|
Part 1
Historical Introduction page sub-index: 1.1 The
early classification of Antoine Lavoisier of 1789 * 1.2 The 1829 work of
Johann Döbereiner *
1.3 The work of John
Newlands 1864 * 1.4 Dmitri Mendeleev's
Periodic Table of 1869 * 1.5 A modern Periodic Table based on the electronic structure of
atoms * 1.6 Where did the elements come from
originally and where do we get the elements from?
Advanced Periodic Table Index *
Part 2
Electronic structure of atoms :
Spectroscopy and the H spectrum :
Ionisation energies *
Part 3
Period 1 survey : 1. Hydrogen
:
2. Helium : Summary of
Period 1 : heavier element
formation-stellar nuclear fusion *
Part 7
s-block metals Groups 1/2 Alkali/Alkaline Earth Metals *
Part 10
3d-block Sc-Zn and Transition Metals *
Part 11
Group and Series data summaries
and links to periodicity plots *

1. A
few snippets of the past and continuing history
of the Periodic Table
Not all
scientists are mentioned who perhaps should be, but I've tried to pick
out a few 'highlight' and added some footnotes on what was happening in
terms of the development of the detailed knowledge of the structure of
atoms, so essential to the modern interpretation of the Periodic Table.
Its a good 'advanced' example of how science works i.e. the relationship
between experimental data and theories to account for it, questions
posed, questions answered, leading to more comprehensive and accurate
theories developing.
1.1 The
early classification of Antoine Lavoisier of 1789
|
Antoine
Lavoisier's 1789 classification of substances into four
'element' groups
|
| acid-making
elements |
gas-like
elements |
metallic
elements |
earthy
elements |
| sulphur |
light |
cobalt,
mercury, tin |
lime
(calcium oxide) |
| phosphorus |
caloric
(heat) |
copper,
nickel, iron, |
magnesia
(magnesium oxide) |
| charcoal
(carbon) |
oxygen |
gold,
lead, silver, zinc |
barytes
(barium sulphate) |
| |
azote
(nitrogen) |
manganese,
tungsten |
argilla
(aluminium oxide) |
| |
hydrogen |
platina
(platinum) |
silex
(silicon dioxide) |
- The understanding that an
element as a unique atomic 'building block' which could not be split
into simpler substances and compound is a chemical combination of
two or more elements were not at all understood at the time of
Lavoisier.
-
'light' and
'caloric' (heat), were considered 'substances' and the last
'scientific' vestige of the elements of 'earth, fire, air and water'
which had there conceptual origin in the Greek civilisation of
2300-2800 years ago.
-
However,
Lavoisier was correct on a few things e.g. the elements sulphur,
phosphorus and carbon and correctly described their oxides as acidic
e.g. dissolved in water turned litmus turns red.
-
Many metallic
elements, were correctly identified though I doubt if they were pure
though!
-
What he
described as the 'earthy elements' are of course compounds, a
chemical combination of a metal plus oxygen or sulfur (both O and S in case
of barium).
-
He didn't have
very high temperature smelting technology, or a reactive metal from
electrolysis (came in about 1806 onwards)' to 'separate' the
elements in some way e.g. he couldn't extract a reactive metal! In
other words, at this time, the wrong 'classification' was due to a
lack of chemical technology as much as lack of knowledge.
-
Atomic
structure history note: You can see from the 1789 'table'
Lavoisier and his contemporaries did not have the experiment
techniques, data or theoretical framework to clearly distinguish
between 'elements' and 'compounds'. It was only in 1808 Dalton
proposed his atomic theory based on experimental data and produced
the first list of 'atomic weights', which we now call relative
atomic masses.

1.2 The 1829 work of
Johann Döbereiner
- Johann
Döbereiner noted that certain elements seemed to occur as
'triads' of similar elements e.g.
- (i)
lithium, sodium and potassium
- (ii)
calcium, strontium and barium
- (iii)
chlorine, bromine and iodine
|
-
Döbereiner
was amongst the first scientists to recognise the 'group'
idea of chemically very similar elements.
-
Three groups he
'recognised' were (i) Group 1
Alkali Metals, (ii) Group 2 Alkaline Earth Metals, (iii) Group 7
Halogens.
-
Atomic structure
history note: The physical and chemical likeness of the three
members of these 'triad groups' should be evident and it was based
purely on observation, however Döbereiner and contemporaries where
unaware of the atomic and molecular nature of these elements e.g. the
atomic nature of the metals (M atoms) and the molecular nature of the
Halogens (X2 diatomic molecules). In fact the concept of a
'molecule' was first realised by Avogadro in 1811 but it took 50 years
before the genius of his experimental work and intuition was fully
realised.

