Difference between revisions of "Extraterrestrial life" - New World Encyclopedia

From New World Encyclopedia
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In order for something to be considered a living organism, there are five biological criteria that must be met: ability to reproduce and grow, it consume nutrients in order to survive, have mobility and respond to external stimuli <ref> (2007) [[http://www.newton.dep.anl.gov/askasci/bio99/bio99171.htm"Definition of Life"]] Retrieved May 1, 2007 </ref> Further, all living organisms on earth are based on the element [[carbon]], depend on water as a meduim for crucial chemical reactions, and are made up of long strands of [[amino acids]], known as [[DNA — Deoxyribonucleic acid]]. The difficulty with trying to understand possible other life forms, is that science currently is unaware of any other composition of life (there has been some speculation that instead of carbon, the element [[silicon]] may consistitue the basis of extraterrestrial life). Therefore, either life in the universe can only exist on planets with similar water and carbon levels and tempeture of Earth, or life exists in some form that we currently do not know about, and raises the issue of how to look for something that does not correspond to current understandings.
 
In order for something to be considered a living organism, there are five biological criteria that must be met: ability to reproduce and grow, it consume nutrients in order to survive, have mobility and respond to external stimuli <ref> (2007) [[http://www.newton.dep.anl.gov/askasci/bio99/bio99171.htm"Definition of Life"]] Retrieved May 1, 2007 </ref> Further, all living organisms on earth are based on the element [[carbon]], depend on water as a meduim for crucial chemical reactions, and are made up of long strands of [[amino acids]], known as [[DNA — Deoxyribonucleic acid]]. The difficulty with trying to understand possible other life forms, is that science currently is unaware of any other composition of life (there has been some speculation that instead of carbon, the element [[silicon]] may consistitue the basis of extraterrestrial life). Therefore, either life in the universe can only exist on planets with similar water and carbon levels and tempeture of Earth, or life exists in some form that we currently do not know about, and raises the issue of how to look for something that does not correspond to current understandings.
  
Most scientists hold that if extraterrestrial life exists, its [[evolution]] would have occurred independently in different places in the [[universe]]. An alternative hypothesis, held by a minority, is [[panspermia]], which suggests that life in the universe could have stemmed from a smaller number of points of origin, and then spread across the universe, from [[Planetary habitability|habitable planet]] to habitable planet. These two hypotheses are not [[mutually exclusive]].
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===Speculation===
  
Given their relative abundance and usefulness in sustaining life it has long been assumed thalife forms elsewhere in the universe will also utilize these basic components. However, other elements and solvents might be capable of providing a basis for [[life]]. [[Silicon]] is usually considered the most likely alternative to carbon, though this remains improbable. Silicon life forms are proposed to have a crystalline morphology, and are theorized to be able to exist in high temperatures, such as planets closer to the sun. Life forms based in [[ammonia]] rather than water are also considered, though this solution appears less optimal than water.<ref>{{cite web| url=http://www.daviddarling.info/encyclopedia/A/ammonialife.html| publisher=daviddarling.info| title=Ammonia based life}}</ref>
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Without concrete facts to analyze or direct phenomena to observe, most scientists studying extraterrestrial life must do so by speculation (Most speculation is, however, based on what is accepted knowledge of astronomy and biology, as well as careful scientific postulating). Even with so many unknown variables, such postulating requires that specific guidelines be established in order to further pursue the notion. For example, scientists must first try to understand if the [[evolution]] of extraterrestrial life would have occurred independently in different places in the [[universe]], or if, as a minority of scientists contend, life in the universe could have stemmed from a smaller number of points of origin, and then spread across the universe, from [[Planetary habitability|habitable planet]] to habitable planet, known as [[panspermia]].
 
 
Recently, scientists have discovered mysterious red cells in India unlike any cells on Earth.<ref>Astrophysics and Space Science 302 #1-6 (2006) 175–187
 
The Red Rain Phenomenon of Kerala and its Possible Extraterrestrial Origin
 
Godfrey Louis and A. Santhosh Kumar</ref>  The cells appear to be replicating without the presence of [[DNA]], raising questions about whether they are a new kind of life altogether, or whether they can even be classified as life at all, without genetic material.  It is believed that these red cells may have been injected into Earth's atmosphere by a comet or meteor from elsewhere in the universe; some believe this may be evidence of panspermia's occurrence.  Little is known about these cells, however, and the issue is controversial.  Some scientists believe the cells may actually be native to Earth.<ref>{{cite news
 
|url=http://www.cnn.com/2006/TECH/science/06/02/red.rain/index.html
 
|publisher=CNN.com
 
|date=2006-06-02
 
|title= Mysterious red cells might be aliens
 
|accessdate=2006-08-09}}
 
</ref>
 
 
 
Along with the biochemical basis of extraterrestrial life, there remains a broader consideration of [[evolution]] and [[comparative anatomy|morphology]]. What might an alien look like? Science fiction has long shown a bias towards humanoid or (often in the case of villains) [[reptiles|reptilian]] forms. The classical alien is light green or grey skinned, with a large head, and the typical four limb and two to five digit structure—i.e., it is fundamentally humanoid with a large [[brain]] to indicate great intelligence. Other subjects from animal [[mythos]] such as [[cats|felines]] and [[insects]] have also featured strongly in fictional representations of aliens.  
 
  
 
In considering the subject more seriously, a useful division has [[Evolving the Alien|been suggested]] between universal and parochial (narrowly restricted)  characteristics. Universals are features which have evolved independently more than once on Earth (and thus presumably are not difficult to develop) and are so intrinsically useful that species will inevitably tend towards them. These include [[flight]], [[sight]], [[photosynthesis]] and [[limbs]], all of which have evolved several times here on Earth with differing materialization. There are a huge variety of [[eye]]s, for example, many of which have radically different working schematics as well as different visual foci: the [[visual spectrum]], [[infrared]], [[polarity]] and [[echolocation]]. Parochials, by contrast, are essentially arbitrary evolutionary forms which often serve little utility (or at least have a function which can be equally served by dissimilar morphology) and probably will not be replicated. Parochials include the five digits of [[mammals]], the [[genitalia]] and sexual mechanics of animals, as well as the curious and often fatal conjunction of the feeding and breathing passages found within many animals.  
 
In considering the subject more seriously, a useful division has [[Evolving the Alien|been suggested]] between universal and parochial (narrowly restricted)  characteristics. Universals are features which have evolved independently more than once on Earth (and thus presumably are not difficult to develop) and are so intrinsically useful that species will inevitably tend towards them. These include [[flight]], [[sight]], [[photosynthesis]] and [[limbs]], all of which have evolved several times here on Earth with differing materialization. There are a huge variety of [[eye]]s, for example, many of which have radically different working schematics as well as different visual foci: the [[visual spectrum]], [[infrared]], [[polarity]] and [[echolocation]]. Parochials, by contrast, are essentially arbitrary evolutionary forms which often serve little utility (or at least have a function which can be equally served by dissimilar morphology) and probably will not be replicated. Parochials include the five digits of [[mammals]], the [[genitalia]] and sexual mechanics of animals, as well as the curious and often fatal conjunction of the feeding and breathing passages found within many animals.  
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The assumption of radical diversity amongst putative extraterrestrials is by no means settled. While many exobiologists do stress that the enormously heterogeneous nature of Earth life foregrounds even greater variety in space, others point out that [[convergent evolution]] dictates substantial similarities between Earth and off-Earth life. These two schools of thought are called "divergionism" and "convergionism," respectively.<ref>{{cite web| url=http://www.daviddarling.info/encyclopedia/E/etlifevar.html| publisher=daviddarling.info| title=Variety of extraterrestrial life}}</ref>
 
