chapter 12 the periodic table the how and why. history u russian scientist dmitri mendeleev taught...

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Chapter 12 The Periodic Table The how and why The how and why

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Page 1: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Chapter 12The Periodic Table

The how and whyThe how and why

Page 2: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

History Russian scientist Dmitri Mendeleev

taught chemistry in terms of properties.

Mid 1800 - molar masses of elements were known.

Wrote down the elements in order of increasing mass.

Found a pattern of repeating properties.

Page 3: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Mendeleev’s Table Grouped elements in columns by similar

properties in order of increasing atomic mass.

Found some inconsistencies - felt that the properties were more important than the mass, so switched order.

Found some gaps. Must be undiscovered elements. Predicted their properties before they

were found.

Page 4: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

The modern table Elements are still grouped by

properties. Similar properties are in the same

column. Order is in increasing atomic number. Added a column of elements Mendeleev

didn’t know about. The noble gases weren’t found because

they didn’t react with anything.

Page 5: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Horizontal rows are called periods

Page 6: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Vertical columns are called groups.

Elements are placed in columns by similar properties.

Also called families

Page 7: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

The group B are called the transition elements

These are called the inner transition elements and they belong here

Page 8: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group 1 are the alkali metals Group 2 are the alkaline earth metals

Page 9: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group 7 is called the Halogens Group 8 are the noble gases

Page 10: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Why? The part of the atom another atom

sees is the electron cloud. More importantly the outside

orbitals. The orbitals fill up in a regular

pattern. The outside orbital electron

configuration repeats. The properties of atoms repeat.

Page 11: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

1s1

1s22s1

1s22s22p63s1

1s22s22p63s23p64s1

1s22s22p63s23p64s23d104p65s1

1s22s22p63s23p64s23d104p65s24d10 5p66s1

1s22s22p63s23p64s23d104p65s24d105p66s2

4f145d106p67s1

H1

Li3

Na11

K19

Rb37

Cs55

Fr87

Page 12: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

He2

Ne10

Ar18

Kr36

Xe54

Rn86

1s2

1s22s22p6

1s22s22p63s23p6

1s22s22p63s23p64s23d104p6

1s22s22p63s23p64s23d104p65s24d105p6

1s22s22p63s23p64s23d104p65s24d10

5p66s24f145d106p6

Page 13: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Atomic Size First problem where do you start

measuring. The electron cloud doesn’t have a

definite edge. They get around this by measuring

more than 1 atom at a time.

Page 14: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Atomic Size

Atomic Radius = half the distance between two nuclei of a diatomic molecule.

}Radius

Page 15: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Trends in Atomic Size Influenced by two factors. Energy Level Higher energy level is further

away. Charge on nucleus More charge pulls electrons in

closer.

Page 16: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group trends As we go down a

group Each atom has

another energy level,

So the atoms get bigger.

HLi

Na

K

Rb

Page 17: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Periodic Trends As you go across a period the radius

gets smaller. Same energy level. More nuclear charge. Outermost electrons are closer.

Na Mg Al Si P S Cl Ar

Page 18: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Overall

Atomic Number

Ato

mic

Rad

ius

(nm

)

H

Li

Ne

Ar

10

Na

K

Kr

Rb

Page 19: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Ionization Energy The amount of energy required to

completely remove an electron from a gaseous atom.

Removing one electron makes a +1 ion.

The energy required is called the first ionization energy.

Page 20: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

What determines IE The greater the nuclear charge the

greater IE. Distance form nucleus increases IE Filled and half filled orbitals have

lower energy, so achieving them is easier, lower IE.

Shielding

Page 21: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Shielding The electron on the

outside energy level has to look through all the other energy levels to see the nucleus

Page 22: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Shielding The electron on the

outside energy level has to look through all the other energy levels to see the nucleus.

A second electron has the same shielding.

Page 23: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group trends As you go down a group first IE

decreases because The electron is further away. More shielding.

Page 24: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Periodic trends All the atoms in the same period

have the same energy level. Same shielding. Increasing nuclear charge So IE generally increases from left to

right. Exceptions at full and 1/2 fill orbitals.

Page 25: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Firs

t Ion

izat

ion

ener

gy

Atomic number

He

He has a greater IE than H.

same shielding greater nuclear

charge

H

Page 26: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Firs

t Ion

izat

ion

ener

gy

Atomic number

H

He

Li has lower IE than H

more shielding further away outweighs greater

nuclear charge

Li

Page 27: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Firs

t Ion

izat

ion

ener

gy

Atomic number

H

He

Be has higher IE than Li

same shielding greater nuclear

charge

Li

Be

Page 28: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Driving Force Full Energy Levels are very low

energy. Noble Gases have full orbitals. Atoms behave in ways to achieve

noble gas configuration.

Page 29: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Ionic Size Cations form by losing electrons. Cations are smaller that the atom

they come from. Metals form cations. Cations of representative elements

have noble gas configuration.

Page 30: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Ionic size Anions form by gaining electrons. Anions are bigger that the atom they

come from. Nonmetals form anions. Anions of representative elements

have noble gas configuration.

Page 31: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Configuration of Ions Ions always have noble gas

configuration. Na is 1s12s22p63s1 Forms a +1 ion - 1s12s22p6 Same configuration as neon. Metals form ions with the

configuration of the noble gas before them - they lose electrons.

Page 32: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Configuration of Ions Non-metals form ions by gaining

electrons to achieve noble gas configuration.

They end up with the configuration of the noble gas after them.

Page 33: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group trends Adding energy level Ions get bigger as

you go down.

Li+1

Na+1

K+1

Rb+1

Cs+1

Page 34: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Electronegativity The tendency for an atom to attract

electrons to itself when it is chemically combined with another element.

How fair it shares. Big electronegativity means it pulls

the electron toward it. Atoms with large negative electron

affinity have larger electronegativity.

Page 35: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Group Trend The further down a group the farther

the electron is away and the more electrons an atom has.

More willing to share. Low electronegativity.

Page 36: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Periodic Trend Metals are at the left end. They let their electrons go easily Low electronegativity At the right end are the nonmetals. They want more electrons. Try to take them away. High electronegativity.

Page 37: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Ionization energy, electronegativity

Electron affinity INCREASE

Page 38: Chapter 12 The Periodic Table The how and why. History u Russian scientist Dmitri Mendeleev taught chemistry in terms of properties. u Mid 1800 - molar

Atomic size increases, shielding constant

Ionic size increases