ATOMIC STRUCTURE 1 The Atom 1.1 Subatomic Particles 1.2 Atomic Number, Mass Number and Isotopes 1.3 Deducing the Number of Protons, Neutrons and Electrons in an Atom / Ion 1.4 Isotopes 1.5 Determination of Relative Atomic Mass 1.5.1 Mass Spectrometry 1.5.2 Features of a Mass Spectrometer 1.5.3 Relative Abundance (Isotopic Composition and Relative Atomic Mass) 1.5.4 Mass Spectra 1.6 Applications of Mass Spectrometry 2 Electron Configuration 2.1 Relative Energies of Orbitals 2.2 Atomic Orbitals and Electron Density Plots 2.3 Writing Electron Configurations 2.4 Drawing Orbital Diagrams 2.5 Relationship between Electron Configurations and Position in the Periodic Table 3 Ionization 3.1 Ionization Energy 3.2 Patterns in Successive Ionization Energies 3.2.1 Evidence of Energy Levels and Sublevels 3.2.2 Deducing the Group of an Element from Successive Ionization Energy Data Recall the following definitions: Relative atomic mass, Ar, of any element is the weighted average mass of its isotopes when compared to one-twelfth the mass of a carbon-12 atom Relative molecular mass, Mr, of an element or compound is the mass of one molecule of that element or compound compared to one-twelfth the mass of a carbon-12 atom 1 The Atom Page 1 of 30 Dalton: all matter is made up of individual particles called atoms, which cannot be created or destroyed; atoms of the same element are alike in every single way Thomson: negatively charged electrons scattered in a positively charged sponge-like substance Rutherford: the atom is mainly empty space with a small dense positively charged centre, the nucleus Bohr: hydrogen pictured as a ‘solar system’, with electrons moving in energy levels around a positively charged nucleus; presence of neutrons (neutral charge) ensures stability of the nucleus of elements with more than 1 proton 1.1 Subatomic Particles Atoms are made up from smaller subatomic particles – protons, neutrons and electrons. Protons and neutrons are found in the positively charged dense nucleus of the atom. Collectively, protons and neutrons are called nucleons. Electrons move about in a volume of space around the nucleus. This volume of space is also called an electron cloud. There are discrete energy levels in this volume of space where there is a high probability of finding an electron. An electron density map represents the probability of finding an electron in a volume of space. Nucleus (protons, neutrons) Electrons (distributed in region of space around nucleus) Subatomic Particle Symbol Relative mass Relative charge proton p 1 +1 neutron n 1 0 electron e 5 10-4 (considered to be negligible) –1 The mass of an atom is concentrated in its small, positively charged nucleus. The electrostatic force of attraction between the protons and electrons holds the atom together; the neutral neutrons stabilise the nucleus. Page 2 of 30 1.2 Atomic Number, Mass Number and Isotopes Atomic number, Z, is the number of protons in the nucleus of an atom. It is the defining property of an element. Mass number, A, is the total number of protons and neutrons in the nucleus of an atom. Mass number = no. of p + n A Z X symbol of the element Atomic number = no. of p (= no. of e for atoms) Isotopes are atoms of the same element which contain the same number of protons but different number of neutrons (i.e. having the same atomic number but different mass numbers). Practice Example 1 Isotopes 12 6 C 13 6 C 14 6 C n+p 12 13 14 p 6 6 6 n 6 7 8 e 6 6 6 Isotopes chlorine-35 chlorine-37 Mass number 35 37 Atomic number 17 17 No. of neutrons 18 20 No. of electrons 17 17 Page 3 of 30 1.3 Deducing the Number of Protons, Neutrons and Electrons in an Atom / Ion The composition of a particular atom or ion can easily be deduced from the proton number, mass number and charge on the ion. Consider an atom, AZ X , a positive ion, A Z Xn+ , or a negative ion AZ Xn- Number of protons Number of neutrons Number of electrons X Z A–Z Z Symbol Atom A Z Cation A Z Xn+ Z A–Z Z–n Anion A Z Xn- Z A–Z Z+n Cations are formed when an atom loses one or more electrons. Anions are