The assumption of radical diversity amongst putative extraterrestrials is by no means settled. While many exobiologists do stress that the enormously heterogeneous nature of Earth life foregrounds even greater variety in space, others point out that [[convergent evolution]] dictates substantial similarities between Earth and off-Earth life. These two schools of thought are called "divergionism" and "convergionism," respectively.<ref>{{cite web| url=http://www.daviddarling.info/encyclopedia/E/etlifevar.html| publisher=daviddarling.info| title=Variety of extraterrestrial life}}</ref>
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Currently, [[Astrobiology]] is a field of study that has gained legitimacy and acceptance in the scientific community. Its main objectives include the search for extraterrestrial life, but in doing so seek to develop a better understanding of life on Earth <ref> (2006) [[http://astrobiology.arc.nasa.gov/about/index.cfm"NASA - Astrobiology"]] Retrieved May 1, 2007 </ref>
  
 
[[Image:arecibo_message.png|160px|right|thumb|The [[Arecibo message]] is a digital message sent to [[Great Globular Cluster in Hercules|globular star cluster M13]], and is a well-known symbol of human attempts to contact extraterrestrials.]]
 
[[Image:arecibo_message.png|160px|right|thumb|The [[Arecibo message]] is a digital message sent to [[Great Globular Cluster in Hercules|globular star cluster M13]], and is a well-known symbol of human attempts to contact extraterrestrials.]]
  
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===The Search For Extraterrestrials===
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Since the last quarter of the 20th century, scientists have been actively searching the universe for other lifeforms with all the different types of technology availble. Yet, even if all of [[NASA]] and the [[The European Space Agency]]'s budgets were directed towards this one goal, the universe is still too large and our technological means still not adequate enough to exhaustively search those areas in space that we know are possibily harboring life. Still, there are undaunted scientists who contuine to search for possible life, whether it be [[bacteria]] or advanced civilizations. There are two different methods scientists use in this search: the direct and indirect method.
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====The Direct Method====
 
Scientists are directly searching for evidence of unicellular life within the [[solar system]], carrying out studies on the surface of Mars and examining [[meteors]] that have fallen to Earth. A mission is also proposed to [[Europa (moon)|Europa]], one of [[Jupiter (planet)|Jupiter]]'s moons with a liquid water layer under its surface, which might contain life.
 
Scientists are directly searching for evidence of unicellular life within the [[solar system]], carrying out studies on the surface of Mars and examining [[meteors]] that have fallen to Earth. A mission is also proposed to [[Europa (moon)|Europa]], one of [[Jupiter (planet)|Jupiter]]'s moons with a liquid water layer under its surface, which might contain life.
  
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It is theorised that any technological society in space will be transmitting information. Projects such as [[SETI]] are conducting an astronomical search for radio activity that would confirm the presence of intelligent life. A related suggestion is that aliens might broadcast pulsed and continuous [[laser]] signals in the optical as well as infrared spectrum;<ref>{{cite web| url=http://www.coseti.org/| publisher=The Columbus Optical SETI Observatory| title=The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum}}</ref> laser signals have the advantage of not "smearing" in the interstellar medium and may prove more conducive to communication between the stars.
 
It is theorised that any technological society in space will be transmitting information. Projects such as [[SETI]] are conducting an astronomical search for radio activity that would confirm the presence of intelligent life. A related suggestion is that aliens might broadcast pulsed and continuous [[laser]] signals in the optical as well as infrared spectrum;<ref>{{cite web| url=http://www.coseti.org/| publisher=The Columbus Optical SETI Observatory| title=The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum}}</ref> laser signals have the advantage of not "smearing" in the interstellar medium and may prove more conducive to communication between the stars.
  
 
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In 1960, [[Cornell University]] astronomer [[Frank Drake]] performed the first modern SETI experiment, named "[[Project Ozma]]," after the [[Princess Ozma|Queen of Oz]] in [[L. Frank Baum]]'s fantasy books. Drake used a 25-meter-diameter radio telescope at [[Green Bank, West Virginia]], to examine the stars [[Tau Ceti]] and [[Epsilon Eridani]] near the 1.420 gigahertz marker frequency. A 400 kilohertz band was scanned around the marker frequency, using a single-channel receiver with a bandwidth of 100 hertz. The information was stored on tape for off-line analysis. Nothing of great interest was found.
 
 
===SETI===
 
  
 
'''SETI''' ([[International Phonetic Alphabet for English|pronounced]] {{IPA|['sɛti]}}) is the acronym for '''Search for Extra-Terrestrial Intelligence'''; organized efforts by humans to detect [[Extraterrestrial life|intelligent aliens]]. A number of efforts with "SETI" in the project name have been organized, including projects funded by the [[United States Government]]. The generic approach of SETI projects is to survey the [[sky]] to detect the existence of [[interstellar communication|transmissions]] from a civilization on a distant planet - an approach widely endorsed by the [[scientific community]] as [[hard science]].
 
'''SETI''' ([[International Phonetic Alphabet for English|pronounced]] {{IPA|['sɛti]}}) is the acronym for '''Search for Extra-Terrestrial Intelligence'''; organized efforts by humans to detect [[Extraterrestrial life|intelligent aliens]]. A number of efforts with "SETI" in the project name have been organized, including projects funded by the [[United States Government]]. The generic approach of SETI projects is to survey the [[sky]] to detect the existence of [[interstellar communication|transmissions]] from a civilization on a distant planet - an approach widely endorsed by the [[scientific community]] as [[hard science]].
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There is also the problem of knowing what to listen for, as we have no idea how a signal sent by aliens might be modulated, and how the data transmitted by it might be encoded.  Narrow-bandwidth signals that are stronger than background noise and constant in intensity are obviously interesting, and if they have a regular and complex pulse pattern are likely to be artificial.  
 
There is also the problem of knowing what to listen for, as we have no idea how a signal sent by aliens might be modulated, and how the data transmitted by it might be encoded.  Narrow-bandwidth signals that are stronger than background noise and constant in intensity are obviously interesting, and if they have a regular and complex pulse pattern are likely to be artificial.  
  
However, while studies have been performed on how to send a signal that could be easily [[decipher]]ed, there is no way to know if the assumptions of those studies are valid, and deciphering the information from an alien signal could be very difficult.
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However, while studies have been performed on how to send a signal that could be easily [[decipher]]ed, there is no way to know if the assumptions of those studies are valid, and deciphering the information from an alien signal could be very difficult.
 
 
There is yet another problem in listening for interstellar radio signals. Cosmic and receiver noise sources impose a threshold to power of signals that we can detect. For us to detect an alien civilization 100 light years away that is broadcasting "omnidirectionally," that is, in all directions, the aliens would have to be using a transmitter power equivalent to several thousand times the entire current power-generating capacity of the entire Earth.
 
 
 
It is much more effective in terms of communication to generate a narrow-beam signal whose "effective radiated power" is very high along the path of the beam, but negligible everywhere else.  This places the transmitter power within reasonable ranges, the problem being now of having the good luck to coincide with the path of the beam, with the possibility approaching to zero as distance increases.
 
 
 
Such a beam might be very hard to detect, not only because it is very narrow, but because it could be blocked by interstellar dust clouds or garbled by "multipath effects," the same phenomenon that causes "ghosted" TV images.  Such ghosts occur when [[television|TV]] transmissions are bounced off a mountain or other large object, while also arriving at our TV antenna by a shorter, direct route, with the TV picking up two signals separated by a delay.
 
