hypothetical types of biochemistry

{{Main|Shadow biosphere}}

File:Arecibo message.svg (1974) sent information into space about basic chemistry of Earth life.]]

A shadow biosphere is a hypothetical microbial biosphere of Earth that uses radically different biochemical and molecular processes than currently known life.{{cite journal | last1 = Davies | first1 = P. C. W. | last2 = Benner | first2 = S.A. | last3 = Cleland | first3 = C.E.|author3-link= Carol Cleland | last4 = Lineweaver | first4 = C.H. | last5 = McKay | first5 = C.P. | last6 = Wolfe-Simon | first6 = F. | s2cid = 5723954 | year = 2009 | title = Signatures of a Shadow Biosphere | journal = Astrobiology | volume = 9 | issue = 2| pages = 241–249 | doi = 10.1089/ast.2008.0251 | bibcode=2009AsBio...9..241D | pmid=19292603}}{{cite journal |last1=Cleland |first1=Carol E. |author1-link=Carol Cleland |last2=Copley |first2=Shelley D. |date=16 January 2006 |title=The possibility of alternative microbial life on Earth |journal=International Journal of Astrobiology |volume=4 |issue=3–4 |pages=165 |bibcode=2005IJAsB...4..165C |citeseerx=10.1.1.392.6366 |doi=10.1017/S147355040500279X |s2cid=364892}} Although life on Earth is relatively well-studied, the shadow biosphere may still remain unnoticed because the exploration of the microbial world targets primarily the biochemistry of the macro-organisms.

Perhaps the least unusual alternative biochemistry would be one with differing chirality of its biomolecules. In known Earth-based life, amino acids are almost universally of the {{small|L}} form and sugars are of the {{small|D}} form. Molecules using {{small|D}} amino acids or {{small|L}} sugars may be possible; molecules of such a chirality, however, would be incompatible with organisms using the opposing chirality molecules. Amino acids whose chirality is opposite to the norm are found on Earth, and these substances are generally thought to result from decay of organisms of normal chirality. However, physicist Paul Davies speculates that some of them might be products of "anti-chiral" life.{{cite journal |last1=Davies |first1=P.C.W. |last2=Lineweaver |first2=Charles H. |title=Finding a Second Sample of Life on Earth |journal=Astrobiology |date=April 2005 |volume=5 |issue=2 |pages=154–163 |doi=10.1089/ast.2005.5.154 |pmid=15815166 |bibcode=2005AsBio...5..154D }}

It is questionable, however, whether such a biochemistry would be truly alien. Although it would certainly be an alternative stereochemistry, molecules that are overwhelmingly found in one enantiomer throughout the vast majority of organisms can nonetheless often be found in another enantiomer in different (often basal) organisms such as in comparisons between members of Archaea and other domains,{{Citation needed|date=January 2012}} making it an open topic whether an alternative stereochemistry is truly novel.

On Earth, all known living things have a carbon-based structure and system. Scientists have speculated about the pros and cons of using elements other than carbon to form the molecular structures necessary for life, but no one has proposed a theory employing such atoms to form all the necessary structures. However, as Carl Sagan argued, it is very difficult to be certain whether a statement that applies to all life on Earth will turn out to apply to all life throughout the universe.{{cite book| title=Carl Sagan's Cosmic Connection: an Extraterrestrial Perspective| first1=Carl| last1= Sagan|first2=Jerome|last2=Agel|edition=2nd|publisher=Cambridge U.P.| date=2000|isbn= 978-0-521-78303-3|page=41}} Sagan used the term "carbon chauvinism" for such an assumption.{{cite book| title=Carl Sagan's Cosmic Connection: an Extraterrestrial Perspective| first=Carl| last= Sagan|edition=2nd|publisher=Cambridge U.P.| date=2000 |page=46}} He regarded silicon and germanium as conceivable alternatives to carbon (other plausible elements include but are not limited to palladium and titanium); but, on the other hand, he noted that carbon does seem more chemically versatile and is more abundant in the cosmos.{{cite book| title=Carl Sagan's Cosmic Connection: an Extraterrestrial Perspective| first=Carl| last= Sagan|edition=2nd|publisher=Cambridge U.P.| date=2000|page=47}} Norman Horowitz devised the experiments to determine whether life might exist on Mars that were carried out by the Viking Lander of 1976, the first U.S. mission to successfully land a probe on the surface of Mars. Horowitz argued that the great versatility of the carbon atom makes it the element most likely to provide solutions, even exotic solutions, to the problems of survival on other planets.Horowitz, N.H. (1986). Utopia and Back and the search for life in the solar system. New York: W.H. Freeman and Company. {{ISBN|0-7167-1766-2}}.{{pn|date=June 2024}} He considered that there was only a remote possibility that non-carbon life forms could exist with genetic information systems capable of self-replication and the ability to evolve and adapt.

{{See also|Organosilicon}}

File:Silane.png, analog of methane]]

File:PDMS.svg (PDMS)]]

File:Diatom2.jpgs{{snd}} carbon-based organisms that extract silicon from sea water, in the form of its oxide (silica) and incorporate it into their cell walls]]

The silicon atom has been much discussed as the basis for an alternative biochemical system, because silicon has many chemical similarities to carbon and is in the same group of the periodic table. Like carbon, silicon can create molecules that are sufficiently large to carry biological information.{{cite journal|last1 = Pace|first1 = N. R. |title = The universal nature of biochemistry |journal = Proceedings of the National Academy of Sciences of the United States of America |volume = 98 |issue = 3 |pages = 805–808 |date = 2001 |pmid = 11158550 |pmc = 33372 |doi = 10.1073/pnas.98.3.805 |bibcode=2001PNAS...98..805P|doi-access = free }}

