🌏
Chapter Introduction: What Is an Atom?
Everything around us — your desk, your food, the air you
breathe, and even your own body — is made of matter. And all matter
is made of incredibly tiny particles called atoms (परमाणु). These atoms are
so small that they cannot be seen with the naked eye!
🏛️
📅 Dalton’s Atomic Theory
(1808)
In 1808, John Dalton proposed the first
scientific atomic theory based on experiments:
- All
matter is composed of tiny, indivisible particles called atoms.
- Atoms
of the same element are identical; atoms of different elements are
different.
- Atoms
cannot be created or destroyed in a chemical reaction.
- Compounds
are formed when atoms of different elements combine in fixed ratios.
📌
💡
🏗️
Historical Journey Through Atomic Models
As scientists performed new experiments, they kept improving
the model of the atom. Each model was a step forward, but none was perfect
until more evidence arrived.
1808
Dalton
Atom = indivisible sphere
1897
Thomson
Plum pudding model
1911
Rutherford
Nuclear / Planetary model
1913
Bohr
Fixed energy shells
Modern
Quantum
Electron cloud model
⚡ Thomson’s Plum Pudding Model
(1897)
In 1897, J. J. Thomson studied cathode rays
by passing electricity through gas at very low pressure. He discovered electrons —
tiny negatively charged particles.
🔬
Since atoms are neutral but contain negative electrons,
Thomson asked: where is the positive charge? His answer was the Plum
Pudding Model:
- The
atom is a sphere of positive charge.
- Electrons
are embedded (scattered) throughout this positive sphere
like plums in a pudding.
- Indian
analogy: think of it like a watermelon 🍉
— the red pulp is the positive charge, and the seeds are the electrons!
Charge of an electron = −1.602 × 10⁻¹⁹ C (represented
as −1 for convenience)
🏆
🥇
The Gold Foil Experiment & Rutherford’s Model
🧪 The Gold Foil
Experiment (1911)
In 1911, Geiger and Marsden, working under Ernest
Rutherford, tested Thomson’s model by firing a beam of positively
charged alpha (α) particles at an extremely thin gold foil.
⚛️
📊 Observations vs.
Expectations
|
What
Thomson’s Model Predicted |
What
Actually Happened |
|
All
α-particles should pass straight through or be deflected only slightly |
Most
particles DID pass straight through ✅ |
|
No
sharp deflections expected |
Some
particles were deflected at very large angles ❌ |
|
Definitely
no particles bouncing back |
A few
particles bounced STRAIGHT BACK ❌ |
⚠️
🌟 Rutherford’s
Conclusions — The Nuclear (Planetary) Model
- Most
of the atom is empty space — this explains why most α-particles
passed through undeflected.
- All
the positive charge and most of the mass are concentrated
in a tiny region at the center called the nucleus (केंद्रक).
- Electrons
revolve around the nucleus in orbits, just like planets orbit the
Sun. Hence, this is called the Planetary Model.
🏏
Diameter of atom ≈ 10⁻¹⁰ m |
Diameter of nucleus ≈ 10⁻¹⁵ m
⚠️ Limitation of Rutherford’s
Model
While it was a big step forward, Rutherford’s model couldn’t
explain why atoms are stable. Here’s the problem:
- A
charged particle moving in a circular path is constantly accelerating
(changing direction).
- An
accelerating charged particle should continuously lose energy.
- If
electrons lose energy, they should spiral inward and
eventually crash into the nucleus.
- But
this DOESN’T happen — atoms are stable! So Rutherford’s model needed
improvement.
🔬
🏆
🔵
Bohr’s Model: Fixed Energy Shells (1913)
To solve the stability problem, Danish physicist Niels
Bohr proposed a new model in 1913 with a revolutionary idea: electrons
move in fixed paths and don’t lose energy while doing so!
📋 Key Postulates of
Bohr’s Model
- Electrons
move in fixed circular paths around the nucleus
called orbits, shells, or stationary states (स्थिर कक्षाएं).
- Each
shell has a definite, fixed energy, so they are also called energy
levels.
