Chapter 3
Periodic Table and Periodicity of Properties

Topic 1


Introduction to the PeriodicTable                                                                         


The Periodic Table is a fundamental tool in chemistry, organizing the known chemical elements based on their atomic number and recurring properties. Its development was a significant milestone in the history of science, stemming from early attempts to classify elements in a systematic manner.

Early Attempts at Classification

In the 19th century, chemists sought to arrange elements in a meaningful way, leading to the discovery of periodic relationships. Notable early attempts include:

·         Dobereiner's Triads: Dobereiner observed that certain groups of three elements, called triads, had atomic masses that followed a pattern. The atomic mass of the middle element was approximately the average of the other two.

·         Newlands' Octaves: Newlands noticed a repeating pattern in the properties of elements when arranged in order of increasing atomic mass, similar to musical notes. He proposed the "law of octaves."

Mendeleev's Periodic Table

The most influential early periodic table was created by Dmitri Mendeleev in 1869. He arranged known elements based on their atomic masses and chemical properties, leading to the formulation of the Periodic Law:

·         Periodic Law: The properties of elements are a periodic function of their atomic masses.

Mendeleev's table was groundbreaking, as it predicted the properties of undiscovered elements and allowed for the correction of inaccurate atomic masses.

Modern Periodic Table

With the discovery of atomic number by Henry Moseley in 1913, the Periodic Law was refined to state that the properties of elements are a periodic function of their atomic numbers. This led to the modern periodic table, which is organized based on increasing atomic number.

Key features of the modern periodic table:

·         Periods: Horizontal rows representing elements with the same number of electron shells.

·         Groups: Vertical columns representing elements with similar chemical properties due to having the same number of valence electrons.

·         Blocks: Sections of the table based on the type of orbital that receives the last electron (s, p, d, or f).

The periodic table is a valuable tool for understanding the relationships between elements, predicting their properties, and understanding chemical reactions. It provides a visual representation of the underlying order in the structure of matter.

 

 


Topic 2                  

Periods and Groups in the Periodic Table

Periods

·         Short Period (Period 1): Contains only two elements: hydrogen and helium.

·         Normal Periods (Periods 2 and 3): Each contains eight elements. Examples:

o    Period 2: Lithium, beryllium, boron, carbon, nitrogen, oxygen, fluorine, neon.

o    Period 3: Sodium, magnesium, aluminum, silicon, phosphorus, sulfur, chlorine, argon.  

·         Long Periods (Periods 4 and 5): Each contains eighteen elements.

·         Very Long Periods (Periods 6 and 7): These periods are longer due to the presence of the Lanthanides (elements 57-71) and Actinides (elements 89-103), which are typically placed separately at the bottom of the periodic table to maintain a manageable format.

Groups

·         Group 1 (Alkali Metals): Hydrogen, lithium, sodium, potassium, rubidium, cesium, francium. These elements have one valence electron.

·         Group 2 (Alkaline Earth Metals): Beryllium, magnesium, calcium, strontium, barium, radium. These elements have two valence electrons.

·         Groups 3-12 (Transition Metals): These elements are characterized by partially filled d orbitals in their outer electron shells. Examples include iron, copper, zinc, and gold.

·         Groups 13-17 (Representative Elements): These elements have varying numbers of valence electrons and exhibit a wide range of properties. Examples include boron, carbon, nitrogen, oxygen, fluorine, aluminum, silicon, phosphorus, sulfur, chlorine.

·         Group 18 (Noble Gases): Helium, neon, argon, krypton, xenon, radon. These elements have completely filled outer electron shells and are generally unreactive.

Key Points:

·         The number of elements in a period is determined by the maximum number of electrons that can occupy a particular energy level (valence shell).

·         Elements within a group share similar chemical properties due to having the same number of valence electrons.

·         The placement of Lanthanides and Actinides at the bottom of the periodic table is a convention to maintain a compact format.

Example:

·         Period 3: The elements in this period have 3 electron shells. The number of valence electrons increases from left to right, from sodium (1 valence electron) to argon (8 valence electrons).

·         Group 1: All alkali metals have 1 valence electron, giving them similar properties such as reactivity with water and formation of ionic compounds.

 

 


Topic 3           

Periodic Trends: Atomic Size and Shielding Effect

Atomic Size

Atomic size is a measure of the average distance between the nucleus and the outermost electrons of an atom. It's generally measured in picometers (pm).  

Trends in Atomic Size:

·         Across a Period:

o    Decreases: As you move from left to right across a period, the number of protons in the nucleus increases, which increases the effective nuclear charge. This stronger attraction pulls the outer electrons closer to the nucleus, reducing atomic size.  

·         Down a Group:

o    Increases: As you move down a group, a new energy level (shell) is added to the atom. This increased distance between the nucleus and the outermost electrons leads to a larger atomic size.

Shielding Effect

The shielding effect is the reduction in the attractive force between the nucleus and the outermost electrons due to the presence of inner electrons.  

Factors Affecting Shielding Effect:

·         Number of Inner Electrons: Atoms with more inner electrons have a greater shielding effect.  

·         Orbital Penetration: Electrons in s orbitals penetrate closer to the nucleus than those in p, d, or f orbitals, leading to a stronger shielding effect.

Trends in Shielding Effect:

·         Across a Period:

o    Shielding effect remains relatively constant: Within a period, the number of inner electrons remains the same, so the shielding effect doesn't change significantly.

·         Down a Group:

o    Increases: As you move down a group, the number of inner electrons increases, leading to a stronger shielding effect.  

Relationship Between Atomic Size and Shielding Effect:

·         A stronger shielding effect reduces the effective nuclear charge felt by the outermost electrons, making them less tightly bound to the nucleus. This results in a larger atomic size.  

