9th Class Chemistry
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ARMCQs DIGITAL STUDY NOTES

Chapter 3: Periodic Table

Chemistry with Sir Aamir Rajper

Clear concepts · Chapter-wise reading · Designed for focused revision

How the Periodic Table Developed

Why classify elements?

Scientists needed a way to organize the growing list of elements. They grouped elements with similar properties. This made the elements easier to study and compare.

Dobereiner’s triads (1829)

Dobereiner put some similar elements into groups of three, called triads. Add the atomic masses of the first and third elements, then divide by two. The result is close to the middle element’s atomic mass.

Triad

Atomic masses

Check

Li, Na, K

7, 23, 39

(7 + 39) ÷ 2 = 23

Cl, Br, I

35.5, 80, 126.5

(35.5 + 126.5) ÷ 2 = 81 (approx.)

Ca, Sr, Ba

40, 88, 137

(40 + 137) ÷ 2 = 88.5 (approx.)

Limitation: only a limited number of elements could be grouped into triads.

Newlands’ law of octaves (1864–1865)

Newlands arranged elements from lower to higher atomic mass. He noticed that every eighth element often had similar properties, like repeating musical notes.

Example: lithium and sodium show similar properties.

Limitation: the rule was successful mainly for lighter elements, up to calcium.

Mendeleev’s periodic law (1869)

The physical and chemical properties of elements are periodic functions of their atomic masses.

Elements with similar chemical properties were placed in the same vertical groups.

He left gaps for undiscovered elements and successfully predicted some of their properties.

Some elements did not fit a strict atomic-mass order. The table also had no clear place for isotopes.

Moseley and the modern periodic law (1913)

The physical and chemical properties of elements are periodic functions of their atomic numbers.

Atomic number is the number of protons. It also gives the electron count in a neutral atom. Arranging elements by atomic number explains the repeating patterns better than arranging them by mass.

Mendeleev

Modern periodic table

Increasing atomic mass

Increasing atomic number

Periodic law based on atomic mass

Periodic law based on atomic number

Modern Periodic Table: Groups and Periods

Understand it simply

The modern periodic table has 118 recognised elements. Atomic number increases across the table. There are 7 horizontal rows, called periods, and 18 vertical columns, called groups.

GUIDED DIAGRAM

Four Blocks · Modern Periodic Table

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s block. The s block occupies the first two groups. Helium has an s configuration but is placed with the noble gases in Group 18.

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Simplified modern periodic table showing periods, group positions and the s, p, d and f blocks.
The four blocks show the type of subshell filled by the differentiating electron. This is the electron added when we move from one element to the next.
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The four blocks show the type of subshell filled by the differentiating electron. This is the electron added when we move from one element to the next.

Periods: horizontal rows

For most elements, the period number tells us the highest occupied shell in the ground state. Ground state means the lowest-energy arrangement. Some transition elements are exceptions.

Moving one place across a period adds one proton. A neutral atom also has one more electron. The outer electron arrangement changes as we move across.

Period

Number of elements

First → last

1

2

H → He

2

8

Li → Ne

3

8

Na → Ar

4

18

K → Kr

5

18

Rb → Xe

6

32

Cs → Rn

7

32

Fr → Og

Period 1 is the shortest. Periods 6 and 7 are the longest, with 32 elements each. Period 7 is complete.

Groups: vertical columns

Elements in the same main group have similar outer electron arrangements. This is why they usually behave in similar ways.

For main-group elements, Group 1 usually means 1 valence electron and Group 2 means 2. Groups 13–18 usually have 3–8 valence electrons. Helium is an exception: it has 2.

Example: Li (2,1), Na (2,8,1) and K (2,8,8,1) each have one valence electron, so all belong to Group 1.

Important Families (Groups 1–18)

Modern group

Old label

Family

Valence e⁻

1

IA

Alkali metals

1

2

IIA

Alkaline earth metals

2

13

IIIA

Boron family

3

14

IVA

Carbon family

4

15

VA

Nitrogen family

5

16

VIA

Oxygen family / chalcogens

6

17

VIIA

Halogens

7

18

VIIIA / zero

Noble gases

8 (He: 2)

Group 1: alkali metals

Li, Na, K, Rb, Cs, Fr. These reactive metals have one valence electron and commonly lose it to form +1 ions. They generally have low melting points. Hydrogen lies above this group but is not an alkali metal.

Group 2: alkaline earth metals

Be, Mg, Ca, Sr, Ba, Ra. They have two valence electrons and commonly form +2 ions. They are generally less reactive than Group 1 metals in the same period.