1.3 The work of John
Newlands 1864
|
Newlands'
Octaves (his 'Periodic Table' of 1864)
|
| H |
Li |
Ga |
B |
C |
N |
O |
| F |
Na |
Mg |
Al |
Si |
P |
S |
| Cl |
K |
Ca |
Cr |
Ti |
Mn |
Fe |
| Co,
Ni |
Cu |
Zn |
Y |
In |
As |
Se |
| Br |
Rb |
Sr |
Ce,
La |
Zr |
Di,
Mo |
Ro,
Ru |
| Pd |
Ag |
Cd |
U |
Sn |
Sb |
Te |
| I |
Cs |
Ba,
V |
Ta |
W |
Nb |
Au |
| Pt,
Ir |
Tl |
Pb |
Th |
Hg |
Bi |
Cs |
-
Newlands
recognised that every 7 elements, the 8th seemed to be very similar
to the 1st of the previous 7 when laid out in a 'periodic' manner
and he was one of the first scientists to derive a 'Periodic Table'
from the available knowledge.
-
e.g. his 'table'
consists of almost
completely genuine elements (Di was a mix of two elements), classified
roughly into groups of similar elements and a real recognition of
'periodicity'
-
He also recognised that the 'groups' had more
than 3 elements (not just 'triads'), and was correct to mix up metals and non-metals in same group
e.g. in 5th column there is carbon, silicon, tin (Sn) from what we
know call Group 4. However, indium is in group 3 but Ti, Zr have a
valency of 4, like Group 4 elements and do form part of vertical
column in what we know call the Transition Metal series
-
Other correct
'patterns' if not precise are recognisable in terms of the
modern
Periodic Table e.g. half of column 2 is Group 1, half of column 3 is
Group 2, half of column 5 is Group 4, half of column 6 is Group 5,
half of column 7 is Group 6. If we put his column 1 as column 7, it
would seem a better match of today!
-
Although none of his
vertical column groups match completely but the basic
pattern of the modern periodic table was emerging. However column's 1 and 7 do seem particularly
mixed up compared to the modern periodic table.

