Title: CP Space Science Unit (Textbook reference Chapters 12, 13, 14, 15 and 16)
1CP Space Science Unit(Textbook reference
Chapters 12, 13, 14, 15 and 16)
2Key Ideas
- Galaxies clusters of stars different shapes
- Stars Sun differ in size, temperature and
color source for all bright objects - Gravity planets, stars, solar system
- Know the appearance, composition, position and
size, and motion of objects in our solar system - Astronomical units for measuring
3What is astronomy?
4?
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5M33, The Pinwheel Galaxy in Triangulum by George
Greaney
What is astronomy?
M33, The Pinwheel Galaxy in Triangulum by George
Greaney
6Basically, if its off this planet its a study of
some realm of astronomy. As one might
imagine that covers an awful lot of subjects,
even more than we know right now.
- NGC 253, galaxy in Sculptor
- by George Greaney
7What is astronomy?
Galaxy M83 in Hydra by George Greaney
8- Stars
- Nebula
- Planets
- The Sun
- Star clusters
- Galaxies
- Galaxy clusters
- Dark matter
- Black holes
- The Great Andromeda Galaxy
- by George Greaney
9What is an astronomer?
Galileo Galilei (1564-1642)
A night watchman with a college education?
10An astronomer is a scientist, skilled in
mathematics, physics, and astronomy.
Most professional astronomers work for
universities or government agencies.
Galileo Observatory in Italy
Source The Berkeley Cosmology Group
11Few astronomers spend much time looking through
a telescope. Most operate telescopes from a
control room or even from their computer at
home via the Internet. Typical astronomers only
spend one or two weeks each year observing, and
the rest of their research time analyzing their
data.
Astronomer Serena Kim at work At Cerro Tololo in
Chili
Source Applied Theoretical and Computational
Physics DivisionLos Alamos National Laboratory
12Amateurs and their tools
13What is an amateurastronomer?
Although the term has different meanings for
different people, a basic definition would
include anyone who looks into the sky, and
wants to see or learn more.
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15The Expanding Universe 15-5
- Theories on How the Universe Formed
- The Big Bang Theory
- Steady-State Theory and Plasma Theory
- Hubbles Law
- Age of the Universe
16What is space like?
- No air
- No gravity-when youre not very close to a
planet, sun, or moon - No wind
- No friction
- No real up or down
- No pressure
17What is a galaxy? (Textbook reference 15-4)
- A large group of stars outside of our own Milky
Way - Made of billions to trillions of stars
- Also may have gas and dust
- Spiral, or elliptical, or irregular shaped
Image at http//hubblesite.org/newscenter/archive/
releases/galaxy/spiral/2007/41/results/50/
18Spiral galaxy--Andromeda
NOAO/AURA/NSF Images at http//www.noao.edu/image_
gallery/html/im0606.html and http//www.noao.edu/i
mage_gallery/html/im0685.html
19Elliptical Galaxies
Images at http//hubblesite.org/newscenter/archive
/releases/galaxy/elliptical/2007/08/image/a/format
/large_web/results/50/ and http//hubblesite.org/n
ewscenter/archive/releases/galaxy/elliptical/1995/
07/results/50/
20Irregular Galaxies
NASA and NOAO/AURA/NSF Images at
http//hubblesite.org/newscenter/archive/releases/
galaxy/irregular/2005/09/results/50/ ,
http//www.noao.edu/image_gallery/html/im0560.html
, and http//www.noao.edu/image_gallery/html/im09
93.html
21Our Galaxy the Milky Way
- has about 200 billion stars, and lots of gas and
dust - is a barred-spiral (we think)
- about 100,000 light-years wide
- our Sun is halfway to the edge, revolving at half
a million miles per hour around the center of the
Galaxy - takes our Solar System about 200 million years to
revolve once around our galaxy
22The Milky Way
Image at http//news.nationalgeographic.com/news/b
igphotos/1945371.html
23Mapping the Milky Way
How do we know what our galaxy looks like?
- We can see
- stars
- star clusters
- nebulae
- galaxies
24Reviewing Galaxies
- Groups of stars, planets, and space debris
- Irregular, Elliptical, Spiral
- Milky Way is our galaxy
25Image of the Sun from Goddard Space Flight Center
26What is a Star? Our Sun is the closest star. At
the simplest, a star is just a ball of gas that
has condensed out of interstellar material. The
largest part of its lifetime is spent as a main
sequence star during which hydrogen is being
converted to helium balancing gravitational
contraction so that the radius and energy output
remain almost constant.