formed when an atom gains one or more electrons. Practice Example 2 No. of protons (Z) No. of neutrons (A – Z) 35 17 17 18 37 17 Cl 17 20 16 8 O2- 8 8 31 15 15 16 Species Cl P3- 1.4 No. of electrons 17 17 8 + 2 = 10 15 + 3 = 18 Isotopes Isotopes of the same element have identical chemical properties but different physical properties. identical chemical properties: presence of same number of electrons (and hence valence electrons) results in isotopes undergoing similar chemical bonding and reactions different physical properties: different number of neutrons (and hence mass numbers) results in isotopes having slightly varying density, boiling point, diffusion rates, with the lighter isotope diffusing more rapidly Page 4 of 30 Applications of radioisotopes Radioisotopes contain nuclei that break up spontaneously with the emission of radiation (which could be alpha particles, beta particles or gamma rays) involving a characteristic half-life which is the time taken for half of the radioactive nuclei to decay cobalt-60 in radiotherapy: damage the DNA of cancer cells by using 60Co (which can undergo beta and gamma decay) so that the cancer cells cannot undergo cell division iodine-125 as medical tracer: kill brain tumour tissue cells using 125I (which can undergo beta and gamma decay) so that the tissue cells cannot undergo cell division iodine-131 as medical tracer: diagnose whether a thyroid gland is functioning normally using 131I (which can undergo beta and gamma decay) so that the path of the radioisotope can be traced carbon-14 in radiocarbon dating: estimate the age of sample by comparing the content of 14C (which can undergo beta decay) in a dead organic sample with that in living tissue 1.5 Determination of Relative Atomic Mass The relative atomic mass (Ar) of an element is the weighted average mass of its isotopes compared to one-twelfth of the mass of carbon-12 atom. Ar = relative isotopic mass of each isotope relative (or percentage) abundance 1.5.1 Mass Spectrometry A mass spectrometer is used for the accurate determination of the i) relative atomic masses of atoms ii) relative molecular masses of molecular compounds iii) accurate mass of an individual nuclide/ isotope iv) identity/ structure of compounds Advantages of mass spectrometry: Requires only very little sample (10-12 g) Accurate Fast Page 5 of 30 1.5.2 Features of a Mass Spectrometer The working of a mass spectrometer may be summarised into 6 key steps: The sample to be tested is vapourized and injected into the mass spectrometer. The vapourised sample is bombarded with highenergy electrons which collide with the atoms of the sample. The beam of positive ions passes through a velocity selector which ensures all ions have the same velocity. The atoms lose an electron to form mainly singly charged positive ions (doubly charged positive ions may also be formed occasionally). The angle of deflection, θ depends on the charge-to-mass ratio )θ angle of deflection θ The ions are then accelerated by an electric field into the magnetic field, which causes the ions to be deflected into circular paths. q of the ion. m Each circular path of ions is brought to focus onto the detector which detects the number of ions passing through at each magnetic field setting and recorded as peaks in the form of a mass spectrum. q m For ions of the same charge, those with smaller mass are deflected to a greater extent. e.g. Angle of deflection: 1H+ > 2H+ > 3H+ For ions of the same mass, the more highly charged ions are deflected to a greater extent. e.g. Angle of deflection: 4He+ < 4He2+ Ions of the same q will be deflected to the same extent. m e.g. Angle of deflection: (12C1H4)+ = (14N1H2)+ Page 6 of 30 A mass spectrum is a plot of relative (or percentage) abundance against mass/charge (m/z ) ratio. 