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Astronomy Unit 2: Stars and Galaxies • What is the relationship between the milky way, our solar system, the universe and Earth ?

Astronomy Unit 2: Stars and Galaxies

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Astronomy Unit 2: Stars and Galaxies. What is the relationship between the milky way, our solar system, the universe and Earth ?. Our Place in the Universe. Stars and Galaxies Astronomy Unit 2. Vocabulary. universe : everything that exists in space, including all matter and energy - PowerPoint PPT Presentation

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Page 1: Astronomy Unit 2: Stars and Galaxies

Astronomy Unit 2:Stars and Galaxies

• What is the relationship between the milky way, our solar system, the universe and Earth ?

Page 2: Astronomy Unit 2: Stars and Galaxies

The Universe

Our GalaxyThe Milkyway

Our Solar System

The Earth

Our Place in the Universe

Page 3: Astronomy Unit 2: Stars and Galaxies

Our Solar System• Planets• Dwarf Planet

Galaxies• 3 types• Elliptical• Spiral • Irregular

Distances• Lightyears • exactly 9,460,730,472,580.8 km (about 9.5 Pm)• about 5,878,625,373,183.6 miles (about 6 trillion miles)

Stars• Life Cycle of Stars• Classification of Stars: Hertzsprung-Russel Diagram• Our Sun• Black Hole• Nebula

Stars and Galaxies Astronomy Unit 2

Page 4: Astronomy Unit 2: Stars and Galaxies

Voca

bula

ry• universe: everything that exists in space, including all matter and energy

• galaxy: a large group of stars, space dust, and gases held together by gravity

• Milky Way: the galaxy in which the Sun is located

• star: a massive ball of hot gases that emits its own light

• Sun: the medium-sized star in the center of the system of objects in space that

includes Earth

• nebula: a cloud of space dust that can clump together to form a star; the plural of

nebula is nebulae (Star Nursery or Stellar Nursery)

• Hertzsprung-Russell (H-R) diagram: a diagram that displays the relationship

between a star’s surface temperature and its magnitude, or brightness

• luminosity: a measure of the energy released each second from the surface of a

star (Brightness)

Page 5: Astronomy Unit 2: Stars and Galaxies

“Earthrise” 1968

Earthrise is the name given to a photograph of the Earth taken by astronaut William Anders in

1968 during the Apollo 8 mission. It has been called "the most influential environmental

photograph ever taken."

Page 6: Astronomy Unit 2: Stars and Galaxies

Our Solar System

• Which planet do you find interesting?

Page 8: Astronomy Unit 2: Stars and Galaxies

The Milky Way Galaxy

• 100,000 light years in diameter• Our sun orbits the center of the

galaxy once every 240 million years

• A Barred spiral galaxy• Contains over 200 billion stars• It is our home galaxy

The Milky Way Galaxy ViewerThis picture, which combines infrared images taken by two different telescopes, shows 1 billion of the Milky Way galaxy's stars all at once.CREDIT: Mike Read (WFAU), UKIDSS/GPS and VVVView full size image

Page 9: Astronomy Unit 2: Stars and Galaxies

What is at the center of the milky way?

Page 10: Astronomy Unit 2: Stars and Galaxies

Galactic Center of the Milky Way • Super massive black hole at the center

Simulated view of a black hole in front of the Large Magellanic Cloud.CREDIT: Alain R. | Wikimedia Commons

How can you see a black hole?

Page 11: Astronomy Unit 2: Stars and Galaxies

Black Hole

An artist's drawing shows a large black hole pulling gas away from a nearby star. Image Credit: NASA E/PO, Sonoma State University, Aurore Simonnet

• A black hole is a place in space where gravity pulls so much that even light can not get out.

• The gravity is so strong because matter has been squeezed into a tiny space.

• This can happen when a star is dying.

Page 12: Astronomy Unit 2: Stars and Galaxies

Types of Galaxies

• Galaxy: A large group of stars, gas, and dust held together by gravity.

Page 13: Astronomy Unit 2: Stars and Galaxies

Elliptical Galaxies

• Elliptical Galaxies: Most common type of galaxy; large three-dimensional football shaped galaxies.-Contain mostly older and dimmer stars.

