Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100...

31
Astronomy Astronomy General Science Spring ‘07

Transcript of Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100...

Page 1: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

AstronomyAstronomy

General Science Spring ‘07

Page 2: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

History of the UniverseHistory of the Universe

Earth = 1 of 9 planetsSun= 1 of 100 billion stars in the Milky

Way, 1 of infinite numbers in our universe

Page 3: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Ancient AstronomyAncient Astronomy

Golden Age= 600 BC-150 AD in GreeceBeliefs relied on philosophy (ideas) and

observations.

Page 4: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Geocentric ViewGeocentric View

At first, we thought the Earth was the center of the universe

Geo=Earth -centric=center

Page 5: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Heliocentric viewHeliocentric view

Eventually, we realized the SUN was the center of our galaxy.

This was called the HELIOcentric view.

Page 6: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Modern AstronomyModern Astronomy

Ideas based more on observation

Nicholas Copernicus (1473-1543, Poland)– Earth rotates– Said Earth is a planet

(only 5 known at this point: Mercury, Venus, Mars, Jupiter, Saturn)

Page 7: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Johannes Kepler (1571-1630)Johannes Kepler (1571-1630)

Laws of Planetary Motion– The path of each planet

is an ellipse– Each planet travels at

its own speed– Astronomical Unit

(AU) = 150 million kilometers

Page 8: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Galileo Galilei (1564-1642)Galileo Galilei (1564-1642)

Around at the same time as Kepler

Favored the heliocentric viewpoint

Created the telescope (which later made him go blind

after looking at the sun through it) Discovered the four

moons of Jupiter

Page 9: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Sir Isaac Newton (1643-1727, Sir Isaac Newton (1643-1727, England)England)

Law of Gravity! Proved Kepler’s idea

that planets orbit in an ellipse.

Page 10: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Trip through our UniverseTrip through our Universe

Light year= how far light

travels in one year Speed of light= 186,000

miles per second!

Billions and billions of stars

Carl Sagan 11/9/34-10/20/96

Page 11: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

ConstellationsConstellations

Star groups that form patterns as seen from Earth

Big dipper (ursa major)Little dipper (ursa minor)Orion

Page 12: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

NovasNovas

When a star suddenly increases in brightness (100x) in a few hrs/days, then dims back to original state.

Gases from one binary star strike the other causing nuclear explosions which we see as light.

Page 13: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

NovasNovas

Page 14: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

NebulaeNebulae

We see light from stars, but most give off other types of radiation– X-Rays, Infared (heat), UV light, radio waves

All types can be seen by different types of telescopes.

Page 15: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

NebulaeNebulae

A huge massive cloud glowing between stars.

Where new stars form

Page 16: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

GalaxiesGalaxies

Contain stars and are major features of our universe.

There are billions of galaxies each with billions of stars of their own.

Page 17: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Three Types of GalaxiesThree Types of Galaxies

Spiral– Shaped like pinwheels– Andromeda– Milky Way

Page 18: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Three Types of GalaxiesThree Types of Galaxies

Elliptical– Vary in shape from

spherical to flat discs– Contain little dust/gas

Page 19: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Three types of GalaxiesThree types of Galaxies

Irregular– No ordinary shape– Least common

Page 20: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

The Milky WayThe Milky Way

100,000 light years across!

15,000 light years thick!

It would take, traveling at the speed of light, 100,000 years to cross!

Page 21: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Earth and its MoonEarth and its Moon

Magnetic field- invisible lines of force that connect poles

Earth has a magnetic core

Made from iron and nickel

Page 22: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Earth= MagnetEarth= Magnet

Van Allen Belts– Doughnut shaped

fields that trap particles from solar wind (e- and p+), produce auroras

– Can see the aurora borealis in Canada and Alaska

Page 23: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Neil Armstrong + Buzz AldrinNeil Armstrong + Buzz Aldrin

First men to land on the moon

July 20,1969 Neil Armstrong first to

step on the moon

Page 24: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

First Step on MoonFirst Step on Moon

Page 25: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

The Moon’s MeasurementsThe Moon’s Measurements

3476 km in diameter Gravity 1/6 that of Earth 384,403 km from Earth 4.6 billion years old No H2O, no atmosphere 100oC @ noon, -175oC at

night

Page 26: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

The Moon’s FeaturesThe Moon’s Features

Galileo was the first to observe the moon

Saw mountains and low areas.

Saw craters formed by asteroids

Page 27: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

The Moon’s movementThe Moon’s movement

Moon revolves around EarthPerigee- closest to Earth (350,000 km)Apogee- furthest (400,00 km)27.5 days to rotate on axis27.5 days to revolve around the Earth

– Why we only see one side of the moon.

Page 28: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.
Page 29: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

The Moon’s OriginThe Moon’s Origin

Several TheoriesAsteroid “captured” by Earth’s gravityFormed from the same nebulae as the

planetsAsteroid (size of Mars) struck Earth, ejected

chunk of Earth outward (widely accepted theory)

Nothing 100% certain

Page 30: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Earth, Moon and Sun Earth, Moon and Sun

The reflection of the sun on the moon results in changing appearance of moon as seen from Earth.

The Moon appears to change shapeThe Moon doesn’t shine, it reflects light.

Page 31: Astronomy General Science Spring ‘07. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite numbers.

Phases of the MoonPhases of the Moon