1.5.3 Relative Abundance (Isotopic Composition and Relative Atomic Mass) Practice Example 3 Chlorine atoms exists as a mixture of 2 isotopes, chlorine-35 and chlorine-37. Given that 25% of naturally chlorine atoms are chlorine-37 atoms, account for the relative atomic mass of chlorine that is reflected in the Periodic Table. % of chlorine-35 = 75 % Ar of Cl = 25 100 37 + 75 100 71 = 35.5 This value of Ar is comparable to the value reflected in the Periodic Table of 35.45. Practice Example 4 The relative atomic mass of gallium is 69.7. Gallium is made up of two isotopes Calculate the percentage abundance of 69Ga. 69 Ga and 71 Ga. Let the percentage abundance of 69Ga be x% 69.7 = x 69 + 71 = 65 The percentage abundance of 69Ga is 65% Page 7 of 30 1.5.4 Mass Spectra The mass spectrum of an element provides the following information: Feature of Mass Spectrum Information deduced number of peaks or lines number of isotopes present m/z value of each peak relative isotopic mass of each isotope (assume z = 1, i.e. only singly charged ions) relative (or percentage) abundance of each isotope Height of each peak The relative atomic mass, Ar, of an element can be calculated by determining the weighted average of isotopic masses according to their relative abundance. Practice Example 5 Deduce the relative atomic mass of boron from the data given in its mass spectrum. m/z Species B+ Isotope Relative Abundance 10 10 10 23 11 11 11 100 B+ 23 B B 100 Ar of B = ( 123 10) + ( 123 11) = 10.8 Page 8 of 30 Self Practice 1 Deduce the relative atomic mass of Mg from its mass spectrum. relative abundance 8 1 24 m/z 25 26 Species m/z Isotope Relative Abundance 24 24 Mg+ 24 8 25 25 Mg+ 25 1 26 26 Mg+ 26 1 Ar of Mg = ( 8 10 24) + ( 1 10 Mg Mg Mg 25) + ( 1 10 26) = 24.3 Self Practice 2 Deduce the relative atomic mass of the element iron from the data given. % abundance 91.68% 5.84% 54 m/z Species Fe+ 2.17% 56 0.31% 57 58 Isotope m/z % Abundance 54 54 54 5.84 56 56 56 91.68 57 57 57 2.17 58 58 58 0.31 Fe+ Fe+ Fe+ Ar of Fe = Fe Fe Fe Fe (54 5.84) + (56 91.68) + (57 2.17) + (58 0.31) 100 = 55.9 Page 9 of 30 For elements that exist as covalently bonded molecules (eg H2, Cl2, P4, S8): mass spectrum consists of peaks corresponding to molecules as well as isotopes molecule will give rise to more than 1 peak if more than 1 isotope is present relative abundance of these peaks can be calculated from the presence/ combination of various isotopes Practice Example 6 The element chlorine has 2 isotopes spectrum of chlorine gas (Cl2). 35 Cl and 37 Cl of relative abundance 3:1. Deduce the mass Possible peaks in mass spectrum of Cl2: m/z Species 35 (35Cl)+ 3 37 (37Cl)+ 1 70 (35Cl35Cl)+ 9 72 (35Cl37Cl)+ 6 74 (37Cl37Cl)+ 1 Relative Intensity Relative abundance Page 10 of 30 1.6 Applications of Mass Spectrometry Some applications of mass spectrometry include: radioactive dating drug testing (detection of anabolic steroids) space research identification of synthesised compounds (in the pharmaceutical industry) Radioactive Dating Depends on radioactive carbon-14 which occurs naturally in the atmosphere. Plants take up CO2 containing 14C (along with 12C) during photosynthesis. The proportion of 14C : 12C in living matter is exactly the same as in the atmosphere When an organism dies, it stops taking in carbon. The unstable radioactive decay over time, causing the 14C : 12C ratio to decrease. Half life of 14C is 5730 years. The level of 14C remaining in a sample can be determined by mass spectrometry. The amount of 14C detected is compared to calibration plots to deduce the age of the sample. 14 C undergoes slow Drug Testing Anabolic steroids, which can be used to build bigger muscles and enhance sport performance, are an artificial form of the male sex hormone testosterone. Both men and women produce testosterone, together with epitestosterone in their bodies. The normal ratio of testosterone to epitestosterone (T:E ratio) does not exceed 4:1. Taking anabolic steroids raises the T:E ratio. The T:E ratio in urine samples can be determined using mass spectrometry. When synthetic testosterone breaks down, its products also have a different ratio of 12 C as compared to the breakdown of natural testosterone. Mass spectrometry can also detect this present in the sample. 