 
 
Similarly, interstellar narrow-beam communications could be bent or "refracted" by [[interstellar cloud]]s to produce multipath effects that could obscure the signal.  If interstellar signals are being transmitted on narrow beams, there is nothing we can do at this end to deal with this problem other than to be alert.
 
 
 
===Early work===
 
In 1960, [[Cornell University]] astronomer [[Frank Drake]] performed the first modern SETI experiment, named "[[Project Ozma]]," after the [[Princess Ozma|Queen of Oz]] in [[L. Frank Baum]]'s fantasy books. Drake used a 25-meter-diameter radio telescope at [[Green Bank, West Virginia]], to examine the stars [[Tau Ceti]] and [[Epsilon Eridani]] near the 1.420 gigahertz marker frequency. A 400 kilohertz band was scanned around the marker frequency, using a single-channel receiver with a bandwidth of 100 hertz. The information was stored on tape for off-line analysis. Nothing of great interest was found.
 
 
 
The first SETI conference took place at Green Bank in 1961. The Soviets took a strong interest in SETI during the 1960s and performed a number of searches with [[omnidirectional antenna]]s in the hope of picking up powerful radio signals beginning in 1964. TV-Host/American astronomer [[Carl Sagan]] and Soviet astronomer [[Iosif Samuilovich Shklovskii|Iosif Shklovskii]] together wrote the pioneering book in the field, ''Intelligent Life in the Universe'' which was published in 1966 <ref name="sagan_shklovskii">{{cite book | first = Carl | last = Sagan | coauthors = Iosif Scklovskii | title = Intelligent Life in the Universe | year = 1966}}</ref>.
 
 
 
In the March 1955 issue of [[Scientific American]], Dr. [[John Kraus]], Professor Emeritus and McDougal Professor of [[Electrical Engineering]] and [[Astronomy]] at the [[Ohio State University]], described a concept to scan the cosmos for natural radio signals using a flat-plane [[radio telescope]] equipped with a parabolic [[reflector]]. Within one year, his concept was approved for construction by the Ohio State University. With the aid of $71,000 in total grants by the [[National Science Foundation]], construction of the first Kraus-style radio telescope began on a 20-acre plot in [[Delaware, Ohio]]. The 360-feet wide, 500-feet long, and 70-feet high telescope was powered up in 1963. This Ohio State University radio telescope was called [[Big Ear]]. Later, it began the world's first continuous SETI program, called the Ohio State University SETI program.
 
 
 
In 1971, the U.S. [[National Aeronautics and Space Administration]] (NASA) funded a SETI study that involved Drake, [[Bernard Oliver]] of [[Hewlett-Packard]] Corporation, and others. The report that resulted proposed the construction of an Earth-based radio telescope array with 1,500 dishes, known as "[[Project Cyclops]]." The price tag for the Cyclops array was $10 billion USD, and, not surprisingly, Cyclops was not built.
 
  
 
===Arecibo message===
 
===Arecibo message===
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Given the limitations of the speed of light for message transmission, no reply would be possible before the year 52,174 (approximately) and hence has been dismissed by some as a [[publicity stunt]].  A controversy arose because the transmission raised the serious question of whether a small group should be allowed to speak for Earth.
 
Given the limitations of the speed of light for message transmission, no reply would be possible before the year 52,174 (approximately) and hence has been dismissed by some as a [[publicity stunt]].  A controversy arose because the transmission raised the serious question of whether a small group should be allowed to speak for Earth.
 
====Sentinel, META, and BETA====
 
In 1980, [[Carl Sagan]], [[Bruce C. Murray|Bruce Murray]], and [[Louis Friedman]] founded the U.S. [[Planetary Society]], partly as a vehicle for SETI studies.
 
 
In the early 1980s, [[Harvard University]] physicist [[Paul Horowitz]] took the next step and proposed the design of a spectrum analyzer specifically intended to search for SETI transmissions. Traditional desktop spectrum analyzers were of little use for this job, as they sampled frequencies using banks of analog filters and so were restricted in the number of channels they could acquire. However, modern integrated-circuit [[digital signal processing]] (DSP) technology could be used to build [[autocorrelation]] receivers to check far more channels. This work led in 1981 to a portable spectrum analyzer named "Suitcase SETI" that had a capacity of 131,000 narrowband channels. After field tests that lasted into 1982, Suitcase SETI was put into use in 1983 with the 26-meter Harvard/Smithsonian [[radio telescope]] at [[Harvard, Massachusetts]]. This project was named "Sentinel," and continued into 1985.
 
 
Even 131,000 channels weren't enough to search the sky in detail at a fast rate, so Suitcase SETI was followed in 1985 by Project "META," for "Megachannel Extra-Terrestrial Assay." The META spectrum analyzer had a capacity of 8.4 million channels and a channel resolution of 0.05 hertz. An important feature of META was its use of frequency [[doppler shift]] to distinguish between signals of terrestrial and extraterrestrial origin.  The project was led by Horowitz with the help of the Planetary Society, and was partly funded by movie maker Steven Spielberg. A second such effort, META II, was begun in Argentina in 1990 to search the southern sky. META II is still in operation, after an equipment upgrade in 1996. The next year, in 1986, UC Berkeley initiated their second SETI effort, SERENDIP II, and has continued with two more SERENDIP efforts to the present day.
 
 
The follow-on to META was named "BETA," for "Billion-channel ExtraTerrestrial Assay," and it commenced observation on October 30, 1995.  The heart of BETA's processing capability consisted of 63 dedicated FFT engines, each capable of performing a 2^22-point [[Complex number#Signal analysis|complex]] [[fast Fourier transform]] in two seconds, and 21 general-purpose [[IBM PC compatible|PC]]s equipped with custom [[digital signal processing]] boards.  This allowed BETA to receive 250 million simultaneous channels with a resolution of 0.5 hertz per channel.  It scanned through the [[microwave]] [[spectrum]] from 1.400 to 1.720 gigahertz in eight hops, with two seconds of observation per hop.  An important capability of the BETA search was rapid and automatic reobservation of candidate signals, achieved by observing the sky with two adjacent beams, one slightly to the east and the other slightly to the west.  A successful candidate signal would first transit the east beam, and then the west beam and do so with a speed consistent with the earth's [[sidereal]] rotation rate.  A third receiver observed the horizon to veto signals of obvious terrestrial origin.  On March 23, 1999 the 26-meter [[radio telescope]] on which Sentinel, META and BETA were based was blown over by strong winds and seriously damaged.  This forced the BETA project to cease operation.
 
 
====MOP and Project Phoenix====
 
In 1992, the U.S. government finally funded an operational SETI program, in the form of the NASA "Microwave Observing Program (MOP)." MOP was planned as a long-term effort, performing a "Targeted Search" of 800 specific nearby stars, along with a general "Sky Survey" to scan the sky.  MOP was to be performed by radio dishes associated with the NASA [[Deep Space Network]], as well as a 43-meter dish at Green Bank and the big Arecibo dish. The signals were to be analyzed by spectrum analyzers, each with a capacity of 15 million channels. These spectrum analyzers could be ganged to obtain greater capacity. Those used in the Targeted Search had a bandwidth of 1 hertz per channel, while those used in the Sky Survey had a bandwidth of 30 hertz per channel.
 