However, silicon has several drawbacks as a carbon alternative. Carbon is ten times more cosmically abundant than silicon, and its chemistry appears naturally more complex. By 1998, astronomers had identified 84 carbon-containing molecules in the interstellar medium, but only 8 containing silicon, of which half also included carbon.{{cite web |url=http://www.faqs.org/faqs/astronomy/faq/part6/section-16.html |title= F.10 Why do we assume that other beings must be based on carbon? Why couldn't organisms be based on other substances? |work=[sci.astro] ET Life (Astronomy Frequently Asked Questions) |access-date=2006-07-21 |first=Joseph |last=Lazio}} Even though Earth and other terrestrial planets are exceptionally silicon-rich and carbon-poor (silicon is roughly 925 times more abundant in Earth's crust than carbon), terrestrial life bases itself on carbon. It may eschew silicon because silicon compounds are less varied, unstable in the presence of water, or block the flow of heat.{{cite web | url = http://biocab.org/Astrobiology.html | title = Astrobiology | access-date = 2011-01-17 | date = September 26, 2006 | publisher = Biology Cabinet | archive-date = 2010-12-12 | archive-url = https://web.archive.org/web/20101212184044/http://biocab.org/Astrobiology.html | url-status = dead }}

Relative to carbon, silicon has a much larger atomic radius, and forms much weaker covalent bonds to atoms — except oxygen and fluorine, with which it forms very strong bonds. Almost no multiple bonds to silicon are stable, although silicon does exhibit varied coordination number.{{sfn|Bains|2004}} Silanes, silicon analogues to the alkanes, react rapidly with water, and long-chain silanes spontaneously decompose. Consequently, most terrestrial silicon is "locked up" in silica, and not a wide variety of biogenic precursors.{{sfn|Bains|2004}}

Silicones, which alternate between silicon and oxygen atoms, are much more stable than silanes, and may even be more stable than the equivalent hydrocarbons in sulfuric acid-rich extraterrestrial environments.{{cite book |first=Stephen |last=Gillette |title=World-Building |publisher=Writer's Digest Books |isbn=978-0-89879-707-7|year=1996 }} Alternatively, the weak bonds in silicon compounds may help maintain a rapid pace of life at cryogenic temperatures. Polysilanols, the silicon homologues to sugars, are among the few compounds soluble in liquid nitrogen.{{cite web |title=The nature of life |website=Astrobiology |author=William Bains |access-date=2015-03-20 |url=http://www.williambains.co.uk/astrobiology/life2.html|archive-url=https://web.archive.org/web/20190127032142/http://www.williambains.co.uk/astrobiology/life2.html|archive-date=27 Jan 2019}}{{reliable?|reason=Self-published srcs are OK *if they're by an expert*, but is Bains one?|date=March 2024}}{{sfn|Bains|2004}}

All known silicon macromolecules are artificial polymers, and so "monotonous compared with the combinatorial universe of organic macromolecules".{{sfn|Bains|2004}} Even so, some Earth life uses biogenic silica: diatoms' silicate skeletons. A. G. Cairns-Smith hypothesized that silicate minerals in water played a crucial role in abiogenesis, in that biogenic carbon compounds formed around their crystal structures.{{Cite book |last=Cairns-Smith |first=A. Graham |title=Seven Clues to the Origin of Life |location=Cambridge |publisher=Cambridge University Press |date=1985 |isbn=978-0-521-27522-4 |url-access=registration |url=https://archive.org/details/sevencluestoorig00cair_0 }}{{cite book | first=Richard | last=Dawkins | author-link=Richard Dawkins | title=The Blind Watchmaker | publisher=W. W. Norton & Company, Inc | location=New York | orig-year=1986 | year=1996 | isbn=978-0-393-31570-7 | pages=[https://archive.org/details/blindwatchmaker0000dawk/page/148 148–161] | url=https://archive.org/details/blindwatchmaker0000dawk/page/148 }} Although not observed in nature, carbon–silicon bonds have been added to biochemistry under directed evolution (artificial selection): a cytochrome c protein from Rhodothermus marinus has been engineered to catalyze new carbon–silicon bonds between hydrosilanes and diazo compounds.{{cite journal |last1=Kan |first1=S. B. Jennifer |last2=Lewis |first2=Russell D. |last3=Chen |first3=Kai |last4=Arnold |first4=Frances H. |title=Directed evolution of cytochrome c for carbon–silicon bond formation: Bringing silicon to life |journal=Science |date=25 November 2016 |volume=354 |issue=6315 |pages=1048–1051 |doi=10.1126/science.aah6219 |pmid=27885032 |pmc=5243118 |bibcode=2016Sci...354.1048K }}

{{See also|Organoboron chemistry}}

• Boranes are dangerously explosive in Earth's atmosphere, but would be more stable in a reducing atmosphere. However, boron's low cosmic abundance makes it less likely as a base for life than carbon.
• Various metals, together with oxygen, can form very complex and thermally stable structures rivaling those of organic compounds;{{Citation needed|date=February 2014}} the heteropoly acids are one such family. Some metal oxides are also similar to carbon in their ability to form both nanotube structures and diamond-like crystals (such as cubic zirconia). Titanium, aluminium, magnesium, and iron are all more abundant in the Earth's crust than carbon. Metal-oxide-based life could therefore be a possibility under certain conditions, including those (such as high temperatures) at which carbon-based life would be unlikely. The Cronin group at Glasgow University reported self-assembly of tungsten polyoxometalates into cell-like spheres.{{cite magazine | url = https://www.newscientist.com/article/dn20906-lifelike-cells-are-made-of-metal.html | title = Life-like cells are made of metal | access-date = 2014-05-25 | date = September 14, 2011 | magazine = New Scientist}} By modifying their metal oxide content, the spheres can acquire holes that act as porous membrane, selectively allowing chemicals in and out of the sphere according to size.
• Sulfur is also able to form long-chain molecules, but suffers from the same high-reactivity problems as phosphorus and silanes. The biological use of sulfur as an alternative to carbon is purely hypothetical, especially because sulfur usually forms only linear chains rather than branched ones. (The biological use of sulfur as an electron acceptor is widespread and can be traced back 3.5 billion years on Earth, thus predating the use of molecular oxygen.{{cite journal |last1=Philippot |first1=Pascal |last2=Van Zuilen |first2=Mark |last3=Lepot |first3=Kevin |last4=Thomazo |first4=Christophe |last5=Farquhar |first5=James |last6=Van Kranendonk |first6=Martin J. |title=Early Archaean Microorganisms Preferred Elemental Sulfur, Not Sulfate |journal=Science |date=14 September 2007 |volume=317 |issue=5844 |pages=1534–1537 |doi=10.1126/science.1145861 |pmid=17872441 |bibcode=2007Sci...317.1534P }} Sulfur-reducing bacteria can utilize elemental sulfur instead of oxygen, reducing sulfur to hydrogen sulfide.)