13 C : 13 C: 12 C to determine is synthetic hormone was Page 11 of 30 Space Research Mass spectrometers are sent into space to identify the gases present in the atmosphere of different planets. Mass spectrometry has also been used to analyse meteorites to provide a better understanding of the environment and life forms on other planets. In space shuttles, mass spectrometry is critical in quickly analysing gases in the shuttle to warn astronauts of any potential problems. Smaller portable mass spectrometers have also been fitted onto the astronauts’ suits to detect traces of leaking gases during space walks to serve as safety warnings to astronauts. 2 Electron Configuration The arrangement of electrons within these energy levels is called its electron configuration and can be deduced from the atomic number of the atom. 2.1 Relative Energies of Orbitals Electrons in an atom exist in discrete energy levels in a region of space around the nucleus. These spaces, each having a characteristic energy level, are known as orbitals. An orbital can be defined as a region of space around the nucleus where there is 90% probability of locating the electron. Some orbitals are close to the nucleus while others are a distance away. The arrangement of electrons (in their orbitals) in an atom is referred to as its electron configuration. Atomic Emission Spectra When energy is provided to a sample of hydrogen atoms, some of the energy is absorbed and electrons are excited from a lower energy level to a higher energy level. The excited state is unstable. The electron will fall back to the lower energy level known as its ground state. Emission spectra are produced when photons are emitted from atoms as excited electrons return to their ground state. An electron in the excited state returning to ground state emits energy corresponding to a particular wavelength in relation to the energy level difference. The emission spectrum is seen as a series of coloured lines at particular wavelengths (the colour corresponds to the wavelength of radiation emitted). Page 12 of 30 The spectrum can thus be regarded as a collection of lines due to different electron transitions. The line emission spectrum of hydrogen provides evidence for the existence of electrons in discrete energy levels. These fixed energy levels are labelled as n = 1, 2, ..., ∞. Main Energy Levels Each main energy level or shell in which electrons are found is assigned a integer number, n, i.e. n = 1, 2, 3 etc. n=4 n=3 n=2 n=1 The number n indicates the average distance of the orbitals from the nucleus. The smaller the value of n, the closer the electron is to the nucleus the more strongly the electron is bound to the nucleus. the lower the energy level of the electron Each main energy level can hold a different number of electrons. Maximum number of electrons each main energy level can hold = 2n2 Main energy level Maximum no. of electrons n=1 n=2 n=3 n=4 2 8 18 32 Electrons occupy energy levels from the lowest possible energy level (i.e. innermost electron shell) to the highest possible energy level (i.e. in the outermost electron shell). An atom in which all electrons are in the lowest possible energy levels is said to be at ground state. Valence electrons have the highest energy The position of an element in Periodic Table in relation to electron arrangement of an atom: Period number: number of electron shells occupied Group number: number of valence electrons Page 13 of 30 Sub-levels (Subshells) Each main energy level, n, is divided into sub-levels. The sub-levels are labelled as s, p, d or f. Generally, the order of energy levels for the sub-levels (within each quantum shell) is: s<p<d<f. Sub-levels contain a fixed number of orbitals (regions of space where there is a high probability of finding an electron). Each orbital has a defined energy state for a given electronic configuration and chemical environment and can hold a maximum of 2 electrons of opposite spin. Subshell No. of Orbitals Type of Orbitals s 1 s p 3 px, py, pz d 5 dxy, dxz, dyz, dz2, dx2-y2 f 7 2.2 Atomic Orbitals and Electron Density Plots s orbitals The s orbitals are spherical