Page 14: Astronomy Unit 2: Stars and Galaxies

Spiral Galaxies• Spiral Galaxies:

Circular galaxies that have arms curve outward from a central hub.

• Contain a super massive black hole at the center

• The Milky Way is a Spiral Galaxy

Page 15: Astronomy Unit 2: Stars and Galaxies

Spiral Galaxies

• Spiral Galaxies: Circular galaxies that have arms curve outward from a central hub.

• Barred spiral galaxies: Have two spiral arms extending out.

Page 16: Astronomy Unit 2: Stars and Galaxies

Irregular Galaxies

• Irregular Galaxies: Come in many different shapes and are smaller and less common than elliptical or spiral galaxies.

Page 17: Astronomy Unit 2: Stars and Galaxies

Light year

Page 18: Astronomy Unit 2: Stars and Galaxies

Lightyears

How far is the Moon from the Earth ? 1.3 light seconds.How far is the Earth from the Sun ? 500 light seconds or 8 light minutes.

light year: a unit of length equal to the distance that light travels in one year

In space, light travels at a speed of nearly 300,000 kilometers per second, or almost 9.5 trillion kilometers per year. A light year is thus equal to about 9.5 trillion kilometers.

Page 19: Astronomy Unit 2: Stars and Galaxies

Lightyears• When you measure distances on Earth, you

typically use units such as meters or kilometers. The distance to most stars, however, is so large that these units are not practical. Instead, scientists use a unit called a light year to measure distances in space. One light year is the distance that light travels in one year. In space, light travels at a speed of nearly 300,000 kilometers per second, or almost 9.5 trillion kilometers per year. A light year is thus equal to about 9.5 trillion kilometers.

• After our Sun, the nearest star to Earth is Proxima Centauri. This star is a little more than 4.2 light years (40 trillion kilometers) away. The distance to a star or galaxy in light years is equal to the number of years needed for the light from that object to reach an observer on Earth. Light from Proxima Centauri takes a little more than 4.2 years to reach Earth. If you observe this star tonight, you would see Proxima Centauri as it looked 4.2 years ago. You will not see what this star looks like at this very moment until 4.2 years from now.

Page 20: Astronomy Unit 2: Stars and Galaxies

LightyearsWhat does a light year measure?

How many kilometers in a lightyear?

How far is the Moon from the Earth ?

How far is the Earth from the Sun ?

How far is the Earth from the next nearest star, Proxima Centauri?

LightyearsWhat does a light year measure?

How many kilometers in a lightyear?

How far is the Moon from the Earth ?

How far is the Earth from the Sun ?

How far is the Earth from the next nearest star, Proxima Centauri?

LightyearsWhat does a light year measure?

How many kilometers in a lightyear?

How far is the Moon from the Earth ?

How far is the Earth from the Sun ?

How far is the Earth from the next nearest star, Proxima Centauri?

LightyearsWhat does a light year measure?

How many kilometers in a lightyear?

How far is the Moon from the Earth ?

How far is the Earth from the Sun ?

How far is the Earth from the next nearest star, Proxima Centauri?

Page 21: Astronomy Unit 2: Stars and Galaxies

Units of DistanceSection

Range (m)Unit Example Items≥ <

Subatomic 0 10−15 am electron, quark, string, Planck length

Atomic to cellular

10−15 10−12 fm proton, neutron10−12 10−9 pm wavelength of gamma rays and X-rays, hydrogen atom

10−9 10−6 nm DNA helix, virus, wavelength of optical spectrum

Human scale

10−6 10−3 µm bacterium, fog water droplet, human hair[1]

10−3 100 mm mosquito, golf ball, football100 103 m human being, football field, Eiffel Tower

103 106 km Mount Everest, length of Panama Canal, larger asteroid

Astronomical

106 109 Mm the Moon, Earth, one light-second109 1012 Gm Sun, one light-minute, Earth's orbit1012 1015 Tm orbits of outer planets, Solar System1015 1018 Pm one light-year; distance to Proxima Centauri1018 1021 Em galactic arm1021 1024 Zm Milky Way, distance to Andromeda Galaxy1024 ∞ Ym visible universe

Page 22: Astronomy Unit 2: Stars and Galaxies

Scale of the Universe

• The Scale of the Universe• The Scale of the Universe Video• http://www.atlasoftheuniverse.com/

Page 23: Astronomy Unit 2: Stars and Galaxies

Stars

Page 24: Astronomy Unit 2: Stars and Galaxies

Stars

star: a massive ball of hot gases that emits its own light

Page 25: Astronomy Unit 2: Stars and Galaxies

Our Galaxy: The Milky Way Galaxy

Our Sun and The Earth

Page 26: Astronomy Unit 2: Stars and Galaxies

The Sun is our closest Star

• Sun: the medium-sized star in the center of the system of objects in space that includes Earth

Page 27: Astronomy Unit 2: Stars and Galaxies

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star.

