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Galaxies and the Universe Ch 25 Sectio n 3

Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

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Page 1: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Galaxies and the UniverseCh 25

Section 3

Page 2: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

What are the objects in the sky?

GALAXIES!Groups of stars, dust, and gases held together

by gravity

Page 3: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Classification of GalaxiesBy shape & age of stars:

As # increases, the shape becomes more elliptical.

As the lowercase letters advance through the alphabet, the arms becomes more tightly wound.

ellipse

spiral bar

spiral

Page 4: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

1. Spiral (disc-like) – has spiral arms

Page 5: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

2. Elliptical – nearly circular shape

Page 6: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

3. Irregular - no distinct shape

Page 7: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Milky Way Galaxy• Spiral shape• 100 billion+ stars• Looks “milky” flat disk we view from inside & see stars in EVERY direction• Solar system completes one orbit in galaxy every 200 million years

• Made of:– Galactic disk: younger stars– Nuclear bulge: center; highest density of stars older

stars– Halo: around bulge & disk; thin gas; 90% of mass is

here

What does this mean about the formation of our galaxy?

Page 8: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

What’s at the center?

A galactic black hole• Found by motion of stars close to Sagittarius A

(near center)• Probably formed early in universe history

– Gas clouds and stars probably collided, formed a massive object, and then collapsed

Page 9: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity
Page 10: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Where Are We?• The Orion arm

(about 3/4 of the way down)• How fast is our solar

system moving?– 220 km/s

• How long does it take our solar system to make one orbit around the Milky Way?– About 240 million years– about 20 times so far

Page 11: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Milky Way

We Are Here

Page 12: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Big Bang Theory• Theory that the universe began as a point and

has been expanding ever since– Thought to have begun as an infinitesimally small,

hot, and dense “singularity”.– About 14 (13.7) billion years ago

• Singularities are zones which defy our current understanding of physics– pressure is thought to be so intense that finite matter

is actually squished into infinite density

Page 13: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity
Page 14: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Radiation Domination• After big bang

– Universe was hot & made of energy (radiation)

– Expansion & cooling sub-atomic particles formed (protons, neutrons, etc.)

– H+ nuclei started to form (still too hot for atom formation)

• Big bang theory constantly being tested– As new discoveries emerge– Scientists come up with

hypotheses & confirm over time using laws of science & infer what happened

Page 15: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Expansion of the UniverseUniverse has two opposing forces:1. Momentum of outward expansion2. Gravity pushing inward to slow expansion

Momentum Expansion

Gravity Gravity

Page 16: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

• What happens depends on which of the forces is stronger

• Creates a period of expansion followed by cooling that continues to happen now

Page 17: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Expanding Universe: Evidence1. Doppler Effect

– Red shifts of galaxies• Edwin Hubble (1929): galaxies shifting away light

waves stretched• Hubble’s Law:

– Objects moving away from Earth universe is expanding– Galaxies are retreating from Earth @ a speed that is

proportional to their distance» Greater red shifts= faster speeds

– Imagine dots on a balloon being blown up

Page 18: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

What do you notice about the galaxies?

Scientists have been able to track the distances between galaxies and how far away they are moving

Page 19: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Expanding Universe Evidence2. Cosmic Background Radiation

• Discovered in 1965 (background noise in

radio antenna)• Shorter wavelengths

(when hot) that became longer (when cooled)

Weak radiation left over from the early, hotstages of the Big Bang expansion

• Today are microwaves (1 mm) in radio portion of electromagnetic spectrum

Page 20: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Outcome of UniverseThree possibilities:1. Open

– expansion will never stop (density insufficient for gravity)

2. Closed– expansion stops and

begins to contract (density high enough gravity pulls mass in)

3. *Flat

– expansion slows to a halt, but does not contract

*widely accepted theory by scientists

Outcome depends on density of universe (unknown).

Page 22: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Another View of the Universe’s Outcome

Page 23: Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity

Solar System vs. Galaxy vs. Universe?

• Solar System: Consists of the Sun, and everything bound to it by gravity. This includes the 8 planets and their moons, the asteroids, the dwarf planets, all the Kuiper belt objects, the meteoroids, comets and interplanetary dust.

• Galaxy: large system of stars held together by mutual gravitation and isolated from similar systems by vast regions of space. The Milky Way measures about 100,000 light-years across, and is thought to contain 200 billion stars.

• Universe: the totality of known or supposed objects and phenomena throughout space; the cosmos; macrocosm.

So to sum it up:• We live on planet Earth which is part of our local Solar System.

• Our Solar System includes the Sun and everything that orbits the Sun.• Our Sun, is just one Star in the Milky Way Galaxy.

• The Milky Way Galaxy is just one Galaxy in the Universe.