Astrobiology

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For the journal, see Astrobiology (journal).
See also: Talk:Abiogenesis#Primitive extraterrestrial life re challenged "Life Before Earth" edits
Nucleic acids may not be the only biomolecules in the Universe capable of coding for life processes.[1]

Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe: extraterrestrial life and life on Earth. This interdisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System, the search for evidence of prebiotic chemistry, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in outer space.[2] Astrobiology addresses the question of whether life exists beyond Earth, and how humans can detect it if it does.[3] (The term exobiology is similar but more specific — it covers the search for life beyond Earth, and the effects of extraterrestrial environments on living things.)[4]

Astrobiology makes use of physics, chemistry, astronomy, biology, molecular biology, ecology, planetary science, geography, and geology to investigate the possibility of life on other worlds and help recognize biospheres that might be different from the biosphere on Earth.[5][6] Astrobiology concerns itself with interpretation of existing scientific data; given more detailed and reliable data from other parts of the universe, the roots of astrobiology itself—physics, chemistry and biology—may have their theoretical bases challenged. Although speculation is entertained to give context, astrobiology concerns itself primarily with hypotheses that fit firmly into existing scientific theories.

Earth is the only place in the universe known to harbor life.[7][8] However, recent advances in planetary science have changed fundamental assumptions about the possibility of life in the universe, raising the estimates of habitable zones around other stars,[9][10] along with the discovery of hundreds of extrasolar planets and new insights into the extreme habitats here on Earth, suggesting that there may be many more habitable places in the universe than considered possible until very recently. On 4 November 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of sun-like stars and red dwarf stars within the Milky Way Galaxy.[11][12] 11 billion of these estimated planets may be orbiting sun-like stars.[13] The nearest such planet may be 12 light-years away, according to the scientists.[11][12]

It has been proposed that viruses are likely to be encountered on other life-bearing planets.[14] Efforts to discover current or past life on Mars is an active area of research. On 24 January 2014, NASA reported that current studies on the planet Mars by the Curiosity and Opportunity rovers will now be searching for evidence of ancient life, including a biosphere based on autotrophic, chemotrophic and/or chemolithoautotrophic microorganisms, as well as ancient water, including fluvio-lacustrine environments (plains related to ancient rivers or lakes) that may have been habitable.[15][16][17][18] The search for evidence of habitability, taphonomy (related to fossils), and organic carbon on the planet Mars is now a primary NASA objective.[15]

Overview[edit]

It is not known whether life elsewhere in the universe would utilize cell structures like those found on Earth. (Chloroplasts within plant cells shown here.)[19]

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In June 2014, the John W. Kluge Center of the Library of Congress held a seminar focusing on astrobiology. Panel members (l to r) Robin Lovin, Derek Malone-France, and Steven J. Dick

Astrobiology is etymologically derived from the Greek ἄστρον, astron, "constellation, star"; βίος, bios, "life"; and -λογία, -logia, study. The synonyms of astrobiology are diverse; however, the synonyms were structured in relation to the most important sciences implied in its development: astronomy and biology. A close synonym is exobiology from the Greek Έξω, "external"; Βίος, bios, "life"; and λογία, -logia, study. The term exobiology was first coined by molecular biologist Joshua Lederberg. Exobiology is considered to have a narrow scope limited to search of life external to earth, whereas subject area of astrobiology is wider and investigates the link between life and the universe, which includes the search for extraterrestrial life, but also includes the study of life on earth, its origin, evolution and limits. Exobiology as a term has tended to be replaced by astrobiology.

Another term used in the past is xenobiology, ("biology of the foreigners") a word used in 1954 by science fiction writer Robert Heinlein in his work The Star Beast.[20] The term xenobiology is now used in a more specialized sense, to mean "biology based on foreign chemistry", whether of extraterrestrial or terrestrial (possibly synthetic) origin. Since alternate chemistry analogs to some life-processes have been created in the laboratory, xenobiology is now considered as an extant subject.[21]

While it is an emerging and developing field, the question of whether life exists elsewhere in the universe is a verifiable hypothesis and thus a valid line of scientific inquiry. Though once considered outside the mainstream of scientific inquiry, astrobiology has become a formalized field of study. Planetary scientist David Grinspoon calls astrobiology a field of natural philosophy, grounding speculation on the unknown, in known scientific theory.[22] NASA's interest in exobiology first began with the development of the U.S. Space Program. In 1959, NASA funded its first exobiology project, and in 1960, NASA founded an Exobiology Program; Exobiology research is now one of four elements of NASA's current Astrobiology Program.[3][23] In 1971, NASA funded the Search for Extra-Terrestrial Intelligence (SETI) to search radio frequencies of the electromagnetic spectrum for signals being transmitted by extraterrestrial life outside the Solar System. NASA's Viking missions to Mars, launched in 1976, included three biology experiments designed to look for possible signs of present life on Mars. The Mars Pathfinder lander in 1997 carried a scientific payload intended for exopaleontology in the hopes of finding microbial fossils entombed in the rocks.[24]

In the 21st century, astrobiology is a focus of a growing number of NASA and European Space Agency Solar System exploration missions. The first European workshop on astrobiology took place in May 2001 in Italy,[25] and the outcome was the Aurora programme.[26] Currently, NASA hosts the NASA Astrobiology Institute and a growing number of universities in the United States (e.g., University of Arizona, Penn State University, Montana State University – Bozeman, University of Washington, and Arizona State University),[27] Britain (e.g., The University of Glamorgan, Buckingham University),[28] Canada, Ireland, and Australia (e.g., The University of New South Wales)[29] now offer graduate degree programs in astrobiology. The International Astronomical Union regularly organizes international conferences through its Bioastronomy Commission.[30]

Advancements in the fields of astrobiology, observational astronomy and discovery of large varieties of extremophiles with extraordinary capability to thrive in the harshest environments on Earth, have led to speculation that life may possibly be thriving on many of the extraterrestrial bodies in the universe. A particular focus of current astrobiology research is the search for life on Mars due to its proximity to Earth and geological history. There is a growing body of evidence to suggest that Mars has previously had a considerable amount of water on its surface, water being considered an essential precursor to the development of carbon-based life.[31]

Missions specifically designed to search for life include the Viking program and Beagle 2 probes, both directed to Mars. The Viking results were inconclusive,[32] and Beagle 2 failed to transmit from the surface and is assumed to have crashed.[33] A future mission with a strong astrobiology role would have been the Jupiter Icy Moons Orbiter, designed to study the frozen moons of Jupiter—some of which may have liquid water—had it not been cancelled. In late 2008, the Phoenix lander probed the environment for past and present planetary habitability of microbial life on Mars, and to research the history of water there.

In November 2011, NASA launched the Mars Science Laboratory (MSL) rover, nicknamed Curiosity, which landed on Mars at Gale Crater in August 2012.[34][35][36] Curiosity rover is currently probing the environment for past and present planetary habitability of microbial life on Mars. On 9 December 2013, NASA reported that, based on evidence from Curiosity studying Aeolis Palus, Gale Crater contained an ancient freshwater lake which could have been a hospitable environment for microbial life.[37][38]

The European Space Agency is currently collaborating with the Russian Federal Space Agency (Roscosmos) and developing the ExoMars astrobiology rover, which is to be launched in 2018.[39]

Methodology[edit]

Planetary habitability[edit]

When looking for life on other planets like the earth, some simplifying assumptions are useful to reduce the size of the task of the astrobiologist. One is to assume that the vast majority of life forms in our galaxy are based on carbon chemistries, as are all life forms on Earth.[40] Carbon is well known for the unusually wide variety of molecules that can be formed around it. Carbon is the fourth most abundant element in the universe and the energy required to make or break a bond is just at an appropriate level for building molecules which are not only stable, but also reactive. The fact that carbon atoms bond readily to other carbon atoms allows for the building of arbitrarily long and complex molecules.

The presence of liquid water is a useful assumption, as it is a common molecule and provides an excellent environment for the formation of complicated carbon-based molecules that could eventually lead to the emergence of life.[41] Some researchers posit environments of ammonia, or more likely, water-ammonia mixtures.[42]

A third assumption is to focus on sun-like stars. This comes from the idea of planetary habitability.[43] Very big stars have relatively short lifetimes, meaning that life would not likely 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.[44] Without a thick atmosphere, one side of the planet would be perpetually baked and the other perpetually frozen. In 2005, the question was brought back to the attention of the scientific community, as the long lifetimes of red dwarfs could allow some biology on planets with thick atmospheres. This is significant, as red dwarfs are extremely common. (See Habitability of red dwarf systems).

It is estimated that 10% of the stars in our galaxy are sun-like; there are about a thousand such stars within 100 light-years of our Sun. These stars would be useful primary targets for interstellar listening. Since Earth is the only planet known to harbor life, there is no evident way to know if any of the simplifying assumptions are correct.

