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The Solar System, stars, the Universe

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Title: The Solar System, stars, the Universe


1
The Solar System, stars, the Universeand 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.

2
The Solar System
  • All the objects within the Suns zone of
    gravitational influence.
  • The Sun
  • 99 of the solar system mass
  • 110 Earths diameter
  • 4.5 billion years old (10 billion year life
    expectancy)
  • An unremarkable star.

3
Tiny Terrestrial Planets
Mercury hot, airless Venus hot, thick
atmosphere Earth moderate atmosphere,
warm. Moon no atmosphere, chillier. Mars
tiny atmosphere, chilly indeed.
4
Giant Jovian Planets
  • Jupiter enormous, about 1 stellar mass.
  • Saturn very large, spectacular rings.
  • Uranus cold, relatively quiet tilted sideways.
  • Neptune strangely turbulent.

5
Solar System Detritus
  • Interplanetary dust
  • Asteroids
  • Asteroid belt (2.1-3.3 au)
  • 1-2106 objects 4 Moons mass. (CONFUSED BY
    SCIENTIFIC NOTATION? Read Appendix C)
  • 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.

6
The Solar Systemdistance scale
(set 1 au15m, 50 ft)
  • Sun diameter17 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

7
The Sun and Jupiter
8
The Solar System distance scale
(set 1 au15m, 50 ft)
  • 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)

9
Sun, Neptune, Kuiper Belt
10
The Solar System distance scale
(set 1 au15m, 50 ft)
  • Öort cloud 750 km (470 miles)
  • (Sierra College to San Diego)
  • Nearest star 4000 km (2500 miles)
  • (Sierra College to New York City)

11
Stars
  • Our Sun is a relatively common type

12
  • 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
The smallest stars have very little raw
fuel but, they use it sparingly ? Tiny stars
live very, very long times
13
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.

14
Supernovae friends and foes
  • Produce atoms more massive than iron.
  • Cause ionizing events there is no defense!

15
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).

16
  • Galactic recycling (star-gas-star cycle)
  • Interstellar medium (ISM) is mostly H, He
  • Star formation occurs
  • Stars produce winds which fertilize the ISM
  • Stars supernovae, further fertilizing the ISM.

17
Types of galaxies
  1. Spirals
  2. Ellipticals
  3. Irregulars

18
Galactic evolution
  • All galaxies seem likely to harbor supermassive
    black holes106 - 108 the mass of the Sun.
  • Central black holes calm down in time
  • Galaxies collide with each other
  • Galaxies consume their interstellar matter

19
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.

20
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?

21
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 Universes
    history, treated by the Big Bang Theory!

22
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 or (especially) Astro 25 for
    details!

23
The Enormity of Timelines
  • Age 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 sapiens
  • 200,000 years (0.0014 of Universes age)
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