Source The British Astronomical Association
27Stars (Textbook reference 15-2 and 15-3)
- Bodies of gases that give off tremendous amounts
of radiant and heat energy - Constellations are groups of stars used for
navigation, storytelling, honoring heroes
Life Cycle of a Star Video
28Nearby Stars Name Distance from
Earth Sun 93 million miles (8 light minutes)
Proxima Centauri 4.22 Light Years Alpha Centuri
A,B 4.39 Light Years Barnards Star 5.94 Light
Years Wolf 359 7.8 Light Years Lalande 21185
8.3 Light Years Sirius A,B 8.6 Light
Years
Image courtesy of Dave DockeryAstronomical
Society of Las Cruces Source The British
Astronomical Association
29Evolution of Stars
30How do Black Holes form?
31Black Holes
- Remains of a neutron star that has collapsed due
to intense gravity - Event horizon surface of a black hole from
which light cannot escape
32Hertzsprung-Russell Diagram
Video on the Hertzsprung-Russell Diagram
The Doppler Effect Red Shift stars moving
away from Earth Blue Shift stars moving toward
Earth
Spectroscopy Video
33Hertzsprung-Russell Diagram
Images from http//www.nasa.gov/centers/goddard/ne
ws/topstory/2007/spectrum_plants.html and
http//sunearthday.gsfc.nasa.gov/2009/TTT/65_surfa
cetemp.php
34Using a Stars Spectrum
- We can use a stars spectrum to classify it.
NOAO/AURA/NSF image at http//antwrp.gsfc.nasa.gov
/apod/ap010530.html
35Time to Create a Stellar Graph
- Everyone will receive several stars
- Place them on the large paper, according to their
color and their brightness - This is a version of the Hertzsprung-Russell
diagram.
36Measuring Distances
- Parallax (lets model it)
- As Earth orbits the Sun, we see nearby stars move
relative to more distant stars - How many degrees did the plate move, relative to
the background? - Can you calculate the distance to the plate?
- The angles involved for stellar observations are
very small and difficult to measure. Proxima
Centauri, has a parallax of 0.77 arcsec. This
angle is approximately the angle subtended by an
object about 2 centimeters in diameter located
about 5.3 kilometers away.
37The Sun (Textbook reference 14-2
- The sun is an ordinary star.
- The sun is the biggest, brightest, and hottest
object in the solar system. - Its energy is the result of the fusion of
hydrogen nuclei into helium nuclei. - The sun is made of about 70 hydrogen and 28
helium.
38Characteristics of the Sun
- Interior Core, Radiation Zone, Convection Zone
- Exterior Photosphere, Chromosphere, Corona
- Features Sunspots, Prominences, Solar Flares
- Central star in our solar system around which
planets revolve - Composed of gases (H2 and He) burning at
15,000,000 o C
39The Sun Seasons (Textbook Reference 12-1)
Seasons Solstices sun directly
overhead two times a year (June 21 and December
21) Junelongest day, Decembershortest
day Equinoxes halfway between
solstices neither hemisphere is tilted toward
the sun daylight and darknessequal
40What causes the seasons?
- 23.5 tilt of Earths axis
- Direct vs. indirect sun rays
- Length of daylight
41Fall
Summer
Sun
Winter
Spring
42The Sun Solar Energy (14-2)
Energy in the Atmosphere Energy reaches earths
atmosphere Reflected back or absorbed clouds,
dust and gases surface Energy is transferred
within the troposphere radiation heats land
and water reflected back into
atmosphere convection moves heat through the
troposphere warm air is replaced by
denser, cool air conduction transfers heat
from land and water directly into the
air nearest Earths surface
43Our Sun is a star that has already spent about 5
billion years on the main sequence.
Scientist believe our Sun is roughly
halfway through it's life.
Source The British Astronomical Association
44Earths Moon
Stars are the source of light for all objects in
outer space
45Phases of the Moon (Textbook reference 12-3)
waxing increasing waning
decreasing gibbous gt ½ crescent lt
½
46Lunar Phases
47Lunar Phases
48Rotate vs. Revolve
- Rotation spin of an object on its axis
- Revolution orbit of an object around another
object
49Moons Orbit and Phases
50Why does one side of the moon always face us?
