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November 2, 2011: CERN Experiment and Violation of Newton’s Second
Law Englishview
October 13, 2011: CERN Experiment and Violation of the Newton’s
Second Law Persianview
November 24, 2008: A New Definition of Gravitonview
July 10, 2007: Zero Point Energy and the Dirac Equationview
July 10, 2007: Zero Point Energy and the Dirac Equationview
June 28, 2007: Unification and CPH Theoryview
June 14, 2007: Summary of Physics Conceptsview
June 14, 2007: Strong Interaction and CPH Theory Rview
June 4, 2007: Quantum Electrodynamics and CPH Theoryview
November 30, 2006: Vocabulary of CPH Theoryview
November 17, 2006: Thermodynamic Laws Entropy and CPH Theoryview
November 17, 2006: Time Function and Absolute Black Holeview
October 14, 2006: CPH and Timeview
October 13, 2006: CPH Theory and Newton's Second Lawview
October 13, 2006: Time Function and Work Energy Theoremview
October 13, 2006: CPH Theory and Special Relativityview
October 13, 2006: Properties of CPHview
July 31, 2006: A New Mechanism of Higgs Bosons in Producing Charge
Particlesview
July 31, 2006: A New Mechanism of Higgs Bosons in Producing Charge
Particlesview
May 14, 2006: Speed of Light and CPH Theoryview
May 14, 2006: Speed of Light and CPH Theoryview
April 28, 2006: Color Charges Curve Spaceview
April 28, 2006: Color Charges Curve Spaceview
April 17, 2006: Effective Nuclear Chargeview
April 17, 2006: Effective Nuclear Chargeview
April 12, 2006: Maxwell's Equations in a Gravitational Fieldview
April 12, 2006: Maxwell's Equations in a Gravitational Fieldview
April 11, 2006: Realization Hawking - End of Physics by CPHview
April 7, 2006: Questions and Answers on CPH Theoryview
April 7, 2006: Opinions on CPH Theoryview
April 7, 2006: Opinions on CPH Theoryview
April 7, 2006: Questions and Answers on CPH Theoryview
March 23, 2006: Analysis of CPH Theoryview
March 23, 2006: Analysis of CPH Theoryview
March 21, 2006: Logical Foundation of CPH Theoryview
March 21, 2006: Definition Principle and Explanation of CPH Theoryview
March 21, 2006: Logical Foundation of CPH Theoryview
March 21, 2006: Definition Principle and Explanation of CPH Theoryview
March 21, 2006: Experimental Foundation of CPH Theoryview
March 21, 2006: Experimental Foundation of CPH Theoryview
March 19, 2006: Color Charge/Color Magnet and CPHview
March 19, 2006: Sub-Quantum Chromodynamicsview
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Life beyond earth: To the sun-like stars |
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Life beyond
earth: To the sun-like stars
Nasa?s deployment of a space telescope to gaze beyond our solar
system provides the best chance so far of detecting alien organisms
? intelligent or otherwise, writes Clive Cookson.
A spacecraft launched from Florida offers the best hope yet of
answering a question people have been asking for aeons: Are there
other worlds like ours or are we alone? Nasa?s $600m (?425m, ?478m)
Kepler space telescope was dispatched from Cape Canaveral to search
the galaxy for planets that could harbour life. The results, says
Debra Fisher, astronomy professor at San Francisco State University,
?will help us chart a course toward one day imaging a pale blue dot
like our planet, orbiting another star?.
The search for extra-solar planets, or exoplanets, has become
astronomy?s hottest activity. Since 1995, telescopes on Earth and in
space have detected 340 planets elsewhere in the galaxy. ?We know
already about an incredibly wild and chaotic range of planets,? says
Prof Fisher. The main point of the planet search, however, is not to
find weird worlds in strange orbits with bizarre geology. What
everyone wants to know is whether there is life beyond the solar
system. If so, its discovery will be among the most important ever
made. It would be the last step in humanity?s scientific demotion
over the past few centuries, by Copernicus, Darwin and others, from
specially created beings at the centre of the cosmos to just one of
myriad life forms in the universe.
Even if the search for extraterrestrial life is unsuccessful, it is
likely to bring benefits closer to home, in the form of new ways to
discover and study micro-organisms on Earth. All exoplanets
discovered so far are too extreme to support life as we know it.
Kepler ? named after Johannes Kepler (1571-1630), who discovered
that planets travel around the sun in elliptical orbits ? is the
first observatory with technology capable of finding Earth-sized
planets that are neither fireballs nor snowballs: worlds with liquid
water and rocky continents.
