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Astronomy 171
Solar System Astronomy
Prof. Paul Martini

Lecture 22: Matter


Key Ideas:

Atoms are composed of
a nucleus of protons and neutrons
orbiting electrons
Chemical Elements and Isotopes
Radioactivity
Four Fundamental Forces
Gravitational and Electromagnetic
Strong and Weak Nuclear Forces


Atoms

Ordinary matter is found primarily in the form of atoms
Range of ordinary matter:
Free subatomic particles (protons and electrons)
Single atoms (hydrogen, helium, gold, etc.)
Simple molecules (O2, H2O, etc.)
Macromolecules (DNA, complex polymers, oil, etc.)
Macroscopic objects (diamonds, trees, people, planets, etc. )


Atomic Structure

Nucleus of a heavy subatomic particle:
proton: positively charged
neutron: uncharged
Electrons orbiting the nucleus
negatively charged particles
1/1836th the mass of a proton
Atoms are mostly empty space
Only 1 part in 1015 of space is occupied
The rest of the volume is threaded by electromagnetic waves


Chemical Elements

Distinguish atoms into Elements by the number of protons in the nucleus
Atomic Number:
1 proton: Hydrogen
2 proton: Helium
3 proton: Lithium
Number of electrons = Number of protons
All elements are Chemically Distinct


Top Ten Most Abundant Elements

10) Sulfur
9) Magnesium
8) Iron
7) Silicon
6) Nitrogen
5) Neon
4) Carbon
3) Oxygen
2) Helium
1) Hydrogen


Variation in Abundance

The average abundances of elements in the Universe need to be measured over a large Volume
For example, the entire Solar System
Local variations can be significant
Oceans mostly Hydrogen and Oxygen
Earth's crust mostly Oxygen, Silicon, Aluminum, and Iron


Known Elements

117 elements are currently known:
87 are metals
11 are gasses
2 occur as liquids (Bromine and Mercury)
26 are natural radioactive elements
24 are made only in particle accelerators
In addition, each element can have a number of different isotopes


Isotopes

A given element can have many Isotopes
Same number of protons
Different number of neutrons
Example:
12C has 6 protons and 6 neutrons
13C has 6 protons and 7 neutrons
14C has 6 protons and 8 neutrons
These isotopes of Carbon are chemically identical, but have different masses.


Radioactivity

If a nucleus has too many or too few neutrons, it is unstable to radioactive decay.
Examples:
3H (1p + 2n) decays to 3He (2p + 1n) + 1 electron + 1 neutrino
14C (6p + 8n) decays to 14N (7p + 7n) + 1 electron + 1 neutrino
This later reaction is the basis of radiocarbon dating
Free neutrons are also unstable
n decays to p + 1 electron + 1 neutrino


Radioactive Half-Life

Radioactive decay is a random process
The activity is measured by the Half-Life
Time for half of the atoms to decay
The more radioactive, the shorter the halflife
Examples:
3H (1p + 2n) decays to 3He (2p + 1n) + 1 electron + 1 neutrino with a 12.26 year half-life
14C (6p + 8n) decays to 14N (7p + 7n) + 1 electron + 1 neutrino with a 5730 year half-life
n decays to p + 1 electron + 1 neutrino with a 12 minute half-life


Fundamental Forces of Nature

All interactions in nature are governed by four "fundamental" forces
Gravitational Force
Electromagnetic Force
Strong Nuclear Force
Weak Nuclear Force


Gravitational Force

Gravitation binds matter over long distances
Long-range attractive force
Weakest force of nature
Obeys the Inverse Square Law of distance


Electromagnetic Force

Electromagnetic force acts between charged particles
Like charges repel each other
Opposite charges attract each other
Long-range, inverse-square law force:
Binds electrons and protons into atoms
Binds atoms together into molecules
Very strong:
1039 times stronger than Gravity


Strong and Weak Nuclear Forces

Short-range forces (<10-15m) in atomic nuclei
Strong force:
Binds protons and neutrons into nuclei
Strongest force of nature
Weak force:
Responsible for radioactivity (what turns a neutron into a proton, electron, and neutrino during neutron decay)
Second strongest force


The Interplay of Forces

Gravity rules on the largest scales:
Binds massive objects together
Controls orbital motions
Electromagnetism rules on atomic scales
Binds electrons to protons and atoms to atoms
Mediates chemical reactions
Strong and Weak Forces rule on nuclear scales
Binds protons to neutrons inside nuclei
Mediates radioactivity and nuclear reactions


See A Note about Graphics to learn why some of the graphics shown in the lectures are not reproduced with these notes.

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Updated: 2007 February 4
Copyright © Paul Martini All Rights Reserved.