in shape. s-orbitals of different shells have the same shape but differ in size. Size of 1s orbital < 2s orbital < 3s orbital Distance of electrons from the nucleus in 1s orbital < 2s orbital < 3s orbital Page 14 of 30 p orbitals The p orbitals have a “dumb-bell” shape. There are 3 types of p orbitals – px, py and pz with different orientations in space. The orbitals within a given subshell (e.g. 2px, 2py, 2pz) have the same energy. p orbitals of different shells have the same shape but differ in size. Size of 2p orbital < 3p orbital Distance of electrons from the nucleus in 2p orbital < 3p orbital Relationship between main energy levels, sub-levels, orbitals and electrons Main energy level, n No. of sub-levels Type of sub-level No. of orbitals within sub-level No. of electrons within sub-level Maximum no. of electrons in main energy level (2n2) 1 1 1s 1 2 2 2 2 2s 1 2 8 2p 3 6 3s 1 2 3p 3 6 3d 5 10 4s 1 2 4p 3 6 4d 5 10 4f 7 14 3 4 3 4 18 32 Page 15 of 30 Relative Energies of Orbitals The relative energies level of the main energy levels and sub-levels in an atom: Energy level n=4 4f 4d 4p Note: 4s subshell has a lower energy level than 3d subshell (when it is not occupied by electrons). 3d n= 3 4s 3p 3s n=2 2p 2s n=1 main energy levels 1s sub-level orbitals Electron Spin Two electrons in the same orbital must have opposite spins. This is so that magnetic attraction which results from their opposite spins can counterbalance the electrical repulsion which results from their identical charges. The direction of spin of electrons can be indicated by arrows, and to represent anti-clockwise spin. to represent clockwise spin Note: Electrons can be thought of as spinning on an axis. Page 16 of 30 2.3 Writing Electron Configurations The electron configuration of an element refers to the arrangement of electrons of its atoms in their main energy levels, sub-levels and orbitals. Notation for writing electron configuration: 2p1 main energy level number of electrons in sub-level / subshell sub-level/ subshell 2.4 Drawing Orbital Diagrams The arrangement of electrons in a specie can also be represented in an orbital diagrams, which shows the arrangement of electrons as well as the spin of the electron. Notation for orbital diagrams to represent electron configuration: Example: For main energy level n = 3, 3s 3p sub-level 3d orbital main energy level, n=3 Aufbau Principle Electrons occupy the lowest energy orbital first before occupying the higher energy orbitals. Order of filling orbitals NOTE When adding electrons, fill up 4s before 3d. When removing electrons, remove from 4s before 3d. Page 17 of 30 Pauli’s Exclusion Principle Each orbital can hold a maximum of 2 electrons. The two electrons must be in opposite spins. NOT 2 electrons can occupy the same orbital (region of space) despite their mutual repulsion as they spin in opposite directions. Hund’s Rule Orbitals of a sub-level (subshell) must be occupied singly and with parallel spins before pairing occurs. This is to ensure electrons are as far apart as possible to minimise electronic repulsion. NOT NOT Note: When an orbital contains only one electron, the electron is said to be unpaired. If the above rules are followed, electrons occupy the lowest possible energy and the resultant arrangement of electrons is known as ground state electronic configuration. (Lowest energy state) When one or more electrons absorb energy and are promoted to a higher energy level, the atom is said to be in an excited state. Ground State Electronic Configurations of Atoms Element Atomic No. He 2 Orbital Diagram for Ground State Electron Configuration Write the Ground State Electron Configuration Full: 1s2 1s Full: 1s2 2s2 2p2 C 6 1s 2s 2p Condensed: [He] 2s2 2p2 Ne Full: 1s2 2s2 2p6 10 1s 2s 2p Page 18 of 30 Element Cl Atomic No. 17 Orbital Diagram for Ground State Electron Configuration 1s 2s 2p 3s Write the Ground State Electron Configuration Full: 1s2 2s2 2p6 3s2 3p5 Condensed: [Ne] 3s2 3p5 3p Ar 18 1s 2s 2p 3s 2s 2p 3s Full: 1s2 2s2 2p6 3s2 3p6 3p Ca 20 1s Full: 1s2 2s2 2p6 3s2 