 
MOP drew the attention of the [[Congress of the United States|U.S. Congress]], where the program was strongly ridiculed, and was canceled a year after its start. SETI advocates did not give up, and in 1995 the nonprofit "SETI Institute" of [[Mountain View, Santa Clara County, California|Mountain View, California]], resurrected the work under the name of Project "Phoenix," backed by private sources of funding.  [[Project Phoenix (SETI)|Project Phoenix]], under the direction of Dr. [[Jill Tarter]], previously Project Scientist for the NASA project, is a continuation of the Targeted Search program, studying roughly 1,000 nearby Sunlike stars.  [[Seth Shostak]] also worked on Project Phoenix. From 1995 through March 2004, Phoenix conducted observing campaigns at the 64-meter [[Parkes Observatory|Parkes radio telescope]] in Australia, the 140 Foot Telescope of the National Radio Astronomy Observatory in West Virginia, USA, and the Arecibo Observatory in Puerto Rico. The project observed the equivalent of 800 stars over the available channels in the frequency range from 1200 to 3000 MHz. The search was sensitive enough to pick up transmitters with power output equivalent to airport radars to a distance of about 200 light years.
 
 
====Allen Telescope Array====
 
 
The SETI Institute is now collaborating with the Radio Astronomy Laboratory at UC Berkeley to develop a specialized radio telescope array for SETI studies, something like a mini-Cyclops array.  The new array concept is named the "Allen Telescope Array" (ATA) (formerly, One Hectare Telescope [1HT]) after the project's benefactor [[Paul Allen]]. Its sensitivity will be equivalent to a single large dish more than 100 meters on a side.  The array is being constructed at the [[Hat Creek Observatory]] in rural northern California. <ref name="Allen">{{cite web | url = http://www.seti.org/site/pp.asp?c=ktJ2J9MMIsE&b=179146 | title = Allen Telescope Array General Overview | publisher = [[SETI Institute]] | accessdate = 2006-06-12}}</ref>
 
 
The full array is planned to consist of 350 or more Gregorian radio dishes, each 6.1 meters (20 feet) in diameter. These dishes are the largest producable with commercially available [[satellite television]] dish technology. The ATA was planned for a 2007 completion date, at a very modest cost of $25 million USD, but the completion date will surely slip. The SETI Institute provides money for building the ATA while UC Berkeley designs the telescope and provides operational funding.  Berkeley astronomers will use the ATA to pursue other deep space radio observations. The ATA is intended to support a large number of simultaneous observations through a technique known as "multibeaming," in which DSP technology is used to sort out signals from the multiple dishes. The DSP system planned for the ATA is extremely ambitious.
 
 
The ATA schedule has slipped, not surprising for an ambitious project on a limited budget.  The individual antennas work, can be fabricated, and meet specifications.  As of summer 2006, roughly 10 of the antennas are complete and 42 are under final construction.  Although not yet capable of significant radio astronomy or SETI observations, the ATA has become a testbed for array technology, as needed for the [[Square Kilometre Array]], the US Navy, and DARPA.  Completion of the full 350 element array will depend on funding and the technical results from the 42 element sub-array.
 
 
===Optical SETI experiments===
 
While most SETI sky searches have studied the radio spectrum, some SETI researchers have considered the possibility that alien civilizations might be using powerful [[laser]]s for interstellar communications at optical wavelengths.
 
The idea was first suggested in a paper published in the British journal ''[[Nature (journal)|Nature]]'' in 1961, and in 1983 [[Charles Townes]], one of the inventors of the laser, published a detailed study of the idea in the US journal ''[[Proceedings of the National Academy of Sciences]]''.
 
 
Most SETI researchers agreed with the idea. The 1971 Cyclops study discounted the possibility of optical SETI, reasoning that construction of a laser system that could outshine the bright central sun of a remote star system would be too difficult. Now some SETI advocates, such as [[Frank Drake]], have suggested that such a judgement was too conservative.
 
 
There are two problems with optical SETI, one of which is easy to deal with, the second of which is troublesome.
 
The first problem is that lasers are highly "monochromatic," that is, they emit light only on one frequency, making it troublesome to figure out what frequency to look for.
 
However, according to [[Harmonic analysis|Harmonic analysis (Fourier analysis)]], emitting light in narrow pulses results in a broad spectrum of emission{{fact}}, with the frequencies becoming higher as the pulse width becomes narrower, and an interstellar communications system could use pulsed lasers.
 
 
The other problem is that while radio transmissions can be broadcast in all directions, lasers are highly directional. This means that a laser beam could be easily blocked by clouds of [[interstellar dust]], and more to the point, we could pick it up only if we happened to cross its line of fire.
 
As it is unlikely an alien civilization would focus an interstellar laser communications beam on Earth deliberately, we would have to cross such a beam by accident.
 
 
However, as discussed earlier, the power requirements for omnidirectional interstellar radio broadcasts are tremendous, and narrow-beam radio communications are technically more plausible.
 
As SETI researchers have adjusted to the idea that interstellar radio communications may be over narrow beams, the idea of hunting for interstellar laser beams has become no more troublesome.
 
 
Several optical SETI experiments are now in progress.
 
A Harvard-Smithsonian group that includes Paul Horowitz designed a laser detector and mounted it on Harvard's 155 centimeter (61 inch) optical telescope.
 
This telescope is currently being used for a more conventional star survey, and the optical SETI survey is "[[piggyback]]ing" on that effort.
 
 
Between October 1998 and November 1999, the survey inspected about 2,500 stars. Nothing that resembled an intentional laser signal was detected, but efforts continue.
 
The Harvard-Smithsonian group is now working with Princeton to mount a similar detector system on Princeton's 91-centimeter (36-inch) telescope.
 
The Harvard and Princeton telescopes will be "ganged" to track the same targets at the same time, with the intent being to detect the same signal in both locations as a means of reducing errors from detector noise.
 
 
The Harvard-Smithsonian group is now building a dedicated all-sky optical survey system along the lines of that described above, featuring a 1.8-meter (72-inch) telescope.
 
The new optical SETI survey telescope is being set up at the [[Oak Ridge Observatory]] in [[Harvard, Massachusetts]].
 
 
The University of California, Berkeley, home of SERENDIP and SETI@home, is also conducting optical SETI searches.
 
One is being directed by [[Geoffrey Marcy]], the well-known extrasolar planet hunter, and involves examination of records of spectra taken during [[extrasolar planet]] hunts for a continuous, rather than pulsed, laser signal.
 
 
The other Berkeley optical SETI effort is more like that being pursued by the Harvard-Smithsonian group and is being directed by Dan Werthimer of Berkeley, who built the laser detector for the Harvard-Smithsonian group.
 
The Berkeley survey uses a 76-centimeter (30-inch) automated telescope and an older laser detector built by Wertheimer.
 
 
 
  
 
===Criticism of SETI===
 
===Criticism of SETI===
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* {{cite book | author = Exers, Ronald, D. Cullers, J. Billingham, L. Scheffer (editors) | title = SETI 2020: A Roadmap for the Search for Extraterrestrial Intelligence | year = 2003 | publisher = SETI Press | id = ISBN 0-9666335-3-9}}
 
* {{cite book | author = Exers, Ronald, D. Cullers, J. Billingham, L. Scheffer (editors) | title = SETI 2020: A Roadmap for the Search for Extraterrestrial Intelligence | year = 2003 | publisher = SETI Press | id = ISBN 0-9666335-3-9}}
 
* {{cite book | last = McConnell | first = Brian | coauthors = Chuck Toporek | title = Beyond Contact: A Guide to SETI and Communicating with Alien Civilizations | year = 2001 | publisher = O'Reilly | id = ISBN 0-596-00037-5}}
 
* {{cite book | last = McConnell | first = Brian | coauthors = Chuck Toporek | title = Beyond Contact: A Guide to SETI and Communicating with Alien Civilizations | year = 2001 | publisher = O'Reilly | id = ISBN 0-596-00037-5}}
 
 
 
 
*Roth, Christopher F., "Ufology as Anthropology: Race, Extraterrestrials, and the Occult."  In ''E.T. Culture: Anthropology in Outerspaces,'' ed. by Debbora Battaglia.  Durham, N.C.: Duke University Press, 2005.
 
