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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Presentation transcript:

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 Galaxies By 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

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

2. Elliptical – nearly circular shape

3. Irregular - no distinct shape

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?

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

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

Milky Way We Are Here

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

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

Expansion of the Universe Universe has two opposing forces: 1.Momentum of outward expansion 2.Gravity pushing inward to slow expansion Momentum Expansion Gravity

What happens depends on which of the forces is stronger Creates a period of expansion followed by cooling that continues to happen now

Exp and in g Universe: Evidence 1.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 a speed that is proportional to their distance » Greater red shifts= faster speeds – Imagine dots on a balloon being blown up

What do you notice about the galaxies? Scientists have been able to track the distances between galaxies and how far away they are moving

Expanding Universe Evidence 2. 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, hot stages of the Big Bang expansion Today are microwaves (1 mm) in radio portion of electromagnetic spectrum

Outcome of Universe Three 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).

ClosedFlatOpen

Another View of the Universe’s Outcome

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.