3p6 4s2 Condensed: [Ar] 4s2 3p 1s V 4s 2s 2p 3s 23 3p 3d Full: 1s2 2s2 2p6 3s2 3p6 3d3 4s2 Condensed: [Ar] 3d3 4s2 4s 1s Cr 2s 2p 3s 24 3p 3d Full: 1s2 2s2 2p6 3s2 3p6 3d5 4s1 Condensed: [Ar] 3d5 4s1 4s 1s Cu 2s 2p 3s 29 3p 3d Full: 1s2 2s2 2p6 3s2 3p6 3d10 4s1 Condensed: [Ar] 3d10 4s1 4s Page 19 of 30 Element Atomic No. Orbital Diagram for Ground State Electron Configuration 1s As 2s 2p 3d 4s Condensed: [Ar] 3d10 4s2 4p3 4p 1s 2s 2p 3s Full: 1s2 2s2 2p6 3s2 3p6 3d10 4s2 4p4 34 3p 3d 4s 2s 2p 3s 36 3p 4s Condensed: [Ar] 3d10 4s2 4p4 4p 1s Kr Full: 1s2 2s2 2p6 3s2 3p6 3d10 4s2 4p3 33 3p Se 3s Write the Ground State Electron Configuration 3d Full: 1s2 2s2 2p6 3s2 3p6 3d10 4s2 4p6 4p Note: In 3d-block elements, the 3d and 4s orbitals are close in energy. The 4s orbitals are filled first, followed by the 3d orbitals (with the exception of Cr and Cu). Cr atom gains extra stability with half-filled 3d subshell. The configuration 1s2 2s2 2p6 3s2 3p6 3d5 4s1 is more stable than 1s2 2s2 2p6 3s2 3p6 3d44s2. Cu atom gains extra stability with a fully-filled 3d subshell. The configuration 1s2 2s2 2p6 3s2 3p6 3d10 4s1 is more stable than 1s2 2s2 2p6 3s2 3p6 3d9 4s2. Page 20 of 30 Ground State Electronic Configurations of Ions Orbital Diagram for Ground State Electronic Configuration Particle Formula Write the Ground State Electronic Configuration Full: 1s2 2s2 2p5 atom ion atom F 1s 2s 2p Condensed: [He] 2s2 2p5 Full: 1s2 2s2 2p6 – F 1s 2s 2p Condensed: [Ne] Full: [Ne] 3s2 Mg 1s 2s 2p 3s Full: 1s2 2s2 2p6 ion Mg2+ 1s 2s 2p Condensed: [Ne] 1s atom 2s 2p 3s Full: 1s2 2s2 2p6 3s2 3p6 3d7 4s2 Co 3p 3d Condensed: [Ar] 3d7 4s2 4s ion Co2+ 1s 2s 2p 3s Full: 1s2 2s2 2p6 3s2 3p6 3d7 4s2 Condensed: [Ar] 3d7 3p 3d Page 21 of 30 Isoelectronic Species Atoms/ions with the same electronic configuration (same number of electrons) are said to be isoelectronic. Isoelectronic species Electronic configuration Note Ne O2- 1s2 2s2 2p6 Na+ Ar P3- 1s2 2s2 2p6 3s2 3p6 Electron configuration can also be represented using a Noble Gas ‘Core’ e.g. electron configuration of O2represented as [Ne] and that of Ca2+ as [Ar] Ca2+ Self Practice 3 For each of the following species, (a) draw the orbital diagram to show its electron configuration (b) write its full electron configuration and its condensed form using the noble gas core. (i) Ge orbital diagram: full electron configuration: 1s2 2s2 2p6 3s2 3p6 3d10 4s2 4p2 condensed electron configuration: [Ar] 3d10 4s2 4p2 (ii) O2– orbital diagram: full electron configuration: 1s2 2s2 2p6 condensed electron configuration: [Ne] (iii) Fe2+ orbital diagram: full electron configuration: 1s2 2s2 2p6 3s2 3p6 3d6 condensed electron configuration: [Ar] 3d6 Page 22 of 30 (iv) Fe3+ orbital diagram: full electron configuration: 1s2 2s2 2p6 3s2 3p6 3d5 condensed electron configuration: [Ar] 3d5 (v) Cu+ orbital diagram: full electron configuration: 1s2 2s2 2p6 3s2 3p6 3d10 condensed electron configuration: [Ar] 3d10 2.5 Relationship between Electron Configurations and Position in the Periodic Table Elements in the same (main) Groups have the same outermost electronic configuration in their atoms. Group I II III IV V VI VII 0 Outermost electron configuration ns1 ns2 ns2np1 ns2np2 ns2np3 ns2np4 ns2np5 ns2np6 except He s-block d-block p-block For main Group elements, No. of valence electrons = Group Number s-block p-block d-block Page 23 of 30 3 Ionization Recall: electrons exist in discrete energy levels around the nucleus. When an electron is at the highest energy level n = , it is no longer in the atom and the atom is said to be ionized. 