Communication attempts[edit]

The illustration on the Pioneer plaque

Research on communication with extraterrestrial intelligence (CETI) focuses on composing and deciphering messages that could theoretically be understood by another technological civilization. Communication attempts by humans have included broadcasting mathematical languages, pictorial systems such as the Arecibo message and computational approaches to detecting and deciphering 'natural' language communication. The SETI program, for example, uses both radio telescopes and optical telescopes to search for deliberate signals from extraterrestrial intelligence.

While some high-profile scientists, such as Carl Sagan, have advocated the transmission of messages,[45][46] scientist Stephen Hawking has warned against it, suggesting that aliens might simply raid Earth for its resources and then move on.[47]

Elements of astrobiology[edit]

Astronomy[edit]

Main article: Astronomy
Artist's impression of the extrasolar planet OGLE-2005-BLG-390Lb orbiting its star 20,000 light-years from Earth; this planet was discovered with gravitational microlensing.
The NASA Kepler mission, launched in March 2009, searches for extrasolar planets.

Most astronomy-related astrobiological research falls into the category of extrasolar planet (exoplanet) detection, the hypothesis being that if life arose on Earth, then it could also arise on other planets with similar characteristics. To that end, a number of instruments designed to detect Earth-sized exoplanets have been considered, most notably NASA's Terrestrial Planet Finder (TPF) and ESA's Darwin programs, both of which have been cancelled. Additionally, NASA has launched the Kepler mission in March 2009, and the French Space Agency has launched the COROT space mission in 2006.[48][49] There are also several less ambitious ground-based efforts underway. (See exoplanet).

The goal of these missions is not only to detect Earth-sized planets, but also to directly detect light from the planet so that it may be studied spectroscopically. By examining planetary spectra, it would be possible to determine the basic composition of an extrasolar planet's atmosphere and/or surface; given this knowledge, it may be possible to assess the likelihood of life being found on that planet. A NASA research group, the Virtual Planet Laboratory,[50] is using computer modeling to generate a wide variety of virtual planets to see what they would look like if viewed by TPF or Darwin. It is hoped that once these missions come online, their spectra can be cross-checked with these virtual planetary spectra for features that might indicate the presence of life. The photometry temporal variability of extrasolar planets may also provide clues to their surface and atmospheric properties.

An estimate for the number of planets with intelligent extraterrestrial life can be gleaned from the Drake equation, essentially an equation expressing the probability of intelligent life as the product of factors such as the fraction of planets that might be habitable and the fraction of planets on which life might arise:[51]

N = R^{*} ~ \times ~ f_{p} ~ \times ~ n_{e} ~ \times ~ f_{l} ~ \times ~ f_{i} ~ \times ~ f_{c} ~ \times ~ L

where:

  • N = The number of communicative civilizations
  • R* = The rate of formation of suitable stars (stars such as our Sun)
  • fp = The fraction of those stars with planets (current evidence indicates that planetary systems may be common for stars like the Sun)
  • ne = The number of Earth-sized worlds per planetary system
  • fl = The fraction of those Earth-sized planets where life actually develops
  • fi = The fraction of life sites where intelligence develops
  • fc = The fraction of communicative planets (those on which electromagnetic communications technology develops)
  • L = The "lifetime" of communicating civilizations

However, whilst the rationale behind the equation is sound, it is unlikely that the equation will be constrained to reasonable error limits any time soon. The first term, N, Number of Stars, is generally constrained within a few orders of magnitude. The second and third terms, fp, Stars with Planets and fe, Planets with Habitable Conditions, are being evaluated for the sun's neighborhood. The problem with the formula is that it is not usable to generate or support hypotheses because it contains units that can never be verified. Drake originally formulated the equation merely as an agenda for discussion at the Green Bank conference,[52] but some applications of the formula had been taken literally and related to simplistic or pseudoscientific arguments.[53] Another associated topic is the Fermi paradox, which suggests that if intelligent life is common in the universe, then there should be obvious signs of it. This is the purpose of projects like SETI, which tries to detect signs of radio transmissions from intelligent extraterrestrial civilizations.

Another active research area in astrobiology is planetary system formation. It has been suggested that the peculiarities of our Solar System (for example, the presence of Jupiter as a protective shield)[54] may have greatly increased the probability of intelligent life arising on our planet.[55][56] No firm conclusions have been reached so far.

Biology[edit]

Hydrothermal vents are able to support extremophile bacteria on Earth and may also support life in other parts of the cosmos.

Unlike in physics, biology cannot state that a process or phenomenon, by being mathematically possible, have to exist forcibly in an extraterrestrial body. Biologists specify what is speculative and what is not.[53]

Until the 1970s, life was thought to be entirely dependent on energy from the Sun. Plants on Earth's surface capture energy from sunlight to photosynthesize sugars from carbon dioxide and water, releasing oxygen in the process, and are then eaten by oxygen-respiring animals, passing their energy up the food chain. Even life in the ocean depths, where sunlight cannot reach, was thought to obtain its nourishment either from consuming organic detritus rained down from the surface waters or from eating animals that did.[57] A world's ability to support life was thought to depend on its access to sunlight. However, in 1977, during an exploratory dive to the Galapagos Rift in the deep-sea exploration submersible Alvin, scientists discovered colonies of giant tube worms, clams, crustaceans, mussels, and other assorted creatures clustered around undersea volcanic features known as black smokers.[57] These creatures thrive despite having no access to sunlight, and it was soon discovered that they comprise an entirely independent food chain. Instead of plants, the basis for this food chain is a form of bacterium that derives its energy from oxidization of reactive chemicals, such as hydrogen or hydrogen sulfide, that bubble up from the Earth's interior. This chemosynthesis revolutionized the study of biology by revealing that life need not be sun-dependent; it only requires water and an energy gradient in order to exist.

Extremophiles (organisms able to survive in extreme environments) are a core research element for astrobiologists. Such organisms include biota which are able to survive several kilometers below the ocean's surface near hydrothermal vents and microbes that thrive in highly acidic environments.[58] It is now known that extremophiles thrive in ice, boiling water, acid, the water core of nuclear reactors, salt crystals, toxic waste and in a range of other extreme habitats that were previously thought to be inhospitable for life.[59] It opened up a new avenue in astrobiology by massively expanding the number of possible extraterrestrial habitats. Characterization of these organisms—their environments and their evolutionary pathways—is considered a crucial component to understanding how life might evolve elsewhere in the universe. According to astrophysicist Dr. Steinn Sigurdsson, "There are viable bacterial spores that have been found that are 40 million years old on Earth - and we know they're very hardened to radiation."[60] Some organisms able to withstand exposure to the vacuum and radiation of space include the lichen fungi Rhizocarpon geographicum and Xanthoria elegans,[61] the bacterium Bacillus safensis,[62] Deinococcus radiodurans,[62] Bacillus subtilis,[62] yeast Saccharomyces cerevisiae,[62] seeds from Arabidopsis thaliana ('mouse-ear cress'),[62] as well as the invertebrate animal Tardigrade.[62] On 29 April 2013, French scientists, funded by NASA, reported that, during spaceflight, microbes (like Pseudomonas aeruginosa) seem to adapt to the space environment in ways "not observed on Earth" and can increase in "virulence".[63] On 27 June 2011, it was reported that a new E. coli bacterium was produced from an engineered DNA in which approximately 90% of its thymine was replaced with the synthetic building block 5-chlorouracil, a substance "toxic to other organisms".[64][65]

Jupiter's moon, Europa,[59][66][67][68][69][70] and Saturn's moon, Enceladus,[71][72] are now considered the most likely locations for extant extraterrestrial life in the solar system.

The origin of life, known as abiogenesis, distinct from the evolution of life, is another ongoing field of research. Oparin and Haldane postulated that the conditions on the early Earth were conducive to the formation of organic compounds from inorganic elements and thus to the formation of many of the chemicals common to all forms of life we see today. The study of this process, known as prebiotic chemistry, has made some progress, but it is still unclear whether or not life could have formed in such a manner on Earth. The alternative hypothesis of panspermia is that the first elements of life may have formed on another planet with even more favorable conditions (or even in interstellar space, asteroids, etc.) and then have been carried over to Earth by a variety of means. Somewhat related to such a hypothesis, two scientists reported studies that life began 9.7±2.5 billion years ago, billions of years before the Earth was formed, based on extrapolating the "genetic complexity of organisms" (from 5 selected extant genomes) to earlier times.[73] However, the peer review was unanimous that the study was deeply flawed and stated the "paper is an example of how not to analyze data."[74] (also see Abiogenesis#Primitive extraterrestrial life and Panspermia#Complexity)