{{See also|GFAJ-1}}

While arsenic, which is chemically similar to phosphorus, is poisonous for most life forms on Earth, it is incorporated into the biochemistry of some organisms.{{cite web|url=http://umbbd.ethz.ch/periodic/elements/as.html |title=Biochemical Periodic Table – Arsenic |publisher=UMBBD |date=2007-06-08 |access-date=2010-05-29}} Some marine algae incorporate arsenic into complex organic molecules such as arsenosugars and arsenobetaines. Fungi and bacteria can produce volatile methylated arsenic compounds. Arsenate reduction and arsenite oxidation have been observed in microbes (Chrysiogenes arsenatis).{{cite journal |last1=Niggemyer |first1=Allison |last2=Spring |first2=Stefan |last3=Stackebrandt |first3=Erko |last4=Rosenzweig |first4=R. Frank |title=Isolation and Characterization of a Novel As(V)-Reducing Bacterium: Implications for Arsenic Mobilization and the Genus Desulfitobacterium |journal=Applied and Environmental Microbiology |date=December 2001 |volume=67 |issue=12 |pages=5568–5580 |doi=10.1128/AEM.67.12.5568-5580.2001 |pmid=11722908 |pmc=93345 |bibcode=2001ApEnM..67.5568N }} Additionally, some prokaryotes can use arsenate as a terminal electron acceptor during anaerobic growth and some can utilize arsenite as an electron donor to generate energy.

It has been speculated that the earliest life forms on Earth may have used arsenic biochemistry in place of phosphorus in the structure of their DNA.{{cite journal |last1=Reilly |first1=Michael |title=Early life could have been based on arsenic |journal=New Scientist |date=April 2008 |volume=198 |issue=2653 |pages=10 |doi=10.1016/S0262-4079(08)61007-6 }} A common objection to this scenario is that arsenate esters are so much less stable to hydrolysis than corresponding phosphate esters that arsenic is poorly suited for this function.{{cite journal |last1=Westheimer |first1=F. H. |title=Why Nature Chose Phosphates |journal=Science |date=6 March 1987 |volume=235 |issue=4793 |pages=1173–1178 |doi=10.1126/science.2434996 |pmid=2434996 |bibcode=1987Sci...235.1173W }}

The authors of a 2010 geomicrobiology study, supported in part by NASA, have postulated that a bacterium, named GFAJ-1, collected in the sediments of Mono Lake in eastern California, can employ such 'arsenic DNA' when cultured without phosphorus.{{cite web |title=NASA-Funded Research Discovers Life Built With Toxic Chemical |publisher=NASA.gov |date=2 December 2010 |access-date=2010-12-02 |url=http://www.nasa.gov/topics/universe/features/astrobiology_toxic_chemical.html |archive-date=2011-08-28 |archive-url=https://web.archive.org/web/20110828203819/http://www.nasa.gov/topics/universe/features/astrobiology_toxic_chemical.html |url-status=dead }}{{cite journal |last1=Wolfe-Simon |first1=Felisa |last2=Blum |first2=Jodi Switzer |last3=Kulp |first3=Thomas R. |last4=Gordon |first4=Shelley E. |last5=Hoeft |last6=Pett-Ridge |first6=Jennifer |last7=Stolz |first7=John F. |last8=Webb |first8=Samuel M. |last9=Weber |first9=Peter K. |last10=Davies |first10=Paul C. W. |last11=Anbar |first11=Ariel D. |last12=Oremland |first12=Ronald S.|author1-link=Felisa Wolfe-Simon|author12-link=Ronald Oremland |title=A Bacterium That Can Grow by Using Arsenic Instead of Phosphorus |journal=Science |date=2 December 2010 |doi=10.1126/science.1197258 |pmid=21127214 |first5=S. E. |volume=332 |issue=6034 |pages=1163–6 |bibcode=2011Sci...332.1163W |s2cid=51834091 |doi-access=free }} They proposed that the bacterium may employ high levels of poly-β-hydroxybutyrate or other means to reduce the effective concentration of water and stabilize its arsenate esters. This claim was heavily criticized almost immediately after publication for the perceived lack of appropriate controls.{{cite web | last=Redfield | first=Rosemary | title=Arsenic-associated bacteria (NASA's claims) | work=rrresearch.blogspot.com/ | date=4 December 2010 | url=http://rrresearch.blogspot.com/2010/12/arsenic-associated-bacteria-nasas.html | access-date=4 December 2010}}{{self-published inline|date=June 2024}}{{cite web |last=Bradley |first=Alex |title=Arsenate-based DNA: a big idea with big holes |work=scienceblogs.com/webeasties/ |date=5 December 2010 |url=http://scienceblogs.com/webeasties/2010/12/guest_post_arsenate-based_dna.php |access-date=9 December 2010 |url-status=dead |archive-url= https://web.archive.org/web/20101208213626/http://scienceblogs.com/webeasties/2010/12/guest_post_arsenate-based_dna.php |archive-date=8 December 2010 }} Science writer Carl Zimmer contacted several scientists for an assessment: "I reached out to a dozen experts ... Almost unanimously, they think the NASA scientists have failed to make their case".{{cite news | last=Zimmer | first=Carl | author-link=Carl Zimmer

| title=Scientists see fatal flaws in the NASA study of arsenic-based life | date=7 December 2010 | url=http://www.slate.com/id/2276919/ | work=Slate | access-date=7 December 2010}}

Other authors were unable to reproduce their results and showed that the study had issues with phosphate contamination, suggesting that the low amounts present could sustain extremophile lifeforms.{{cite web | url = http://www.biotechniques.com/news/Arsenic-Life-Claim-Refuted/biotechniques-332691.html#.UQBYhx3O3zk | title="Arsenic Life" Claim Refuted | access-date = 23 January 2013 | last = Williams | first = Sarah | date = 7 November 2012 | work = BioTechniques | archive-url = https://web.archive.org/web/20160304054417/http://www.biotechniques.com/news/Arsenic-Life-Claim-Refuted/biotechniques-332691.html#.UQBYhx3O3zk | archive-date = 4 March 2016 | url-status = dead }}