Example:

·         Sodium (Na) vs. Potassium (K): Both sodium and potassium are in Group 1. Potassium has a larger atomic size than sodium because it has a greater number of inner electrons, which shield the outer electron more effectively, reducing the effective nuclear charge.  

In summary: Atomic size decreases across a period due to increased effective nuclear charge, while it increases down a group due to the addition of new energy levels. The shielding effect, influenced by the number of inner electrons and orbital penetration, plays a significant role in determining atomic size.  

 

 


Topic 4

Ionization Energy

Ionization energy is the energy required to remove an electron from a neutral gaseous atom. It is typically measured in kilojoules per mole (kJ/mol).

In simpler terms, it's the energy needed to break the bond between an atom and its outermost electron. This process creates a positively charged ion (cation).

First Ionization Energy:

·         The energy needed to remove the first electron from a neutral atom.

·         For example, the first ionization energy of sodium (Na) is +496 kJ/mol.

Successive Ionization Energies:

·         Atoms with multiple valence electrons can have multiple ionization energies.

·         Removing a second electron requires more energy than removing the first, and so on.

Trends in Ionization Energy:

·         Across a Period:

o    Increases: As you move from left to right across a period, the atomic size decreases, and the effective nuclear charge increases. This stronger attraction between the nucleus and valence electrons makes it more difficult to remove an electron, resulting in higher ionization energies.  

·         Down a Group:

o    Decreases: As you move down a group, the atomic size increases, and the shielding effect of inner electrons becomes stronger. This reduces the effective nuclear charge felt by the valence electrons, making it easier to remove them, resulting in lower ionization energies.

Example:

·         Group 1 elements (alkali metals): Have low first ionization energies because they have only one valence electron, which is relatively easy to remove.

·         Group 17 elements (halogens): Have high first ionization energies because they have seven valence electrons, making it difficult to remove an electron without disrupting the stable configuration.

In summary: Ionization energy increases across a period due to increased effective nuclear charge and decreases down a group due to increased atomic size and shielding effect. These trends are important for understanding the reactivity and chemical properties of elements.

 

 

 


Topic 5      

Electron Affinity

Electron affinity is a measure of an atom's ability to attract an additional electron. It's defined as the energy change (either released or absorbed) when an electron is added to a neutral gaseous atom to form a negative ion (anion).

Key points:

·         Energy Release or Absorption: Electron affinity can be either positive or negative:

o    Positive: If energy is absorbed when an electron is added, the electronaffinity is positive, indicating that the atom is less likely to accept an electron.

o    Negative: If energy is released when an electron is added, the electron affinity is negative, indicating that the atom has a strong affinity for electrons.

·         Trend Across a Period:

o    Increases: Generally, electron affinity increases from left to right across a period. As atomic size decreases, the nucleus has a stronger attraction for electrons, making it more likely to accept one.

·         Trend Down a Group:

o    Decreases: Electron affinity generally decreases from top to bottom within a group. As atomic size increases, the shielding effect of inner electrons becomes stronger, reducing the attraction between the nucleus and the incoming electron.

Examples:

·         Halogens (Group 17): Halogens typically have high negative electron affinities, indicating a strong tendency to gain electrons and form anions.

·         Noble Gases (Group 18): Noble gases have relatively low electron affinities, as their filled outer electron shells make them relatively stable and less likely to accept additional electrons.

Factors affecting electronaffinity:

·         Atomic size: Smaller atoms generally have higher electron affinities due to stronger nuclear attraction.

·         Shielding effect: The presence of inner electrons can shield the nucleus from the incoming electron, reducing the attraction.

·         Electron configuration: Atoms with half-filled or completely filled subshells may have slightly higher electron affinities due to the stability associated with these configurations.

In summary: Electron affinity is a measure of an atom's ability to attract an electron. It generally increases across a period and decreases down a group, reflecting trends in atomic size and shielding effects. Understanding electron affinity is important for understanding the formation of ions and chemical bonding.

 

 

 


Topic no 6      

Electronegativity

Electronegativity is a measure of an atom's ability to attract shared electrons towards itself in a covalent bond. It's a crucial property in understanding the nature of chemical bonds, particularly covalent bonds.

Trends in Electronegativity:

·         Across a Period:

o    Increases: Electronegativity generally increases from left to right across a period. As atomic size decreases and effective nuclear charge increases, the nucleus has a stronger attraction for electrons, including shared electrons in covalent bonds.

·         Down a Group:

o    Decreases: Electronegativity generally decreases from top to bottom within a group. As atomic size increases, the shielding effect of inner electrons weakens the attraction between the nucleus and shared electrons.

Examples:

·         Group 17 elements (halogens): Halogens have high electronegativities, making them highly electronegative elements. This means they strongly attract shared electrons in covalent bonds, often forming polar covalent bonds or ionic bonds.

·         Group 1 elements (alkali metals): Alkali metals have low electronegativities, making them electropositive elements. They are less likely to attract shared electrons and often form ionic bonds by losing electrons.

Factors affecting electronegativity:

·         Atomic size: Smaller atoms have higher electronegativities due to stronger nuclear attraction.

·         Shielding effect: The presence of inner electrons can shield the nucleus from shared electrons, reducing the attraction.

·         Electron configuration: Atoms with half-filled or completely filled subshells may have slightly higher electronegativities due to the stability associated with these configurations.

In summary: Electronegativity is a measure of an atom's ability to attract shared electrons in a covalent bond. It increases across a period and decreases down a group, reflecting trends in atomic size and shielding effects. Electronegativity is crucial for understanding the polarity of covalent bonds and the nature of chemical interactions between atoms.