3.1 Ionization Energy The first ionization energy (1st I.E.) of an element is the energy required to remove one mole of electrons from one mole of gaseous its atoms. X(g) X+(g) + eExample 1st I.E. of magnesium: Mg (g) Mg+(g) + e 1st I.E. = +736 kJ mol-1 The second ionisation energy (2nd I.E.) of an element is the energy required to remove one mole of electrons from one mole of singly positively charged gaseous ions. X+ (g) X2+ (g) + e Example 2nd I.E. of magnesium: Mg+ (g) Mg2+ (g) + e 2nd I.E. = +1450 kJ mol-1 Note: The higher the ionisation energy of an element, the more difficult it is to remove an electron. The 2nd I.E. > 1st I.E. because more energy is required to remove an electron from a positive ion (compared to a neutral atom) due to greater net electrostatic attraction. COMMON MISTAKE: Mg(g) Mg2+(g) + 2e represents 2nd ionisation energy !!WRONG!! The above equation represents the sum of 1St I.E. and 2nd I.E. 3.2 Patterns in Successive Ionization Energies There is a general increase in successive ionisation energy because an increasing amount of energy required to remove successive electrons from an increasingly positive ion due to an increasing NET electrostatic attraction between the nucleus and valence electrons. X (g) X+(g) + e 1st I.E. X+(g) X2+(g) + e 2nd I.E. X2+(g) X3+(g) + e 3rd I.E. Page 24 of 30 3.2.1 Evidence of Energy Levels and Sublevels Successive ionization energy data for an element can show the arrangement of electrons around the nucleus, i.e. the electron configuration of the element. The following information can be obtained from a plot of successive ionization energies against the order of removal of electrons: (a) Number of electrons in an atom (b) Number of main energy levels occupied and the number of electrons in each (c) Number of sub-levels occupied and the number of electrons in each (d) Number of valence electrons in the atom Evidence of Main Energy Levels The following plot is obtained when all the electrons are successively removed from an atom. lg I.E. 6 5 4th main energy level 1 electron 2 electrons 1st main energy level 4 3 8 electrons 3rd main energy level 2 8 electrons 2nd main energy level 1 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 order of electrons removed Observation from plot Sharp increase in I.E. for removal of 2nd electron Deductions There is 1 valence electron The 2nd electron is in a different main energy level This is the highest-energy main energy level (furthest from nucleus) n=4 Gradual increase in I.E. for next 8 electrons There are 8 electrons in this main energy level This is the 2nd highest-energy main energy level (one inwards from the outermost) n=3 Another sharp increase in I.E. for removal of the 10th electron The 10th electron is removed from a different main energy level This is the 3rd highest-energy main energy level (two inwards from the outermost) n=2 Gradual increase in I.E. for next 8 electrons There are 8 electrons in this main energy level n=2 Page 25 of 30 Observation from plot Deductions The 18th electron is removed from a different main energy level Another sharp increase in I.E. for removal of the 18th electron This is the lowest-energy main energy level (closest to nucleus) n=1 There are 2 electrons in this main energy level Electron configuration of the atom may be deduced to be: 1s22s22p63s23p64s1 This is a Group 1 element Note: Some graphs may not show the successive removal of all electrons. In these cases, electron configuration of the element cannot be determined but Group number of the element can still be deduced. Evidence of Sub-levels in Main Energy Levels lg I.E. 3s 3p 1 2 3 4 5 6 7 8 9 order of electrons removed Zooming in on the section corresponding to the 3rd main energy level in the previous graph, it is observed that there is a steady increase in I.E.s for the removal of 2nd to 7th electrons these 6 electrons are in the same sub-level a minor increase (jump) in I.E. for the removal of the 8th electron 8th electron is removed from a different sub-level which is closer to the nucleus. There is stronger electrostatic force of attraction between the 8th electron and nucleus (since it is closer to the nucleus) and more energy is required to remove it. The above shows that the main energy level is further divided into sub-levels (labelled as 3s and 3p) which are occupied by two and six electrons respectively. Page 26 of 30 3.2.2 Deducing the Group of an Element from Successive Ionization Energy Data To determine the Group to which an element belongs to, we must determine the number of valence electrons. The point where a big increase in I.E. occurs indicates the removal of successive electrons from an inner main energy level. Practice Example 7 From the following data, predict the Group to which this element belongs and write its electron configuration. I.E. kJ mol-1 1st 2nd 3rd 4th 900 1758 14905 21060 Work out the difference between the 1st & 2nd IE, 2nd & 3rd IE, 3rd & 4th IE. There is a sharp increase in I.E. for removal of the 3rd electron (as indicated by the largest difference in IE between 2nd IE & 3rd IE). 