Alternatively, it was suggested that GFAJ-1 cells grow by recycling phosphate from degraded ribosomes, rather than by replacing it with arsenate.{{cite journal |first=Harris TK and Deutscher MP | last=Basturea GN | title= Growth of a bacterium that apparently uses arsenic instead of phosphorus is a consequence of massive ribosome breakdown | date=17 August 2012 | pmid=22798070 | doi=10.1074/jbc.C112.394403 | volume=287 | issue=34 | journal=J Biol Chem | pages=28816–9 | pmc=3436571| doi-access=free }}

In addition to carbon compounds, all currently known terrestrial life also requires water as a solvent. This has led to discussions about whether water is the only liquid capable of filling that role. The idea that an extraterrestrial life-form might be based on a solvent other than water has been taken seriously in recent scientific literature by the biochemist Steven Benner,{{cite journal |last1=Benner |first1=Steven A. |last2=Ricardo | first2=Alonso |last3=Carrigan |first3=Matthew A |title=Is there a common chemical model for life in the universe? |date=2004 |journal=Current Opinion in Chemical Biology |volume=8|pages=676–680 |doi=10.1016/j.cbpa.2004.10.003 |issue=6 |pmid=15556414 }} and by the astrobiological committee chaired by John A. Baross.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=69 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; pages 69–79. Solvents discussed by the Baross committee include ammonia,Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=72 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; p. 72. sulfuric acid,Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=73 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; p. 73. formamide,Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=74 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; p. 74. hydrocarbons, and (at temperatures much lower than Earth's) liquid nitrogen, or hydrogen in the form of a supercritical fluid.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=75 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; p. 75.

Water as a solvent limits the forms biochemistry can take. For example, Steven Benner, proposes the polyelectrolyte theory of the gene that claims that for a genetic biopolymer such as, DNA, to function in water, it requires repeated ionic charges.{{cite journal |last1=Benner |first1=Steven A. |last2=Hutter |first2=Daniel |title=Phosphates, DNA, and the Search for Nonterrean Life: A Second Generation Model for Genetic Molecules |journal=Bioorganic Chemistry |date=February 2002 |volume=30 |issue=1 |pages=62–80 |doi=10.1006/bioo.2001.1232 |pmid=11955003 }} If water is not required for life, these limits on genetic biopolymers are removed.

Carl Sagan once described himself as both a carbon chauvinist and a water chauvinist;{{cite book |author=Sagan, Carl |title=Cosmos |date=2002 |isbn=978-0-375-50832-5 |publisher=Random House |pages=126–127}} however, on another occasion he said that he was a carbon chauvinist but "not that much of a water chauvinist".{{cite book |author1=Sagan, Carl |author2=Head, Tom |title=Conversations with Carl Sagan |url=https://archive.org/details/conversationswit00saga |url-access=registration |date=2006 |publisher=University Press of Mississippi |isbn=978-1-57806-736-7 |page=[https://archive.org/details/conversationswit00saga/page/10 10]}}

He speculated on hydrocarbons,{{rp|11}} hydrofluoric acid,{{cite book |author=Sagan, Carl |title=Cosmos |date=2002 |isbn=978-0-375-50832-5 |publisher=Random House |page=128}} and ammonia as possible alternatives to water.

Some of the properties of water that are important for life processes include:

• A complexity which leads to a large number of permutations of possible reaction paths including acid–base chemistry, H⁺ cations, OH⁻ anions, hydrogen bonding, van der Waals bonding, dipole–dipole and other polar interactions, aqueous solvent cages, and hydrolysis. This complexity offers a large number of pathways for evolution to produce life, many other solvents{{which|date=November 2018}} have dramatically fewer possible reactions, which severely limits evolution.
• Thermodynamic stability: the free energy of formation of liquid water is low enough (−237.24 kJ/mol) that water undergoes few reactions. Other solvents are highly reactive, particularly with oxygen.
• Water does not combust in oxygen because it is already the combustion product of hydrogen with oxygen. Most alternative solvents are not stable in an oxygen-rich atmosphere, so it is highly unlikely that those liquids could support aerobic life.
• A large temperature range over which it is liquid.
• High solubility of oxygen and carbon dioxide at room temperature supporting the evolution of aerobic aquatic plant and animal life.
• A high heat capacity (leading to higher environmental temperature stability).
• Water is a room-temperature liquid leading to a large population of quantum transition states required to overcome reaction barriers. Cryogenic liquids (such as liquid methane) have exponentially lower transition state populations which are needed for life based on chemical reactions. This leads to chemical reaction rates which may be so slow as to preclude the development of any life based on chemical reactions.{{citation needed|date=November 2018}}
• Spectroscopic transparency allowing solar radiation to penetrate several meters into the liquid (or solid), greatly aiding the evolution of aquatic life.
• A large heat of vaporization leading to stable lakes and oceans.
• The ability to dissolve a wide variety of compounds.
• The solid (ice) has lower density than the liquid, so ice floats on the liquid. This is why bodies of water freeze over but do not freeze solid (from the bottom up). If ice were denser than liquid water (as is true for nearly all other compounds), then large bodies of liquid would slowly freeze solid, which would not be conducive to the formation of life.

Water as a compound is cosmically abundant, although much of it is in the form of vapor or ice. Subsurface liquid water is considered likely or possible on several of the outer moons: Enceladus (where geysers have been observed), Europa, Titan, and Ganymede. Earth and Titan are the only worlds currently known to have stable bodies of liquid on their surfaces.

Not all properties of water are necessarily advantageous for life, however.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=70 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; page 70. For instance, water ice has a high albedo, meaning that it reflects a significant quantity of light and heat from the Sun. During ice ages, as reflective ice builds up over the surface of the water, the effects of global cooling are increased.

There are some properties that make certain compounds and elements much more favorable than others as solvents in a successful biosphere. The solvent must be able to exist in liquid equilibrium over a range of temperatures the planetary object would normally encounter. Because boiling points vary with the pressure, the question tends not to be does the prospective solvent remain liquid, but at what pressure. For example, hydrogen cyanide has a narrow liquid-phase temperature range at 1 atmosphere, but in an atmosphere with the pressure of Venus, with {{convert|92|bar|atm}} of pressure, it can indeed exist in liquid form over a wide temperature range.

