The structure of an atom, theoretically consisting of a positively charged nucleus surrounded and neutralised by negatively charged electrons revolving in orbits at varying distances from the nucleus, the formation of the nucleus and the arrangement of different electrons with different chemical elements.
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The first definite theory about the structure of matter was put forward by John Dalton in 1890.
The concept of atomic number was given by Moseley. He also observed that when a metal is bombarded with high-speed electrons, X-rays are emitted.
Atomic number = Number of protons in the nucleus
= Number of electrons
The sum of number of protons and neutrons present in the nucleus is called mass number and is a whole number.
Mass number (A)
= Number of protons + Number of neutrons
= Number of electrons + Number of neutrons
= Atomic number + Number of neutrons
The first simple model of the atom was proposed by JJ Thomson. According to this model, an atom has a uniform region (radius approximately 10-¹⁰ m) of positive charge with electrons embedded in such a way as to give the most stable electronic arrangement. This model had failed.
The α-particle scattering experiments conducted by Rutherford are related to the discovery of nuclei.
The following conclusions were drawn from these experiments
A major portion of atom is empty space because most ot α-particles passed straight through the atom.
An atom has a very small, rigid, positively charged body called a nucleus. Due to this positively charged part α-particles are repelled from the metal foil.
The entire mass of an atom is concentrated in the nucleus, so it is very heavy and hard.
Main Postulates
Niels Bohr proposed this atomic model which is based upon the Planck's quantum theory of radiations.
The electrons in an atom move around the nucleus in only selected circular paths called orbits. Each orbit has a certain amount of energy.
Electron in the particular orbit, does not lose or gain energy.
Only those orbits are permitted in which the angular momentum ot the electron is a whole number multiple of h/2Ï€ ⇒ ('h' is Planck's constant).
Energy is emitted when an electron jumps from a higher energy level to a lower energy level and energy is absorbed when an electron jumps from a lower energy level to a higher energy level.
The arrangement of electrons in different shells of an atom is known as electronic configuration of the element.
Following rules are used to write the electronic configuration
According to this principle, "the sub-shells are filled with electrons in increasing order of their energy." That is, the lower energy subshells will be filled with electrons first.
Cr = 1s², 2s², 2p⁶, 3s², 3p⁶, 3d⁵, 4s¹
Cu = 1s², 2s², 2p⁶, 3s², 3p⁶, 3d¹⁰, 4s¹
According to this rule, "Pairing of electrons in a sub-shell starts after all the available atomic orbitals or the sub-shell are singly filled (half filled)"
It states that, "No two electrons can have the same value of the four quantum numbers".
Knowledge Update
- Exactly half filled subshells have less energy and thus assume greater stability than any other arrangement. Thus, p³ is more stable arrangement than p², p⁴ or p⁵.
Species having same number of electrons are known as iso-electronic, e.g, NH3 or H3O^+ are iso-electronic.
Radioactivity can be defined as the spontaneous emission of suitable particle and electromagnetic radiations by unstable nuclei.
It was discovered by Prof. Henre Becquerel in 1896.
The three rays emitted from radioactive substance are
Nuclear Stability
Due to the very small size of the nucleus, there are very high repulsive forces between protons. The presence of neutrons in the nucleus reduces these forces. Therefore, the stability of the nucleus depends on the ratio of n and p, i.e., n/p. For stable nucleus, n/p should be 1.0 - 1.6.
During disintegration of an atom, either an α-particle or a β-particle is emitted.
α-Emission During α-emission from a nucleus, its mass number decreases by 4 and charge number by 2, i.e.,
β-Emission During β-Emission from a nucleus, its mass number remains same while atomic number increases by 1, e.g.,
γ-Emission During γ--emission, mass number and atomic number remain same.
Half-Life Period (t1/2) The time during which half the number of atoms present initially in the element decay is known as half life period.
N = N0 × (1/2)^n and T = t1/2 × n
Where, N0 = Initial amount
N = Remaining amount
T = Total time
n = Number of half lives
t1/2 = 0.693/k
Where, k = decay constant
Average Life Period = T = 1/k = t1/2/0.693 = 1.44 t1/2
The transformation of a stable nucleus into another nucleus by pre-bombing it with suitable high energy particles is called artificial transformation, e.g., -------
It is the phenomenon of the splitting of a heavy nucleus into two or more lighter nuclei with the evolution of a large amount of energy, for example,
92U²³⁵ + 0n¹ → 56Ba¹³⁹ + 36Kr⁹⁴ + 30n¹ + E
Two types of chain reactions occur in nuclear fission.
It is the phenomenon of fusion of two or more lighter nuclei to form a heavier nucleus that contains a large amount of energy, Example, the energy of the hydrogen bomb and sum.
1H² + 1H² → 2He⁴ + 17.6 MeV
Important TIPS
- Isotopes have same number of protons but different number of neutrons
- Isotones have same number of neutrons.
- Radioactivity does not change with temperature, pressure, etc.
- Extranuclear part of atom contains electrons.
Half life period, t1/2 = 0.693/k (k = decay constant)
Average life = 1/k 1.44 × t1/2
- Nuclear fusion is source of sun's energy.
- The principle of the atomic bomb is based on nuclear fission and the hydrogen bomb is nuclear fusion.
- β-particle is strongest reducing agent.
- Cu and Cr are exceptions to Aufbau's principle.
Energy of an electron in
nth orbit (En) = -13.6Z²/n² eV/atom
Radius of nth orbit (rn) = 5.53n²/Z Ã…
Velocity of e- in nth orbit = 2.18 × 108Z cm/s
Z = Atomic number
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