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2/25/2015 1 Bell-Ringer 1. Write out what you know about astronomy. 2. How does the size of the Sun compare to the size of the Earth? 3. What types of tools do astronomers use? Earth’s Address

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1

Bell-Ringer 1. Write out what you know

about astronomy.

2. How does the size of the Sun compare to the size of the Earth?

3. What types of tools do astronomers use?

Earth’s Address

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2

Earth

Solar System

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Milky Way Galaxy

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Milky Way Galaxy

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The Sun-Earth-Moon System

Tools of Astronomy:

Have you ever used a magnifying lens to read fine print?

If so, you have used a tool that gathers and focuses light.

Astronomers use telescopes to gather and focus light from distant objects.

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Tools of Astronomy:

What is radiation?

Astronomers study electromagnetic radiation.

Electromagnetic radiation includes visible light, infrared and ultraviolet radiation, radio waves, microwaves, X-rays, and gamma rays

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15

Parts of the wave

amplitude

trough wavelength

crest

rest position

16

Wavelength measures the distance

between two equivalent parts of a wave

The distance from the crest of one wave to the crest of the next wave is called the wavelength.

In longitudinal waves, the wavelength is the distance between two compressions or two rarefactions.

The distance between two successive identical parts of a wave.

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17

Frequency measures the rate of

vibrations

The frequency of a wave is the number of full wavelengths that pass a point in a given time interval.

Measures how rapidly vibrations occur in the medium

Symbol for frequency is f.

18

Frequency measures the rate of

vibrations

SI unit of frequency is hertz (Hz)

Unit named after Heinrich Hertz, who in 1888 became the first person to experimentally demonstrate the existence of electromagnetic waves

One vibration per second is 1 Hz

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Check for Understanding

In what ways do we

use electromagnetic

radiation on a daily

basis?

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Wavelength & Frequency

C = λf

C = speed of

light

Speed of light

C = 300,000,000 m/s

C = 186,000 miles per second

C = 671 million miles per hour

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Telescopes:

Objects in space emit

radiation in all

proportions of the

electromagnetic

spectrum.

Telescopes:

Telescopes give us

the ability to observe

wavelengths beyond

what the human eye

can detect.

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China Radio Telescope:

4m-Blanco Light Telescope:

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Hubble space telescope

:

Mars Landing Rover

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Voyager space probe

Jupitor from earth based

telescope

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Jupiter from Hubble

Jupiter from Voyager

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Telescopes:

The pupil of your eye

has a diameter of up

to 7mm when it is

adapted to darkness.

Telescopes:

If you compared the ratio of head size to eye size of a great horned owl and humans, your eyes would be the size of grapefruits.

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Telescopes:

Similarly, a telescopes opening,

called an aperture, might be as

large as 10 meters in diameter.

The larger the aperture, the more

light or electromagnetic radiation

can be gathered or collected.

Benefits of

Telescopes:

Telescopes can detect radiation beyond what the human eye can detect.

The larger aperture allows more radiation to be gathered so objects that are too dim to see can be recorded.

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Benefits of

Telescopes:

Another way that the telescope

surpasses the human eye is with the

aid of cameras, or other imaging

devices to create time exposures.

Telescopes can detect objects that

are too faint for the human eye to

see.

Time Exposure:

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Time Exposure:

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Refracting Telescope

Reflecting Telescope

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Reflecting Telescope

Interferometry:

Interferometry is a technique that

uses the images from several

telescopes to produce a single

image.

By combining multiple images,

astronomers can create detailed

images that could only be achieved

from larger telescopes.

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Bell-Ringer

What proof is there

that we have landed

on the moon?

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Refracting Telescope

Reflecting Telescope

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Interferometry:

Interferometry is a technique that

uses the images from several

telescopes to produce a single

image.

By combining multiple images,

astronomers can create detailed

images that could only be achieved

from larger telescopes.

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Reflector Array

Exploring the Moon

Astronomers have learned

much about the moon from

observations with telescopes.

Most of our knowledge about

the moon comes from

explorations by space probes

and landings by astronauts.

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Exploring the Moon

The first step toward reaching the moon was in 1957 when the Soviet Union launched the first artificial satellite, Sputnik I

4 Years later, Soviet Cosmonaut Yuri A. Gagarin became the first human in space.

Sputnik 1

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Exploring the Moon

Exploring the Moon

In 1961, Alan B. Shepard, Jr.

was the first American in

space.