*Roth, Christopher F., "Ufology as Anthropology: Race, Extraterrestrials, and the Occult."  In ''E.T. Culture: Anthropology in Outerspaces,'' ed. by Debbora Battaglia.  Durham, N.C.: Duke University Press, 2005.
 
 
* [[Carl Sagan|Sagan, Carl]]. 1996. ''The Demon-Haunted World: Science as a Candle in the Dark: chapter 4: "Aliens"
 
* [[Carl Sagan|Sagan, Carl]]. 1996. ''The Demon-Haunted World: Science as a Candle in the Dark: chapter 4: "Aliens"
 
 
 
 
 
 
* {{cite book
 
* {{cite book
 
| author = [[David Grinspoon (scientist)|David Grinspoon]]
 
| author = [[David Grinspoon (scientist)|David Grinspoon]]
Line 271: Line 181:
  
 
==External links==
 
==External links==
*[http://www.vega.org.uk/video/programme/9 'Is There Anybody Out There?'] Freeview video by the Vega Science Trust and the BBC/OU.
+
*[http://astrobiology.arc.nasa.gov/about/index.cfm ''NASA: Astrobiology'']
*[http://www.actualaliens.com Actual Aliens]: Extraterrestrial News and Current Events
 
 
*[http://www.pbs.org/lifebeyondearth/index.html ''PBS: Life Beyond Earth'' a film by Timothy Ferris]
 
*[http://www.pbs.org/lifebeyondearth/index.html ''PBS: Life Beyond Earth'' a film by Timothy Ferris]
 
*[http://www.pbs.org/exploringspace/ ''PBS: Exploring Space - The Quest for Life'' by Scott Pearson]
 
*[http://www.pbs.org/exploringspace/ ''PBS: Exploring Space - The Quest for Life'' by Scott Pearson]
*[http://www.ufoskeptic.org ''ufoskeptic.org'' by Bernard Haisch]
 
 
*[http://www.rfreitas.com/Astro/Xenopsychology.htm ''Xenopsychology'' by Robert A. Freitas Jr.]
 
*[http://www.rfreitas.com/Astro/Xenopsychology.htm ''Xenopsychology'' by Robert A. Freitas Jr.]
 
*[http://news.nationalgeographic.com/news/2005/05/0520_050520_tv_aliens.html "What Aliens Might Look Like"] from [[National Geographic]]
 
*[http://news.nationalgeographic.com/news/2005/05/0520_050520_tv_aliens.html "What Aliens Might Look Like"] from [[National Geographic]]
*[http://www.sylviaengdahl.com/space/poetry1.htm Sylvia Engdahl , "Early Space Poetry" Part I]: Didactic and other poetry concerning other inhabited worlds, well-known and obscure poets, 17th-18th centuries. [http://www.sylviaengdahl.com/space/poetry2.htm "Part II":] 19th century
 
 
*[http://news.bbc.co.uk/1/hi/sci/tech/4728228.stm Top stars picked in alien search]
 
*[http://news.bbc.co.uk/1/hi/sci/tech/4728228.stm Top stars picked in alien search]
 
 
* [http://ufologie.net/htm/caponi.htm ufologie.net - The Filiberto Caponi close encounter of the 3rd kind, 1993]
 
* [http://www.ufocasebook.com/caponi.html ufocasebook.com - Filiberto Caponi Close Encounter 1993]
 
* [http://ufologie.net/htm/ilkleymoor.htm The Ilkley Moor encounter of the 3rd kind, 1987]
 
 
{{cleanup-date|2006 September}}<!-- too many links surely? —>
 
 
* [http://www.seti.org/ SETI Institute]
 
* [http://www.seti.org/ SETI Institute]
* [http://setiathome.ssl.berkeley.edu/ SETI@home], the [[shared computing]] project
 
 
* [http://www.planetary.org/ The Planetary Society]
 
* [http://www.planetary.org/ The Planetary Society]
 
* [http://www.setileague.org/ The SETI League]
 
* [http://www.setileague.org/ The SETI League]
:* [http://www.setileague.org/iaaseti/index.html IAA SETI Permanent Study Group]
 
:* [http://www.setileague.org/editor/clarke.htm Where Is Everybody?] : an [[essay]] by [[Arthur C. Clarke]] on SETI
 
 
* [http://www.iaaweb.org/ International Academy of Astronautics]
 
* [http://www.iaaweb.org/ International Academy of Astronautics]
 
* [http://www.boulder.swri.edu/CSEPR/projects/readings/race-need_for_operating_guidelines.pdf ''SETI Principles''] as defined from the [[Department of Space Studies]] of the [[Southwest Research Institute]] (PDF File)
 
* [http://www.boulder.swri.edu/CSEPR/projects/readings/race-need_for_operating_guidelines.pdf ''SETI Principles''] as defined from the [[Department of Space Studies]] of the [[Southwest Research Institute]] (PDF File)
* [http://seti.harvard.edu/seti/ Harvard University SETI page]
 
* [http://www.coseti.org The Columbus Optical SETI Observatory, Dr. Stuart A, Kingsley]
 
* [http://www.spacedaily.com/news/seti-04e.html ''First Contact Within 20 Years: Shostak''] &ndash; From SpaceDaily.com, 22 July 2004 (based on calculations to be published in [[Acta Astronautica]])
 
 
* [http://SkyandTelescope.com/resources/seti/ ''SETI: Searching for Life''] &ndash; Article series in [[Sky & Telescope]] magazine
 
* [http://SkyandTelescope.com/resources/seti/ ''SETI: Searching for Life''] &ndash; Article series in [[Sky & Telescope]] magazine
 
* Cirkovic, Milan M., and Bradbury, R. J., 200n, "[http://www.anthropic-principle.com/preprints/milan-seti.pdf Galactic Gradients, Postbiological Evolution, and the Apparent Failure of SETI.]"
 
* Cirkovic, Milan M., and Bradbury, R. J., 200n, "[http://www.anthropic-principle.com/preprints/milan-seti.pdf Galactic Gradients, Postbiological Evolution, and the Apparent Failure of SETI.]"
 
* [http://history.nasa.gov/garber.pdf ''Searching for Good Science: The Cancellation of NASA's SETI Program''] ([[Portable Document Format|PDF]]) &ndash; By [[Stephen J. Garber]], [[NASA History Office]].  ''Journal of the British Interplanetary Society'', Vol. 52, pp. 3-12, 1999. Provides more details on the elimination of SETI funding by the US Congress in 1993.
 
