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The following Technical Notes are hyperlinked from appropriate locations within
the Site. They are meant to give a little more information , or
background, to a particular issue.
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The Drake Equation.
The Drake Equation provides an approximate number of planets, N, with
intelligent life (communicative civilizations). It is , of course,
only as accurate as the estimates of the variables.
There's nothing magic about this equation...take a look at the definition of
the factors and you will see it is all pretty logical. N = R* fp ne fl
fi fc L
where,
 | N = The number of communicative civilizations |
 | R* = The rate of formation of suitable stars (stars such as our
Sun). In the Milky Way, 100 billion
stars. |
 | fp = The fraction of those stars with planets.
(Current evidence indicates that planetary systems may be common for
stars like the Sun.) Say ...¼,
1 in 4. |
 | ne = The number of Earth-like worlds per planetary
system. Maybe... ½,
2 per solar system. |
 | fl = The fraction of those Earth-like planets where
life actually develops. Maybe ....
⅛, 1 in
8. |
 | fi = The fraction of life sites where intelligence
develops. Say ....
¼, 1 in 4. |
 | fc = The fraction of communicative planets (those on
which electromagnetic communications technology develops).
Many scientists will argue that this is a large
fraction ....maybe ½, 1 in 2. |
 | L = The "lifetime" of communicating civilizations as
related to the lifetime of the solar system they are a apart of.
Using
Earth as an example this would be maybe
40 years out of 4 billion, or 1 over 100 million. (That is to say, Earth
has been capable of communicating extra-terrestrial for 40 years.)
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Given the numbers in green above, N would equal
2,500 communicative civilizations for the Milky Way. Of course,
any other estimates would be just as valid, given our present knowledge of
the Milky Way, however, the exercise allows us to more readily appreciate
the sensitivity for the existence of life on other planets.
Note also that this gives the odds of finding a civilization which has
developed far enough to communicate with us. On the other hand
maybe we just want to know the odds of finding a caveman
civilization. Variable L would be higher in that case.
Radioactive Dating Methods. Carbon-14 method is the most
common method and is used for dating the age of once living articles less
than about 60,000 years old. Carbon -14 is a radioisotope found in
all living matter. It has a half life of 5,750 years, which means that
after about 60,000 years there is so little Carbon 14 left in the tissue
that it cannot be accurately measured. Articles dating back between
40,000 and 60,000 years ago have so little of their original radio-carbon in
them (maybe 0.1%) that it is nearly impossible to accurately distinguish
from background levels. However for time periods less
than 50,000 years, Carbon-14 dating is a viable option.
Other methods of Radioactive
Dating can be used for longer periods. For example Uranium-235 has a
half life of 700 million years and Uranium-238 has a half life of 4,400
million years! These methods are used in dating non-living material
such as rocks and minerals.
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We get to see all sides. Imagine you are on a
Merry-go-round......the carousel horse you are riding is the Earth and it's orbiting
the center of the Merry-go-Round, the Sun. You pass your friend
standing on the side and wave to him/her....6 seconds later (6 months later,
for the Earth) you cannot see your friend who is now on the other side of
the "Sun". However, you do see many other people, who could not
be seen before. Not to worry, another 6 seconds (another 6 months for the
Earth) and there is your friend, still there, just as before. .....and
the cycle repeats itself, over and over again. Every 12 seconds
(months for the Earth) you see the same scenery alongside the
Merry-go-Round....it is the same for the night sky as we travel around the
sun every year.
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Panoramic view of the Milky Way. Cool! A photo of our
Milky Way? our galaxy?? Well....not quite. It's tempting to see
this photo as having been taken from outside the Milky Way. Of course
that would be amazing! ...but it would be a false impression. It
is actually a photo from the inside looking out! Interesting illusion,
ya? This photo is made from many still photos over a period of one year and represents a 360° view of
the night sky. Imagine this photo stretched out and placed
in a circle around your head so that as you turned you could see the night
sky as it would appear around the earth (ignoring for a moment the sun).
The age of the photo - 1940 - should be of no concern.....
in cosmic terms it is but a fleeting instant. Should the same be
taken today with similar photographic equipment there would be no measurable
difference in appearance.
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Come back this way. This refers
to the question of whether this universe, which has been expanding ever
since the Big Bang, will continue to expand forever, or, if the expansion
will slow, then stop, and begin to collapse upon itself. If it
is the latter, then we will, in a sense, "come back this way".
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Big Bang Theory.
Most astronomers today will tell you that the Big Bang theory is "...99
percent certain". Some few very knowledgeable scientists will tell you
"...not so fast, there are a lot of things wrong with that theory".