The ammonia molecule (NH₃), like the water molecule, is abundant in the universe, being a compound of hydrogen (the simplest and most common element) with another very common element, nitrogen. The possible role of liquid ammonia as an alternative solvent for life is an idea that goes back at least to 1954, when J. B. S. Haldane raised the topic at a symposium about life's origin.{{Cite journal |author=J. B. S. Haldane |date=1954 |title=The Origins of Life |journal=New Biology |volume=16 |pages=12–27}} cited in {{cite web |url=http://www.daviddarling.info/encyclopedia/A/ammonialife.html/ |title=Ammonia-based life |last=Darling |first=David |archive-url=https://web.archive.org/web/20121018095038/http://www.daviddarling.info/encyclopedia/A/ammonialife.html |archive-date=2012-10-18 |url-status=dead |access-date=2012-10-01 }}

Numerous chemical reactions are possible in an ammonia solution, and liquid ammonia has chemical similarities with water.{{cite web | url = http://www.daviddarling.info/encyclopedia/A/ammonialife.html | title = ammonia-based life | access-date = 2012-10-01 | last = Darling | first = David}} Ammonia can dissolve most organic molecules at least as well as water does and, in addition, it is capable of dissolving many elemental metals. Haldane made the point that various common water-related organic compounds have ammonia-related analogs; for instance the ammonia-related amine group (−NH₂) is analogous to the water-related hydroxyl group (−OH).

Ammonia, like water, can either accept or donate an H⁺ ion. When ammonia accepts an H⁺, it forms the ammonium cation (NH₄⁺), analogous to hydronium (H₃O⁺). When it donates an H⁺ ion, it forms the amide anion (NH₂⁻), analogous to the hydroxide anion (OH⁻). Compared to water, however, ammonia is more inclined to accept an H⁺ ion, and less inclined to donate one; it is a stronger nucleophile. Ammonia added to water functions as an Arrhenius base: it increases the concentration of the anion hydroxide. Conversely, using a solvent system definition of acidity and basicity, water added to liquid ammonia functions as an acid, because it increases the concentration of the cation ammonium. The carbonyl group (C=O), which is much used in terrestrial biochemistry, would not be stable in ammonia solution, but the analogous imine group (C=NH) could be used instead.

However, ammonia has some problems as a basis for life. The hydrogen bonds between ammonia molecules are weaker than those in water, causing ammonia's heat of vaporization to be half that of water, its surface tension to be a third, and reducing its ability to concentrate non-polar molecules through a hydrophobic effect. Gerald Feinberg and Robert Shapiro have questioned whether ammonia could hold prebiotic molecules together well enough to allow the emergence of a self-reproducing system.{{cite book |title=Life Beyond Earth |url=https://archive.org/details/lifebeyondearthi0000fein |url-access=registration |first=Gerald |last= Feinberg |author2=Robert Shapiro |publisher=Morrow |date=1980 |isbn=978-0-688-03642-3}} cited in {{cite web | url = http://www.daviddarling.info/encyclopedia/A/ammonialife.html/ | title = ammonia-based life | access-date = 2012-10-01 | last = Darling | first = David | url-status = dead | archive-url = https://web.archive.org/web/20121018095038/http://www.daviddarling.info/encyclopedia/A/ammonialife.html | archive-date = 2012-10-18 }} Ammonia is also flammable in oxygen and could not exist sustainably in an environment suitable for aerobic metabolism.{{cite book |title=Life in the Universe: Expectations and Constraints |url=https://archive.org/details/lifeuniverseexpe00schu |url-access=limited |first1=Dirk |last1= Schulze-Makuch |first2=Louis Neal |last2=Irwin |publisher=Springer |edition=2 |date=2008 |isbn= 978-3-540-76816-6 |page=[https://archive.org/details/lifeuniverseexpe00schu/page/n130 119]}}

File:Layers of titan.jpg

A biosphere based on ammonia would likely exist at temperatures or air pressures that are extremely unusual in relation to life on Earth. Life on Earth usually exists between the melting point and boiling point of water, at a pressure designated as normal pressure, between {{convert|0|and|100|°C|K|abbr=on|lk=out}}. When also held to normal pressure, ammonia's melting and boiling points are {{convert|-78|°C|K|abbr=on}} and {{convert|-33|°C|K|abbr=on}} respectively. Because chemical reactions generally proceed more slowly at lower temperatures, ammonia-based life existing in this set of conditions might metabolize more slowly and evolve more slowly than life on Earth. On the other hand, lower temperatures could also enable living systems to use chemical species that would be too unstable at Earth temperatures to be useful.

A set of conditions where ammonia is liquid at Earth-like temperatures would involve it being at a much higher pressure. For example, at 60 atm ammonia melts at {{convert|-77|°C|K|abbr=on}} and boils at {{convert|98|°C|K|abbr=on}}.

Ammonia and ammonia–water mixtures remain liquid at temperatures far below the freezing point of pure water, so such biochemistries might be well suited to planets and moons orbiting outside the water-based habitability zone. Such conditions could exist, for example, under the surface of Saturn's largest moon Titan.{{cite web |url=http://www.es.ucl.ac.uk/research/planetary/undergraduate/dom/titan/titan.htm |title=Exobiological Implications of a Possible Ammonia-Water Ocean Inside Titan |last=Fortes |first=A. D. |date=1999 |access-date=7 June 2010}}

Methane (CH₄) is a simple hydrocarbon: that is, a compound of two of the most common elements in the cosmos: hydrogen and carbon. It has a cosmic abundance comparable with ammonia. Hydrocarbons could act as a solvent over a wide range of temperatures, but would lack polarity. Isaac Asimov, the biochemist and science fiction writer, suggested in 1981 that poly-lipids could form a substitute for proteins in a non-polar solvent such as methane. Lakes composed of a mixture of hydrocarbons, including methane and ethane, have been detected on the surface of Titan by the Cassini spacecraft.