- Shells
are represented by letters K, L, M, N, … or numbers n
= 1, 2, 3, 4, …
- While
in a fixed shell, an electron does NOT lose energy.
- The K-shell
(n=1) is closest to the nucleus and has the least energy.
- Energy
of shells increases as we move farther from the nucleus.
- An
electron can jump to another shell by absorbing or releasing a
fixed amount of energy equal to the energy difference between the two
levels.
NucleusK (n=1)e⁻L (n=2)e⁻M (n=3)e⁻↑ Energy increases outward
Fig: Bohr’s model showing K, L, M shells (energy levels)
around the nucleus
📌
🏆
🚀
🧩
Subatomic Particles: Protons, Neutrons & Electrons
An atom is made of three fundamental subatomic particles.
Let’s understand each one!
|
Particle |
Symbol |
Charge |
Location |
Relative
Mass |
Discovered
By |
|
Electron
(इलेक्ट्रॉन) |
e⁻ |
−1 |
Shells
(outside nucleus) |
~1/1836
of proton |
J. J.
Thomson (1897) |
|
Proton
(प्रोटॉन) |
p⁺ |
+1 |
Inside
Nucleus |
1 unit |
Rutherford |
|
Neutron
(न्यूट्रॉन) |
n⁰ |
0
(neutral) |
Inside
Nucleus |
~1 unit
(≈ proton) |
James
Chadwick (1932) |
🔍 Discovery of the
Neutron (1932)
Scientists noticed a puzzle: Helium has 2 protons, but its
mass is about 4 times that of Hydrogen (which has 1 proton). So where
is the extra mass coming from?
In 1932, James Chadwick (a student of
Rutherford) solved this puzzle by discovering the neutron — a
particle with nearly the same mass as a proton but no electrical charge.
Neutrons are present in the nucleus of all atoms except hydrogen.
⚖️
🏆
🔢
Atomic Number, Mass Number & Notation
📌 Atomic Number (Z)
The atomic number (परमाणु संख्या) is
the number of protons in the nucleus of an atom. It is denoted
by the symbol Z.
- Atomic
number uniquely identifies an element. No two different
elements have the same atomic number.
- Since
atoms are electrically neutral, number of protons = number of
electrons.
- Example:
Hydrogen has 1 proton → Z = 1. Helium has 2 protons → Z = 2.
Atomic Number (Z) = Number of Protons = Number
of Electrons (in neutral atom)
⚖️ Mass Number (A)
The mass number (द्रव्यमान संख्या) is
the total number of protons + neutrons in the nucleus. It is
denoted by the symbol A. Protons and neutrons together are called nucleons.
Mass Number (A) = Number of Protons (p⁺) +
Number of Neutrons (n⁰)
|
Element |
Protons
(Z) |
Neutrons |
Mass
Number (A) |
Electrons |
|
Hydrogen
(H) |
1 |
0 |
1 |
1 |
|
Helium
(He) |
2 |
2 |
4 |
2 |
|
Lithium
(Li) |
3 |
4 |
7 |
3 |
|
Carbon
(C) |
6 |
6 |
12 |
6 |
|
Sodium
(Na) |
11 |
12 |
23 |
11 |
📝 Standard Atomic
Notation
The symbol, atomic number, and mass number of an element are
written in a standard way:
C126↑ Mass Number (A)↑ Atomic Number (Z)← Element Symbol
Standard notation for Carbon: Mass number 12, Atomic
number 6
🔍 Finding Neutrons from
Atomic & Mass Numbers:
Given: Atomic number (Z) = 17 (Chlorine), Mass
number (A) = 35
Number of neutrons = A − Z = 35 − 17
Number of Neutrons = 18
⚠️
🔤 Symbols of Elements
In 1803, Dalton introduced pictorial symbols. In 1813, Berzelius suggested
alphabetical symbols from Latin names. Today, IUPAC approves
all element names and symbols.
📌
🔵
Electronic Configuration: How Electrons Fill Shells
The arrangement of electrons in different energy
levels/shells of an atom is called its electronic configuration (इलेक्ट्रॉनिक विन्यास).
📋 Bohr-Bury Rules for
Filling Electrons
- Maximum
electrons in a shell = 2n², where n is the shell number.