- Moon rotates once every 27.3 days
- Moon revolves once every 29.5 days
- Moons rotation approximately equal to its
revolution
51Eclipses
- Lunar Eclipse
- Solar Eclipse
- Total Eclipse
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54A total eclipse of the sun occurs during the day!
Only the corona is visible.
55Tides
- Effect of gravity between the moon and the sun
56Spring Tides
- When the sun, the moon, and the Earth are all
aligned in a 180o angle
57Neap Tide
- When the sun, the moon, and the Earth form a 90
angle
58Stars are the source of light for all objects in
outer space
- Complete the standards-based reading handed out
in class to address this concept - Answer the assessment questions that accompany
the handout
59SOLAR SYSTEM
- Sixty-one satellites of the planets
- Many Comets and asteroids
60Formation of the Solar System(Textbook reference
15-5)
61A collapsing interstellar cloud
- Stars and planets form from interstellar clouds
- They appear dark because of dust blocking out the
light - The light can cause it to glow, or even become
heated - Stars and solar systems are born this way
- Collapse accelerates
- The collapse of this cloud is slow, but it
accelerates and becomes denser at the center - This collapse and spin results in a flattening at
the equatorial plane
62- Matter condenses
- Our solar system may have formed this way when
temperature and pressure caused hydrogen to fuse
into helium - The temperature differential allowed for
different elements to concentrate in different
areas around the sun - This is why the inner planets are rocky and have
a higher melting point - Outer ones are less dense and made of ice and gas
63Planetesimals
- The planetesimals combined to get larger and in
many cases to become the known planets. - Gas giants form
- Jupiter was the first to form
- Icy planetesimals combined to form it
- Its mass (gravity) caused it to collect much of
the debris - The others formed the same way, but Jupiter took
most of the extraneous material
64- Terrestrial planets form
- the merging of planetesimals in the inner portion
of the disk - Made of materials that resist vaporization
- Most of the gaseous material and smaller stuff
consumed by the sun, hence fewer satellites. - Debris
- All of the junk left over
- Some became comets
- Some ejected from solar system or destroyed in
collisions - The asteroid belt between mars and Jupiter is the
rest
65The Greeks called the five points of light that
seemed to move among the stars ______, meaning
______.
PlanetsWandering Stars?
66The ancient Romans later called these planets
- Mercury
- Venus
- Mars
- Jupiter
- Saturn
67Greek Ideas Earth at the Center(Textbook
reference 14-1)
- Initially the geocentric theory stated that
everything moved around the earth. - Retrograde motion (apparent westward movement)
led astronomers to find a different explanation
68Describe the ancient Greek beliefs of the solar
system.
- The ancient Greeks thought Earth was a stationary
object and the sun, moon, and planets were on a
rotating celestial sphere
69Checkpoint What is a geocentric system?
- A geocentric system is one in which Earth is at
the center of a system of revolving planets.
70Figure 2 Interpreting DiagramsWhere is Earth
located in this illustration?
- The Earth is in the middle of the solar system
- The sun, moon, and a planet are orbiting Earth on
a large circle, while moving on a smaller cirlce
71How is Ptolemys model of the solar system differ
from the Greeks before him?
- The Greeks before Ptolemy thought the universe
was unchanging and the sun, moon, and planets
moved together on a celestial sphere (like a
carousel). Earth was stationary - Ptolemy introduced the idea of the sun, moon and
planets rotating on little circles which rotate
on bigger circles
72Copernicuss Idea Sun at the Center
- The heliocentric model (Copernicus) put the sun
at the center and planets in orbit around it. - Proximity to the sun caused planets to move at
different speeds - This explained retrograde
73Heliocentric
- A description of the solar system which all
planets revolve around the sun
74Guide For Reading How do the heliocentric and
geocentric descriptions of the solar system
differ?
- In a geocentric system, Earth is at the center of
the revolving planets. - In a heliocentric system, Earth and the other
planets revolve around the sun.
75What two discoveries made by Galileo supported
the heliocentric description of the solar system?
- Jupiters four moons revolve around the planet.