There is debate about the effectiveness of methane and other hydrocarbons as a solvent for life compared to water or ammonia.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=74 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; page 74.{{cite journal |title=Solubility of Polyethers in Hydrocarbons at Low Temperatures. A Model for Potential Genetic Backbones on Warm Titans |journal=Astrobiology |date=March 2015 |last1=McLendon |first1=Christopher |last2=Opalko |first2=F. Jeffrey |volume=15 |issue=3 |pages= 200–206 |doi=10.1089/ast.2014.1212 |bibcode=2015AsBio..15..200M |pmid=25761113}}{{cite news |last=Hadhazy |first=Adam |url=http://www.space.com/29389-alien-life-hydrocarbon-exoplanets-ether-dna.html?adbid=10152808883996466&adbpl=fb&adbpr=17610706465&short_code=2ze6t |title=Alien Life on Oily Exoplanets Could Have Ether-based 'DNA' |work=Astrobiology Magazine |publisher=Space.com |date=13 May 2015 |access-date=2015-05-21 }} Water is a stronger solvent than the hydrocarbons, enabling easier transport of substances in a cell.{{cite web |title=What is Consuming Hydrogen and Acetylene on Titan? |publisher=NASA/JPL |date=2010 |access-date=2010-06-06 |url=http://www.jpl.nasa.gov/news/news.cfm?release=2010-190 |url-status=dead |archive-url=https://web.archive.org/web/20110629185640/http://www.jpl.nasa.gov/news/news.cfm?release=2010-190 |archive-date=June 29, 2011 }} However, water is also more chemically reactive and can break down large organic molecules through hydrolysis. A life-form whose solvent was a hydrocarbon would not face the threat of its biomolecules being destroyed in this way. Also, the water molecule's tendency to form strong hydrogen bonds can interfere with internal hydrogen bonding in complex organic molecules. Life with a hydrocarbon solvent could make more use of hydrogen bonds within its biomolecules. Moreover, the strength of hydrogen bonds within biomolecules would be appropriate to a low-temperature biochemistry.

Astrobiologist Chris McKay has argued, on thermodynamic grounds, that if life does exist on Titan's surface, using hydrocarbons as a solvent, it is likely also to use the more complex hydrocarbons as an energy source by reacting them with hydrogen, reducing ethane and acetylene to methane.{{cite journal |journal = Icarus |volume= 178 |issue = 1 |pages = 274–276 |date= 2005 |doi = 10.1016/j.icarus.2005.05.018 |title = Possibilities for methanogenic life in liquid methane on the surface of Titan |author1=McKay, C. P. |author2=Smith, H. D. |bibcode=2005Icar..178..274M|url= https://zenodo.org/record/1259025 }} Possible evidence for this form of life on Titan was identified in 2010 by Darrell Strobel of Johns Hopkins University; a greater abundance of molecular hydrogen in the upper atmospheric layers of Titan compared to the lower layers, arguing for a downward diffusion at a rate of roughly 10²⁵ molecules per second and disappearance of hydrogen near Titan's surface. As Strobel noted, his findings were in line with the effects Chris McKay had predicted if methanogenic life-forms were present.{{cite journal |last1=Strobel |first1=Darrell F. |title=Molecular hydrogen in Titan's atmosphere: Implications of the measured tropospheric and thermospheric mole fractions |journal=Icarus |date=August 2010 |volume=208 |issue=2 |pages=878–886 |doi=10.1016/j.icarus.2010.03.003 |bibcode=2010Icar..208..878S }} The same year, another study showed low levels of acetylene on Titan's surface, which were interpreted by Chris McKay as consistent with the hypothesis of organisms reducing acetylene to methane. While restating the biological hypothesis, McKay cautioned that other explanations for the hydrogen and acetylene findings are to be considered more likely: the possibilities of yet unidentified physical or chemical processes (e.g. a non-living surface catalyst enabling acetylene to react with hydrogen), or flaws in the current models of material flow.{{cite web |title=Have We Discovered Evidence For Life On Titan |author=Mckay, Chris |date=2010 |url=http://astronomy.nmsu.edu/tharriso/ast105/making_sense.php.html |work=New Mexico State University |access-date=2014-05-15 |archive-url=https://web.archive.org/web/20160309224810/http://astronomy.nmsu.edu/tharriso/ast105/making_sense.php.html |archive-date=2016-03-09 |url-status=dead }} He noted that even a non-biological catalyst effective at 95 K would in itself be a startling discovery.

A hypothetical cell membrane termed an azotosome, capable of functioning in liquid methane in Titan conditions was computer-modeled in an article published in February 2015. Composed of acrylonitrile, a small molecule containing carbon, hydrogen, and nitrogen, it is predicted to have stability and flexibility in liquid methane comparable to that of a phospholipid bilayer (the type of cell membrane possessed by all life on Earth) in liquid water.{{cite journal |last1=Stevenson |first1=James |last2=Lunine |first2=Jonathan |last3=Clancy |first3=Paulette |title=Membrane alternatives in worlds without oxygen: Creation of an azotosome |journal=Science Advances |date=27 Feb 2015 |volume=1 |issue=1 |doi=10.1126/sciadv.1400067 |pmid=26601130 |pmc=4644080 |pages=e1400067 |bibcode=2015SciA....1E0067S}}[http://phys.org/news/2015-02-life-saturn-moon-titan.html Life 'not as we know it' possible on Saturn's moon Titan]. An analysis of data obtained using the Atacama Large Millimeter / submillimeter Array (ALMA), completed in 2017, confirmed substantial amounts of acrylonitrile in Titan's atmosphere.{{cite web |last=Wall |first=Mike |title=Saturn Moon Titan Has Molecules That Could Help Make Cell Membranes |url=https://www.space.com/37653-saturn-moon-titan-cell-membrane-molecules.html |date=28 July 2017 |work=Space.com |access-date=29 July 2017 }}{{cite journal |author=Palmer, Maureen Y.|display-authors=etal |title=ALMA detection and astrobiological potential of vinyl cyanide on Titan |date=28 July 2017 |journal=Science Advances |volume =3 |number=7 |doi= 10.1126/sciadv.1700022 |pmc=5533535 |bibcode=2017SciA....3E0022P |pmid=28782019 |page=e1700022}} Later studies questioned whether acrylonitrile would be able to self-assemble into azotosomes.{{Cite journal|last1=Sandström|first1=H.|last2=Rahm|first2=M.|date=January 2020|title=Can polarity-inverted membranes self-assemble on Titan?|journal=Science Advances|volume=6 |issue=4 |pages=eaax0272 |language=EN|doi=10.1126/sciadv.aax0272|pmc=6981084|pmid=32042894|bibcode=2020SciA....6..272S }}

Hydrogen fluoride (HF), like water, is a polar molecule, and due to its polarity it can dissolve many ionic compounds. At atmospheric pressure, its melting point is {{convert|189.15|K|C}}, and its boiling point is {{convert|292.69|K|C}}; the difference between the two is a little more than 100 K. HF also makes hydrogen bonds with its neighbor molecules, as do water and ammonia. It has been considered as a possible solvent for life by scientists such as Peter Sneath{{cite book |title=Planets and Life |last=Sneath |first=P. H. A. |date=1970 |publisher=Thames and Hudson}} cited in {{cite book |title=Extraterrestrial Encounter |last=Boyce |first=Chris |date=1981 |publisher=New English Library |pages=125, 182}} and Carl Sagan.