- K-shell
(n=1): max 2 electrons | L-shell (n=2): max 8 electrons
| M-shell (n=3): max 18 electrons
- The
maximum number of electrons in the outermost shell is
always 8 (except K-shell which holds only 2).
- Electrons
fill in order K → L → M → N, moving to the next shell only
after the current one is full.
Max electrons in shell = 2n² | K:
2×1²=2 | L: 2×2²=8 | M:
2×3²=18
|
Element |
Symbol |
Atomic
No. (Z) |
K |
L |
M |
Config. |
|
Hydrogen |
H |
1 |
1 |
– |
– |
1 |
|
Helium |
He |
2 |
2 |
– |
– |
2 |
|
Lithium |
Li |
3 |
2 |
1 |
– |
2, 1 |
|
Carbon |
C |
6 |
2 |
4 |
– |
2, 4 |
|
Neon |
Ne |
10 |
2 |
8 |
– |
2, 8 |
|
Sodium |
Na |
11 |
2 |
8 |
1 |
2, 8, 1 |
|
Magnesium |
Mg |
12 |
2 |
8 |
2 |
2, 8, 2 |
|
Chlorine |
Cl |
17 |
2 |
8 |
7 |
2, 8, 7 |
|
Argon |
Ar |
18 |
2 |
8 |
8 |
2, 8, 8 |
📝 Example: Electronic
Configuration of Phosphorus (P, Z=15)
🔗
Valency: Combining Capacity of an Atom
🔑 Key Terms
✅ The Octet Rule
Atoms are most stable when their outermost shell has 8
electrons (octet) — or 2 electrons in the case of helium (only has
K-shell).
- Elements
with a complete octet (like Ne, Ar) are inert/unreactive (noble
gases).
- Elements
with incomplete valence shells are reactive.
They lose, gain, or share electrons to complete the octet.
Valency (संयोजकता) =
Number of electrons gained, lost, or shared to complete the octet
|
Element |
Electron
Config. |
Valence
Electrons |
Action |
Valency |
|
Sodium
(Na) |
2, 8, 1 |
1 |
Loses 1
electron |
1 |
|
Oxygen
(O) |
2, 6 |
6 |
Gains 2
electrons |
2 |
|
Carbon
(C) |
2, 4 |
4 |
Shares
4 electrons |
4 |
|
Chlorine
(Cl) |
2, 8, 7 |
7 |
Gains 1
electron |
1 |
|
Neon
(Ne) |
2, 8 |
8
(complete) |
No
gain/loss (stable) |
0 |
💡
🧬
Isotopes & Isobars: Special Atomic Pairs
🔬 Isotopes (समस्थानिक)
Atoms of the same element that have the same atomic
number (Z) but different mass numbers (A) — i.e.,
different numbers of neutrons — are called isotopes.
📌
💧 Isotopes of Hydrogen
Naturally occurring hydrogen is a mixture of three isotopes:
🔬
☢️ Important Uses of Isotopes
- ²³⁵U —
Used as fuel in nuclear reactors to generate electricity.
- ⁶⁰Co —
Radioactive cobalt used in cancer radiation therapy.
- ¹³¹I —
Iodine isotope used to treat goitre and thyroid cancer.
- ¹⁴C —
Carbon-14 used in carbon dating — determining the age of
fossils and ancient artefacts in archaeology!
💡
⚖️ Average Atomic Mass
Since isotopes exist in nature in different proportions, the
atomic mass of an element is calculated as the weighted average of
its isotopes based on their abundance.
📐 Example: Weighted
Average Atomic Mass of Chlorine
Chlorine has two isotopes: ³⁵Cl (75%) and ³⁷Cl
(25%)
Note: This doesn’t mean any single Cl atom has mass 35.5
u. It’s just a weighted average over millions of atoms!
🔄 Isobars (समभारिक)
Atoms of different elements that have
the same mass number (A) but different atomic numbers
(Z) are called isobars.
|
Element |
Atomic
Number (Z) |
Mass
Number (A) |
Relation |
|
Argon
(Ar) |
18 |
40 |
All are
isobars — same mass number (40), different atomic numbers |
|
Potassium
(K) |
19 |
40 |
|
|
Calcium
(Ca) |
20 |
40 |
📝 Quick Revision Summary
⚛️ Dalton (1808)Atoms are
indivisible particles — the building blocks of matter.