3rd electron is removed from an inner main energy level which is closer to the nucleus. Hence, there is stronger electrostatic force of attraction between the 3rd electron and nucleus and more energy is required to remove it The element has 2 valence electrons The element belongs to Group 2. Hence, the valence electron configuration of the element is ns2. Page 27 of 30 Practice Example 8 The following element has the following successive ionisation energies when all its electrons are successively removed. (i) Deduce the Group number of the element. (ii) Deduce the total number of quantum shells. (iii) Write the electron configuration of the element. (i) There is a sharp increase in I.E. for removal of the 3rd electron (as indicated by the largest difference in IE between 2nd IE & 3rd IE). (ii) 3rd electron is removed from an inner main energy level which is closer to the nucleus. Hence, there is a stronger electrostatic force of attraction between the 3rd electron and nucleus and more energy is required to remove it. The element has 2 valence electrons The element belongs to Group 2. From the graph, Total number of electrons = 12 There should be 3 main energy levels / 3 electron shells ( i.e. n = 3 ) (Note also there are 3 regions of gradual increase in I.E.) (iii) Electron configuration: 1s22s22p63s2 Challenge yourself to explain this: Group I elements have high 2nd I.E. Group II elements have high 3rd I.E. Group III elements have high 4th I.E. Group IV elements have high 5th I.E. Group V elements have high 6th I.E. Group VI elements have high 7th I.E. Group VII elements have high 8th I.E. Page 28 of 30 Self Practice 4 Deuce the electron configuration of the element from its successive ionization energies given. Successive removal of 20 electrons from element Removal of 1st electron: Ca(g) → Ca+(g) + eRemoval of 2nd electron: Ca+(g) → Ca2+(g) + e...... Removal of 19th electron: Ca18+(g) → Ca19+(g) + eRemoval of 20th electron: Ca19+(g) → Ca20+(g) + e- No. of electrons removed There is a sharp increase in I.E. for removal of the 3rd , 11th and 19th electrons 3rd , 11th and 19th electrons are removed from main energy levels successively closer to the nucleus. There are stronger electrostatic forces of attraction between the nucleus and the electrons closer to it and more energy is required to remove these electrons 1st and 2nd electrons removed are from the outermost electron shell (highest energy level) (The element has 2 valence electrons) 3rd to 10th electrons removed are from an inner main energy level (one inwards from the outermost) 11th to 18th electrons removed are from an inner main energy level closer to nucleus 19th and 20th electrons removed are from the innermost energy level electron configuration: 1s2 2s2 2p6 3s2 3p6 4s2 Page 29 of 30 Self Practice 5 Deduce the group number for an unknown element given its first eight successive ionization energies in kJ mol-1. 580 1800 2750 11580 14850 18400 23300 27500 There is a sharp increase in I.E. for removal of the 4th electron 4th electron is removed from an inner main energy level which is closer to the nucleus. Hence, there is stronger electrostatic force of attraction between the 4th electron and nucleus and more energy is required to remove it 1st to 3rd electrons removed are from the outermost energy level 4th to 8th electrons removed are from an inner shell (one inwards from the outermost) The element has 3 valence electrons The element belongs to Group 13. (valence electron configuration of the element is ns2 np1) Page 30 of 30