HF is dangerous to the systems of molecules that Earth-life is made of, but certain other organic compounds, such as paraffin waxes, are stable with it. Like water and ammonia, liquid hydrogen fluoride supports an acid–base chemistry. Using a solvent system definition of acidity and basicity, nitric acid functions as a base when it is added to liquid HF.{{cite book |title=Chemistry in Nonaqueous Ionizing solvents: Inorganic Chemistry in Liquid Hydrogen Cyanide and Liquid hydrogen Fluoride |first1=Gerhart |last1= Jander |first2=Hans |last2= Spandau |first3=C. C. |last3=Addison |publisher=Pergamon Press |location=N.Y. |date=1971 |volume=II}} cited in {{cite book |title=Xenology: An Introduction to the Scientific Study of Extraterrestrial Life, Intelligence, and Civilization |first=Robert A. |last= Freitas |publisher=Xenology Research Institute |location=Sacramento, CA |date=1979 |chapter=8.2.2 |chapter-url=http://www.xenology.info/Xeno/8.2.2.htm}}

However, hydrogen fluoride is cosmically rare, unlike water, ammonia, and methane.{{cite book |title=Xenology: An Introduction to the Scientific Study of Extraterrestrial Life, Intelligence, and Civilization |first=Robert A. |last= Freitas |publisher=Xenology Research Institute |location=Sacramento, CA |date=1979 |chapter=8.2.2 |chapter-url=http://www.xenology.info/Xeno/8.2.2.htm}}

Hydrogen sulfide is the closest chemical analog to water,{{cite web | url=http://www.daviddarling.info/encyclopedia/S/solvent.html | title = solvent | access-date = 2012-10-12 | last = Darling | first = David}} but is less polar and is a weaker inorganic solvent.{{cite book| title=Ionizing Solvents| first1=J.| last1= Jander| first2=C.| last2=Lafrenz | publisher=John Wiley & Sons Ltd., Verlag Chemie| location=Weinheim/Bergstr.| date=1970|volume=I}} cited in {{cite book| title=Xenology: An Introduction to the Scientific Study of Extraterrestrial Life, Intelligence, and Civilization| first=Robert A.| last= Freitas| publisher=Xenology Research Institute| location=Sacramento, CA| date=1979 |chapter=8.2.2 |chapter-url=http://www.xenology.info/Xeno/8.2.2.htm}} Hydrogen sulfide is quite plentiful on Jupiter's moon Io and may be in liquid form a short distance below the surface; astrobiologist Dirk Schulze-Makuch has suggested it as a possible solvent for life there.{{cite web |url=http://www.astrobio.net/exclusive/3518/the-chance-for-life-on-io | title = The Chance for Life on Io | access-date = 2013-05-25 | last = Choi | first = Charles Q.| date = 2010-06-10 |archive-url=https://web.archive.org/web/20121027183552/http://www.astrobio.net/exclusive/3518/the-chance-for-life-on-io |archive-date=2012-10-27 |url-status=usurped}} On a planet with hydrogen sulfide oceans, the source of the hydrogen sulfide could come from volcanoes, in which case it could be mixed in with a bit of hydrogen fluoride, which could help dissolve minerals. Hydrogen sulfide life might use a mixture of carbon monoxide and carbon dioxide as their carbon source. They might produce and live on sulfur monoxide, which is analogous to oxygen (O₂). Hydrogen sulfide, like hydrogen cyanide and ammonia, suffers from the small temperature range where it is liquid, though that, like that of hydrogen cyanide and ammonia, increases with increasing pressure.

Silicon dioxide, also known as silica and quartz, is very abundant in the universe and has a large temperature range where it is liquid. However, its melting point is {{convert|1,600|to|1,725|C|F}}, so it would be impossible to make organic compounds in that temperature, because all of them would decompose. Silicates are similar to silicon dioxide and some have lower melting points than silica. Feinberg and Shapiro have suggested that molten silicate rock could serve as a liquid medium for organisms with a chemistry based on silicon, oxygen, and other elements such as aluminium.{{cite book |author1=David W. Koerner |author2=Simon LeVay |title=Here Be Dragons : The Scientific Quest for Extraterrestrial Life |date=2000 |isbn=978-0-19-803337-0 |publisher=Oxford U.P. |pages=202}}

File:Sulfuric-acid-Givan-et-al-1999-3D-balls.png

Other solvents sometimes proposed:

• Supercritical fluids: supercritical carbon dioxide and supercritical hydrogen.{{cite journal |last1=Budisa |first1=Nediljko |last2=Schulze-Makuch |first2=Dirk |title=Supercritical Carbon Dioxide and Its Potential as a Life-Sustaining Solvent in a Planetary Environment |journal=Life |date=8 August 2014 |volume=4 |issue=3 |pages=331–340 |doi=10.3390/life4030331 |pmc=4206850 |pmid=25370376|bibcode=2014Life....4..331B |doi-access=free }}
• Simple hydrogen compounds: hydrogen chloride.{{Cite book | last1 = Ward | first1 = Peter D. | last2 = Benner | first2 = Steven A. | contribution = Alien biochemistries | date = 2007 | title = Planets and Life | editor-last = Sullivan | editor-first = Woodruff T. | editor2-last = Baross | editor2-first = John A. | page = 540 | place = Cambridge | publisher = Cambridge | isbn = 978-0-521-53102-3}}
• More complex compounds: sulfuric acid, formamide, methanol.
• Very-low-temperature fluids: liquid nitrogen and hydrogen.
• High-temperature liquids: sodium chloride.[http://www.astrobio.net/news-exclusive/the-methane-habitable-zone/ The methane habitable zone].