- Venus goes through phases similar to those of
Earths moon.
76Brahe, a ______ ______, made much more accurate
observations by carefully observing the positions
of the planets for almost _____ years.
Brahe and Kepler
77What did Kepler discover about the orbits of the
planets?
- Kepler had discovered that the orbit of each
planet is an ellipse. - Ellipse an elongated circle or oval shape.
78The Space Program (textbook reference 13-2)
- Space Race began in 1957 with the launch of the
Soviet satellite Sputnik I - Satellite an object revolving around another
object - Humans in Space
- Soviets launched the first human in 1961
- The Moon Landing
- 1969, Apollo 11, and Neil Armstrong and Buzz
Aldrin
79Exploring the Solar System (textbook reference
14-1 continued)
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81Ellipse
- An elongated circle, or oval shape the shape of
the planets orbit
82- Keplers Laws
- 1st law in general, the planets orbit the sun in
an ellipse - The eccentricity of the orbit is how squashed
the orbit is - 2nd law a line drawn from the sun to any planet,
sweeps out equal areas in equal times (although
the orbital distance may be different) - 3rd law he defined the size of the ellipse and
the orbital period (year)
83Which planets orbit did Kepler calculate to
discover that a planets orbit is not a circle?
84Inertia and Gravity (textbook reference 12-2)
85Inertia
- Inertia tendency of a moving object to continue
in a straight line or a stationary object to
remain in place.
86The more _____ an object has, the more ______ it
has.
87Gravity
- Gravity The attractive force between two
objects its magnitude depends on their masses
and the distance between them.
88The strength of gravity depends on the ______ of
the objects and the ______ between them.
89Figure 5 Interpreting Diagrams -What would
happen if a planet had no inertia?
- The planet would be pulled into the sun
90Figure 5 Interpreting Diagrams -What would
happen if a planet had no gravity?
- The planet would continue to travel straight off
into space
91Guide For Reading What two factors keep the
planets in their orbits?
- Newton concluded that two factors inertia and
gravity combine to keep the planets in orbit. - Inertia keeps the planets the moving
- Gravity from the sun keeps the planets from
traveling off in space
92Reviewing Gravity
- Gravity is the attractive force between 2 objects
- It is affected by mass and distance
- Gravity is what determines the orbit planets
follow - Newtons explanation of gravity supported
Keplers laws of planetary motion.
Dark Matter helps Gravitational Pull
93Solar System Characteristics (Textbook reference
14-3)
- Inner Planets
- Mercury, Venus, Earth, Mars
- Terrestrial planets with atmosphere and crust
94The Inner Planets
- Terrestrial Planets
- 4 inner planets
- Similar densities to Earth
- Solid rocky surfaces
95Mercury
- closest to the sun
- 1/3 Earths size(or the size of Earths moon)
- no moons
- solid and covered with craters
- almost no atmosphere
- the eighth largest planet(second smallest planet)
96- Surface
- covered with craters and plains
- the plains formed much like the maria on the moon
- the craters are smaller with less ejecta
- Interior
- the density suggests a dense core similar to the
Earth - the magnetic field suggests its partially molten
97Venus
- Sixth largest planet
- Sister planet to Earth
- About three-fourths the size of Earth
- Has no moons or rings
- The brightest object in our sky besides the sun
and moon because of proximity and albedo 75
- Surface is rocky and very hot (covered in
craters, volcanoes and mountains) - Atmosphere completely hides the surface and
traps the heat. - Probes and satellites have provided radar images
of 98 of the surface
98Earth
- Third planet from the sun
- Fifth largest planet
- Liquid covers 71 percent of the Earths surface.
- The Earth has one moon.
- Only planet known to have life and liquid water
- Atmosphere composed of composed of Nitrogen
(78), Oxygen (21), and other gases (1).
99Earth, from 6,100,000,000 km (3,700,000,000
miles) away can you find it?
