Our Place in the Cosmos Our Place in the Cosmos Course Aims and - - PDF document

our place in the cosmos our place in the cosmos
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Our Place in the Cosmos Our Place in the Cosmos Course Aims and - - PDF document

Our Place in the Cosmos Our Place in the Cosmos Course Aims and and To explain primarily at a descriptive Introduction to Introduction to level the contents, dimensions and history of the Universe, and our place Astrophysics Astrophysics


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Our Place in the Cosmos Our Place in the Cosmos and and Introduction to Introduction to Astrophysics Astrophysics

Jon Loveday Astronomy Centre Department of Physics & Astronomy

Course Aims

To explain primarily at a descriptive level the contents, dimensions and history of the Universe, and our place within it. This will include a survey of the basic astronomical tools, and will seek to explain the way in which some basic physical laws can be applied in

  • rder to understand the observed

phenomena.

Class organisation

Lectures

Monday 9am Arts A5 Friday 9am Pev1 1A6

Workshops Friday 10am

Our Place in the Cosmos: Pev1-2A2 Informal discussion, quizzes, student

presentations

Intro to Astrophysics: Arundel 1B Mathematical background, problem sheets Taken by Peter Thomas

Assessment

Our Place in the

Cosmos

15 minute presentation (weeks 5-10; 20%) In-class quiz (week 10; 20%) 2000-word essay (week 10; 60%)

Introduction to

Astrophysics

4 x problem sheets (10% each) In-class quiz (week 9; 40%) Briefing paper (week 9; 20%)

Lecturer

Jon Loveday Pev2 5A5 x 7719 J.Loveday@sussex.ac.uk Office hour: Tuesday 1.30-2.30

Web Resources

Sussex Direct has links to the official

course document (click on the course code: F3095 or F3156)

Study Direct includes copies of these

slides and other useful resources

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Course textbooks

21st Century Astronomy by Hester et al.

is very good, though expensive at £42

Introductory Astronomy by Holliday is

cheaper

Other useful books you should find in the

library include:

Universe Freedman & Kaufmann In Quest of the Universe Kuhn & Koupelis

Student Feedback

Please feel free to stop me and ask for

clarification at any time during classes if anything I have said is unclear

Feedback on any aspect of the course is

welcome during the Friday seminar

Formal feedback will be requested via

the Study Direct website during weeks 8-9. Please note that feedback provided in this way is completely anonymous

What is Astronomy?

Literally means “naming the stars” The earliest astronomers simply tracked the

motions of the heavenly bodies

Modern astronomers use observations to help

understand the Universe and our place within it via scientific reasoning

Astrology is not astronomy, but a pseudo-

science

Why Astrology is not a Science

The constellations are only imaginary,

not physical associations of stars

Constellations have shifted relative to

  • ur calendar due to precession of

equinoxes since founding of astrology

Rigorous tests of astrological

“predictions” have shown they do not work

The Scientific Method

Guided by observations, posit a theory that

explains them

A good theory makes testable predictions

about future observations, and thus is falsifiable

Scientific theories can never be definitively

proved, they can only be ruled out by contrary

  • bservations

A theory that stands the test of time becomes

generally accepted and possibly modified

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Why Study Astronomy?

Early astronomers used positions of the stars

to track the seasons and later as a vital navigational aid

Help understand phenomena such as tides and

eclipses

Understand and appreciate even more the

beauty of the night sky

Learn about the origin and fate of the

Universe

Course Outline

Brief tour - scales in the Universe Historical overview Earth, Moon and Sun Orbits and Gravity Solar System Stars Galaxies The Milky Way The Universe

A brief tour

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Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto

Solar System Milky Way

Milky Way as Viewed from Earth NGC 891

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Milky Way in the near-IR NGC 4414 A cluster of galaxies

Virgo Galaxy Cluster

Infrared Universe The Deep Universe Hubble Ultra-Deep Field CMB Temperature Map

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Scales in the Universe

Astronomical distances are commonly

given in terms of light travel time, ie. distance light will travel in that time at its speed of 300,000 km/s

Distances as light travel times - not to scale!

Prehistoric astronomy

Since prehistoric times, man has observed the

changing phases of the moon during the lunar month, and the changing passage of the Sun during the year

One can understand how, as well as indicating

the change of the seasons, man might well have thought of the stars as causing the change

Hence religious significance of the heavenly

bodies, and birth of astrology

Dots below horses thought to represent changing phases

  • f the Moon

Earliest depictions of the skies are found in the Cave paintings in Lascaux, SW France (c15,000 BC) The Great Bull: An Ice Age Star Map?

Pleiades Hyades Orion

Prehistoric astronomy

Observations of the changing passage of the

Sun and the star patterns in the night sky enabled tracking of the seasons, and hence the best times to plant and harvest crops

Observations of the Moon’s phase allowed

fishermen to predict the tides

Observatories were built to track the positions

  • f the heavenly bodies, most famously

Stonehenge, 3000-1500 BC

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Stonehenge

An early astronomical calculator? On summer solstice, Sun rises exactly above

the Heelstone

In Stonehenge Decoded (1965), Gerald Hawkins

claimed large number of alignments with Lunar and Solar phenomena, and hence that eclipses could be predicted

These claims are still controversial

At sunset close to the spring and autumn equinoxes, shadows give the effect of a snake slithering down the stairway.

El Castillo, Chichen Itza (Mayan, c1000 AD) The Planets

It must have been noticed very early

that some bodies moved faster in the night sky than the surrounding stars.

The word "planet" comes from the Greek

word "planetes," which means "nomad”

  • r “wanderer”.

To the Babylonians and Sumerians before

them, the planets were "stray sheep”.

The Ancient Greeks

By far the most famous early astronomers are the ancient

  • Greeks. Between about 500BC and 100BC, they built a

picture of the Universe which dominated for over 1000 years.

Thales (624 - 545 BC)

Realised that celestial objects were at different distances, that the Earth was spherical, and that the light of the moon was reflected sunlight.

Pythagoras (582 - 500 BC)

Produced the first geocentric model of the Universe, with everything making perfectly circular orbits around the Earth.

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Geocentric Model