Title: What is your Cosmic Address?
1What is your Cosmic Address?
Street City State Country Continent Hemisphere P
lanet
2Realm Guesses Guesses Guesses Guesses Guesses Guesses
Realm Group 1 Group 2 Group 3 Group 4 Group 5 Group 6
Earth Salt grain Salt grain Salt grain Salt grain Salt grain Salt grain
Sun
Solar System
Solar Neighborhood
Galaxy
Local Group
Local Supercluster
Universe
3Realm Actual Size (km) Actual Size (light-years) Multiple X larger than Earth Scale Model
Earth 12,700(1.27E4) 1.4 billionths(1.4E-9) 1 salt grain(0.1 mm)
Sun 1.39 million(1.39E6) 1.5 ten-millionths(1.5E-7) 109(1.09E2) gum ball(1.9 cm)
Solar System 30 billion(3.0E10) 0.0032(3.2E-3) 2.34 million(2.34E6) football stadium(234 meters)
Solar Neighborhood 617 trillion(6.17E14) 65(6.5E1) 48 billion(4.8E10) Mercury(4,800 km)
Galaxy 963 quadrillion(9.63E17) 100,000(1.0E5) 75 trillion(7.5E13) 5.4 x Sun(7.5 million km)
Local Group 31 quintillion(3.1E19) 6.5 million(6.5E6) 2.4 quadrillion(2.4E15) Orbit of Mars(1.6 AU)
Local Supercluster 1.2 sextillion(1.2E21) 130 million(1.3E8) 97 quadrillion(9.7E16) Orbit of Eris (68 AU)
Universe 860.9 sextillion(8.6E23) 91 billion(9.1E10) 68 quintillion(6.8E19) Oort Cloud(48,000 AU or 0.76 ly)
4Realms of the Universe
Image courtesy of The Cosmic Perspective by
Bennett, Donahue, Schneider, Voit Addison
Wesley, 2002
5Earth
- Planet where we all live
- Comprised primarily of rock
- Spherical in shape
- 12,700 km in diameter
- It would take 17 days to circumnavigate the globe
driving a car at 100 km/hr - At the speed of light, it would take 0.13 seconds
to go all the way around Earth.
6Sun
- Star that Earth orbits
- Composed primarily of hydrogen and helium gas
- Uses nuclear fusion in its core to generate heat
and light to allow itself to resist the crushing
weight of its own mass - Spherical in shape
- 1.39 Million km in diameter
7Earth Sun
- The Suns diameter is 109 times greater than that
of Earth - Over 1 million Earths would fit inside the Suns
volume - Earth orbits the Sun at an average distance of
150 million kilometers. This distance is called
an Astronomical Unit (AU) - It would take 11,780 Earths lined up side to side
to bridge the 1 AU between Earth and Sun.
8The Solar System
- 8 planets, thousands and thousands of dwarf
planets and asteroids, trillions of comets and
meteoroids - Mostly distributed in a disk about the Sun
- Sun blows a constant wind of charged gas into
interplanetary space, called the Solar Wind
Boundary between Solar Wind and interstellar
space at 100 AU from the Sun (200 AU diameter)
9The Solar Neighborhood
- The region of the Galaxy within about 32.6
light-years of the Sun (65 light-years diameter)
is considered its neighborhood. - Here stars move generally with the Sun in its
orbit around the center of the Galaxy - This region is inside a large bubble of hot
interstellar gas called the Local Bubble. Here
the gas temperature is about 1 million degrees
Kelvin and the density is 1000 times less than
average interstellar space.
To Center of Galaxy
The image is 390 light-years across.
Direction of Galactic Rotation
10The Milky Way Galaxy
The Milky Way Galaxy is a giant disk of stars
100,000 light-years across and 1,000 light-years
thick.
The Sun is located at the edge of a spiral arm,
30,000 light-years from the center It takes 250
Million years for the Sun to complete one orbit
There are over 100 Billion stars in the Milky
Way The Spiral arms are only 5 more dense than
average, and are the locations of new star
formation
11The Local Group
- Contains 3 large spiral galaxies--Milky Way,
Andromeda (M31), and Triangulum (M33)plus a few
dozen dwarf galaxies with elliptical or irregular
shapes. - Gravitationally bound togetherorbiting about a
common center of mass - Ellipsoidal in shape
- About 6.5 million light-years in diameter
12- A cluster of many groups and clusters of galaxies
- Largest cluster is the Virgo cluster containing
over a thousand galaxies. - Clusters and groups of galaxies are
gravitationally bound together, however the
clusters and groups spread away from each other
as the Universe expands. - The Local Supercluster gets bigger with time
- It has a flattened shape
- The Local Group is on the edge of the majority of
galaxies - The Local Supercluster is about 130 Million
light-years across
The Local Supercluster
13The Universe
- Surveys of galaxies reveal a web-like or
honeycomb structure to the Universe - Great walls and filaments of matter surrounding
voids containing no galaxies - Probably 100 Billion galaxies in the Universe
The plane of the Milky Way Galaxy obscures our
view of what lies beyond. This creates the
wedge-shaped gaps in all-sky galaxy surveys such
as those shown here.
14The Universe
The observable Universe is 91 Billion light-years
in diameter.
Computer Simulation
151) The Standard Ruler
There are two basic methods for measuring
astronomical distances
- Use knowledge of physical and/or geometric
properties of an object to relate an angular size
with a physical size to determine distance. - Ex Parallax, Moving Clusters, Time Delays, Water
MASERs - Considered to be a direct or absolute
measurement.
R
?
d
d R/Tan(?) ? R/?
16Trigonometric Parallax
- Requires very precise measurements of stellar
positions, and long baselines - Need telescopes with high resolution, and must
observe over several years. - Hipparchos satellite measured distances to tens
of thousands of stars within 1,500 light-years of
the Sun.
172) The Standard Candle
- Use knowledge of physical and/or empirical
properties of an object to determine its
Luminosity, which yields distance via the Inverse
Square Law of Light. - Ex Cepheid Variables, Supernovae, TRGB,
Tully-Fisher - Considered to be relative until tied to an
absolute calibration.
b L/4?d2
18Cepheid Variable Stars
- There is a kind of giant star whose surface
pulsates in and out with a regular period. That
period of pulsation is related to the Luminosity
of the star. - LMC contains hundreds of known Cepheids all at
the same distance. Which allows for robust
determination of the Period Luminosity
Relationship.
19To measure cosmological distances a ladder of
methods is used to reach further out into the
Universe.
Each rung in the ladder of distance measuring
methods depends on the calibration of the methods
below.