A small number of elements make up >99% of the solid Earth.
O = oxygen
Na = sodium
Mg = magnesium
Al = aluminum
Si = silicon
S = sulfur
Ca = calcium
Fe = iron
Ni = nickel
Slide 15
The crust is a little more elementally interesting (again, as a result of differentiation), but it is still mainly made of a small number of elements.
C = carbon
P = phosphorus
K = potassium
Ti = titanium
Mn = manganese
Slide 16
Since electrons weigh virtually nothing, the mass of an atom is concentrated in its nucleus.
Each atom can be described by its atomic weight (or mass),
which is the sum of the protons and neutrons.
lithium:
atomic number = 3
3 protons
4 neutrons
atomic weight = 3 + 4 = 7
BUT . although each element has a defined number of protons,
the number of neutrons is not fixed.
Atoms with the same atomic number but variable numbers of neutrons are called isotopes.
Slide 17
Carbon (atomic # 6) has three natural isotopes
with atomic weights of 12, 13 and 14.
isotope #p #n
====== == ==
C-12 6 6
C-13 6 7
C-14 6 8
Tin (Sn, atomic # 50) has ten natural isotopes with atomic masses of 112, 114, 115, 116, 117, 118, 119, 120, 122 and 124. How many protons and neutrons do these isotopes have?
Slide 18
Radioactivity is a nuclear phenomenon: it comes as a result of a particular structure in a nucleus.
A radioactive atom is considered unstable. All unstable atoms emit radioactivity (usually by ejecting nuclear particles) in order to reach a stable configuration.
This is the process of radioactive decay
(about which we will talk on 6/9).
So, not all atoms will be radioactive, just a small proportion of isotopes with unstable nuclei.
The bulk of isotopes are stable, or non-radioactive.
Slide 19
Carbon (atomic # 6) has three natural isotopes
with atomic weights of 12, 13 and 14.
isotope #p #n
====== == ==
C-12 6 6
C-13 6 7
C-14 is a radioactive isotope; C-12 and C-13 are stable.
Over time the proportion of C-12/C-14 and C-13/C-14
will increase until there is no C-14.
(unless some process makes new C-14 .)
C-14 6 8
Slide 20