In October 2011, scientists found that the cosmic dust permeating the universe contains complex organic matter ("amorphous organic solids with a mixed aromatic-aliphatic structure") that could be created naturally, and rapidly, by stars.[75][76][77] As one of the scientists noted, "Coal and kerogen are products of life and it took a long time for them to form ... How do stars make such complicated organics under seemingly unfavorable conditions and [do] it so rapidly?"[75] Further, the scientist suggested that these compounds may have been related to the development of life on earth and said that, "If this is the case, life on Earth may have had an easier time getting started as these organics can serve as basic ingredients for life."[75] In September 2012, NASA scientists reported that polycyclic aromatic hydrocarbons (PAHs), subjected to interstellar medium (ISM) conditions, are transformed, through hydrogenation, oxygenation and hydroxylation, to more complex organics - "a step along the path toward amino acids and nucleotides, the raw materials of proteins and DNA, respectively".[78][79] Further, as a result of these transformations, the PAHs lose their spectroscopic signature which could be one of the reasons "for the lack of PAH detection in interstellar ice grains, particularly the outer regions of cold, dense clouds or the upper molecular layers of protoplanetary disks."[78][79]

On 29 August 2012, and in a world first, astronomers at Copenhagen University reported the detection of a specific sugar molecule, glycolaldehyde, in a distant star system. The molecule was found around the protostellar binary IRAS 16293-2422, which is located 400 light years from Earth.[80][81] Glycolaldehyde is needed to form ribonucleic acid, or RNA, which is similar in function to DNA. This finding suggests that complex organic molecules may form in stellar systems prior to the formation of planets, eventually arriving on young planets early in their formation.[82]

On 21 February 2014, NASA announced a greatly upgraded database for tracking polycyclic aromatic hydrocarbons (PAHs) in the universe. According to scientists, more than 20% of the carbon in the universe may be associated with PAHs, possible starting materials for the formation of life. PAHs seem to have been formed shortly after the Big Bang, are widespread throughout the universe, and are associated with new stars and exoplanets.[83]

Astroecology[edit]

Main article: Astroecology

Astroecology concerns the interactions of life with space environments and resources, in planets, asteroids and comets. On a larger scale, astroecology concerns resources for life about stars in the galaxy through the cosmological future. Astroecology attempts to quantify future life in space, addressing this area of astrobiology.

Experimental astroecology investigates resources in planetary soils, using actual space materials in meteorites.[84] The results suggest that Martian and carbonaceous chondrite materials can support bacteria, algae and plant (asparagus, potato) cultures, with high soil fertilities. The results support that life could have survived in early aqueous asteroids and on similar materials imported to Earth by dust, comets and meteorites, and that such asteroid materials can be used as soil for future space colonies.[84][85]

On the largest scale, cosmoecology concerns life in the universe over cosmological times. The main sources of energy may be red giant stars and white and red dwarf stars, sustaining life for 1020 years.[84][84][86] Astroecologists suggest that their mathematical models may quantify the immense potential amounts of future life in space, allowing a comparable expansion in biodiversity, potentially leading to diverse intelligent life-forms.[87]

Astrogeology[edit]

Astrogeology is a planetary science discipline concerned with the geology of the celestial bodies such as the planets and their moons, asteroids, comets, and meteorites. The information gathered by this discipline allows the measure of a planet's or a natural satellite's potential to develop and sustain life, or planetary habitability.

An additional discipline of astrogeology is geochemistry, which involves study of the chemical composition of the Earth and other planets, chemical processes and reactions that govern the composition of rocks and soils, the cycles of matter and energy and their interaction with the hydrosphere and the atmosphere of the planet. Specializations include cosmochemistry, biochemistry and organic geochemistry.

The fossil record provides the oldest known evidence for life on Earth.[88] By examining the fossil evidence, paleontologists are able to better understand the types of organisms that arose on the early Earth. Some regions on Earth, such as the Pilbara in Western Australia and the McMurdo Dry Valleys of Antarctica, are also considered to be geological analogs to regions of Mars, and as such, might be able to provide clues on how to search for past life on Mars.

Consistent with the above, the earliest evidence for life on Earth are graphite found to be biogenic in 3.7 billion-year-old metasedimentary rocks discovered in Western Greenland[89] and microbial mat fossils found in 3.48 billion-year-old sandstone discovered in Western Australia.[90][91] Nonetheless, several studies suggest that life on Earth may have started even earlier, as early as 4.25 billion years ago according to one study.[92][93][94]

Life in the Solar System[edit]

Europa, due to the ocean that exists under its icy surface, might host some form of microbial life.

People have long speculated about the possibility of life in settings other than Earth, however, speculation on the nature of life elsewhere often has paid little heed to constraints imposed by the nature of biochemistry.[95] The likelihood that life throughout the universe is probably carbon-based is encouraged by the fact that carbon is one of the most abundant of the higher elements. Only two of the natural atoms, carbon and silicon, are known to serve as the backbones of molecules sufficiently large to carry biological information. As the structural basis for life, one of carbon's important features is that unlike silicon it can readily engage in the formation of chemical bonds with many other atoms, thereby allowing for the chemical versatility required to conduct the reactions of biological metabolism and propagation.

The various organic functional groups, composed of hydrogen, oxygen, nitrogen, phosphorus, sulfur, and a host of metals, such as iron, magnesium, and zinc, provide the enormous diversity of chemical reactions necessarily catalyzed by a living organism. Silicon, in contrast, interacts with only a few other atoms, and the large silicon molecules are monotonous compared with the combinatorial universe of organic macromolecules.[53][95] Indeed, it seems likely that the basic building blocks of life anywhere will be similar to our own, in the generality if not in the detail.[95] Although terrestrial life and life that might arise independently of Earth are expected to use many similar, if not identical, building blocks, they also are expected to have some biochemical qualities that are unique. If life has had a comparable impact elsewhere in the solar system, the relative abundances of chemicals key for its survival - whatever they may be - could betray its presence. Whatever extraterrestrial life may be, its tendency to chemically alter its environment might just give it away.[96]

Thought on where in the Solar System life might occur was limited historically by the belief that life relies ultimately on light and warmth from the Sun and, therefore, is restricted to the surfaces of planets.[95] The three most likely candidates for life in the Solar System are the planet Mars, the Jovian moon Europa, and Saturn's moon Titan.[97][98][99][100][101] More recently, Saturn's moon Enceladus may be considered a likely candidate as well.[72][102] This speculation of likely candidates of life is primarily based on the fact that (in the cases of Mars and Europa) the planetary bodies may have liquid water, a molecule essential for life as we know it, for its use as a solvent in cells.[31]

Water on Mars is found in its polar ice caps, and newly carved gullies recently observed on Mars suggest that liquid water may exist, at least transiently, on the planet's surface.[103][104] At the Martian low temperatures and low pressure, liquid water is likely to be highly saline.[105] As for Europa, liquid water likely exists beneath the moon's icy outer crust.[67][97][98] This water may be warmed to a liquid state by volcanic vents on the ocean floor (an especially intriguing theory considering the various types of extremophiles that live near Earth's volcanic vents), but the primary source of heat is probably tidal heating.[106] On 11 December 2013, NASA reported the detection of "clay-like minerals" (specifically, phyllosilicates), often associated with organic materials, on the icy crust of Europa.[107] The presence of the minerals may have been the result of a collision with an asteroid or comet according to the scientists.[107]

Another planetary body that could potentially sustain extraterrestrial life is Saturn's largest moon, Titan.[101] Titan has been described as having conditions similar to those of early Earth.[108] On its surface, scientists have discovered the first liquid lakes outside Earth, but they seem to be composed of ethane and/or methane, not water.[109] After Cassini data was studied, it was reported on March 2008 that Titan may also have an underground ocean composed of liquid water and ammonia.[110] Additionally, Saturn's moon Enceladus may have an ocean below its icy surface[111] and, according to NASA scientists in May 2011, "is emerging as the most habitable spot beyond Earth in the Solar System for life as we know it".[72][102]

On 26 April 2012, scientists reported that lichen survived and showed remarkable results on the adaptation capacity of photosynthetic activity within the simulation time of 34 days under Martian conditions in the Mars Simulation Laboratory (MSL) maintained by the German Aerospace Center (DLR).[112][113] In June, 2012, scientists reported that measuring the ratio of hydrogen and methane levels on Mars may help determine the likelihood of life on Mars.[114][115] According to the scientists, "...low H2/CH4 ratios (less than approximately 40) indicate that life is likely present and active."[114] Other scientists have recently reported methods of detecting hydrogen and methane in extraterrestrial atmospheres.[116][117]

On 11 August 2014, astronomers released studies, using the Atacama Large Millimeter/Submillimeter Array (ALMA) for the first time, that detailed the distribution of HCN, HNC, H2CO, and dust inside the comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON).[118][119]

Rare Earth hypothesis[edit]

Main article: Rare Earth hypothesis

This hypothesis states that based on astrobiological findings, multi-cellular life forms found on Earth may actually be more of a rarity than scientists initially assumed. It provides a possible answer to the Fermi paradox which suggests, "If extraterrestrial aliens are common, why aren't they obvious?" It is apparently in opposition to the principle of mediocrity, assumed by famed astronomers Frank Drake, Carl Sagan, and others. The Principle of Mediocrity suggests that life on Earth is not exceptional, but rather that life is more than likely to be found on innumerable other worlds.