1.4 Dmitri Mendeleev's
Periodic Table of 1869

-
Mendeleev
laid out all the known elements in order of
'atomic weight' (what we know call relative atomic mass, Ar) except for
several examples like tellurium (Te, Ar = 127.60) and iodine (I,
Ar = 126.90) whose order he
reversed because chemically they seemed to be in the wrong vertical
column! Smart thinking!
-
Argon (Ar, Ar
= 39.95) and potassium (K, Ar = 39.10) is the 2nd example,
but that was not a problem for chemists at the time, because the Group 0
Noble Gases hadn't been discovered by then!
-
These 'anomalies' in
the order of 'atomic weights' are explained by the existence of isotopes
which were discovered ~1916 and the neutron finally characterised in
1932.
-
Isotopes of elements
are atoms of the same proton number with different numbers of neutrons,
hence atoms of the same element with different mass numbers.
-
The most abundant
stable isotope of potassium is 39K, and that of argon is
40Ar, hence the anomaly.
-
Naturally occurring
iodine is 100% 127I, but tellurium has a range of isotopic
masses from 120Te to 130Te but more the heavier
isotopes are more abundant than the lighter isotopes.
-
By 1869, Mendeleev
and Lothar Meyer had an advantage over Newlands because there was an
increased
number of known elements and hence 'groups' of similar elements were becoming more clearly defined.
-
Mendeleev
used a double column approach which is NOT incorrect, i.e. a sort of
group xA and xB classification. This is due to the 'insert' of
transition metals, some of whom show chemical similarities to the
vertical 'groups'. We now recognise theses dual columns as
-
His 'presentation'
was sufficiently accurate to predict missing elements and their
properties * e.g. germanium (Ge) below silicon (Si) and above tin (Sn) in Group IV and
Mendeleev is rightly called the 'father of the modern Periodic
Table'.
-
Atomic structure
history notes: In 1897 Wien and J J Thompson measured the charge
mass ratio of the 'particles' of the cathode rays (electrons) and also
showed that the smallest positively charged particle was obtained from
hydrogen gas. This 'smallest particle' we now know is the proton.
-
Between 1910-1914
Millikan established the value of the electric charge on an electron in
his famous 'oil drop' experiments, hence the mass of the electron could
be calculated.
-
From 1902-1910
Rutherford, Geiger and Marsden and others used
alpha particle scattering
experiments (GCSE-AS atomic structure notes) to establish the
concept of the nucleus and were even able to make an estimate of the
value of its positive charge (which we now know equals the atomic/proton
number). Even at that stage it was recognised that this positive nuclear
charge bore some relationship to the order of the elements, as given by
'atomic weights', which Mendeleev and others were using to construct
their periodic table.
-
Experimentally the
'atomic number' of an element was established by Chadwick in 1920 from
beta particle scattering experiments (an atoms electrons deflecting the
bombarding beta particle electrons) and from the X-ray spectra results
of Moseley in 1913. Moseley showed that when atoms were bombarded with
cathode rays (electrons) X-rays where produced. It was found that the
square root of the highest energy emission line (called the K alpha
line, Kα) gave a linear plot with the apparent atomic number.
However the plot of √Kα against atomic weight (relative
atomic mass) gave a zig-zag plot. Therefore finally establishing that
the really important 'chemical identity number' was the charge on the
nucleus, i.e. what we know as the atomic/proton number and this would be
the crucial number for ordering the elements, ultimately into the modern
periodic table.
-
However, there was
still the problem of why the atomic mass and atomic number where
different i.e. in the case of the lighter elements, the atomic weight
was often about twice the atomic number. In 1919 Aston developed a
cathode ray tube i.e. like those used by Wien and Thompson etc. into a
'mass spectrograph', which we now know as a
mass spectrometer (GCSE-AS
atomic structure notes). This showed that atoms of the same
element had different masses but there was no experimental evidence that
they had different atomic numbers (which of course they didn't). In 1920
Rutherford suggested there might be a 'missing' neutral particle and in
1932 Chadwick discovered the neutron by bombarding beryllium atoms with
alpha particles which produced a beam of neutrons
1.5
A modern
version of the Periodic Table based on the electronic structure of
atoms
The electronic basis of the periodic table is
explained in Part 2.
| Pd |
s block |
3d to
6d blocks of Transition Metals (Periods 4
to 7), note that the 1st (d1) and 10th (d10) are NOT true
transition elements. |
p block |
| Gp1 |
Gp2 |
Gp3 |
Gp4 |
Gp5 |
Gp6 |
Gp7 |
Gp0 |
| 1 |
1H
Note: (i) H does not readily fit into any group, (ii) He not
strictly a 'p' element but does belong in Gp 0/8
|
2He |
| 2 |
3Li |
4Be |
The
full IUPAC modern Periodic Table of Elements (ZSymbol, z = atomic or proton
number) |
5B |
6C |
7N |
8O |
9F |
10Ne |
| 3 |
11Na |
12Mg |
13Al |
14Si |
15P |
16S |
17Cl |
18Ar |
| 4 |
19K |
20Ca |
21Sc |
22Ti |
23V |
24Cr |
25Mn |
26Fe |
27Co |
28Ni |
29Cu |
30Zn |
31Ga |
32Ge |
33As |
34Se |
35Br |
36Kr |
| 5 |
37Rb |
38Sr |
39Y |
40Zr |
41Nb |
42Mo |
43Tc |
44Ru |
45Rh |
46Pd |
47Ag |
48Cd |
49In |
50Sn |
51Sb |
52Te |
53I |
54Xe |
| 6 |
55Cs |
56Ba |
*57-71 |
72Hf |
73Ta |
74W |
75Re |
76Os |
77Ir |
78Pt |
79Au |
80Hg |
81Tl |
82Pb |
83Bi |
84Po |
85At |
86Rn |
| 7 |
87Fr |
88Ra |
*89-103 |
104Rf |
105Db |
106Sg |
107Bh |
108Hs |
109Mt |
110Ds |
111Rg |
112? |
113? |
114? |
115? |
116? |
117? |
118? |
| Gp
1 Alkali Metals
Gp 2 Alkaline Earth Metals
Gp 7/17 Halogens
Gp 0/18 Noble Gases
Take note of the four
points on the right |
|
|
*57La |
58Ce |
59Pr |
60Nd |
61Pm |
62Sm |
63Eu |
64Gd |
65Tb |
66Dy |
67Ho |
68Er |
69Tm |
70Yb |
71Lu |
|
*89Ac |
90Th |
91Pa |
92U |
93Np |
94Pu |
95Am |
96Cm |
97Bk |
98Cf |
99Es |
100Fm |
101Md |
102No |
103Lr |
|
*Horizontal insert
in Period
6 of the
Lanthanide
Metal Series (Lanthanides/Lanthanoids) Z=57 to 71
including the 4f-block
series.
*Horizontal insert
in Period 7 of the
Actinide Series of Metals
(Actinides/Actinoids) Z=89-103
including the
5f-block
series. |
-
Using 0 to
denote the Group number of the Noble Gases is historic i.e. when its valency was
considered zero since no compounds were known. However, from
1961 stable compounds of
xenon have been synthesised exhibiting up to the maximum possible valency of 8
e.g. in XeO4.
-
Because of the
horizontal series of elements e.g. like the Sc to Zn block (10 elements), Groups 3 to
0 can also be numbered as
Groups 13 to 18 to fit in with the maximum number of vertical columns of elements
in periods 4 and 5 (18 elements per period).
-
This means
that 21Sc to 30Zn can be now considered
as the top elements in the vertical Groups 3 to 12.
-
I'm afraid
this can make things confusing, but there
it is, classification is still in progress!
|
-
With are knowledge
the modern Periodic Table is now laid out in order of
atomic (proton) number.
-
Due to
isotopic masses, the relative atomic mass does go 'up/down' occasionally
(there is no obvious 'nuclear' rule that accounts for this, at least
at GCSE/GCE level!). BUT chemically Te
is like S and Se etc. and I is like Cl and Br etc. and so are placed
in their correct 'chemically similar family' group and this is now backed up by
modern knowledge of the electron structure
of atoms.
-
We now know the electronic structure of elements and can
understand sub-levels and the 'rules' in electron structure e.g. 2 in
shell 1 (period 1, 2 elements H to He), 8 in shell 2 (period 2, 8
elements Li to Ne), there is a sub-level which allows an extra 10
elements (the transition metals) in period 4 (18 elements, K to Kr).
this also explains the sorting out of Mendeleev's A and B double
columns in a group. The
periods are complete now that we know about Noble Gases.
-
The use and
function of the Periodic Table will never cease! Newly 'man-made' elements
are being synthesised.
-
In the 1940's
Glenn Seaborg was part of a research team developing the materials
required to produce the first atomic bombs dropped on Hiroshima and
Nagasaki. He specialised in separating all the substances made in the
first nuclear reactors and helped discover the series of 'nuclear
synthesised' elements beyond the naturally occurring limit of uranium
(92U). From element 93 to 113 are now known, so the structure of the bottom part of the periodic
table will continue to grow. There is plenty of scope for present day, and
future Mendeleev's!!!! (will you be one of em'?).
-
Atomic structure
history note: From 1913 onwards the electron structure of atoms was
gradually being understood and paralleling the developing knowledge of
the structure of the nucleus and its importance in determining which
element an atom was i.e. the atomic/proton number.
The Bohr theory of the hydrogen spectrum
(see section 2.6) postulated that the electrons surrounding the
positive nucleus could only exist in specific energy levels and that any
electron level change must involve a specific input/output of energy -
the quanta e.g. a photon of light or X-rays etc.
-
In the 1920's and
1930's scientist-mathematicians like Heisenberg and Schrödinger were
developing the mathematical equations known as wave mechanics. These
mathematical theories describe the detailed behaviour of electrons, and
out of these equations come the four quantum numbers from which are
derived the set of rules we use to
assign electrons in their respective levels (see section 2.2),
which ultimately determines the chemistry of an element.