* [http://history.nasa.gov/garber.pdf ''Searching for Good Science: The Cancellation of NASA's SETI Program''] ([[Portable Document Format|PDF]]) &ndash; By [[Stephen J. Garber]], [[NASA History Office]].  ''Journal of the British Interplanetary Society'', Vol. 52, pp. 3-12, 1999. Provides more details on the elimination of SETI funding by the US Congress in 1993.
* [http://www.openseti.org Open SETI Initiative] &ndash; Gerry Zeitlin's site concerned with reforming SETI's approach
 
* [http://groups.myspace.com/galacticdrifterseti Galactic Drifter SETI] &ndash; Example of an economical SETI contact strategy in terms of look direction and timing constraints
 
* [http://history.nasa.gov/SP-419/sp419.htm ''The Search For Extraterrestrial Intelligence'' (NASA SP-419, 1977)]
 
* [http://www.winlab.rutgers.edu/~crose/cgi-bin/cosmic23.html  ET Might Write, Not Radiate]
 
* [http://www.satsig.net/seticalc.htm  SETI radio link-budget range calculator]
 
* [http://www.ccnmag.com/story.php?id=146  IT & SETI: The Role of Computer Technology in the Search for Extraterrestrial Intelligence]
 
* [http://www.markelowitz.com/exobiology.htm Mark Elowitz's Web site on Exobiology and SETI]
 
* [http://www.bigear.org/ Big Ear Memorial Website] - discovered the "Wow!" signal and has entry in Guinness Book of Records
 
* [http://www.naapo.org/ NAAPO], North American AstroPhysical Observatory (formerly Big Ear)
 
* [http://spsr.utsi.edu/ SPSR] The Society for Planetary SETI Research
 
* [http://www.setifaq.org/ SETI@home FAQ for newsgroups alt.sci.seti and sci.astro.seti]
 
* [http://www.spacedaily.com/reports/Has_Seti_Been_Barking_Up_The_Wrong_Tree_Mostly_999.html Has SETI Been Barking Up the Wrong Tree (Mostly?]
 
* {{cite news | title=Top stars picked in alien search | publisher=BBC News | date=2006-02-19 | url=http://news.bbc.co.uk/1/hi/sci/tech/4728228.stm | accessdate=2006-08-13 }}
 
 
 
 
{{Credit3|Extraterrestrial_life|79457760|Extraterrestrial_life_in_popular_culture|78634268|SETI|79467501|}}
 

Revision as of 02:59, 2 May 2007


Extraterrestrial life is life that may exist and originate outside the planet Earth, the only place in the universe known to support life. Its existence is currently hypothetical; there is yet no evidence of extraterrestrial life that has been widely accepted by the scientific community.

Speculative forms of extraterrestrial life range from humanoid and monstrous beings seen in works of science fiction to life at the much smaller scale of bacteria. Extraterrestrial life forms, especially intelligent ones, are often referred to in popular culture as aliens or ETs. The putative study and theorisation of ET life is known as astrobiology or xenobiology.

Historical Belief in Extraterrestrial Life

Astronomy played a significant role in ancient societies, the arrangment of heavenly bodies inspiring cultural beliefs and especially mythology. Beliefs in creatures and lifeforms that populated the sky world became almost common place in the ancient world. The atomists of Greece took up the idea of an infinite universe, with an infinity of populated worlds. The Jewish Talmud states that there are at least 18,000 other worlds. The Babylonians, Egyptians, Sumerians, Chinese and Aztecs all held somewhat similar ideas of multiple worlds that existed amongst the stars. However, these beliefs were often spiritually focused, as the sky and stars was often the domain of dieties and supernatural powers. The notion of alien biological lifeforms as they are thought of today, did take shape for centuries.

Giordano Bruno, De l'Infinito, Univirso e Mondi, 1584

This situation changed, however, with the dramatic shift in thinking initiated by the invention of the telescope and the Copernican assault on geocentric cosmology. Once it became clear that the Earth was merely one planet amongst countless bodies in the universe the extraterrestrial idea moved towards the scientific mainstream. God's omnipotence, it could be argued, not only allowed for other worlds and other life, on some level it necessitated them. The best known early-modern proponent of such ideas was Giordano Bruno, who argued in the 16th century for an infinite universe in which every star is surrounded by its own solar system; he was eventually burned at the stake for heretical ideas.[1] Dominican monk Tommaso Campanella wrote about a Solarian alien race in his Civitas Solis. The possibility of extraterrestrials remained a widespread speculation as scientific discovery accelerated. William Herschel, the discoverer of Uranus, was one of many 18th-19th century astronomers convinced that our Solar System, and perhaps others, would be well populated by alien life. Other luminaries of the period who championed "cosmic pluralism" included Immanuel Kant and Benjamin Franklin. At the height of the Enlightenment even the Sun and Moon were considered candidates for hosting aliens.

Extraterrestrials and the Modern era

This enthusiasm towards the possibility of alien life continued well into the 20th century. As long as human kind was unable to travel into space, extraterrestrial life seemed as probable to scientists and the general public alike. However, a split in the belief in E.T. life forms occured in the beginning half of the 20th century. With advancement in the scientific areas of physics, astronomy and evolutionary biology, scientists started to understand how complicated and fragile it was for life to develop on Earth, let alone elsewhere in a largely dangerous and inhospitable universe. Furthermore, the early explorations of space by probes showed no signs of life on the barren planet of Mars and exposed Venus to be a planet of such dramatic climate it is not condusive to support any known forms of life. The major scientific arguement against extraterrestrial life was formed; Earth was unique in its evolution, randomly composed of the exact conditions to support the fragile, and somewhat random itself, process that led to life. Most scientists believed, and still do that for such conditions to happen twice, even in a universe as big as ours, is unlikely (See Scientific Debate below)

Yet, as science was dismissing the notion of extraterrestrial life, it was becoming more popular in the public's imagination. The connection between extraterrestrials, the sudden frequent reports of UFOs, and the anthropromorphizing of extraterrestrals into the common identity of aliens, as they are known today, happened in a time period between 1920 and 1950. The possibility of intelligent life forms became an almost alluring mystery to the public. Early science fiction of the period used aliens frequently in its stories. Even those who claimed not to believe in aliens, shared a widespread fear of malevolent creatures from space, possibly best demonstrated by Orson Welles' infamous radio broadcast of The World of the Wars in which hundreds of people in the New York and New Jersey area were led to believe an invasion by aliens was taking place.

Artistic depiction of a Grey Alien

Belief in aliens has become one of the most interesting and complicated aspects of pop culture, the paranormal and the new age movement in the later half of the 20th century. Not only is commonly believed that UFOs are in fact alien space craft, but reports of contact between humans and aliens have been prevalent since the 1950s. One popular phenomeon is the abduction of humans by aliens, during which humans are unwittingly brought aboard space craft and subjected to medical examinations. Conspiracy theorists have claimed that world governments have clandestine relationships with aliens or are otherwise covering up alien existence. Some new age socities believe aliens hold a special place in the spiritual realm. These beliefs are fueled by overwhelming reports, observations, and the media, in which aliens are commonplace elements of movies and television shows, as well as books and documentaries. Commonly, these aliens are seen as small, with greyish skin, large head and black, lidless eyes. They are sometimes refered to as Greys. Other depictions percieve aliens as repitilian, insect-like, or even resembling people of Nordic descent.

File:Grey alien close1.jpg
A grey alien close-up

Aliens are depicted in numerous different ways; some portray and believe aliens exist to help mankind, while other times aliens are seen as hostile and using mankind for their own advancement. Either way, the notion that there are other life forms that possess similar intelligence and cognitant abilities as humans seems to strike a cord in humanity. Perhaps it is an overactive imagination projecting onto the infinity of the cosmos, of which we still know little. Or perhaps the fear of the ultimate unknown, that which is alien to mankind that helps fuel the belief.

Scientific Approach

Since there is no solid proof for the existence of extraterrestrial life, most of the scientific community since the mid 20th century have not given the idea much thought, especially with the stigma of the more outlandish pop culture perspectives on the matter. However, there have been, and continue to be, scientists who engage the idea, on many different levels.

