order of:
Explanation: Lower-energy orbitals are filled first.
77. According to n+l rule, lower value of n+l means:
Explanation: This rule is used to predict filling order.
78. Between 4s and 3d, the lower energy orbital during filling is:
Explanation: Because 4s has lower n+l value than 3d.
79. No two electrons in an atom can have the same set of:
Explanation: This is Pauli exclusion principle.
80. Hund's rule says electrons in degenerate orbitals occupy them:
Explanation: This maximizes multiplicity and lowers repulsion.
81. Electronic configuration of oxygen (Z = 8) is:
Explanation: Eight electrons fill in this order.
82. Electronic configuration of sodium (Z = 11) is:
Explanation: The eleventh electron enters 3s.
83. Electronic configuration of chromium is exceptional because it is:
Explanation: Half-filled d-subshell offers extra stability.
84. Electronic configuration of copper is exceptional because it is:
Explanation: Completely filled d-subshell gives additional stability.
85. Valence electrons are electrons in the:
Explanation: They largely determine chemical behavior.
86. Nitrogen (Z = 7) has number of unpaired electrons equal to:
Explanation: Configuration $1s^22s^22p^3$ places one electron in each p orbital.
87. Oxygen (Z = 8) has number of unpaired electrons equal to:
Explanation: In $2p^4$, one pair forms and two electrons remain unpaired.
88. The number of unpaired electrons in $Fe^{3+}$ is:
Explanation: Fe is [Ar]3d$^6$4s$^2$; Fe$^{3+}$ becomes [Ar]3d$^5$.
89. The number of unpaired electrons in $Cu^{2+}$ is:
Explanation: Cu is [Ar]3d$^{10}$4s$^1$; Cu$^{2+}$ becomes [Ar]3d$^9$.
90. A species with one or more unpaired electrons is:
Explanation: Unpaired electrons cause attraction in a magnetic field.
91. A species with all electrons paired is:
Explanation: All paired electrons cancel magnetic moments.
92. For a 3p electron, n and l are respectively:
Explanation: p-subshell corresponds to l = 1.
93. For a 4d electron, allowed m values are:
Explanation: For d, l = 2 and m ranges from -l to +l.
94. Maximum number of electrons in 4th shell is:
Explanation: Use $2n^2$ with n = 4.
95. Maximum number of electrons in f-subshell is:
Explanation: Seven orbitals each holding two electrons give 14.
96. The correct filling order among these is:
Explanation: This follows increasing orbital energy.
97. When transition metals form cations, electrons are generally removed first from:
Explanation: Though 4s fills before 3d, it is removed first during ionisation.
98. Chromium and copper are exceptions mainly because half-filled or fully filled subshells are:
Explanation: Extra stability comes from symmetry and exchange energy.
99. Hund rule mainly helps predict:
Explanation: It determines how electrons occupy equal-energy orbitals.
100. Electronic configuration acts as the bridge between atomic structure and:
Explanation: Outer-electron arrangement controls chemical behavior.
101. Which quantum number determines the size of orbital?
Explanation: Higher n usually means larger orbital size.
102. Which quantum number determines the shape of orbital?
Explanation: l determines whether the orbital is s, p, d, or f.
103. Which quantum number determines orientation in space?
Explanation: m differentiates orbitals of same subshell.
104. For n = 4, total number of orbitals in the shell is:
Explanation: Total orbitals in a shell = n$^2$.
105. For n = 3, total number of orbitals is:
Explanation: n$^2$ gives total orbital count.
106. An orbital with n = 3 and l = 2 is:
Explanation: l = 2 corresponds to d-subshell.
107. An orbital with n = 2 and l = 0 is:
Explanation: l = 0 denotes s-subshell.
108. Number of radial nodes in 3p orbital is:
Explanation: n - l - 1 = 3 - 1 - 1 = 1.
109. Number of angular nodes in 4d orbital is:
Explanation: Angular nodes equal l, and for d, l = 2.
110. Total nodes in 4s orbital are:
Explanation: Total nodes = n - 1 = 3.
111. Species $Ne$ is:
Explanation: All electrons are paired in neon.
112. Species $O_2^-$ has unpaired electrons and is therefore:
Explanation: Adding one electron to oxygen molecule still leaves one unpaired electron.
113. Emission spectrum appears as:
Explanation: Emission occurs when excited atoms release light.
114. Absorption spectrum appears as:
Explanation: Certain wavelengths are absorbed from a continuous source.
115. Electron diffraction is evidence for:
Explanation: Diffraction is a wave property.
116. Greater certainty in position implies:
Explanation: This is the trade-off in uncertainty principle.
117. Among 3s, 3p, and 3d orbitals of a multi-electron atom, increasing energy order is:
Explanation: Within the same shell, energy increases with l for multi-electron atoms.
118. Among 4s and 3d orbitals during filling, the lower energy is usually:
Explanation: n+l rule places 4s below 3d during filling.
119. For hydrogen atom, energy depends only on:
Explanation: All orbitals with same n are degenerate in hydrogen.
120. In multi-electron atoms, orbitals of same n have different energies because of:
Explanation: Electron-electron repulsion breaks the hydrogen-like degeneracy.
121. Threshold frequency in photoelectric effect means:
Explanation: Below threshold, photons lack sufficient energy.
122. Increasing intensity of light below threshold frequency does not eject electrons because:
Explanation: Photon energy depends on frequency, not intensity.
123. An orbital and an orbit differ because an orbital is:
Explanation: Orbit is a Bohr path, orbital is a quantum mechanical region.
124. The set of quantum numbers not allowed for an electron is:
Explanation: For n = 2, l can only be 0 or 1.
125. Atomic structure becomes NEET-friendly when you connect models, spectra, orbitals, and configurations through:
Explanation: That single framework ties together the chapter.