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Introduction

The evolution of atomic models unfolds a compelling narrative in scientific history. Beginning with Dalton's assumption of an indivisible atom, subsequent discoveries by Goldstein, Thomson, and Chadwick reshaped our understanding. Thomson's plum pudding and Rutherford's nuclear models provided insights, while Bohr's model addressed some issues. Concepts such as electron distribution, valency, atomic, and mass numbers gained significance. The discovery of isotopes and isobars expanded our knowledge, finding applications in diverse fields, from nuclear reactors to medical sciences. 

Important Points: Structure of the Atom | Science Class 9

Historical Perspective

Discoveries in Atomic TheoryDiscoveries in Atomic Theory

  • Dalton's Assumption (1803): Atom is indivisible.
  • Goldstein's Discovery (1866): Discovered canal rays, leading to the identification of protons (positively charged particles).
  • Thomson's Discovery (1897): Discovered electrons with a negative charge.
  • Chadwick's Discovery: Identified neutrons with no charge.

Thomson's Model

  • Electrons are distributed in the sphere of protons.
  • Atom is electrically neutral.
  • Known as the plum pudding model.

Rutherford's Model

  • Experiment with α-particles on thin gold foil.
  • Conclusions: Atom mostly empty space.
  • +ve charge concentrated in a small volume (nucleus).
  • Nuclear model: Nucleus (protons) at the center, electrons orbiting.
  • Drawback: Electrons should lose energy and collapse, making atoms unstable.

Bohr's Model

  • Electrons in discrete orbits (energy levels).
  • Electrons in these orbits do not radiate energy.
  • Drawbacks: Violates Heisenberg Uncertainty Principle, fails for larger atoms.

Atomic StructureAtomic Structure

Discovery of Neutron

  • In 1932, J. Chadwick made a groundbreaking discovery in the realm of atomic particles by identifying a subatomic particle with no charge and a mass nearly equivalent to that of a proton. 
  • This neutral particle, eventually named the neutron, is a constituent of the nucleus in all atoms, excluding hydrogen.
  • Neutrons, denoted as 'n,' play a crucial role in determining the mass of an atom. The total mass of an atom is the sum of the masses of protons and neutrons residing within the nucleus.

Electron Distribution Rules

The distribution of electrons within different orbits of an atom was proposed by Bohr and Bury. The following rules guide the assignment of electron numbers to various energy levels or shells:

1. Maximum Electrons in a Shell: The maximum number of electrons present in a shell is determined by the formula 2n², where 'n' denotes the orbit number or energy level index (1, 2, 3, ...). This leads to specific maximum electron counts for various shells: 2 in the first orbit (K-shell), 8 in the second orbit (L-shell), 18 in the third orbit (M-shell), 32 in the fourth orbit (N-shell), and so forth.

Important Points: Structure of the Atom | Science Class 9

2. Maximum Electrons in Outermost Orbit: The outermost orbit can accommodate a maximum of 8 electrons.

3. Step-wise Filling of Shells: Electrons are allocated to shells in a step-wise manner, ensuring that inner shells are filled before accommodating electrons in a given shell.

Valency

  • Valency refers to the combining capacity of an atom, indicating its tendency to react with other atoms and form molecules. 
  • This property is associated with the arrangement of electrons in the outermost shell of an atom.

Atomic Number (Z)

  • Total protons in an atom's nucleus.
  • Represents the element.

Mass Number (A)

  • Protons + Neutrons.
  • Element representation: AXZ.

Important Points: Structure of the Atom | Science Class 9

Isotopes

  • Atoms of the same element with different mass numbers.
  • Same chemical properties, different physical properties.
  • Applications in nuclear reactors, cancer treatment, and medical fields.

Important Points: Structure of the Atom | Science Class 9

Isobars

  • Atoms of different elements with the same mass number.
  • Different chemical properties.Important Points: Structure of the Atom | Science Class 9

Practice Questions

Ques. Is it possible for the atom of an element to have one electron, one proton and no neutron? If so, name the element.

Ans. Yes, it is true for the hydrogen atom which is represented as 1H1 . It is having one electron, one proton and no neutron.

Ques. What do you understand by the ground state of an atom?

Ans. The state of an atom where all the electrons in the atom are in their lowest energy levels is called the ground state. 

Ques. Who identified the sub-atomic particle electron?

Ans. J.J. Thomson discovered the sub-atomic particle electron and proved that it existed without ever being able to see or isolate one. 

Ques. Who discovered the nucleus of the atom?

Ans. Rutherford and his co-workers performed alpha-particle scattering experiments which led to the discovery of the atomic nucleus of atom.

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FAQs on Important Points: Structure of the Atom - Science Class 9

1. What is the historical perspective of atomic theory?
Ans. The historical perspective of atomic theory traces back to ancient Greek philosophers like Democritus, who proposed that matter is composed of indivisible particles called atoms. In the early 19th century, John Dalton further developed the theory by introducing the concept of atomic weights and the idea that atoms combine in fixed ratios to form compounds. Later, J.J. Thomson discovered the electron, leading to the plum pudding model, which was eventually replaced by Ernest Rutherford's nuclear model after his gold foil experiment revealed the nucleus. Niels Bohr later refined the model with his planetary model of the atom, which incorporated quantized electron orbits. This historical evolution reflects the increasing complexity and understanding of atomic structure.
2. What are the rules for electron distribution in an atom?
Ans. The rules for electron distribution in an atom are based on principles such as the Aufbau principle, Pauli exclusion principle, and Hund's rule. The Aufbau principle states that electrons fill the lowest energy orbitals first. The Pauli exclusion principle asserts that no two electrons can have the same set of four quantum numbers, meaning each orbital can hold a maximum of two electrons with opposite spins. Hund's rule states that electrons will occupy degenerate orbitals singly before pairing up, ensuring maximum spin multiplicity. These rules help predict the electron configuration of elements, which is crucial for understanding chemical behavior.
3. What is valency and how is it determined?
Ans. Valency is the measure of an atom's ability to bond with other atoms, determined by the number of electrons in its outermost shell. It reflects the capacity of an element to form chemical bonds, either by losing, gaining, or sharing electrons. For main group elements, valency is often equivalent to the number of electrons needed to fill or empty the outer shell to achieve a stable electronic configuration, typically resembling that of noble gases. For example, carbon has a valency of four because it can form four covalent bonds by sharing its four valence electrons.
4. What are isotopes and how do they differ from each other?
Ans. Isotopes are variants of a chemical element that have the same number of protons but different numbers of neutrons, resulting in different atomic masses. For example, carbon-12 and carbon-14 are both isotopes of carbon; they both have six protons but differ in neutron count (six for carbon-12 and eight for carbon-14). While isotopes exhibit similar chemical properties due to their identical electron configurations, they can differ significantly in physical properties and stability, leading to applications in fields such as radiocarbon dating and medical imaging.
5. What are isobars and what distinguishes them from isotopes?
Ans. Isobars are atoms of different elements that have the same atomic mass but different atomic numbers. This means that isobars contain the same total number of nucleons (protons and neutrons) but differ in the number of protons and neutrons individually. For example, carbon-14 (6 protons and 8 neutrons) and nitrogen-14 (7 protons and 7 neutrons) are isobars because they both have a total mass number of 14. Unlike isotopes, which are variants of the same element, isobars belong to different elements, leading to different chemical properties.
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