Basis of Life

In order for something to be considered a living organism, there are five biological criteria that must be met: ability to reproduce and grow, it consume nutrients in order to survive, have mobility and respond to external stimuli [2] Further, all living organisms on earth are based on the element carbon, depend on water as a meduim for crucial chemical reactions, and are made up of long strands of amino acids, known as DNA — Deoxyribonucleic acid. The difficulty with trying to understand possible other life forms, is that science currently is unaware of any other composition of life (there has been some speculation that instead of carbon, the element silicon may consistitue the basis of extraterrestrial life). Therefore, either life in the universe can only exist on planets with similar water and carbon levels and tempeture of Earth, or life exists in some form that we currently do not know about, and raises the issue of how to look for something that does not correspond to current understandings.

Speculation

Without concrete facts to analyze or direct phenomena to observe, most scientists studying extraterrestrial life must do so by speculation (Most speculation is, however, based on what is accepted knowledge of astronomy and biology, as well as careful scientific postulating). Even with so many unknown variables, such postulating requires that specific guidelines be established in order to further pursue the notion. For example, scientists must first try to understand if the evolution of extraterrestrial life would have occurred independently in different places in the universe, or if, as a minority of scientists contend, life in the universe could have stemmed from a smaller number of points of origin, and then spread across the universe, from habitable planet to habitable planet, known as panspermia.

In considering the subject more seriously, a useful division has been suggested between universal and parochial (narrowly restricted) characteristics. Universals are features which have evolved independently more than once on Earth (and thus presumably are not difficult to develop) and are so intrinsically useful that species will inevitably tend towards them. These include flight, sight, photosynthesis and limbs, all of which have evolved several times here on Earth with differing materialization. There are a huge variety of eyes, for example, many of which have radically different working schematics as well as different visual foci: the visual spectrum, infrared, polarity and echolocation. Parochials, by contrast, are essentially arbitrary evolutionary forms which often serve little utility (or at least have a function which can be equally served by dissimilar morphology) and probably will not be replicated. Parochials include the five digits of mammals, the genitalia and sexual mechanics of animals, as well as the curious and often fatal conjunction of the feeding and breathing passages found within many animals.

A consideration of which features are ultimately parochial challenges many taken for granted notions about morphological necessity. Skeletons, in some form, are likely to be replicated elsewhere, yet the vertebrate spine—while a profound development on Earth—is just as likely to be unique. Similarly, it is reasonable to expect some type of egg laying amongst off-Earth creatures but the mammary glands which set apart mammals may be a singular case.

The assumption of radical diversity amongst putative extraterrestrials is by no means settled. While many exobiologists do stress that the enormously heterogeneous nature of Earth life foregrounds even greater variety in space, others point out that convergent evolution dictates substantial similarities between Earth and off-Earth life. These two schools of thought are called "divergionism" and "convergionism," respectively.[3]

Currently, Astrobiology is a field of study that has gained legitimacy and acceptance in the scientific community. Its main objectives include the search for extraterrestrial life, but in doing so seek to develop a better understanding of life on Earth [4]

The Arecibo message is a digital message sent to globular star cluster M13, and is a well-known symbol of human attempts to contact extraterrestrials.

The Search For Extraterrestrials

Since the last quarter of the 20th century, scientists have been actively searching the universe for other lifeforms with all the different types of technology availble. Yet, even if all of NASA and the The European Space Agency's budgets were directed towards this one goal, the universe is still too large and our technological means still not adequate enough to exhaustively search those areas in space that we know are possibily harboring life. Still, there are undaunted scientists who contuine to search for possible life, whether it be bacteria or advanced civilizations. There are two different methods scientists use in this search: the direct and indirect method.

The Direct Method

Scientists are directly searching for evidence of unicellular life within the solar system, carrying out studies on the surface of Mars and examining meteors that have fallen to Earth. A mission is also proposed to Europa, one of Jupiter's moons with a liquid water layer under its surface, which might contain life.

There is some limited evidence that microbial life might possibly exist or have existed on Mars. An experiment on the Viking Mars lander reported gas emissions from heated Martian soil that some argue are consistent with the presence of microbes. However, the lack of corroborating evidence from other experiments on the Viking indicates that a non-biological reaction is a more likely hypothesis. Recently, Circadian rhythms have been allegedly discovered in Viking data. The interpretation is controversial. Independently in 1996 structures resembling bacteria were reportedly discovered in a meteorite, ALH84001, thought to be formed of rock ejected from Mars. This report is also controversial and scientific debate continues. (See Viking biological experiments.)

In February 2005, NASA scientists reported that they had found strong evidence of present life on Mars.[5] The two scientists, Carol Stoker and Larry Lemke of NASA's Ames Research Center, based their claims on methane signatures found in Mars' atmosphere that resemble the methane production of some forms of primitive life on Earth, as well as their own study of primitive life near the Rio Tinto river in Spain. NASA officials soon denied the scientists' claims, and Stoker herself backed off from her initial assertions.[6] However, only a few days after Stoker and Lemke made their claims, scientists from the European Space Agency reported that their own measurements of methane on Mars suggested an organic origin.[7]

Though such findings are still very much in debate, support among scientists for the belief in the existence of life on Mars seems to be growing. In an informal survey conducted at the conference in which the European Space Agency presented its findings, 75 percent of the scientists in attendance reported to believe that life once existed on Mars; 25 percent reported a belief that life currently exists there.[7]

Terrestrial Planet Finder - Infrared interferometer concept of finding Earth-like extrasolar planets

Astronomers also search for extrasolar planets that would be conducive to life, especially those like OGLE-2005-BLG-390Lb which have been found to have Earth-like qualities. Current radiodetection methods have been inadequate for such a search, as the resolution afforded by recent technology is inadequate for detailed study of extrasolar planetary objects. Future telescopes should be able to image planets around nearby stars, which may reveal the presence of life (either directly or through spectrography which would reveal key information such as the presence of free oxygen in a planet's atmosphere). Darwin is an ESA mission designed to find Earth-like planets, and analyse their atmosphere. It has been argued that one of the best candidates for the discovery of life-supporting planets may be Alpha Centauri, the closest star system to Earth, given that two of the three stars in the system are broadly sun-like.

Indirect search

It is theorised that any technological society in space will be transmitting information. Projects such as SETI are conducting an astronomical search for radio activity that would confirm the presence of intelligent life. A related suggestion is that aliens might broadcast pulsed and continuous laser signals in the optical as well as infrared spectrum;[8] laser signals have the advantage of not "smearing" in the interstellar medium and may prove more conducive to communication between the stars.

In 1960, Cornell University astronomer Frank Drake performed the first modern SETI experiment, named "Project Ozma," after the Queen of Oz in L. Frank Baum's fantasy books. Drake used a 25-meter-diameter radio telescope at Green Bank, West Virginia, to examine the stars Tau Ceti and Epsilon Eridani near the 1.420 gigahertz marker frequency. A 400 kilohertz band was scanned around the marker frequency, using a single-channel receiver with a bandwidth of 100 hertz. The information was stored on tape for off-line analysis. Nothing of great interest was found.

SETI (pronounced ['sɛti]) is the acronym for Search for Extra-Terrestrial Intelligence; organized efforts by humans to detect intelligent aliens. A number of efforts with "SETI" in the project name have been organized, including projects funded by the United States Government. The generic approach of SETI projects is to survey the sky to detect the existence of transmissions from a civilization on a distant planet - an approach widely endorsed by the scientific community as hard science.

There are great challenges in searching across the sky to detect a first transmission that can be characterised as intelligent, since its direction, spectrum and method of communication are all unknown beforehand. SETI projects necessarily make assumptions to narrow the search, and thus no exhaustive search has so far been conducted. Visiting another civilization on a distant world is presently beyond human capabilities (see Project Orion and Project Daedalus for some hypothetical explorations of the concept). However, it is currently technologically feasible to develop a communications system which uses a powerful transmitter and a sensitive receiver to search the sky for extraterrestrial worlds whose citizens have a similar inclination as terrestrials.