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star.

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star.

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star.

Page 29: Astronomy Unit 2: Stars and Galaxies

Lifecycle of Star

Page 31: Astronomy Unit 2: Stars and Galaxies

Hertzprung Russell Diagram

Page 32: Astronomy Unit 2: Stars and Galaxies

Nebula –

Horsehead Nebula

Pillars of Creation in the Eagle Nebula

nebula: a cloud of space dust that can clump together to form a star; the plural of nebula is nebulae

Stellar Nursery

Space Cats

Video about Pillars of Creation

Page 33: Astronomy Unit 2: Stars and Galaxies

Average Star and Massive Stars

Page 34: Astronomy Unit 2: Stars and Galaxies

Red Giant

Page 35: Astronomy Unit 2: Stars and Galaxies
Page 36: Astronomy Unit 2: Stars and Galaxies

White Dwarf

Page 37: Astronomy Unit 2: Stars and Galaxies

Red Super giant

Page 38: Astronomy Unit 2: Stars and Galaxies

Supernova

• SupernovaBLAST FROM THE PAST: Type IIn supernovae are believed to represent the collapse of massive stars surrounded by dense shrouds. Eta Carinae in the Milky Way is shown for illustration; it is a massive star (or pair of stars) surrounded by a nebula of material it cast off in the past.

Page 39: Astronomy Unit 2: Stars and Galaxies

Neutron Stars

A very small dense star that is composed mostly of tightly-packed neutrons (neutronium).

The Crab Nebula

Page 41: Astronomy Unit 2: Stars and Galaxies

Life Cycle Stars

Massive Star Main Sequence Star

Our Sun is medium sized main sequence star

Page 42: Astronomy Unit 2: Stars and Galaxies

Life Cycle of Stars

Page 43: Astronomy Unit 2: Stars and Galaxies

Hertzsprung – Russell Diagram

Hotter

Brighter

Page 44: Astronomy Unit 2: Stars and Galaxies

Hertzsprung – Russell Diagram

• Hertzsprung-Russell (H-R) diagram is used to classify stars

Page 45: Astronomy Unit 2: Stars and Galaxies
Page 46: Astronomy Unit 2: Stars and Galaxies

_____________ - ____________ Diagram

_____________ - ____________ Diagram_____________ - ____________ Diagram

_____________ - ____________ Diagram

Page 47: Astronomy Unit 2: Stars and Galaxies

___________- _________ Diagram ___________- _________ Diagram

___________- _________ Diagram ___________- _________ Diagram

Page 48: Astronomy Unit 2: Stars and Galaxies

Glue Nows

Page 49: Astronomy Unit 2: Stars and Galaxies

Star Type #4

Star Type #3

Star Type #2

Star Type #1

_____________________________________DiagramUsed to classify stars

Do N

ow!!

!!

Page 50: Astronomy Unit 2: Stars and Galaxies
Page 51: Astronomy Unit 2: Stars and Galaxies

