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The Solar System, stars, the Universe… …and you Setting a context for us in the Universe The solar system; Other stars; Our Milky Way Galaxy; Other galaxies; The Big Bang; The enormity of timelines; Take home message: a good idea of our place in space, and how the building blocks of life came to be.

The Solar System, stars, the Universe… …and you

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The Solar System, stars, the Universe… …and you. Setting a context for us in the Universe The solar system; Other stars; Our Milky Way Galaxy; Other galaxies; The Big Bang; The enormity of timelines; - PowerPoint PPT Presentation

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Page 1: The Solar System, stars, the Universe… …and you

The Solar System, stars, the Universe……and you

Setting a context for us in the Universe• The solar system;• Other stars;• Our Milky Way Galaxy;• Other galaxies;• The Big Bang;• The enormity of timelines;

Take home message: a good idea of our place in space, and how the building blocks of life came to be.

Page 2: The Solar System, stars, the Universe… …and you

Scientific notation

Before we can even begin…

10,000 = 1×104

600,000 = 6×105

0.00008 = 8×10-5

Page 3: The Solar System, stars, the Universe… …and you

The Solar System

All the objects within the Sun’s zone of gravitational influence.

The Sun– 99% of the solar system mass;

– 110 × Earth’s diameter;

– 4.5 billion years old (10 billion year life expectancy);

– An unremarkable star.

Page 4: The Solar System, stars, the Universe… …and you

Tiny Terrestrial Planets

Mercury – hot, airless;

Venus – hot, thick atmosphere;

Earth – moderate atmosphere, warm.

Moon – no atmosphere, chillier.

Mars – tiny atmosphere, chilly indeed.

Page 5: The Solar System, stars, the Universe… …and you

Giant Jovian Planets

Jupiter – enormous, about 1% stellar mass.

Saturn – very large, spectacular rings.

Uranus – cold, relatively quiet; tilted sideways.

Neptune – strangely turbulent.

Page 6: The Solar System, stars, the Universe… …and you

Solar System Detritus

Interplanetary dust

Asteroids—Asteroid belt (2.1-3.3 au); —1-2×106 objects; 4% Moon’s mass.

Kuiper belt—30-50 au;—105 cometary objects;—Largest known is Eris (2500 km diameter).

Comets—Periodic (i.e., Tempel, 5.5y orbit); —Öort cloud (50,000 au);—1012 cometary objects.

Page 7: The Solar System, stars, the Universe… …and you

The Solar System:distance scale

Sun: diameter=17 cm (6.6 inches)

Earth: diameter = 2 mm (1/16 inches);

15 m from Sun

Jupiter: diameter = 1.4 cm (1/2 inch);

80 m from Sun

(set 1 au=15m, 50 ft)

Page 8: The Solar System, stars, the Universe… …and you

The Sun and Jupiter

Page 9: The Solar System, stars, the Universe… …and you

The Solar System: distance scale

Neptune: diameter = 0.5 cm (1/5 inch); 450 m from Sun (1/4 mile)

Kuiper belt: 450-750 m from Sun (1/4 – 1/2 miles)

(set 1 au=15m, 50 ft)

Page 10: The Solar System, stars, the Universe… …and you

Sun, Neptune, Kuiper Belt

Page 11: The Solar System, stars, the Universe… …and you

The Solar System: distance scale

Öort cloud = 750 km (470 miles)

(Sierra College to San Diego)

Nearest star = 4000 km (2500 miles)

(Sierra College to New York City)

(set 1 au=15m, 50 ft)

Page 12: The Solar System, stars, the Universe… …and you

Stars

Our Sun is a relatively common type

Page 13: The Solar System, stars, the Universe… …and you

Stars

Each different kind has a different life history…

The bigger stars have more raw fuel……but, they use it faster

Big stars burn out quickly

Big stars produce a great deal of harmful radiation

The smallest stars have very little raw fuel……but, they use it sparingly

Tiny stars live very, very long times

Tiny stars produce low energy radiation

Page 14: The Solar System, stars, the Universe… …and you

Stars and nucleosynthesis

Stars turn hydrogen into helium via nuclear fusion;

Stars also fuse helium into carbon, and the most massive engage in even more complicated atomic fusion reactions that produce other atoms such as phosphorus, nitrogen, etc.

Carbon stars are giants that lose up to half their mass via huge winds that blow off their surfaces.

Page 15: The Solar System, stars, the Universe… …and you

Supernovae: friends and foes

Produce atoms more massive than iron.

Cause ionizing events – there is no defense!

Page 16: The Solar System, stars, the Universe… …and you

The Milky Way Galaxy

A massive grouping of stars, dust, and gas, and related phenomena.

Dimensions– Disk 100,000 LY across; 1000 LY thick;– We are 28,000 LY from center;– 100 billion times mass of Sun (interior to Rsun).

Page 17: The Solar System, stars, the Universe… …and you

Galactic recycling (star-gas-star cycle)

Interstellar medium (ISM) is mostly H, He;

Star formation occurs;

Stars produce winds which churn and fertilize the ISM;

Stars supernovae, further fertilizing the ISM.

Page 18: The Solar System, stars, the Universe… …and you

Types of galaxies

1. Spirals

2. Ellipticals

3. Irregulars

4. Active

All galaxies seem likely to harbor supermassive black holes (108 × the mass of the Sun).

These black holes were apparently more active in the distant past.

Page 19: The Solar System, stars, the Universe… …and you

Galactic evolution

Central black holes calm down in time;

Galaxies collide with each other;

Galaxies consume their interstellar matter;

Important: not all galaxies have as much dust and gas as ours does!

Page 20: The Solar System, stars, the Universe… …and you

Galaxy groups

Galaxies occur in clusters

Clusters occur in superclusters

– Nearest large galaxy (Andromeda galaxy) is

2.5 MLY away.

– Superclusters are about 100 MLY across.

Page 21: The Solar System, stars, the Universe… …and you

Receding galaxies

Redshift studies have revealed that nearly all galaxies are rushing away from us.

The farther a galaxy is from us, the faster it is rushing away.

Truly distant galaxies are rushing away from us at speeds approaching the speed of light!

What is the matter with us?

Page 22: The Solar System, stars, the Universe… …and you

The Big Bang

Galaxies are receding from us because space is expanding.

This is NOT a cosmic explosion in space. It is a cosmic explosion OF space.

All points in the Universe see galaxies receding from them.

This was the first hint of the Universe’s history, treated by the Big Bang Theory!

Page 23: The Solar System, stars, the Universe… …and you

Consequences of the Big Bang theory

The Universe…… enlarged and cooled with time… started out as pure H and He.… continues to age…

The Big Bang theory accurately explains the relative H and He concentrations in the Universe, its clumpiness, age, background radiation, and other things.

Dark Matter and Dark Energy are recent discoveries needed to explain some observations.

… See Astro 5, Astro 10, or (especially) Astro 25 for details!

Page 24: The Solar System, stars, the Universe… …and you

The Enormity of TimelinesAge of Universe:

13.5-14 billion years

Age of Milky Way Galaxy:at least 13.2 billion years

Age of Sun:4.6 billion years

Age of Earth:4.5 billion years

First life on Earth:3.7 billion years

Homo sapiens200,000 years (0.0014% of Universe’s age)