1.6
Where did the elements come from originally? and where do we
get the elements from?
-
The ultimate origin of all elements
is the nuclear reactions that go on when stars are formed from
inter-stellar dust and gas forming a huge combined mass due to
gravity, and then 'chunks' of a star cool down to form planets. The
heaviest elements are formed in nuclear fusion reactions when stars
self-destruct in super-nova explosions.
-
All
the elements from atomic numbers 1-92 (H-U) naturally occur on
Earth, though some are very unstable-radioactive and decay to form
more nuclear stable elements.
-
Everything around you is made up of
the elements of the periodic table, BUT most are chemically
combined with other elements in the form of many naturally
occurring compounds e.g.
-
hydrogen and oxygen in water,
sodium and chlorine in sodium chloride ('common salt'), iron,
oxygen and carbon as iron carbonate, carbon and oxygen as carbon
dioxide etc. etc.!
-
Therefore, most elements can only be
obtained by some kind of chemical process to separate or
extract an element from a compound e.g.
-
Less reactive metals are obtained
by reduction of their oxides with carbon and more reactive
metals are extracted by electrolysis of their chlorides or
oxides (see GCSE-AS notes on Metal Extraction)
-
Non-metals are obtained by a
variety of means e.g. chlorine is obtained by electrolysis of
sodium chloride solution (see
GCSE notes on Group 7 The Halogens).
-
However some elements never occur
as compounds or they occur in their elemental form as well as
in compounds e.g.
-
The Group 0 Noble Gases are so
unreactive they are only present in the atmosphere as individual
atoms. Since air is a mixture, these gases are separated from
air by a physical method of separation by distillation of
liquified air. The elements oxygen and nitrogen are obtained
from air at the same time, which is far more convenient than
trying to get them from compounds like oxides and nitrates etc.
-
Gold/platinum is are the least
reactive metals and are usually found 'native' as the
yellow/silver elemental metal.
-
Relatively unreactive metals like
copper and silver can also be found in their elemental form in
mineral deposits as well as in metal ores containing compounds
like copper carbonate, copper sulphide and silver sulphide.
-
The non-metal sulphur is found
combined with oxygen and a metal in compounds known as
sulphates, but it can occur as relatively pure sulphur in yellow
mineral beds of the element.
-
-