William Borucki, the mission?s chief scientist, says it will survey
100,000 sunlike stars over the next four years, looking for orbiting
planets in the ?habitable zone? ? sometimes known as the ?Goldilocks
zone? ? where conditions ?are not too hot and not too cold but just
right? for life. If Earth-sized planets are common, Kepler will
detect hundreds of them, including dozens in the habitable zone. ?If
we find that many, it will mean that life may well be common
throughout our galaxy,? he adds. ?If we do not find any, that would
be another profound discovery?, implying that Earth is a lonely
outpost of life.
Most astronomers are optimistic, given the latest theories of
planetary formation and the number and variety of giant planets
already discovered. ?We already know enough to say that the universe
is probably loaded with terrestrial planets similar to Earth,? says
Alan Boss of the Carnegie Institution for Science in Washington.
Boss believes that most stars similar in size and temperature to our
sun are accompanied by one or more habitable planets. Given that
there are an estimated 100bn sunlike stars in our Milky Way galaxy
and 100bn galaxies in the known universe, the potential number of
Earth-like planets is a humbling 10 to the power of 22 (one followed
by 22 zeros).
Paul Davies, cosmology professor at Arizona State University, says
there has been a huge change in attitude during his career. ?When I
was a student in the 1960s, no one believed that there was life
beyond Earth,? he says. ?Recently the pendulum has swung in the
opposite direction, towards a universe teeming with life.?
Enthusiasts for exobiology ? life beyond Earth ? are encouraged not
only by the plethora of planets around distant stars but also by the
recent discovery that interstellar space is rich in organic
chemicals. An intensive search with radiotelescopes has identified
150 molecules by their spectroscopic ?signatures?; these include
complex chemicals such as alcohols, sugars and amino acids, which
are precursors of life.
The origin
The origin of these ?prebiotic? molecules is mysterious. Anthony
Remijan of the US National Radio Astronomy Observatory says they may
form on the surface of interstellar dust grains, heated just enough
by nearby stars to catalyse chemical reactions. Once formed,
prebiotic chemicals could reach the surface of planets, where a
process of proto-evolution would lead the molecules to organise
themselves into increasingly complex self-replicating forms.
Yet the fact remains that we have evidence for life having started
only once in the universe: On Earth 3.5bn-4bn years ago. Within our
solar system, hopes remain high that, within the next decade, robot
missions to Mars will prove the existence of past ? and perhaps of
present ? microbial life. Later missions might possibly find that
some moons of Jupiter and Saturn harbour life too.
Prof Davies also raises the possibility that life started
independently on Earth on two or more occasions. ?Has there been a
blind spot to the possibility of ?alien? life on Earth?? he asks.
?Might it exist on Earth today in extreme environments and remain
undetected because our techniques are customised to the biochemistry
of known life?? He advocates a systematic search on Earth for
micro-organisms with an alternative biochemistry to the DNA, RNA and
proteins that control all known forms of life from viruses and
bacteria to humans. ?If we found life happened more than once here,
then it means that the universe really is teeming with life,? says
Prof Davies.
Beyond Earth and the solar system, there is no realistic possibility
of making direct physical contact with alien life. So astronomers
will use an increasingly sophisticated series of indirect means over
the next two or three decades to look for it. The Kepler space
telescope represents the first step. It will find Earth-like worlds
by detecting tiny differences in the light coming from distant stars
as orbiting planets pass in front of them. The light variations
during these ?transits? are equivalent to an insect flying across a
powerful searchlight beam ? previous observatories have not been
powerful enough to record them.
Astronomers can deduce a surprising amount of information about a
planet by observing a series of transits: its size, from the way its
parent star changes brightness; its orbital period, from the time
between transits; its orbital dimensions, from the star?s mass and
size; and its surface temperature, from its orbit and the star?s
temperature. This will tell whether the planet is potentially
habitable but not, of course, whether it is inhabited.
After three years of Kepler observations, Nasa expects to have a
reliable estimate for the number of Earth-like planets in our
galaxy. Assuming that those are reasonably plentiful, space agencies
can then plan the next stage: a mission to image planets directly ?
possibly showing clouds, continents and oceans ? and analyse their
atmospheres for chemical signatures of life, such as oxygen, methane
and water. Although the European Space Agency has such a mission on
the drawing board, called Darwin, and Nasa is thinking of something
similar called Terrestrial Planet Finder, these are unlikely to be
funded, developed and launched in less than 15 years.
The whole process could be short-circuited, however, by a dramatic
coup de th颴re: The detection of signals transmitted by intelligent
beings elsewhere. The search for extraterrestrial intelligence,
known as Seti, started in 1960 at the Green Bank radiotelescope in
West Virginia, under the direction of the American astronomer Frank
Drake. The failure to hear a peep from ET after almost 50 years has
not discouraged advocates of Seti, who say we have not listened long
enough or hard enough ? or in the right way.