universe: everything that exists in space, including all matter

and energy

galaxy: a large group of stars, space dust, and gases held

together by gravity

Milky Way: the galaxy in which the Sun is located

star: a massive ball of hot gases that emits its own light

Sun: the medium-sized star in the center of the system of

objects in space that includes Earth

nebula: a cloud of space dust that can clump together to form a

star; the plural of nebula is nebulae

Hertzsprung-Russell (H-R) diagram: a diagram that displays the

relationship between a star’s surface temperature and its

magnitude, or brightness

luminosity: a measure of the energy released each second from

the surface of a star

light year: a unit of length equal to the distance that light

travels in one year

Astronomy Unit 2 Vocabulary

universe: everything that exists in space, including all matter

and energy

galaxy: a large group of stars, space dust, and gases held

together by gravity

Milky Way: the galaxy in which the Sun is located

star: a massive ball of hot gases that emits its own light

Sun: the medium-sized star in the center of the system of

objects in space that includes Earth

nebula: a cloud of space dust that can clump together to form a

star; the plural of nebula is nebulae

Hertzsprung-Russell (H-R) diagram: a diagram that displays the

relationship between a star’s surface temperature and its

magnitude, or brightness

luminosity: a measure of the energy released each second from

the surface of a star

light year: a unit of length equal to the distance that light

travels in one year

Astronomy Unit 2 Vocabulary

Page 52: Astronomy Unit 2: Stars and Galaxies

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

__________________________

Page 53: Astronomy Unit 2: Stars and Galaxies

Planets Inner Rocky Planets1.2.3.4.Asteroid BeltGaseous Giants5.6.Ice Giants7.8.Dwarf Planets9.

Planets Inner Rocky Planets1.2.3.4.Asteroid BeltGaseous Giants5.6.Ice Giants7.8.Dwarf Planets9.

PlanetsInner Rocky Planets1.2.3.4.Asteroid BeltGaseous Giants5.6.Ice Giants7.8.Dwarf Planets9.

PlanetsInner Rocky Planets1.2.3.4.Asteroid BeltGaseous Giants5.6.Ice Giants7.8.Dwarf Planets9.

Page 54: Astronomy Unit 2: Stars and Galaxies

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star;

Our _________ is a ________________-sized star near the edge of a ___________ galaxy named ____________________.

Our Sun is many thousands of times closer to Earth than any other star;

SectionRange (m)

Unit Example Items≥ <

Subatomic 0 10−15 am electron, quark, string, Planck length

Atomic to cellular

10−15 10−12 fm proton, neutron

10−12 10−9 pm wavelength of gamma rays and X-rays, hydrogen atom

10−9 10−6 nm DNA helix, virus, wavelength of optical spectrum

Human scale

10−6 10−3 µm bacterium, fog water droplet, human hair[1]

10−3 100 mm mosquito, golf ball, football

100 103 m human being, football field, Eiffel Tower

103 106 km Mount Everest, length of Panama Canal, larger asteroid

Astronomical

106 109 Mm the Moon, Earth, one light-second

109 1012 Gm Sun, one light-minute, Earth's orbit

1012 1015 Tm orbits of outer planets, Solar System

1015 1018 Pm one light-year; distance to Proxima Centauri

1018 1021 Em galactic arm

1021 1024 Zm Milky Way, distance to Andromeda Galaxy

1024 ∞ Ym visible universe

SectionRange (m)

Unit Example Items≥ <

Subatomic 0 10−15 am electron, quark, string, Planck length

Atomic to cellular

10−15 10−12 fm proton, neutron

10−12 10−9 pm wavelength of gamma rays and X-rays, hydrogen atom

10−9 10−6 nm DNA helix, virus, wavelength of optical spectrum

Human scale

10−6 10−3 µm bacterium, fog water droplet, human hair[1]

10−3 100 mm mosquito, golf ball, football

100 103 m human being, football field, Eiffel Tower

103 106 km Mount Everest, length of Panama Canal, larger asteroid

Astronomical

106 109 Mm the Moon, Earth, one light-second

109 1012 Gm Sun, one light-minute, Earth's orbit

1012 1015 Tm orbits of outer planets, Solar System

1015 1018 Pm one light-year; distance to Proxima Centauri

1018 1021 Em galactic arm

1021 1024 Zm Milky Way, distance to Andromeda Galaxy

1024 ∞ Ym visible universe

Page 55: Astronomy Unit 2: Stars and Galaxies
Page 56: Astronomy Unit 2: Stars and Galaxies

Elliptical

Spiral

Irregular

Elliptical

Spiral

Irregular

Page 57: Astronomy Unit 2: Stars and Galaxies

• Hertzsprung-Russell (H-R) diagram: a diagram that displays the relationship between a star’s surface temperature and its magnitude, or brightness

Hertzsprung – Russell Diagram

Page 58: Astronomy Unit 2: Stars and Galaxies
Page 59: Astronomy Unit 2: Stars and Galaxies
Page 60: Astronomy Unit 2: Stars and Galaxies