Group 13: boron family

B, Al, Ga, In, Tl. They have three valence electrons. Boron is a metalloid; the other members are metals. +3 is a common oxidation state, but not universal.

Group 14: carbon family

C, Si, Ge, Sn, Pb. They have four valence electrons. Carbon is a nonmetal; silicon and germanium are metalloids; tin and lead are metals. Tin and lead commonly show +2 and +4 oxidation states.

Group 15: nitrogen family

N, P, As, Sb, Bi. They have five valence electrons. Metallic character increases down the group. Common oxidation states include −3, +3 and +5.

Group 16: oxygen family

O, S, Se, Te, Po. They have six valence electrons and are also called chalcogens. Oxygen, sulfur and selenium are nonmetals; tellurium is a metalloid and polonium is usually classified as a metal.

Group 17: halogens

F, Cl, Br, I, At. They have seven valence electrons, are reactive and commonly gain one electron to form −1 ions.

At room temperature

Halogens

Gases

F₂ and Cl₂

Liquid

Br₂

Solid

I₂ (astatine is also solid)

Group 18: noble gases

He, Ne, Ar, Kr, Xe, Rn, Og. Their valence shell is filled: helium has two electrons; the others typically have eight. These elements are generally very unreactive. Oganesson’s bulk physical properties are not yet experimentally established.

Transition elements

Most d-block elements are metals. Many form coloured ions or complexes (a central metal joined to surrounding atoms or groups). They often have more than one oxidation state, a signed value assigned using electron-counting rules.

A transition element has an incomplete d subshell in its atom or a common positive ion.

s-, p-, d- and f-Blocks

Understand it simply

The block of an element is identified by the type of subshell occupied by its differentiating electron (the electron added when moving from the preceding element).

Block

Position

General filling

Main character

s

Groups 1–2; He has an s configuration

ns¹–ns²

Representative elements

p

Groups 13–18, excluding He

ns²np¹–ns²np⁶

Representative elements

d

Groups 3–12

(n−1)d subshell

Mostly transition metals

f

Two rows below the main table

(n−2)f subshell

Inner transition series

Lanthanoids: the 4f series in Period 6; actinoids: the 5f series in Period 7.

Helium has configuration 1s². Its electrons are in an s subshell, but it sits in Group 18 because it behaves like the noble gases.

A d subshell holds up to 10 electrons, so the d block has 10 columns. An f subshell holds up to 14 electrons.

Why Periodic Properties Repeat

Meaning of periodicity

Periodicity is the recurrence of similar physical and chemical properties when elements are arranged in increasing atomic number. It occurs because similar valence-shell configurations recur.

Three controlling ideas

Factor

Meaning

Result

Effective nuclear charge (Zeff)

The nuclear attraction felt by an electron after allowing for the screening effect of other electrons

Stronger pull generally decreases atomic size

Number of occupied shells

How many main energy levels contain electrons

More shells generally increase size

Shielding

Inner electrons partly screen outer electrons from nuclear attraction

More shielding weakens the pull on outer electrons

Across a period, the nucleus gains protons. Inner electrons do not add much extra shielding. The nucleus therefore pulls more strongly on outer electrons. Down a group, extra shells put outer electrons farther away and increase shielding.

Atomic Size and Atomic Radius

Definition

Atomic radius is a measure of atomic size. For two identical covalently bonded atoms, the covalent radius equals half the distance between their nuclei: r = d ÷ 2.

Understand it simply

A larger radius means a larger atom. For two identical bonded atoms, half the distance between their centres gives the covalent radius.

GUIDED DIAGRAM

Atomic Radius

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Distance between centres. For two identical covalently bonded atoms, measure the distance d between their nuclei.

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Two identical atoms with centres separated by distance d. Each has atomic radius r = d over two.
A simplified model of covalent radius; an atom has no perfectly sharp outer boundary.
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A simplified model of covalent radius; an atom has no perfectly sharp outer boundary.

Common units are pm and Å.

1 Å = 10⁻¹⁰ m = 100 pm.

Atomic size can be measured in different ways. Compare values found by the same method.

Across a period: generally decreases (→)

Across a period, protons increase while added electrons enter the same main shell. The stronger pull brings the electron cloud closer. Atoms usually become smaller.

Example (approximately, covalent radii): Li > Be > B > C > N > O > F.

Down a group: increases (↓)

Down a group, each new occupied shell puts the outer electrons farther from the nucleus. Inner electrons also shield them more. Atoms become larger.

Example: Li < Na < K < Rb < Cs.

Lanthanoids slowly become smaller across their series. Their 4f electrons do not shield the nucleus well. This decrease in size is called lanthanide contraction.