S earch
for ET
Nasa had trouble funding Seti in the face of ridicule from
politicians such as the late Senator William Proxmire, a scourge of
what he saw as frivolous public spending. But private donors stepped
in to fill the gap, notably Paul Allen, co-founder of Microsoft. He
has contributed $26m to the construction in California of an array
of 350 radio dishes, each 6 metres in diameter, dedicated to
listening for extraterrestrial signals.
Until now, Seti has had to beg for time on radiotelescopes designed
for other purposes. Estimating how many intelligent civilisations
exist in our galaxy is not much easier today than it was when Drake
published an equation for the purpose in 1961. ?The numbers that
came out of the Drake equation then were between one and 50m,? says
Duncan Forgan, an Edinburgh university astronomer who has just
carried out a new calculation, based on the latest knowledge of
planetary formation and biological evolution. Prof Forgan estimates
that between 360 and 38,000 intelligent life forms capable of
interstellar communications have evolved over the lifetime of our
galaxy so far ? but he says no one can put a sensible figure on the
number of civilisations in existence now, let alone the chance of
picking up a message from one of them.
Even if the Kepler mission gives a good estimate of the number of
habitable planets, we will still have little idea of the chance that
life will actually start, let alone evolve into a civilisation
transmitting radio waves or laser pulses. Perhaps the biggest
uncertainty is how long an average civilisation exists before it is
destroyed. Or, more optimistically, perhaps some civilisations have
become too technologically advanced for primitive Earthlings of the
21st century to detect signs of their existence. Astronomers still
have little idea of the identity of the mysterious ?dark matter? and
?dark energy? that make up 95 per cent of the universe. Could aliens
use them to communicate? Could they even exist in dark matter?
If we do hear from ET, elaborate diplomatic protocols will clank
into action on Earth, to control how the momentous discovery is
disseminated. Any reply to the aliens would have to wait for an
international agreement. Although some astronomers are surprised
that Seti has detected no signs of intelligent life elsewhere, they
do not expect an alien visit to Earth. Short of a ?wormhole? or some
other propulsion system beyond the ken of contemporary physics, the
timescales required for interstellar travel are too vast; it would
take several millennia to travel a few light-years to our nearest
planetary neighbours. The energy required would be prohibitive, too.
?Actual visits would be ruled out by the laws of physics,? says
Boss. Realistically, we can expect to know within 20-30 years
whether there is life of some sort beyond Earth. As for intelligent
life, we may have to wait an eternity.
The meaning of life is of increasing interest to scientists as well
as philosophers. As the search for extraterrestrial life gathers
pace, the exobiologists who specialise in this are studying the
potential range of chemical and physical characteristics in living
systems. Silicon-based life has featured in science fiction but most
chemists say only carbon-based systems such as on Earth would be
versatile and robust enough to evolve elsewhere.
These would have to follow the rules of organic chemistry - and of
Darwinian evolution. ?Whatever its shape or chemistry, there is one
important expectation that many if not all biologists share about
life in the universe,? says Sean Carroll, professor of genetics at
the University of Chicago. ?Wherever life has arisen, it has evolved
by the two principles Darwin formulated: By descent with
modification and natural selection.?
A universal requirement for life, then, is a biochemical store of
genetic information passed down through the generations, with small
changes to make evolution possible. On Earth this role is carried
out by the DNA and RNA molecules, which carry data on chemical
letters called nucleotides. Although scientists have not thought up
a completely different genetic system, they have developed
alternative forms of DNA incorporating synthetic nucleotides.
Last month at the American Association for the Advancement of
Science meeting in Chicago, Steven Benner announced the first
laboratory experiment in which artificial DNA underwent Darwinian
evolution. ?If you are looking for alien life, it is helpful to have
an alternative system to study,? says Dr Benner of the Foundation
for Applied Molecular Evolution in Florida.
Instead of carrying out ?wet? experiments in a biochemistry lab, a
different approach uses computers and software to simulate the
creation of life under various conditions elsewhere in the universe.
On an Earth-like planet, with oceans, continents and climate broadly
similar to ours, any advanced life forms would probably not look
wildly different to their terrestrial counterparts. For example, the
history of life on Earth shows that features such as eyes and ears,
which give organisms a huge competitive advantage, evolved
independently on several occasions. It is conceivable, however, that
any super-advanced civilisation could be unrecognisable to ours, if
biological organisms have melded with machine intelligence to form
some sort of hybrid biocomputer life form. The concept is
controversial, but some futurists such as Ray Kurzweil predict that
something like it will happen on Earth later this century.
Source: The
peninsola
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@2003-2012 The CPH theory, All right reserved
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