Chemistry topic 2 Fundamental Particles Atoms have a central nucleus (protons and neutrons) surrounded by orbiting electrons in shells. Protons have a +1 charge, neutrons have 0 charge, and electrons have a -1 charge. Relative mass: proton = 1, neutron = 1, electron = 1/1840. Maximum electrons per shell: 2n^2 (n = shell number). Atomic number (Z) = number of protons. Mass number (A) = sum of protons and neutrons. Isotopes Isotopes: atoms of the same element with the same atomic number but different neutron numbers. Same chemical behavior due to identical proton and electron configurations. Different physical properties due to varying mass numbers. Relative Masses Relative atomic mass (Ar): Mean mass of an element's atom relative to 1/12 of carbon-12. Relative isotopic mass: Isotopic mass relative to 1/12 of carbon-12. Relative molecular mass (Mr): Mean mass of a compound's molecule relative to 1/12 of carbon-12, calculated by adding Ar values of component elements. Relative formula mass: Similar to Mr, used for giant structures. Ions and Mass Spectrometry Ions are formed when atoms gain or lose electrons, resulting in an overall charge. Mass spectrometry identifies isotopes and determines relative atomic mass. Time of Flight (TOF) Mass Spectrometry Ionization: Vaporized sample ionized, forming +1 ions. Acceleration: Ions accelerated towards a negative plate. Ion drift: Magnetic field deflects ions. Detection: Ions hit the detector, producing a current proportional to abundance. Analysis: Spectra generated, displaying isotope abundance. Ions with a 2+ charge have half the expected m/z ratio. Ar = \frac{\sum(m/z \times abundance)}{\sum abundance}. Predicting Mass Spectra Spectra can be predicted from isotope abundances. Example: Chlorine spectra show characteristic patterns due to the presence of ^{35}Cl and ^{37}Cl isotopes. Ionisation Energy Ionization energy: Minimum energy to remove one mole of electrons from one mole of gaseous atoms (kJmol^{-1}). Na(g) \rightarrow Na^+(g) + e^- Successive ionization energies increase due to increasing electrostatic attraction. Factors influencing ionization energy: number of protons, electron shielding, and subshell. Ionization energy increases across a period and decreases down a group. Sudden large increases in successive ionization energies indicate a change in energy level. Electron Orbitals Electrons are held in orbitals (s, p, d, f), each holding up to 2 electrons with opposite spins. Electron Configurations Fill the lowest energy orbital first. Electrons with the same spin fill orbitals before pairing. No orbital holds more than 2 electrons. Exceptions: Half-full or completely full d sublevels are more stable. Chromium: 1s^22s^22p^63s^23p^63d^54s^1 Copper: 1s^22s^22p^63s^23p^63d^{10}4s^1 Periodicity Periodicity: Repeating patterns of physical/chemical properties in the Periodic Table. Elements in the same period have the same number of electron shells. Elements in the same group have the same number of outer electrons. Blocks: s-block (groups 1, 2), p-block (groups 3-0), d-block (transition metals), f-block (radioactive elements). Atomic radius decreases across a period and increases down a group. Ionization energy increases across a period and decreases down a group. Physical Properties of Period 2 Melting points peak towards the middle due to bond strength and structure. Li and Be: Metallic bonding, MP increases (Be > Li). B and C: Giant covalent lattices, high melting points. N, O, F, Ne: Simple covalent molecules, low melting points due to weak van der Waals forces. Ionization energies generally increase across the period (exceptions: B and O). Physical Properties of Period 3 Melting points: Na, Mg, Al (metallic, MP increases), Si (macromolecular, very high MP), P, S, Cl (simple covalent, low MP), Ar (noble gas, very low MP). Ionization energies generally increase across the period (exceptions: Al and S). Knowt Play Call Kai