The anthropic principle states that fundamental laws of the universe work specifically in a way that life would be possible. The anthropic principle supports the Rare Earth Hypothesis by arguing the overall elements that are needed to support life on Earth are so fine-tuned that it is nearly impossible for another just like it to exist by random chance (note that these terms are used by scientists in a different way from the vernacular conception of them). However, Stephen Jay Gould compared the claim that the universe is fine-tuned for the benefit of our kind of life to saying that sausages were made long and narrow so that they could fit into modern hot dog buns, or saying that ships had been invented to house barnacles.[120][121]

Research[edit]

The systematic search for possible life outside Earth is a valid multidisciplinary scientific endeavor.[122] The University of Glamorgan, UK, started just such a degree in 2006,[28] and the American government funds the NASA Astrobiology Institute. However, characterization of non-Earth life is unsettled; hypotheses and predictions as to its existence and origin vary widely, but at the present, the development of theories to inform and support the exploratory search for life may be considered astrobiology's most concrete practical application.

Biologist Jack Cohen and mathematician Ian Stewart, amongst others, consider xenobiology separate from astrobiology. Cohen and Stewart stipulate that astrobiology is the search for Earth-like life outside our solar system and say that xenobiologists are concerned with the possibilities open to us once we consider that life need not be carbon-based or oxygen-breathing, so long as it has the defining characteristics of life. (See carbon chauvinism).

Research outcomes[edit]

Asteroid(s) may have transported life to Earth.

As of 2014, no evidence of extraterrestrial life has been identified. Examination of the Allan Hills 84001 meteorite, which was recovered in Antarctica in 1984 and originated from Mars, is thought by David McKay, Chief Scientist for Astrobiology at NASA's Johnson Space Center, as well as other scientists, to contain microfossils of extraterrestrial origin; this interpretation is controversial.[123][124][125]

Yamato 000593 is the second largest meteorite from Mars, and was found on Earth in 2000. At a microscopic level, spheres are found in the meteorite that are rich in carbon compared to surrounding areas that lack such spheres. The carbon-rich spheres may have been formed by biotic activity according to NASA scientists.[126][127][128]

On 5 March 2011, Richard B. Hoover, a scientist with the Marshall Space Flight Center, speculated on the finding of alleged microfossils similar to cyanobacteria in CI1 carbonaceous meteorites.[129][130] However, NASA formally distanced itself from Hoover's claim.[131][132][133] According to American astrophysicist Neil deGrasse Tyson: "At the moment, life on Earth is the only known life in the Universe, but there are compelling arguments to suggest we are not alone."[134]

Extreme environments on the Earth

On 17 March 2013, researchers reported data that suggested microbial life forms thrive in the Mariana Trench, the deepest spot on the Earth.[135][136] Other researchers reported related studies that microbes thrive inside rocks up to 1900 feet below the sea floor under 8500 feet of ocean off the coast of the northwestern United States.[135][137] According to one of the researchers,"You can find microbes everywhere — they're extremely adaptable to conditions, and survive wherever they are."[135]

Methane

In 2004, the spectral signature of methane was detected in the Martian atmosphere by both Earth-based telescopes as well as by the Mars Express probe. Because of solar radiation and cosmic radiation, methane is predicted to disappear from the Martian atmosphere within several years, so the gas must be actively replenished in order to maintain the present concentration.[138][139] The Mars Science Laboratory rover will perform precision measurements of oxygen and carbon isotope ratios in carbon dioxide (CO2) and methane (CH4) in the atmosphere of Mars in order to distinguish between a geochemical and a biological origin.[140][141][142]

Planetary systems

It is possible that some planets, like the gas giant Jupiter in our solar system, may have moons with solid surfaces or liquid oceans that are more hospitable. Most of the planets so far discovered outside our solar system are hot gas giants thought to be inhospitable to life, so it is not yet known whether our solar system, with a warm, rocky, metal-rich inner planet such as Earth, is of an aberrant composition. Improved detection methods and increased observing time will undoubtedly discover more planetary systems, and possibly some more like ours. For example, NASA's Kepler Mission seeks to discover Earth-sized planets around other stars by measuring minute changes in the star's light curve as the planet passes between the star and the spacecraft. Progress in infrared astronomy and submillimeter astronomy has revealed the constituents of other star systems. Infrared searches have detected belts of dust and asteroids around distant stars, underpinning the formation of planets.

Planetary habitability

Efforts to answer questions such as the abundance of potentially habitable planets in habitable zones and chemical precursors have had much success. Numerous extrasolar planets have been detected using the wobble method and transit method, showing that planets around other stars are more numerous than previously postulated. The first Earth-sized extrasolar planet to be discovered within its star's habitable zone is Gliese 581 c, which was found using radial velocity.[143]

Missions[edit]

Research into the environmental limits of life and the workings of extreme ecosystems is ongoing, enabling researchers to better predict what planetary environments might be most likely to harbor life. Missions such as the Phoenix lander, Mars Science Laboratory, ExoMars to Mars, and the Cassini probe to Saturn's moon Titan hope to further explore the possibilities of life on other planets in our solar system.

Viking program[edit]

Carl Sagan posing with a model of the Viking Lander.

The two Viking spacecraft each carried four types of biological experiments to the surface of Mars in the late 1970s. These were the only Mars landers to carry out experiments to look specifically for biosignatures of life on Mars. The landers used a robotic arm to put soil samples into sealed test containers on the craft. The two landers were identical, so the same tests were carried out at two places on Mars' surface; Viking 1 near the equator and Viking 2 further north.[144] The result was inconclusive,[145] and is still disputed by some scientists.[146][147][148][149]

Beagle 2[edit]

Main article: Beagle 2
Replica of the 33.2 kg Beagle-2 lander
Mars Science Laboratory rover concept artwork

Beagle 2 was an unsuccessful British Mars lander that formed part of the European Space Agency's 2003 Mars Express mission. Its primary purpose was to search for signs of life on Mars, past or present. All contact with it was lost upon its entry into the atmosphere.[150]

EXPOSE[edit]

Main article: EXPOSE

EXPOSE was a multi-user facility mounted in 2008 outside the International Space Station dedicated to astrobiology.[151][152] EXPOSE was developed by the European Space Agency (ESA) for long-term spaceflights that allowed to expose organic chemicals and biological samples to outer space for one and a half years in low Earth orbit.[153]

Mars Science Laboratory[edit]

The Mars Science Laboratory (MSL) mission landed a rover that is currently in operation on Mars.[154] It was launched 26 November 2011, and landed at Gale Crater on 6 August 2012.[36] Mission objectives are to help assess Mars' habitability and in doing so, determine whether Mars is or has ever been able to support life,[155] collect data for a future manned mission, study Martian geology, its climate, and further assess the role that water, an essential ingredient for life as we know it, played in forming minerals on Mars.

ExoMars[edit]

Main article: ExoMars
ExoMars rover model

ExoMars is a robotic mission to Mars to search for possible biosignatures of Martian life, past or present. This astrobiological mission is currently under development by the European Space Agency (ESA) with likely collaboration by the Russian Federal Space Agency (Roscosmos); it is planned for a 2018 launch.[156][157][158]

Mars 2020 rover mission[edit]

The 'Mars 2020 rover mission' is a concept under study by NASA with a possible launch in 2020. It is intended to investigate astrobiologically relevant environments on Mars, investigate its surface geological processes and history, including the assessment of its past habitability and potential for preservation of biosignatures within accessible geological materials.[159] The Science Definition Team is proposing the rover collect and package as many as 31 samples of rock cores and soil for a later mission to bring back for more definitive analysis in laboratories on Earth. The rover could make measurements and technology demonstrations to help designers of a human expedition understand any hazards posed by Martian dust and demonstrate how to collect carbon dioxide (CO2), which could be a resource for making oxygen (O2) and rocket fuel. Improved precision landing technology that enhances the scientific value of robotic missions also will be critical for eventual human exploration on the surface.[160][161]

Red Dragon[edit]

Red Dragon is a proposed concept for a low-cost Mars lander mission that would utilize a SpaceX Falcon Heavy launch vehicle, and a modified Dragon capsule to enter the Martian atmosphere. The lander's primary mission would be to search for evidence of life on Mars (biosignatures), past or present. The concept had been scheduled to propose for funding on 2012/2013 as a NASA Discovery mission, for launch in 2018.[162][163]

Icebreaker Life[edit]

Main article: Icebreaker Life

Icebreaker Life is a lander mission that is being proposed for NASA's Discovery Program for the 2018 launch opportunity.[164] If selected and funded, the stationary lander would be a near copy of the successful 2008 Phoenix and it would carry an upgraded astrobiology scientific payload, including a 1 meter-long drill to sample ice-cemented ground in the northern plains to conduct a search for organic molecules and evidence of current or past life on Mars.[165][166] One of the key goals of the Icebreaker Life mission is to test the hypothesis that the ice-rich ground in the polar regions has significant concentrations of organics due to protection by the ice from oxidants and radiation.