SETI is not generally viewed by scientists as a trivial task. Our galaxy, the Milky Way, is 100,000 light years across and contains approximately a hundred billion stars. Searching the entire sky for some far-away and faint signal is an exhausting exercise. A number of assumptions are needed for SETI to be feasible.

A basic assumption of SETI is that of "Mediocrity": the idea that humanity is not exotic in the cosmos but in a sense "typical" or "medium" when compared with other intelligent species.[citation needed] This would mean that humanity has sufficient similarities with other intelligent beings that communications would be mutually desirable and understandable. If this basic assumption of Mediocrity is correct, and other intelligent species are present in any number in the galaxy at our technological level or above, then communications between the two worlds should be inevitable.

Another assumption is to focus on Sun-like stars. Very big stars have relatively short lifetimes, meaning that intelligent life would likely not have time to evolve on planets orbiting them. Very small stars provide so little heat and warmth that only planets in very close orbits around them would not be frozen solid, and in such close orbits these planets would be tidally locked to the star, with one side of the planet perpetually baked and the other perpetually frozen. (However, some speculate that a thick cloud cover may mitigate these differences. [1])

About 10% of the stars in the Milky Way galaxy are Sun-like, and there are about a thousand such stars within 100 light-years of the Sun. These stars would be useful primary targets for interstellar listening.

However, we know of only one planet where life exists, our own. There is no way to know if any of the simplifying assumptions are correct, and so as a second priority the entire sky must be searched.

Searching the Electromagnetic Spectrum

In order to find an electromagnetic transmission from an alien civilization we also have to search through most of the useful radio spectrum, as there is no way to know what frequencies aliens might be using. Trying to transmit a powerful signal over a wide range of wavelengths is impractical, and so it is likely that such a signal would be transmitted on a relatively narrow band. This means that a wide range of frequencies must be searched at every spatial coordinate of the sky.

There is also the problem of knowing what to listen for, as we have no idea how a signal sent by aliens might be modulated, and how the data transmitted by it might be encoded. Narrow-bandwidth signals that are stronger than background noise and constant in intensity are obviously interesting, and if they have a regular and complex pulse pattern are likely to be artificial.

However, while studies have been performed on how to send a signal that could be easily deciphered, there is no way to know if the assumptions of those studies are valid, and deciphering the information from an alien signal could be very difficult.

Arecibo message

In 1974, a largely symbolic attempt was made to send a message to other worlds. To celebrate a substantial upgrading of the 305 meter Arecibo Radio Telescope in Puerto Rico, a coded message of 1,679 bits was transmitted towards the Globular Cluster M13, about 25,100 light years away.

The pattern of 0s and 1s contained in the message defines a 23 × 73 two dimensional grid which when plotted reveals some data about our location in the Solar System, a stylized figure of a human being, chemical formulae and an outline of the radio telescope itself. The 23 by 73 grid was chosen because both 23 and 73 are prime numbers, which makes it easier to decode the message.

Given the limitations of the speed of light for message transmission, no reply would be possible before the year 52,174 (approximately) and hence has been dismissed by some as a publicity stunt. A controversy arose because the transmission raised the serious question of whether a small group should be allowed to speak for Earth.

Criticism of SETI

SETI has occasionally been the target of criticism by those who suggest that it is a form of pseudoscience. In particular, critics allege that no observed phenomena suggest the existence of extraterrestrial intelligence, and furthermore that the assertion of the existence of extraterrestrial intelligence has no good Popperian criteria for falsifiability [2]. Science fiction writer Michael Crichton, in a 2003 lecture at Caltech, stated that "The Drake equation cannot be tested and therefore SETI is not science. SETI is unquestionably a religion." [3].

In response, SETI advocates note, among other things, that the existence of intelligent life on Earth is a plausible reason to expect it elsewhere, and that individual SETI projects have clearly defined "stop" conditions. Concerning the latter argument, the justification for SETI projects doesn't necessarily require an acceptance of the Drake equation. The search for extra-terrestrial intelligence is not an assertion that extra-terrestrial intelligence exists, and conflating the two can be seen as a straw man argument. There is an effort to distinguish the SETI projects from UFOlogy, the study of UFOs considered to be pseudoscience by many.

In 1983 Stanislaw Lem, disappointed with the lack of results of SETI in spite of the huge effort, has noted that he considers the Universe silent, coining the moniker silencium universi.

References
ISBN links support NWE through referral fees

  1. Helden, Al Van (1995) [Bruno (1548-1600)"] Retrieved April 28, 2007
  2. (2007) ["Definition of Life"] Retrieved May 1, 2007
  3. Variety of extraterrestrial life. daviddarling.info.
  4. (2006) ["NASA - Astrobiology"] Retrieved May 1, 2007
  5. Berger, Brian, "Exclusive: NASA Researchers Claim Evidence of Present Life on Mars", 2005.
  6. "NASA denies Mars life reports", spacetoday.net, 2005.
  7. 7.0 7.1 Michelson, , "European Scientists Believe in Life on Mars", Yahoo News, 2005.
  8. The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum. The Columbus Optical SETI Observatory.

Further reading

  • Exers, Ronald, D. Cullers, J. Billingham, L. Scheffer (editors) (2003). SETI 2020: A Roadmap for the Search for Extraterrestrial Intelligence. SETI Press. ISBN 0-9666335-3-9. 
  • McConnell, Brian and Chuck Toporek (2001). Beyond Contact: A Guide to SETI and Communicating with Alien Civilizations. O'Reilly. ISBN 0-596-00037-5. 
  • Roth, Christopher F., "Ufology as Anthropology: Race, Extraterrestrials, and the Occult." In E.T. Culture: Anthropology in Outerspaces, ed. by Debbora Battaglia. Durham, N.C.: Duke University Press, 2005.
  • Sagan, Carl. 1996. The Demon-Haunted World: Science as a Candle in the Dark: chapter 4: "Aliens"
  • David Grinspoon (2003). Lonely Planets: The Natural Philosophy of Alien Life. HarperCollins. ISBN 0-06-018540-6. 
  • Jack Cohen and Ian Stewart (2002). Evolving the Alien: The Science of Extraterrestrial Life. Ebury Press. ISBN 0-09-187927-2. 
  • John C. Baird (1987). The Inner Limits of Outer Space: A Psychologist Critiques Our Efforts to Communicate With Extraterrestrial Beings. Hanover: University Press of New England. ISBN 0-87451-406-1. 
  • Donald Goldsmith (1997). The Hunt for Life on Mars. New York: A Dutton Book. ISBN 0-525-94336-6. 
  • Michael T. Lemnick (1998). Other Worlds: The Search for Life in the Universe. New York: A Touchstone Book. 
  • Cliff Pickover (2003). The Science of Aliens. New York: Basic Books. ISBN 0-465-07315-8. 
  • Roth, Christopher F. (2005) "Ufology as Anthropology: Race, Extraterrestrials, and the Occult." In E.T. Culture: Anthropology in Outerspaces, ed. by Debbora Battaglia. Durham, N.C.: Duke University Press.
  • Crowe, Michael J.. The Extraterrestrial Life Debate, 1750—1900. Dover Publications. 
  • Sagan, Carl and I.S. Shklovskii (1966). Intelligent Life in the Universe. Random House. 
  • Sagan, Carl (1973). Communication with Extraterrestrial Intelligence. MIT Press. 

External links