July 20, 1969, the Apollo 11

mission landed Neil Armstrong

and Edwin “Buzz” Aldrin on

the Moon.

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Exploring the Moon

Exploring the Moon

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Exploring the Moon

The last mission of the Apollo program was Apollo 17 - December 7, 1972

Eugene “Gene” Cernan, Commander of Apollo 17, was the last person to set foot on the Moon.

No person has set foot on the Moon since 1972.

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The Lunar Surface:

Albedo is the amount of

sunlight that is reflected from

an objects surface.

The albedo of the moon is very

low. 7- 8%

Earth’s albedo is 31%

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The Lunar Surface:

The Lunar Surface:

Lunar highlands are heavily

cratered regions of the Moon

that are light in color and

mountainous.

Other regions called maria are

dark, smooth planes. 3km

lower in elevation

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A Trip to the Moon: 1902 Silent Film

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The Lunar Surface:

Craters on the Moon, called

impact craters, formed when

objects from space crashed

into the lunar surface.

The Lunar Surface:

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The Lunar Surface:

The material blasted out during

impacts falls back to the

Moon’s surface as ejecta.

Some craters have long trails

of ejecta, called rays, that

radiate outward from the

impact site.

Fresh ejecta

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The Lunar Surface:

Rilles are meandering,

valleylike structures that might

be collapsed lava tubes.

Lunar Properties

Our moon is unique among all

the moons in the solar system.

It is one of the largest moons

compared to the mass of the

planet it orbits.

It is solid and rocky, in contrast

with the icy composition of

most other moons.

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Lunar Properties

Our moon orbits very far from

Earth relative to other moons

and the planets they orbit.

Composition

The moon is made up of

minerals similar to those found

on Earth (mostly silicates).

The maria are mostly basalt,

but unlike basalt on earth, they

contain no water.

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Far Side

Far Side

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History of the Moon

The lunar surface is about the same

age of Earth (3.8-4.6 billion years)

We know this by radiometric dating

of rocks from the surface.

Based on the frequency of impact

craters, scientists theorize the Moon

was heavily bombarded during its

first 800 million years.

History of the Moon

A layer of loose

ground up rock

(regolith) several

meters thick formed

on the surface of the

moon due to heavy

bombardment of

asteroids.

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Layered Structure

Scientists infer from seismic data

collected by seismographs left on the

Moon that the Moon has a layered

structure, similar to Earth.

Layered Structure

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Formation of Maria

After the period of heavy bombardment,

lava welled up from the Moon’s interior

and in the large impact basins.

This created the dark smooth plains of

the maria that we see today.

Tectonics

The moon is no longer

tectonically active (No

volcanoes, no magnetic

field)

However, the moon

experiences an annual

moonquake.

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Giant Impact Theory

There are several theories to

explain how the moon came

into existence.

The most accepted theory by

astronomers is the “Giant

Impact Theory”

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Driving Question

Why is there no change of

season at the equator?

Effects of Earth’s Tilt:

Earth is tilted 23.5° relative to the ecliptic

plane

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Effects of Earth’s Tilt:

The ecliptic plane is the plane of Earth’s

orbit.

Effects of Earth’s Tilt

Earth’s orbit around the Sun and the tilt

of Earth contributes to the changes of

season we are familiar with.

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Effects of Earth’s Tilt:

At a solstice, the Sun is overhead at its

farthest distance either north or south of

the Equator.

Effects of Earth’s Tilt:

At an equinox, Earth’s axis is

perpendicular to the Sun’s rays and at

noon the sun is directly overhead at the

equator.

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Lunar Motions

Synchronous rotation explains why

only one side of the moon always faces

Earth.

It is the state at which the Moon’s orbital

period and rotation periods are equal.

The Moon’s orbital period (lunar month)

is 27.3 days.

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Today: Turn in any worksheets:

Eclipse simulation from Friday.

Lunar Phases

Lunar Phases Quiz Tomorrow!

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Tides:

The Sun and the Moon both contribute

to Earth’s tides by their gravitational pull

which creates bulges of ocean water.

Tides are observed every 12 hours as

the Earth rotates and the Moon orbits

the Earth.

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Spring and Neap Tides:

Solar Eclipse

A solar eclipse occurs when the Moon

passes directly between the Sun and the

Earth.

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Types of Solar Eclipses

Depending on whether the Moon is at

perigee or apogee during a solar

eclipse, we may experience a total

eclipse or an annular eclipse

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Types of Solar Eclipses

A total eclipse occurs when the moon is

lined up directly between the Earth and

the Sun while at Perigee.