Europa Clipper[edit]

Main article: Europa Clipper

Europa Clipper is a mission concept under study by NASA that would conduct detailed reconnaissance of Jupiter's moon Europa and would investigate whether the icy moon could harbor conditions suitable for life.[167][168] It would also aid in the selection of future landing sites.[169][170]

See also[edit]


References[edit]

  1. ^ "Launching the Alien Debates (part 1 of 7)". Astrobiology Magazine. NASA. 8 December 2006. Retrieved 5 May 2014. 
  2. ^ "How the search for aliens can help sustain life on Earth". CNN News. 4 October 2012. Retrieved 8 October 2012. 
  3. ^ a b "About Astrobiology". NASA Astrobiology Institute. NASA. 21 January 2008. Archived from the original on 11 October 2008. Retrieved 20 October 2008. 
  4. ^ Mirriam Webster Dictionary entry "Exobiology" (accessed 11 April 2013)
  5. ^ iTWire - Scientists will look for alien life, but Where and How?
  6. ^ Ward, P. D.; Brownlee, D. (2004). The life and death of planet Earth. New York: Owl Books. ISBN 0-8050-7512-7. 
  7. ^ Graham, Robert W. (February 1990). "NASA Technical Memorandum 102363 - Extraterrestrial Life in the Universe" (PDF). NASA (Lewis Research Center, Ohio). Retrieved July 7, 2014. 
  8. ^ Altermann, Wladyslaw (2008). "From Fossils to Astrobiology - A Roadmap to Fata Morgana?". In Seckbach, Joseph; Walsh, Maud. From Fossils to Astrobiology: Records of Life on Earth and the Search for Extraterrestrial Biosignatures 12. p. xvii. ISBN 1-4020-8836-1. 
  9. ^ Horneck, Gerda; Petra Rettberg (2007). Complete Course in Astrobiology. Wiley-VCH. ISBN 3-527-40660-3. 
  10. ^ Davies, Paul (18 November 2013). "Are We Alone in the Universe?". New York Times. Retrieved 20 November 2013. 
  11. ^ a b Overbye, Dennis (4 November 2013). "Far-Off Planets Like the Earth Dot the Galaxy". New York Times. Retrieved 5 November 2013. 
  12. ^ a b Petigura, Eric A.; Howard, Andrew W.; Marcy, Geoffrey W. (31 October 2013). "Prevalence of Earth-size planets orbiting Sun-like stars". Proceedings of the National Academy of Sciences of the United States of America. arXiv:1311.6806. Bibcode:2013PNAS..11019273P. doi:10.1073/pnas.1319909110. Retrieved 5 November 2013. 
  13. ^ Khan, Amina (4 November 2013). "Milky Way may host billions of Earth-size planets". Los Angeles Times. Retrieved 5 November 2013. 
  14. ^ Griffin, Dale Warren (14 August 2013). "The Quest for Extraterrestrial Life: What About the Viruses?". Astrobiology (journal) 13 (8): 774–783. Bibcode:2013AsBio..13..774G. doi:10.1089/ast.2012.0959. Retrieved 6 September 2013. 
  15. ^ a b Grotzinger, John P. (24 January 2014). "Introduction to Special Issue - Habitability, Taphonomy, and the Search for Organic Carbon on Mars". Science 343 (6169): 386–387. Bibcode:2014Sci...343..386G. doi:10.1126/science.1249944. Retrieved 24 January 2014. 
  16. ^ Various (24 January 2014). "Special Issue - Table of Contents - Exploring Martian Habitability". Science 343 (6169): 345–452. Retrieved 24 January 2014. 
  17. ^ Various (24 January 2014). "Special Collection - Curiosity - Exploring Martian Habitability". Science. Retrieved 24 January 2014. 
  18. ^ Grotzinger, J.P. et al. (24 January 2014). "A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars". Science 343 (6169). doi:10.1126/science.1242777. Retrieved 24 January 2014. 
  19. ^ Gutro, Robert (4 November 2007). "NASA Predicts Non-Green Plants on Other Planets". Goddard Space Flight Center. Archived from the original on 6 October 2008. Retrieved 20 October 2008. 
  20. ^ Heinlein R and Harold W (21 July 1961). "Xenobiology". Science 134 (3473): 223, 225. Bibcode:1961Sci...134..223H. doi:10.1126/science.134.3473.223. JSTOR 1708323. 
  21. ^ Markus Schmidt (9 March 2010). "Xenobiology: A new form of life as the ultimate biosafety tool". BioEssays 32 (4): 322–331. doi:10.1002/bies.200900147. PMC 2909387. PMID 20217844. 
  22. ^ Grinspoon 2004
  23. ^ Steven J. Dick and James E. Strick (2004). The Living Universe: NASA and the Development of Astrobiology. New Brunswick, NJ: Rutgers University Press. 
  24. ^ Jack D. Famer, David J. Des Marais, and Ronald Greeley; Des Marais; Greeley (5 September 1996). "Exopaleontology at the Pathfinder Landing Site". Abstracts of the Lunar and Planetary Science Conference (NASA Ames Research Center) 26: 393. Bibcode:1995LPI....26..393F. Retrieved 21 November 2009. 
  25. ^ "First European Workshop on Exo/Astrobiology". ESA Press Release. European Space Agency. 2001. Retrieved 20 October 2008. 
  26. ^ Gavaghan, H. (1 June 2001). "ESA Embraces Astrobiology". Science 292 (5522): 1626–1627. doi:10.1126/science.292.5522.1626. PMID 11387447. 
  27. ^ Astrobiology at Arizona State University
  28. ^ a b CASE Undergraduate Degrees
  29. ^ The Australian Centre for Astrobiology, University of New South Wales
  30. ^ Commission 51: Bioastronomy
  31. ^ a b NOVA | Mars | Life's Little Essential | PBS
  32. ^ Klein HP and Levin GV (1 October 1976). "The Viking Biological Investigation: Preliminary Results". Science 194 (4260): 99–105. Bibcode:1976Sci...194...99K. doi:10.1126/science.194.4260.99. PMID 17793090. Retrieved 15 August 2008. 
  33. ^ "Possible evidence found for Beagle 2 location". European Space Agency. 21 December 2005. Archived from the original on 30 September 2008. Retrieved 18 August 2008. 
  34. ^ Webster, Guy; Brown, Dwayne (22 July 2011). "NASA's Next Mars Rover To Land At Gale Crater". NASA JPL. Retrieved 22 July 2011. 
  35. ^ Chow, Dennis (22 July 2011). "NASA's Next Mars Rover to Land at Huge Gale Crater". Space.com. Retrieved 22 July 2011. 
  36. ^ a b Amos, Jonathan (22 July 2011). "Mars rover aims for deep crater". BBC News. Archived from the original on 22 July 2011. Retrieved 22 July 2011. 
  37. ^ Chang, Kenneth (9 December 2013). "On Mars, an Ancient Lake and Perhaps Life". New York Times. Retrieved 9 December 2013. 
  38. ^ Various (9 December 2013). "Science - Special Collection - Curiosity Rover on Mars". Science. Retrieved 9 December 2013. 
  39. ^ "ExoMars: ESA and Roscosmos set for Mars missions". European Space Agency (ESA). 14 March 2013. Retrieved 14 March 2013. 
  40. ^ "Polycyclic Aromatic Hydrocarbons: An Interview With Dr. Farid Salama". Astrobiology magazine. 2000. Retrieved 20 October 2008. 
  41. ^ "Astrobiology". Macmillan Science Library: Space Sciences. 2006. Retrieved 20 October 2008. 
  42. ^ "The Ammonia-Oxidizing Gene". Astrobiology Magazine. 19 August 2006. Retrieved 20 October 2008. 
  43. ^ "Stars and Habitable Planets". Sol Company. 2007. Archived from the original on 1 October 2008. Retrieved 20 October 2008. 
  44. ^ "M Dwarfs: The Search for Life is On". Red Orbit & Astrobiology Magazine. 29 August 2005. Retrieved 20 October 2008. 
  45. ^ Sagan, Carl. Communication with Extraterrestrial Intelligence. MIT Press, 1973, 428 pgs.
  46. ^ An Awkward History of Our Space Transmissions
  47. ^ Don’t talk to aliens, warns Stephen Hawking. (25 April 2010)
  48. ^ "Kepler Mission". NASA. 2008. Archived from the original on 31 October 2008. Retrieved 20 October 2008. 
  49. ^ "The COROT space telescope". CNES. 17 October 2008. Archived from the original on 8 November 2008. Retrieved 20 October 2008. 
  50. ^ "The Virtual Planet Laboratory". NASA. 2008. Retrieved 20 October 2008. 