GENERAL
REVISION
NOTES

SITE PURPOSE EDUCATION - online learning
or 'self-private-tuition' using revision notes, quizzes, practice
tests involving ADVANCED LEVEL CHEMISTRY in the areas of REVISING
only the CHEMISTRY at Doc Brown's Chemistry Clinic via HOMEPAGE in
secondary school/schools, 6th form college/colleges,
academy/academies or home self-study and may help with 1st year undergraduate
university chemistry courses. Hopefully it will encourage
interest and understanding of Chemistry, Earth Science and Radioactivity
in any country of the world, though the site is written entirely in English. The website is designed to help
and unofficially support students/teachers revise-learn/teach the chemistry for modular
or co-ordinated examination science
courses from UK QCA based AQA, OCR (Oxford and Cambridge),
Nuffield, Salters, Cambridge International (CIE), London International, WJEC, CCEA etc.
Also, national award assessments-examinations for BTEC-NVQ
applied, additional and chemistry science courses, Advanced Subsidiary
Level GCE-AS-A2-IB-KS5-BTEC-NVQ exams. National Chemistry assessment levels, International Baccalaureate,
K12 higher US grade level examinations for the
national curriculum for secondary schools and colleges. The notes should also provide some background theory
for a coursework assignment or project. BUT please note that
my on-line revision notes and quizzes are no substitute for good classroom
teaching-lecturing and thorough studying of your own notes and textbooks, practicing past papers
and a copy of the syllabus which are readily downloaded from the
examination board sites, but I hope here and there they will lend a
tutoring hand on some topic, unit, module etc. For final revision you
have to be intellectually honest about what you don't know or follow, YOU have to
take the stuff to pieces, analyse what you do/do not understand
and reconstruct it so it all makes sense in the end. There is no other
way, there are no magic secrets on how to revise and learn, its mainly
down to hard work and just good old fashioned study and employing teach-yourself
strategies without the need for extra tutors and tutoring lessons. I also think
there is too much hit and miss revision using past papers (which I do NOT
supply) and not enough
systematic revision. I also hope it will help teachers in planning
lessons and developing schemes of work for science-chemistry. There are no
lesson plans on the site but there are plenty of quizzes to incorporate into
classroom activities whether photocopied or on electronic whiteboard projector
for use as self-tuition-assessment purposes and a variety of teaching and
learning styles and the images may be used in Microsoft Word documents and powerpoint projections.
The site seems to be used by a large number of home study tutors, particularly
the revision notes. An individual tutor may print out the notes for
science-chemistry learning teaching-tuition purposes and for background material
for assignments and projects. I have no interest or time in producing WORD.doc or xxxx.pdf files
of the notes at the moment. Neither have I time to write up many practical
laboratory experiments ('lab'-'labs') at the moment, but the notes contain lots
of background information of chemical reactions in terms of
observations-balanced equations-reactants-products-theory etc. I also find it
difficult to recommend specific exam websites or syllabus textbooks, it depends exactly on
what you need, what you have time for, and there are so many of them to choose
from and I do not supply past examination papers. Dr W P Brown GCE A AS A2
IB Advanced-Subsidiary Level Chemistry 25-09-07
 
AQA Cambridge CIE London
Edexcel Nuffield Salters OCR GCE AS A2 IB advanced level chemistry revision
AQA Cambridge CIE London
Edexcel Nuffield Salters OCR GCE AS A2 IB advanced level chemistry revision
AQA Cambridge CIE London
Edexcel Nuffield Salters OCR GCE AS A2 IB advanced level chemistry revision
AQA Cambridge CIE London
Edexcel Nuffield Salters OCR GCE AS A2 IB advanced level chemistry revision
 |