⚡ Thomson (1897)Plum pudding
model — electrons embedded in positive sphere.
🥇 Rutherford (1911)Nuclear
model — dense nucleus at center, electrons orbit outside.
🔵 Bohr (1913)Electrons
move in fixed energy shells K, L, M, N. Stability explained.
🔢 Atomic Number (Z)Number
of protons. Uniquely identifies an element. Z = electrons.
⚖️ Mass Number (A)A = Protons
+ Neutrons. Neutrons = A − Z.
🔵 Shell Capacity: 2n²K=2,
L=8, M=18. Outermost shell max = 8 electrons.
🔗 ValencyElectrons
gained/lost/shared to complete octet. Noble gases: valency = 0.
🧬 IsotopesSame Z,
different A. Same chemical properties. Used in medicine, energy, dating.
🔄 IsobarsDifferent Z,
same A. Different elements with equal nucleon count.
⚖️ Average Atomic MassWeighted
average based on abundance of isotopes in nature.
🧩 Neutron (1932)Chadwick
discovered neutron — neutral particle adding mass to nucleus.
📋 Important Exam
Questions
Q1. What were the main observations of Rutherford’s gold
foil experiment and what conclusions did he draw? (CBSE — 5 Marks)
Observations: (1) Most alpha particles passed
straight through the gold foil. (2) A few alpha particles were deflected at
large angles. (3) A very few bounced straight back.
Conclusions: (1) Since most particles passed
through undeflected, most of an atom is empty space. (2) Since some
particles were sharply deflected and a few bounced back, there must be a very
small, dense, positively charged nucleus at the center of the atom.
(3) Electrons revolve around the nucleus in orbits (planetary model). The
nucleus is about 10⁵ times smaller than the atom.
Q2. Why did Rutherford’s model fail to explain atomic
stability? How did Bohr’s model solve this problem? (CBSE — 3 Marks)
Rutherford’s failure: According to classical
physics, a charged particle moving in a circular path constantly accelerates.
An accelerating charged particle continuously loses energy. If electrons lose
energy, they would spiral inward and fall into the nucleus — making atoms
collapse. But atoms are stable, so this model was incomplete.
Bohr’s solution: Bohr proposed that electrons
move in fixed stationary states (shells) where they do NOT
lose energy. Energy remains constant in a fixed shell. An electron only
gains/loses energy when jumping between shells, releasing a fixed quantum of
energy. This explained stability.
Q3. An element X has mass number 35 and 18 neutrons. Find
its (i) Atomic number (ii) Electronic configuration (iii) Valency. (CBSE — 3
Marks)
Q4. Define isotopes. Give two examples and state any two
uses of isotopes in daily life. (CBSE — 3 Marks)
Definition: Isotopes are atoms of the same
element that have the same atomic number (Z) but different mass numbers (A) due
to different numbers of neutrons.
Examples: (1) Isotopes of Hydrogen: Protium
(¹H), Deuterium (²H), Tritium (³H) — all have Z=1. (2) Isotopes of Carbon: ¹²C,
¹³C, ¹⁴C — all have Z=6.
Uses: (1) ¹⁴C (carbon-14) is used in carbon
dating to determine the age of fossils and archaeological artefacts.
(2) ²³⁵U (uranium-235) is used as fuel in nuclear reactors to
generate electricity.
Q5. Differentiate between Isotopes and Isobars with one
example each. (CBSE — 2 Marks)
Isotopes: Atoms of the same element with
same atomic number (Z) but different mass numbers (A). They have different
numbers of neutrons. Example: ¹⁶O and ¹⁸O — both have Z=8 (oxygen), but
different mass numbers.
Isobars: Atoms of different elements with
different atomic numbers (Z) but same mass number (A). Example: Argon (Z=18,
A=40), Potassium (Z=19, A=40), Calcium (Z=20, A=40) — all have mass number 40
but are different elements.