  51. ^ Ford, Steve (August 1995). "What is the Drake Equation?". SETI League. Archived from the original on 29 October 2008. Retrieved 20 October 2008. 
  52. ^ Amir Alexander. "The Search for Extraterrestrial Intelligence: A Short History - Part 7: The Birth of the Drake Equation". 
  53. ^ a b c "Astrobiology". Biology Cabinet. 26 September 2006. Archived from the original on 12 December 2010. Retrieved 17 January 2011. 
  54. ^ Horner, Jonathan; Barrie Jones (24 August 2007). "Jupiter: Friend or foe?". Europlanet. Retrieved 20 October 2008. 
  55. ^ Jakosky, Bruce; David Des Marais, et al. (14 September 2001). "The Role Of Astrobiology in Solar System Exploration". NASA. SpaceRef.com. Retrieved 20 October 2008. 
  56. ^ Bortman, Henry (29 September 2004). "Coming Soon: "Good" Jupiters". Astrobiology Magazine. Retrieved 20 October 2008. 
  57. ^ a b Chamberlin, Sean (1999). "Black Smokers and Giant Worms". Fullerton College. Retrieved 11 February 2011. 
  58. ^ Carey, Bjorn (7 February 2005). "Wild Things: The Most Extreme Creatures". Live Science. Retrieved 20 October 2008. 
  59. ^ a b Cavicchioli, R. (Fall 2002). "Extremophiles and the search for extraterrestrial life". Astrobiology 2 (3): 281–92. Bibcode:2002AsBio...2..281C. doi:10.1089/153110702762027862. PMID 12530238. 
  60. ^ BBC Staff (23 August 2011). "Impacts 'more likely' to have spread life from Earth". BBC. Retrieved 24 August 2011. 
  61. ^ Article: Lichens survive in harsh environment of outer space
  62. ^ a b c d e f The Planetary Report, Volume XXIX, number 2, March/April 2009, "We make it happen! Who will survive? Ten hardy organisms selected for the LIFE project, by Amir Alexander
  63. ^ Tengra FK et al. (29 April 2013). "Spaceflight Promotes Biofilm Formation by Pseudomonas aeruginosa". PLOS ONE 8 (4): e6237. Bibcode:2013PLoSO...862437K. doi:10.1371/journal.pone.0062437. Retrieved 5 July 2013. 
  64. ^ Marlière, Philippe; Patrouix, Julien; Döring, Volker; Herdewijn, Piet; Tricot, Sabine; Cruveiller, Stéphane; Bouzon, Madeleine; Mutzel, Rupert (27 June 2011). "Chemical Evolution of a Bacterium's Genome". Angewandte Chemie 50 (31): 7109. doi:10.1002/anie.201100535. 
  65. ^ Staff (29 June 2011). "Bacterium Engineered With DNA in Which Thymine Is Replaced by Synthetic Building Block". Science Daily. Retrieved 30 June 2011. 
  66. ^ "Jupiter's Moon Europa Suspected Of Fostering Life" (PDF). Daily University Science News. 2002. Retrieved 8 August 2009. 
  67. ^ a b Weinstock, Maia (24 August 2000). "Galileo Uncovers Compelling Evidence of Ocean On Jupiter's Moon Europa". Space.com. Retrieved 20 October 2008. 
  68. ^ Cavicchioli, R. (Fall 2002). "Extremophiles and the search for extraterrestrial life". Astrobiology 2 (3): 281–92. Bibcode:2002AsBio...2..281C. doi:10.1089/153110702762027862. PMID 12530238. 
  69. ^ David, Leonard (7 February 2006). "Europa Mission: Lost In NASA Budget". Space.com. Retrieved 8 August 2009. 
  70. ^ "Clues to possible life on Europa may lie buried in Antarctic ice". Marshal Space Flight Center (NASA). 5 March 1998. Archived from the original on 31 July 2009. Retrieved 8 August 2009. 
  71. ^ Lovett, Richard A. (31 May 2011). "Enceladus named sweetest spot for alien life". Nature (Nature). doi:10.1038/news.2011.337. Retrieved 3 June 2011. 
  72. ^ a b c Kazan, Casey (2 June 2011). "Saturn's Enceladus Moves to Top of "Most-Likely-to-Have-Life" List". The Daily Galaxy. Retrieved 3 June 2011. 
  73. ^ Sharov, Alexei A.; Gordon, Richard (28 March 2013). "Life Before Earth". arXiv. arXiv:1304.3381v1. Retrieved 16 April 2013. 
  74. ^ Sharov, Alexei A. (12 June 2006). "Genome increase as a clock for the origin and evolution of life". Biology Direct 1: 1–17. doi:10.1186/1745-6150-1-17. PMC 1526419. 
  75. ^ a b c Chow, Denise (26 October 2011). "Discovery: Cosmic Dust Contains Organic Matter from Stars". Space.com. Retrieved 26 October 2011. 
  76. ^ ScienceDaily Staff (26 October 2011). "Astronomers Discover Complex Organic Matter Exists Throughout the Universe". ScienceDaily. Retrieved 27 October 2011. 
  77. ^ Kwok, Sun; Zhang, Yong (26 October 2011). "Mixed aromatic–aliphatic organic nanoparticles as carriers of unidentified infrared emission features". Nature 479 (7371): 80–3. Bibcode:2011Natur.479...80K. doi:10.1038/nature10542. PMID 22031328. 
  78. ^ a b Staff (20 September 2012). "NASA Cooks Up Icy Organics to Mimic Life's Origins". Space.com. Retrieved 22 September 2012. 
  79. ^ a b Gudipati, Murthy S.; Yang, Rui (1 September 2012). "In-Situ Probing Of Radiation-Induced Processing Of Organics In Astrophysical Ice Analogs—Novel Laser Desorption Laser Ionization Time-Of-Flight Mass Spectroscopic Studies". The Astrophysical Journal Letters 756 (1): L24. Bibcode:2012ApJ...756L..24G. doi:10.1088/2041-8205/756/1/L24. Retrieved 22 September 2012. 
  80. ^ Than, Ker (29 August 2012). "Sugar Found In Space". National Geographic. Retrieved 31 August 2012. 
  81. ^ Staff (29 August 2012). "Sweet! Astronomers spot sugar molecule near star". AP News. Retrieved 31 August 2012. 
  82. ^ Jørgensen, J. K.; Favre, C.; Bisschop, S.; Bourke, T.; Dishoeck, E.; Schmalzl, M. (2012). "Detection of the simplest sugar, glycolaldehyde, in a solar-type protostar with ALMA". The Astrophysical Journal Letters. eprint 757: L4. arXiv:1208.5498. Bibcode:2012ApJ...757L...4J. doi:10.1088/2041-8205/757/1/L4. 
  83. ^ Hoover, Rachel (21 February 2014). "Need to Track Organic Nano-Particles Across the Universe? NASA's Got an App for That". NASA. Retrieved 22 February 2014. 
  84. ^ a b c d Mautner, Michael N. (2002). "Planetary bioresources and astroecology. 1. Planetary microcosm bioessays of Martian and meteorite materials: soluble electrolytes, nutrients, and algal and plant responses". Icarus 158: 72–86. Bibcode:2002Icar..158...72M. doi:10.1006/icar.2002.6841. PMID 12449855. 
  85. ^ Mautner, Michael N. (2002). "Planetary resources and astroecology. Planetary microcosm models of asteroid and meteorite interiors: electrolye solutions and microbial growth. Implications for space populations and panspermia". Astrobiology 2 (1): 59–76. Bibcode:2002Icar..158...72M. doi:10.1006/icar.2002.6841. PMID 12449855. 
  86. ^ Mautner, Michael N. (2005). "Life in the cosmological future: Resources, biomass and populations". Journal of the British Interplanetary Society 58: 167–180. Bibcode:2005JBIS...58..167M. 
  87. ^ Mautner, Michael N. (2000). Seeding the Universe with Life: Securing Our Cosmological Future. Washington D. C.: Legacy Books (www.amazon.com). ISBN 0-476-00330-X. 
  88. ^ "Fossil SUccession". U.S. Geological Survey. 14 August 1997. Archived from the original on 14 October 2008. Retrieved 20 October 2008. 
  89. ^ Yoko Ohtomo, Takeshi Kakegawa, Akizumi Ishida, Toshiro Nagase, Minik T. Rosing (8 December 2013). "Evidence for biogenic graphite in early Archaean Isua metasedimentary rocks". Nature Geoscience. doi:10.1038/ngeo2025. Retrieved 9 December 2013. 
  90. ^ Borenstein, Seth (13 November 2013). "Oldest fossil found: Meet your microbial mom". AP News. Retrieved 15 November 2013. 