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101Mars
- Fourth planet from the sun
- A thin atmosphere that contains mostly carbon
dioxide - Appears as bright reddish color in the night sky
- Surface features volcanoes and huge dust storms
- Has 2 moons Phobos and Deimos
102Moons of Mars
103Solar System Characteristics(Textbook reference
25-4)
- Outer Planets
- Jupiter, Saturn, Uranus, Neptune, Pluto
- Jovian planets have ring systems and gas
atmospheres (J, S, U, N) - Pluto is neither terrestrial or Jovian
104The Outer Planets(Textbook reference 14-4)
- The Gas Giants
- These planets include Jupiter, Saturn, Uranus
and Neptune - All larger than Earth by 15-300 times
105Jupiter
- The largest planet (1/10 of the sun and 11X
Earths) - Better than 70 of the planetary mass of the
solar system - 52 albedo
- Has a banded appearance
106Jupiter
- Rings have 3 parts Halo Ring, Main Ring,
Gossamer Ring - Brightest planet in sky
- Strong magnetic field
- 60 moons, 5 visible from Earth
107- Density is relatively low for its size
- The is because of it composition (H and He in gas
or liquid form. - Rotation
- Shortest day in the solar system about 10hrs
- This fast spin distorts the shape
- This also contributes to its banded appearance
- Belts are low lying dark-colored clouds
- Zones are high light-colored clouds
- Moons
- More than 60, but some are very small
- Mostly composed of ice and rock
- Gravity assist
108Jupiters Red Spot
- the great spot is a storm of swirling gas that
has lasted for better than 300 years - Jupiter does not have a solid surface. The planet
is a ball of liquid surrounded by gas.
109Moons of Jupiter
- Jupiter has four large Galilean moons, twelve
smaller named moons and twenty-three more
recently discovered but not named moons. - Well take a look at the four large Galilean
moons which were first observed by Galileo in
1610.
110Io
- Io is the fifth moon of Jupiter. Its the third
largest of Jupiters moons. - Io has hundreds of volcanic calderas. Some of the
volcanoes are active.
111Europa
- Europa is the sixth of Jupiters moons and is the
fourth largest. - It is slightly smaller than the Earths moon.
- The surface strongly resembles images of sea ice
on Earth. There may be a liquid water sea under
the crust. - Europa is one of the five known moons in the
solar system to have an atmosphere.
112Ganymede
- Ganymede is the seventh and largest of Jupiters
known satellites. - Ganymede has extensive cratering and an icy crust.
113Callisto
- Callisto is the eighth of Jupiters known
satellites and the second largest. - Callisto has the oldest, most cratered surface of
any body yet observed in the solar system.
114Saturn
- Second largest planet
- Sixth from the sun.
- Slightly smaller than Jupiter
- Easily visible in the night sky
- Voyager explored Saturn and its rings.
- Made of materials that are lighter than water.
(If you could fit Saturn in a lake, it would
float!)
115Rings of Saturn
- 7 major rings made up of ringlets
- Gravity keeps the rings in place
- rings are not solid
- composed of small countless particles
- rings are very thin.
- Though theyre 250,000 km or more in diameter,
theyre less than one kilometer thick
116- Moons
- 55 moons
- 31 moons
- Largest moon, Titan,
- Titan, the largest is bigger than Mercury
- Odd among moons because of content with dense
atmosphere and methanes existence in 3 states
117Uranus
- 7th planet from sun
- Has a faint ring system (they are dark and hard
to observe) - 27 known moons
- Covered with clouds
- Uranus sits on its side with the north and south
poles sticking out the sides. - 4x larger and 15Xmass of the Earth
118Uranus
- Atmosphere
- Bluish appearance cause by methane gas
- Clouds are similar in appearance to the surface
- Liquid surface with a small solid core
- Rotation
- Almost a top to bottom rotation
- Poles vacillate between 42 years of darkness and
light
119URANUS
- Uranus has more moons (15) than any other planet
except Jupiter (16) and Saturn (23)!
120Neptune
- 4th largest planet
- 8th planet from sun
- Because of the orbits, from 1979 to 1999, Neptune
was the ninth planet. - Discovered through math
- 7 known moons
- Great Dark Spot thought to be a hole, similar to
the hole in the ozone layer on Earth - Like Uranus, the methane gives Neptune its color.
121Neptune
- Atmosphere
- Smaller and denser than Uranus but 4XEarth
- Similar in color to Uranus (twins??) but does
have some color variation on surface - Belts and zones give it texture
- Moons and Rings
- 13 moons Triton being the largest
- Triton has retrograde orbit
- Also has nitrogen geysers when heated by the sun
- Rings are invisible from Earth but exist
122The blue coloration of Neptune is probably due to
the presence of methane
Note the apparent storms
123Plutoa planet?