The most recent is the Witt Theory. The important
thing for us who have day jobs is to understand what the Big Bang
theory is...just so we can appreciate the mystery of it all. As more
and more discoveries are made the truth will become more clear. But
for now, the Big Bang theory is front and center.
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144 moons. There are a lot of moons in
our Solar System...as noted here:
There will likely be more
moons discovered around the Planets in the near future.
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Hot gas clouds. The Gas clouds in
intergalactic space consist of individual gas atoms (mainly hydrogen and
helium), or particles
which can have very high energies. The energy of these gas clouds
is expressed as a temperature, the cooler gas clouds consist of neutral
atoms and the hotter clouds consisting of gas plasmas, which are the gas
atoms stripped of their electrons. The latter can be a very high
temperature but because
the density of these gas molecules in space is so low, the
total heat in a given
volume is also extremely low, relative to earthly conditions. Do not
confuse the high temperatures of the gas plasmas with the earthly affect of touching a hot
object of the same temperature, where the density of the hot object is
billions of times more than the density of the gas clouds. A spacecraft flying through these high
temperature plasmas will not melt away simply because the heat
available to cause damage is vastly reduced. The gas molecules are so
thin, i.e., widely spaced, that the extreme density of the spacecraft
(relative to the plasma) easily absorbs the energy of the small
number of gas
ions it encounters.
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American power of 10
The following table gives the
name for the power-of-10. The number represents the number of
zeros...
| billion |
9 |
| trillion |
12 |
| quadrillion |
15 |
| quintillion |
18 |
| sextillion |
21 |
| septillion |
24 |
| octillion |
27 |
| nonillion |
30 |
|
decillion |
33 |
|
undecillion |
36 |
|
duodecillion |
39 |
|
tredecillion |
42 |
|
quattuordecillion |
45 |
|
quindecillion |
48 |
|
sexdecillion |
51 |
|
septendecillion |
54 |
|
octodecillion |
57 |
|
novemdecillion |
60 |
|
vigintillion |
63 |
| |
|
| googol * |
100 |
| |
|
|
centillion |
303 |
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* Hummmm...this looks
like....google!
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Large Hadron Collider. The LHC was recently completed at a cost of several
billions of dollars and is located near Geneva, Switzerland.
Colliders of this size and complexity are built by governments since the
cost is so high that private institutions cannot afford them. The LHC will study the physics which existed
between .1 and 1 microsecond after the Big Bang. A Collider of this size
was being constructed in the US (New Mexico)
in the 70's but was cancelled by Congress. Cutting edge physics
will now be done in Europe....a further erosion of our technology lead!
A Collider is an energy
particle accelerator. In layman's terms the Collider accelerates
particles close to the speed of light and and causes a head-on collision in
which matter is destroyed, energy created, and new matter in the form of
elementary particles is created from energy. The collisions result in
temperatures of trillions of degrees. Essentially recreating
the conditions which scientists believe existed during the Big Bang.
This is cutting edge physics.....
While the LHC may now be the world's highest energy particle accelerator at
energies of 1,000,000 GeV, the US has the 2nd largest Collider...the
Relativistic Heavy Ion Collider RHIC, known as "rick". The RHIC was completed
in 2001 at the Brookhaven Laboratory on Long Island and can attain energies up
to 20,000 GeV. Prior to the RHIC, the largest Collider was the SPS also
at Geneva. The SPS was capable of energies as high as 450 GeV. It
is still in use today,
as the last link in the accelerator chain providing beams for the LHC.
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Hubble Telescope.
The Hubble Space Telescope (HST) was the first telescope to be placed
in earth orbit. The single advantage of earth orbit is that the HST is
free from the distortion and interference of the earth's atmosphere.
This is a huge advantage and even today, 14 years after its initial
operation. the Hubble is capable of observations far better than the newest
and larger earth bound telescopes. The Hubble is capable of
observations in a wide spectrum....from ultraviolet, through the visual
spectrum, to infrared. It has
a diameter of 95-inches, just over 2-meter, compared to earth telescopes
much larger. tens of meters in diameter.
In 1993, shortly after it was
placed in service, the Hubble made the first Deep-field observation and
recorded images of galaxies further away than ever seen before....peering
very deep into the night sky. The light from these galaxies began
their journey over 1 billion years after the Big Bang, when the
galaxies where very young. In 2002, the Hubble got an upgrade and was
able to see further into the night sky....going back to just 700 million
years after the Big Bang. In 2009, the last upgrade of the Hubble will
allow it to see even further...just 500 million years after the Big Bang.
these incredible images will allow scientists to further refine their
theories on how the universe was formed and the processes that occurred.
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