  91. ^ Noffke, Nora; Christian, Daniel; Wacey, David; Hazen, Robert M. (8 November 2013). "Microbially Induced Sedimentary Structures Recording an Ancient Ecosystem in the ca. 3.48 Billion-Year-Old Dresser Formation, Pilbara, Western Australia". Astrobiology (journal). Bibcode:2013AsBio..13.1103N. doi:10.1089/ast.2013.1030. Retrieved 15 November 2013. 
  92. ^ Tenenbaum, David (October 14, 2002). "When Did Life on Earth Begin? Ask a Rock". Astrobiology Magazine. Retrieved April 13, 2014. 
  93. ^ Courtland, Rachel (July 2, 2008). "Did newborn Earth harbour life?". New Scientist. Retrieved April 13, 2014. 
  94. ^ Steenhuysen, Julie (May 20, 2009). "Study turns back clock on origins of life on Earth". Reuters. Retrieved April 13, 2014. 
  95. ^ a b c d Pace, Norman R. (30 January 2001). "The universal nature of biochemistry". Proceedings of the National Academy of Sciences of the USA 98 (3): 805–808. Bibcode:2001PNAS...98..805P. doi:10.1073/pnas.98.3.805. PMC 33372. PMID 11158550. Retrieved 20 March 2010. 
  96. ^ "Telltale chemistry could betray ET". New Scientists. 21 January 2011. Retrieved 22 January 2011. 
  97. ^ a b Tritt, Charles S. (2002). "Possibility of Life on Europa". MilwaukeeSchool of Engineering. Retrieved 20 October 2008. 
  98. ^ a b Friedman, Louis (14 December 2005). "Projects: Europa Mission Campaign". The Planetary Society. Archived from the original on 20 September 2008. Retrieved 20 October 2008. 
  99. ^ David, Leonard (10 November 1999). "Move Over Mars – Europa Needs Equal Billing". Space.com. Retrieved 20 October 2008. 
  100. ^ Than, Ker (28 February 2007). "New Instrument Designed to Sift for Life on Mars". Space.com. Retrieved 20 October 2008. 
  101. ^ a b Than, Ker (13 September 2005). "Scientists Reconsider Habitability of Saturn's Moon". Science.com. Retrieved 11 February 2011. 
  102. ^ a b Lovett, Richard A. (31 May 2011). "Enceladus named sweetest spot for alien life". Nature (Nature). doi:10.1038/news.2011.337. Retrieved 3 June 2011. 
  103. ^ "NASA Images Suggest Water Still Flows in Brief Spurts on Mars". NASA. 2006. Archived from the original on 16 October 2008. Retrieved 20 October 2008. 
  104. ^ "Water ice in crater at Martian north pole". European Space Agency. 28 July 2005. Archived from the original on 23 September 2008. Retrieved 20 October 2008. 
  105. ^ Landis, Geoffrey A. (1 June 2001). "Martian Water: Are There Extant Halobacteria on Mars?". Astrobiology 1 (2): 161–164. Bibcode:2001AsBio...1..161L. doi:10.1089/153110701753198927. PMID 12467119. Retrieved 20 October 2008. 
  106. ^ Kruszelnicki, Karl (5 November 2001). "Life on Europa, Part 1". ABC Science. Retrieved 20 October 2008. 
  107. ^ a b Cook, Jia-Rui c. (11 December 2013). "Clay-Like Minerals Found on Icy Crust of Europa". NASA. Retrieved 11 December 2013. 
  108. ^ "Titan: Life in the Solar System?". BBC - Science & Nature. Retrieved 20 October 2008. 
  109. ^ Britt, Robert Roy (28 July 2006). "Lakes Found on Saturn's Moon Titan". Space.com. Archived from the original on 4 October 2008. Retrieved 20 October 2008. 
  110. ^ Lovett, Richard A. (20 March 2008). "Saturn Moon Titan May Have Underground Ocean". National Geographic News. Archived from the original on 24 September 2008. Retrieved 20 October 2008. 
  111. ^ "Saturn moon 'may have an ocean'". BBC News. 10 March 2006. Retrieved 5 August 2008. 
  112. ^ Baldwin, Emily (26 April 2012). "Lichen survives harsh Mars environment". Skymania News. Retrieved 27 April 2012. 
  113. ^ de Vera, J.-P.; Kohler, Ulrich (26 April 2012). "The adaptation potential of extremophiles to Martian surface conditions and its implication for the habitability of Mars". European Geosciences Union. Retrieved 27 April 2012. 
  114. ^ a b Oze, Christopher; Jones, Camille; Goldsmith, Jonas I.; Rosenbauer, Robert J. (7 June 2012). "Differentiating biotic from abiotic methane genesis in hydrothermally active planetary surfaces". PNAS 109 (25): 9750–9754. Bibcode:2012PNAS..109.9750O. doi:10.1073/pnas.1205223109. PMC 3382529. PMID 22679287. Retrieved 27 June 2012. 
  115. ^ Staff (25 June 2012). "Mars Life Could Leave Traces in Red Planet's Air: Study". Space.com. Retrieved 27 June 2012. 
  116. ^ Brogi, Matteo; Snellen, Ignas A. G.; de Krok, Remco J.; Albrecht, Simon; Birkby, Jayne; de Mooij, Ernest J. W. (28 June 2012). "The signature of orbital motion from the dayside of the planet t Boötis b". Nature 486 (7404): 502–504. arXiv:1206.6109. Bibcode:2012Natur.486..502B. doi:10.1038/nature11161. Retrieved 28 June 2012. 
  117. ^ Mann, Adam (27 June 2012). "New View of Exoplanets Will Aid Search for E.T.". Wired (magazine). Retrieved 28 June 2012. 
  118. ^ Zubritsky, Elizabeth; Neal-Jones, Nancy (11 August 2014). "RELEASE 14-038 - NASA’s 3-D Study of Comets Reveals Chemical Factory at Work". NASA. Retrieved 12 August 2014. 
  119. ^ Cordiner, M.A. et al. (11 August 2014). "Mapping the Release of Volatiles in the Inner Comae of Comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON) Using the Atacama Large Millimeter/Submillimeter Array". The Astrophysical Journal 792 (1). doi:10.1088/2041-8205/792/1/L2. Retrieved 12 August 2014. 
  120. ^ Gould, Stephen Jay (1998). "Clear Thinking in the Sciences". Lectures at Harvard University. 
  121. ^ Gould, Stephen Jay (2002). Why People Believe Weird Things: Pseudoscience, Superstition, and Other Confusions of Our Time. 
  122. ^ NASA Astrobiology Institute
  123. ^ Crenson, Matt (6 August 2006). "Experts: Little Evidence of Life on Mars". Associated Press (on discovery.com). Archived from the original on 16 April 2011. Retrieved 8 March 2011. 
  124. ^ McKay DS, Gibson EK, ThomasKeprta KL, Vali H, Romanek CS, Clemett SJ, Chillier XDF, Maechling CR, Zare RN (1996). "Search for past life on Mars: Possible relic biogenic activity in Martian meteorite ALH84001". Science 273 (5277): 924–930. Bibcode:1996Sci...273..924M. doi:10.1126/science.273.5277.924. PMID 8688069. 
  125. ^ McKay DS, Thomas-Keprta KL, Clemett, SJ, Gibson, EK Jr, Spencer L, Wentworth SJ (2009). "Life on Mars: new evidence from martian meteorites". In Hoover, Richard B; Levin, Gilbert V; Rozanov, Alexei Y; Retherford, Kurt D. Proc. SPIE. Proceedings of SPIE 7441 (1): 744102. doi:10.1117/12.832317. Retrieved 8 March 2011. 
  126. ^ Webster, Guy (27 February 2014). "NASA Scientists Find Evidence of Water in Meteorite, Reviving Debate Over Life on Mars". NASA. Retrieved 27 February 2014. 
  127. ^ White, Lauren M.; Gibson, Everett K.; Thomnas-Keprta, Kathie L.; Clemett, Simon J.; McKay, David (19 February 2014). "Putative Indigenous Carbon-Bearing Alteration Features in Martian Meteorite Yamato 000593". Astrobiology 14 (2): 170–181. Bibcode:2014AsBio..14..170W. doi:10.1089/ast.2011.0733. Retrieved 27 February 2014. 
  128. ^ Gannon, Megan (28 February 2014). "Mars Meteorite with Odd 'Tunnels' & 'Spheres' Revives Debate Over Ancient Martian Life". Space.com. Retrieved 28 February 2014. 
  129. ^ Tenney, Garrett (5 March 2011). "Exclusive: NASA Scientist Claims Evidence of Alien Life on Meteorite". FoxNews. Archived from the original on 6 March 2011. Retrieved 6 March 2011. 
  130. ^ Hoover, Richard B. (2011). "Fossils of Cyanobacteria in CI1 Carbonaceous Meteorites: Implications to Life on Comets, Europa, and Enceladus". Journal of Cosmology 13: xxx. Retrieved 6 March 2011. 
  131. ^ "NASA shoots down alien fossil claims". ABC News. 7 March 2011. Retrieved 7 March 2011. 