Ionization Energy

Definition

First ionization energy is the minimum energy needed to remove one electron from each atom in one mole of separate gaseous atoms. The atoms must be in their ground state, or lowest-energy state. Isolated means that they are separate, rather than bonded to other atoms.

Understand it simply

Imagine taking an electron away from a gas atom. The more strongly the atom holds it, the more energy you need.

Na(g) + energy → Na⁺(g) + e⁻ (ΔH > 0)

Unit: kJ mol⁻¹. A higher value means more energy is needed to remove an electron.

Across a period: generally increases (→)

Across a period, atoms usually get smaller and hold outer electrons more strongly. Removing an electron usually takes more energy.

Down a group: generally decreases (↓)

Down a group, outer electrons are farther away and more shielded. They are usually easier to remove.

Exam-important exceptions

Be needs more energy than B. Be loses a 2s electron, which is held more strongly than B’s 2p electron.

N needs more energy than O. N has a half-filled 2p³ arrangement. O has a paired 2p electron, which is easier to remove.

Helium has the highest first ionization energy of all elements.

Selected first ionization energies

kJ mol⁻¹

Li

520

Na

496

K

419

Rb

403

Cs

376

Electron Affinity

Definition

Electron affinity is related to the energy change when a separate gaseous atom gains an electron. When this process releases energy, its electron-gain enthalpy is negative. Electron-gain enthalpy means the energy change per mole for adding electrons to gaseous atoms.

Understand it simply

Now imagine adding an electron to a gas atom. The energy change tells us whether energy is released or taken in.

Cl(g) + e⁻ → Cl⁻(g) + energy released

Use the sign carefully. “Electron affinity” often means the amount of energy released, written as positive. Electron-gain enthalpy gives the energy change: it is negative when energy is released.

Across a period: generally more favourable (→)

Across a period, the stronger nuclear pull often makes electron gain more favourable. Noble gases and some stable subshell arrangements are exceptions.

Down a group: generally less favourable (↓)

Down a group, greater distance and shielding usually weaken the pull on an added electron.

Why chlorine exceeds fluorine

Cl releases more energy than F when it gains an electron. F is very small, so its 2p electrons are crowded. They push the new electron away more strongly. Cl has a larger 3p subshell with more room.

Halogen order (energy released): Cl > F > Br > I.

Element

Electron-gain enthalpy (approx.)

F

−328 kJ mol⁻¹

Cl

−349 kJ mol⁻¹

Br

−325 kJ mol⁻¹

I

−295 kJ mol⁻¹

Shielding Effect

Definition

The shielding effect is the reduction in the attraction felt by outer electrons because inner electrons partially screen them from the positive nucleus.

Understand it simply

Inner electrons partly block the nucleus’s pull on outer electrons. More inner shells usually mean more shielding.

GUIDED DIAGRAM

Shielding Effect

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Sodium. Sodium has arrangement 2,8,1. Inner electrons partly screen the attraction between the nucleus and its outer electron.

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Shell diagrams of sodium, configuration 2 8 1, and potassium, configuration 2 8 8 1, showing the greater shielding in potassium.
Potassium has an additional occupied shell, so its outermost electron experiences greater shielding than sodium’s.
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Potassium has an additional occupied shell, so its outermost electron experiences greater shielding than sodium’s.

Across a period: approximately constant

Across a period, the number of inner occupied shells stays nearly the same. Electrons in the same shell shield one another less well. The pull felt by outer electrons usually increases.

Down a group: increases (↓)

Down a group, there are more inner shells to shield the outer electrons. K (2,8,8,1) has more shielding than Na (2,8,1).

More shielding and greater distance make an outer electron easier to remove. This helps explain the decrease in ionization energy down a group.

Electronegativity

Definition

Electronegativity describes how strongly an atom in a bond attracts the shared electrons towards itself.

Understand it simply

Bonded atoms pull on shared electrons. The atom with higher electronegativity pulls more strongly.

Electronegativity compares how strongly bonded atoms pull shared electrons. It has no unit. The Pauling scale is a common way to compare it.

Fluorine is the most electronegative element.

Across a period: generally increases (→)

Across a period, atoms usually become smaller and the nuclear pull grows stronger. They attract shared electrons more strongly.

Down a group: generally decreases (↓)

Down a group, greater size and shielding weaken the pull on shared electrons.

Halogen

Electronegativity (Pauling)

F

3.98 ≈ 4.0

Cl

3.16 ≈ 3.2

Br

2.96 ≈ 3.0

I

2.66 ≈ 2.7

Keep these ideas separate: ionization energy concerns removing an electron; electron affinity concerns adding one; electronegativity concerns pulling shared electrons in a bond.