Types of Solar Eclipses

An annular eclipse occurs when the

moon is lined up directly between the

Earth and the Sun while at Apogee

During an annular eclipse, a ring of light

is visible.

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Lunar Eclipse

A lunar eclipse occurs when the Moon

passes through Earth’s Shadow

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ECLIPSE CALANDER

May 25, 2013 - Penumbral Lunar Eclipse.

The eclipse will be visible throughout most of

North America, South America, western

Europe, and western Africa.

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ECLIPSE CALANDER

August 21, 2017 - Total Solar Eclipse. This is a

rare, once-in-a-lifetime event for viewers in the

United States. The last total solar eclipse visible in

the United States occurred in 1979 and the next

one will not take place until 2024. The path of

totality will begin in the Pacific Ocean and travel

through the center of the United States. The total

eclipse will be visible in parts of Oregon, Idaho,

Wyoming, Nebraska, Missouri, Kentucky,

Tennessee, North Carolina, and South Carolina

before ending in the Atlantic Ocean. A partial

eclipse will be visible in most of North America and

parts of northern South America.

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Foucault Pendulum

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Foucault Pendulum

For the Test: What you need to know:

Types of electromagnetic radiation

Types of telescopes

Surface features of the moon

Theory of the formation of the moon

Motion of the earth and moon around the sun.

Solstices, equinoxes, and eclipses

Phases of the moon

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1. Linking telescopes to

improve the detail in the

images obtained is called

________________.

Interferometry

Review:

2. A telescope that uses

curved lenses to focus

visible light is called a(an)

______________________

Refracting Telescope

Review:

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3. The Moon’s __________ is

the amount of sunlight

that its surface reflects.

Albedo

Review:

4. The __________ is the

point in the Moon’s orbit

when it is farthest from

Earth

Apogee

Review:

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5. Loose, ground-up rock,

such as the layer covering

much of the surface of the

moon.

Regolith

Review:

6. In the following diagram,

would it be winter or

summer in the northern

hemisphere?

Summer

Review:

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7. The far side of the moon has many more ________ than the near side?

a) maria

b) solstices

c) impact craters

d) equinoxes

Review:

7. The far side of the moon has many more ________ than the near side?

a) maria

b) solstices

c) impact craters

d) equinoxes

Review:

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8. A ____________ occurs when the Moon passes directly between the sun and the Earth.

a) Solstice

b) Solar Eclipse

c) Equinox

d) Lunar Eclipse

Review:

8. A ____________ occurs when the Moon passes directly between the sun and the Earth.

a) Solstice

b) Solar Eclipse

c) Equinox

d) Lunar Eclipse

Review:

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9. Who was the first person

to set foot on the moon?

a) Neil Armstrong

b) Buzz Aldrin

c) Yuri Gagarin

d) Alan Shepard

Review:

9. Who was the first person

to set foot on the moon?

a) Neil Armstrong

b) Buzz Aldrin

c) Yuri Gagarin

d) Alan Shepard

Review:

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9. During what time is the most

direct sunlight furthest north

of the equator?

a) Vernal Equinox

b) Autumnal Equinox

c) Summer Solstice

d) Winter Solstice

Review:

9. During what time is the most

direct sunlight furthest north

of the equator?

a) Vernal Equinox

b) Autumnal Equinox

c) Summer Solstice

d) Winter Solstice

Review:

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10. Approximately how long does it take for the moon to make one complete orbit around the earth?

a) 1 day

b) 1 week

c) 1 month

d) 1 year

Review:

10. Approximately how long does it take for the moon to make one complete orbit around the earth?

a) 1 day

b) 1 week

c) 1 month

d) 1 year

Review:

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The Sun-Earth-Moon System

For the Test: What you need to know:

Types of electromagnetic radiation

Types of telescopes

Surface features of the moon

Theory of the formation of the moon

Motion of the earth and moon around the sun.

Solstices, equinoxes, and eclipses

Phases of the moon

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Bell-Ringer:

Come up with a test question

that I will use on the Test

tomorrow.

Write it as a true/false or

multiple choice style question

Must be over a topic from

Chapter 27

Types of Telescopes

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Space-Based Astronomy

What benefit do robotic probes

have over human exploration?

The Lunar Surface

A

B Maria

Highlands

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The Lunar Surface

E

Rilles

The Lunar Surface

Regolith

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