  132. ^ Borenstein, Seth (7 March 2011). "Scientists skeptical of meteorite alien life claim". Associated Press (on Starnewsonline.com). Retrieved 7 March 2011. 
  133. ^ Redfield, Rosemary (6 March 2011). "Is this claim of bacteria in a meteorite any better than the 1996 one?". RR Research blog. Archived from the original on 8 March 2011. Retrieved 7 March 2011. 
  134. ^ "The Search for Life in the Universe". Department of Astrophysics and Hayden Planetarium. NASA. 23 July 2001. Retrieved 7 March 2011. 
  135. ^ a b c Choi, Charles Q. (17 March 2013). "Microbes Thrive in Deepest Spot on Earth". LiveScience. Retrieved 17 March 2013. 
  136. ^ Glud, Ronnie; Wenzhöfer, Frank; Middleboe, Mathias; Oguri, Kazumasa; Turnewitsch, Robert; Canfield, Donald E.; Kitazato, Hiroshi (17 March 2013). "High rates of microbial carbon turnover in sediments in the deepest oceanic trench on Earth". Nature Geoscience. Bibcode:2013NatGe...6..284G. doi:10.1038/ngeo1773. Retrieved 17 March 2013. 
  137. ^ Oskin, Becky (14 March 2013). "Intraterrestrials: Life Thrives in Ocean Floor". LiveScience. Retrieved 17 March 2013. 
  138. ^ Vladimir A. Krasnopolsky (February 2005). "Some problems related to the origin of methane on Mars". Icarus 180 (2): 359–367. Bibcode:2006Icar..180..359K. doi:10.1016/j.icarus.2005.10.015. 
  139. ^ Planetary Fourier Spectrometer website (ESA, Mars Express)
  140. ^ "Sample Analysis at Mars (SAM) Instrument Suite". NASA. October 2008. Archived from the original on 7 October 2008. Retrieved 9 October 2008. 
  141. ^ Tenenbaum, David (9 June 2008). "Making Sense of Mars Methane". Astrobiology Magazine. Archived from the original on 23 September 2008. Retrieved 8 October 2008. 
  142. ^ Tarsitano CG and Webster CR (2007). "Multilaser Herriott cell for planetary tunable laser spectrometers". Applied Optics, 46 (28): 6923–6935. Bibcode:2007ApOpt..46.6923T. doi:10.1364/AO.46.006923. PMID 17906720. 
  143. ^ Than, Ker (24 April 2007). "Major Discovery: New Planet Could Harbor Water and Life". Space.com. Archived from the original on 15 October 2008. Retrieved 20 October 2008. 
  144. ^ Chambers, Paul (1999). Life on Mars; The Complete Story. London: Blandford. ISBN 0-7137-2747-0. 
  145. ^ Levin, G and P. Straaf. 1976. Viking Labeled Release Biology Experiment: Interim Results. Science: 194. 1322-1329.
  146. ^ Bianciardi, Giorgio; Miller, Joseph D.; Straat, Patricia Ann; Levin, Gilbert V. (March 2012). "Complexity Analysis of the Viking Labeled Release Experiments". IJASS 13 (1): 14–26. Bibcode:2012IJASS..13...14B. doi:10.5139/IJASS.2012.13.1.14. Retrieved 15 April 2012. 
  147. ^ Klotz, Irene (12 April 2012). "MARS VIKING ROBOTS 'FOUND LIFE'". DiscoveryNews. Retrieved 16 April 2012. 
  148. ^ Navarro-González, R. et al. (2006). "The limitations on organic detection in Mars-like soils by thermal volatilization–gas chromatography–MS and their implications for the Viking results". PNAS 103 (44): 16089–16094. Bibcode:2006PNAS..10316089N. doi:10.1073/pnas.0604210103. PMC 1621051. PMID 17060639. Retrieved 2 April 2012. 
  149. ^ Paepe, Ronald (2007). "The Red Soil on Mars as a proof for water and vegetation" (PDP). Geophysical Research Abstracts 9 (1794). Retrieved 2 May 2012. 
  150. ^ Beagle 2 lander
  151. ^ Gerda Horneck, Petra Rettberg, Jobst-Ulrich Schott, Corinna Panitz, Andrea L’Afflitto, Ralf von Heise-Rotenburg, Reiner Willnecker, Pietro Baglioni, Jason Hatton, Jan Dettmann, René Demets and Günther Reitz., Elke Rabbow (9 July 2009). "EXPOSE, an Astrobiological Exposure Facility on the International Space Station - from Proposal to Flight" (PDF). Orig Life Evol Biosph. Bibcode:2009OLEB...39..581R. doi:10.1007/s11084-009-9173-6. Retrieved 8 July 2013. 
  152. ^ Karen Olsson-Francis; Charles S. Cockell (23 October 2009). "Experimental methods for studying microbial survival in extraterrestrial environments" (PDF). Journal of Microbiological Methods 80: 1–13. doi:10.1016/j.mimet.2009.10.004. Retrieved 31 July 2013. 
  153. ^ Centre national d'études spatiales (CNES). "EXPOSE - home page". Retrieved 8 July 2013. 
  154. ^ "Name NASA's Next Mars Rover". NASA/JPL. 27 May 2009. Archived from the original on 22 May 2009. Retrieved 27 May 2009. 
  155. ^ "Mars Science Laboratory: Mission". NASA/JPL. Retrieved 12 March 2010. 
  156. ^ "Europe still keen on Mars missions". BBC News. 15 March 2012. Retrieved 16 March 2012. 
  157. ^ "Europe Joins Russia on Robotic ExoMars". Aviation Week. 16 March 2012. Retrieved 16 March 2012. 
  158. ^ "ESA Ruling Council OKs ExoMars Funding". Space News. 15 March 2012. Retrieved 16 March 2012. 
  159. ^ "Science Definition Team for the 2020 Mars Rover". NASA. Science Ref. 21 December 2012. Retrieved 21 December 2012. 
  160. ^ "Science Team Outlines Goals for NASA's 2020 Mars Rover". Jet Propulsion Laboratory (NASA). 9 July 2013. Retrieved 10 July 2013. 
  161. ^ "Mars 2020 Science Definition Team Report - Frequently Asked Questions" (PDF). NASA. 9 July 2013. Retrieved 10 July 2013. 
  162. ^ Wall, Mike (31 July 2011). "'Red Dragon' Mission Mulled as Cheap Search for Mars Life". SPACE.com. Retrieved 1 May 2012. 
  163. ^ "NASA ADVISORY COUNCIL (NAC) - Science Committee Report" (PDF). Ames Research Center, NASA. 1 November 2011. Retrieved 1 May 2012. 
  164. ^ McKay, Christopher P.; Carol R. Stoker, Brian J. Glass, Arwen I. Davé, Alfonso F. Davila, Jennifer L. Heldmann, Margarita M. Marinova, Alberto G. Fairen, Richard C. Quinn, Kris A. Zacny, Gale Paulsen, Peter H. Smith, Victor Parro, Dale T. Andersen, Michael H. Hecht, Denis Lacelle, and Wayne H. Pollard. (5 April 2013). "The Icebreaker Life Mission to Mars: A Search for Biomolecular Evidence for Life". Astrobiology 13 (4): 334–353. Bibcode:2013AsBio..13..334M. doi:10.1089/ast.2012.0878. Retrieved 30 June 2013. 
  165. ^ "Icebreaker Life Mission". Astrobiology Magazine. 16 May 2013. Retrieved 1 July 2013. 
  166. ^ McKay, C. P.; Carol R. Stoker, Brian J. Glass, Arwen I. Davé, Alfonso F. Davila, Jennifer L. Heldmann, Margarita M. Marinova, Alberto G. Fairen, Richard C. Quinn, Kris A. Zacny, Gale Paulsen, Peter H. Smith, Victor Parro, Dale T. Andersen, Michael H. Hecht, Denis Lacelle, and Wayne H. Pollard. (2012), "THE ICEBREAKER LIFE MISSION TO MARS: A SEARCH FOR BIOCHEMICAL EVIDENCE FOR LIFE" (PDF), Concepts and Approaches for Mars Exploration, Lunar and Planetary Institute, retrieved 1 July 2013 
  167. ^ "Europa Clipper". Jet Propulsion Laboratory (NASA). November 2013. Retrieved 13 December 2013. 
  168. ^ Kane, Van (26 May 2013). "Europa Clipper Update". Future Planetary Exploration. Retrieved 13 December 2013. 
  169. ^ Pappalardo, Robert T.; S. Vance, F. Bagenal, B.G. Bills, D.L. Blaney, D.D. Blankenship, W.B. Brinckerhoff, et al. (2013). "Science Potential from a Europa Lander". Astrobiology 13 (8). doi: 10.1089/ast.2013.1003. Retrieved 14 December 2013. 
  170. ^ Senske, D. (2 October 2012), "Europa Mission Concept Study Update" (PDF), Presentation to Planetary Science Subcommittee, retrieved 14 December 2013 

Bibliography[edit]

External links[edit]

Further reading[edit]

  • The Search For Life In The Universe, D. Goldsmith, T. Owen. Second edition. ISBN 0-201-56949-3 Addison-Wesley Publishing Company