- Today, Pluto is called a "dwarf planet.
- A dwarf planet orbits the sun just like other
planets, but it is smaller. - A dwarf planet is so small it cannot clear other
objects out of its path.
124Per NASA.gov.
- In 2003, an astronomer saw a new object beyond
Pluto. The astronomer thought he had found a new
planet. The object he saw was larger than Pluto.
He named the object Eris (EER-is). Finding Eris
caused other astronomers to talk about what makes
a planet a "planet." There is a group of
astronomers that names objects in space. This
group decided that Pluto was not really a planet
because of its size and location in space. So
Pluto and objects like it are now called dwarf
planets. Pluto is also called a plutoid. A
plutoid is a dwarf planet that is farther out in
space than the planet Neptune. The three known
plutoids are Pluto, Eris and Makemake
(MAH-kee-MAH-kee). Astronomers use telescopes to
discover new objects like plutoids.
125Dwarf Planet Pluto
- Pluto, is one of three plutoids.
- It is a small (smaller than Earths moon), solid
and icy - It is so far from the sun that it has never been
visited by spacecraft. - It orbits the sun very slowly.
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131Sample Quiz Questions
Question Which of the planets are rocky?
Answer The inner planets Mercury, Venus,
Earth and Mars
132Sample Question 2
- Which of the planets has the most satellites?
Saturn!
133Image by Dave DockeryAstronomical Society of
Las Cruces
What Are Comets, Asteroids and Meteors?
(textbook reference 14-5) Space Debris
Comet Ikeya Zhang
134Comets A comet is basically a ball of ice and
dust in space. The typical comet is less than
10 kilometers across. Most of their time is
spent frozen solid in the outer reaches of our
solar system.
Comet Hale Bopp
Image by Harvard-Smithsonian Center for
Astrophysics
135A comet orbits around the sun, in a wide,
elliptical path. When a comet gets within a few
million miles of the sun, it begins to melt,
leaving a tail of gas and dust that is blown by
solar winds
Source NASA
Comet Hale Bopp
Image by Harvard-Smithsonian Center for
Astrophysics
136Reviewing Comets
- Small icy bodies
- Travel past the Sun
- Give off gas and dust as they pass by
- Tail of gasses called a coma
137Asteroids
- Asteroid rocks orbiting in space
- Asteroid belt 100,000 asteroids located between
Mars and Jupiter - separates inner and outer planets
138Asteroids
- Small bodies
- Believed to be left over from the beginning of
the solar system billions of years ago - Largest asteroids have been given names
139Meteoroids
- Meteoroid smallest asteroids or comets
- Come from asteroids colliding in space
- Come from a comet breaking up and creating a
cloud of dust continuing to move through the
solar system
140Meteors
- Meteor meteoroid striking Earths atmosphere
- Meteorite meteor that hits Earths surface
141Solar SystemActivities
- Order the Planets
- Fun with Planets
- Constellations of the Northern Sky
- Planets
- Solar System
142Units of Time from Space
- Year 1 revolution of Earth
- Day 1 rotation of Earth
- Month 1 revolution and/or rotation of Moon
143Measuring Distances
- What is a Light Year?
- A light year is the distance light travels in a
year. Light moves at a velocity of about 300,000
kilometers (km) each second how far would it
move in a year? - About 10 trillion km (or about 6 trillion miles).
- Why do we use light years?
- Show me how far 5 centimeters is.
- Now show me 50 centimeters.
- Now tell me (without thinking about it, or
calculating it in meters) how far 500 centemeters
is. 2000? 20,000? - We need numbers that make sense to us in
relationship to objects we scale up and use
meters and kilometers for large numbers.
144Measurements in Space
- Light year distance light travels in one Earth
year - Astronomical Unit distance from Earth to Sun
http//www.youtube.com/watch?v3bmb0YE9VGM
145Are We Alone in the Universe?(textbook reference
14-6)
- SETI http//www.seti.org/seti-institute/about-seti
/scientists vs Pseudoscience http//www.chem1.com/
acad/sci/pseudosci.html - If it is just us, it seems like an awful waste
of space. - Ellie Arroway in Carl Sagans Contact