The Elements Periodic Trends
Where did the elements come from? Naturally-from the centers of the stars Technetium, Promethium, Neptunium are not found on earth but have been detected in the spectra of stars Synthetically-made by cyclotrons and synchrotrons
Nuclear Reactions Fusion is the nuclear reaction that creates newer and larger elements from simpler elements Nuclear Fusion reactions can only take place under conditions of extreme heat (such as the conditions found in stars) where the kinetic energy of the particles is so great (high temperature) that it can overcome the repulsion between positively charged protons
Big Bang 12-16 billion years ago the entire universe could fit on the head of a pin Huge, violent explosion that occurred within a split second (the big bang) Immediately afterwards temperatures were in the millions of Kelvins (extremely high kinetic energy)
Matter as we know it… At extremely high temperatures matter existed as energy only  E=mc 2 Universe cooled as it expanded As it cooled the energy converted to matter in the form of electrons, protons, and neutrons
Nebula-the birthplace of stars
More Matter… As the Universe continued to cool the particles formed the first atoms All Hydrogen The H accumulated and formed first generation stars Nuclear reactions took place in the centers of stars forming the elements
Natural States of the Elements on Earth Most are found in compounds Few are found as pure elements Gold, silver, copper, platinum relatively inactive and found in pure states Francium and astatine only found in minute amounts Transuranium elements are synthesized and are not naturally occurring
Periodic Trends and Definitions Periodic Trends arise from the arrangement of the periodic table in periods, and groups that have similar chemical and physical properties A trend is a predictable change in a property towards a particular direction  Properties include electronegativity, ionization energy, atomic radius, density, melting point, boiling point
Electronegativity The ability of an atom to attract electrons to itself (electron affinity) A calculated value based on the attraction of shared electrons to a particular atom in a chemical bond
Ionization Energy The energy needed to remove an outer electron from an atom (in the ground state, gas phase) Calculated as the minimum energy required to be absorbed by the electron/atom in order to remove an electron from an isolated atom in it’s ground state
Atomic Radius The volume occupied by the electrons surrounding the nucleus Difficult to determine Usually determined for atoms that are chemically bonded Defined as 1/2 the distance between the nuclei of the atoms on a molecule Called the  bond radius
Density Mass per unit volume Usually determined at ambient temperatures (20  o C) Determined for the most thermodynamically stable allotrope Often in g/cm 3
Melting Point/Boiling Point Melting point is the temperature at which the solid and liquid phases coexist in equilibrium (at a standard pressure) Boiling Point is the temperature at which the vapor pressure of a liquid is equal to the external atmospheric pressure at 1 atm

Minooka-Elements Periodic Trends

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  • 2.
    Where did theelements come from? Naturally-from the centers of the stars Technetium, Promethium, Neptunium are not found on earth but have been detected in the spectra of stars Synthetically-made by cyclotrons and synchrotrons
  • 3.
    Nuclear Reactions Fusionis the nuclear reaction that creates newer and larger elements from simpler elements Nuclear Fusion reactions can only take place under conditions of extreme heat (such as the conditions found in stars) where the kinetic energy of the particles is so great (high temperature) that it can overcome the repulsion between positively charged protons
  • 4.
    Big Bang 12-16billion years ago the entire universe could fit on the head of a pin Huge, violent explosion that occurred within a split second (the big bang) Immediately afterwards temperatures were in the millions of Kelvins (extremely high kinetic energy)
  • 5.
    Matter as weknow it… At extremely high temperatures matter existed as energy only E=mc 2 Universe cooled as it expanded As it cooled the energy converted to matter in the form of electrons, protons, and neutrons
  • 6.
  • 7.
    More Matter… Asthe Universe continued to cool the particles formed the first atoms All Hydrogen The H accumulated and formed first generation stars Nuclear reactions took place in the centers of stars forming the elements
  • 8.
    Natural States ofthe Elements on Earth Most are found in compounds Few are found as pure elements Gold, silver, copper, platinum relatively inactive and found in pure states Francium and astatine only found in minute amounts Transuranium elements are synthesized and are not naturally occurring
  • 9.
    Periodic Trends andDefinitions Periodic Trends arise from the arrangement of the periodic table in periods, and groups that have similar chemical and physical properties A trend is a predictable change in a property towards a particular direction Properties include electronegativity, ionization energy, atomic radius, density, melting point, boiling point
  • 10.
    Electronegativity The abilityof an atom to attract electrons to itself (electron affinity) A calculated value based on the attraction of shared electrons to a particular atom in a chemical bond
  • 11.
    Ionization Energy Theenergy needed to remove an outer electron from an atom (in the ground state, gas phase) Calculated as the minimum energy required to be absorbed by the electron/atom in order to remove an electron from an isolated atom in it’s ground state
  • 12.
    Atomic Radius Thevolume occupied by the electrons surrounding the nucleus Difficult to determine Usually determined for atoms that are chemically bonded Defined as 1/2 the distance between the nuclei of the atoms on a molecule Called the bond radius
  • 13.
    Density Mass perunit volume Usually determined at ambient temperatures (20 o C) Determined for the most thermodynamically stable allotrope Often in g/cm 3
  • 14.
    Melting Point/Boiling PointMelting point is the temperature at which the solid and liquid phases coexist in equilibrium (at a standard pressure) Boiling Point is the temperature at which the vapor pressure of a liquid is equal to the external atmospheric pressure at 1 atm