Sulfuric acid in liquid form is strongly polar. It remains liquid at higher temperatures than water, its liquid range being 10 °C to 337 °C at a pressure of 1 atm, although above 300 °C it slowly decomposes. Sulfuric acid is known to be abundant in the clouds of Venus, in the form of aerosol droplets. In a biochemistry that used sulfuric acid as a solvent, the alkene group (C=C), with two carbon atoms joined by a double bond, could function analogously to the carbonyl group (C=O) in water-based biochemistry.

A proposal has been made that life on Mars may exist and be using a mixture of water and hydrogen peroxide as its solvent.{{cite journal | title = A Possible Biogenic Origin for Hydrogen Peroxide on Mars | journal = International Journal of Astrobiology | volume = 6 | issue = 2 | pages = 147 | date = 2007-05-22 | first = Joop M. | last = Houtkooper |author2=Dirk Schulze-Makuch | doi = 10.1017/S1473550407003746 | arxiv = physics/0610093 |bibcode = 2007IJAsB...6..147H | s2cid = 8091895 }}

A 61.2% (by mass) mix of water and hydrogen peroxide has a freezing point of −56.5 °C and tends to super-cool rather than crystallize. It is also hygroscopic, an advantage in a water-scarce environment.{{cite journal |url=http://www.cosis.net/abstracts/EPSC2007/00439/EPSC2007-J-00439.pdf |archive-url=https://web.archive.org/web/20070926102728/http://www.cosis.net/abstracts/EPSC2007/00439/EPSC2007-J-00439.pdf |archive-date=2007-09-26 |url-status=live |journal=EPSC Abstracts |volume= 2 |id= EPSC2007-A-00439 |date=2007 |title=The H₂O₂–H₂O Hypothesis: Extremophiles Adapted to Conditions on Mars? |first=Joop M. |last= Houtkooper |author2=Dirk Schulze-Makuch |bibcode=2007epsc.conf..558H |pages=558}}{{cite web |url=http://www.planetary.org/blog/article/00001109/ |title=Europlanet : Life's a bleach |date=2007-08-24 |first=Doug |last=Ellison |publisher=Planetary.org |access-date=2007-08-25 |archive-date=2010-09-25 |archive-url=https://web.archive.org/web/20100925041103/http://www.planetary.org/blog/article/00001109/ |url-status=dead }}

Supercritical carbon dioxide has been proposed as a candidate for alternative biochemistry due to its ability to selectively dissolve organic compounds and assist the functioning of enzymes and because "super-Earth"- or "super-Venus"-type planets with dense high-pressure atmospheres may be common.

Physicists have noted that, although photosynthesis on Earth generally involves green plants, a variety of other-colored plants could also support photosynthesis, essential for most life on Earth, and that other colors might be preferred in places that receive a different mix of stellar radiation than Earth.{{cite web|url=http://www.nasa.gov/centers/goddard/news/topstory/2007/spectrum_plants.html |title=NASA – NASA Predicts Non-Green Plants on Other Planets |publisher=Nasa.gov |date=2008-02-23 |access-date=2010-05-29}}{{Cite journal | last = Kiang | first = Nancy Y. |author2=Segura, Antígona |author2-link=Antígona Segura |author3=Tinetti, Giovanna |author4=Jee, Govind|author5-link=Robert E. Blankenship |author5=Blankenship, Robert E. |author6=Cohen, Martin |author7=Siefert, Janet |author8=Crisp, David |author9= Meadows, Victoria S. | title = Spectral signatures of photosynthesis. II. Coevolution with other stars and the atmosphere on extrasolar worlds | journal = Astrobiology | volume = 7 | issue = 1 | pages = 252–274 | date = 2007-04-03 | doi = 10.1089/ast.2006.0108 | bibcode=2007AsBio...7..252K | pmid=17407410|arxiv = astro-ph/0701391 | s2cid = 9172251 }}

These studies indicate that blue plants would be unlikely; however yellow or red plants may be relatively common.

Many Earth plants and animals undergo major biochemical changes during their life cycles as a response to changing environmental conditions, for example, by having a spore or hibernation state that can be sustained for years or even millennia between more active life stages.{{cite web |url=https://www.pbs.org/wnet/nature/yellowstone/hibernate.html |title=Christmas in Yellowstone |publisher=Pbs.org |access-date=2010-05-29 |archive-date=2008-10-08 |archive-url=https://web.archive.org/web/20081008005741/http://www.pbs.org/wnet/nature/yellowstone/hibernate.html |url-status=dead }} Thus, it would be biochemically possible to sustain life in environments that are only periodically consistent with life as we know it.

For example, frogs in cold climates can survive for extended periods of time with most of their body water in a frozen state, whereas desert frogs in Australia can become inactive and dehydrate in dry periods, losing up to 75% of their fluids, yet return to life by rapidly rehydrating in wet periods.{{Cite journal|title=Main and Bentley, Ecology, "Water Relations of Australian Burrowing Frogs and Tree Frogs" (1964)|journal = Ecology|volume = 45|issue = 2|pages = 379–382|jstor = 1933854|last1 = Main|first1 = A. R.|last2 = Bentley|first2 = P. J.|year = 1964|doi = 10.2307/1933854}} Either type of frog would appear biochemically inactive (i.e. not living) during dormant periods to anyone lacking a sensitive means of detecting low levels of metabolism.

File:Early genetic code.svg

The genetic code may have evolved during the transition from the RNA world to a protein world.{{cite journal | first=Abdrew J. | last=Doig | title=Frozen, but no accident – why the 20 standard amino acids were selected | date=7 December 2016 | doi=10.1111/febs.13982 | volume=284 | issue=9 | journal=FEBS J. | pages=1296–1305| pmid=27926995 | doi-access=free }} The Alanine World Hypothesis postulates that the evolution of the genetic code (the so-called GC phase{{cite journal | first1=Hyman | last1=Hartman | first2=Temple F. | last2=Smith | title=The Evolution of the Ribosome and the Genetic Code | date=20 May 2014 | doi=10.3390/life4020227 | volume=4 | issue=2 | journal=Life | pages=227–249| pmid=25370196 | pmc=4187167 | bibcode=2014Life....4..227H | doi-access=free }}) started with only four basic amino acids: alanine, glycine, proline and ornithine (now arginine).{{cite journal|last1=Kubyshkin|first1=Vladimir|last2=Budisa|first2=Nediljko|title=The Alanine World Model for the Development of the Amino Acid Repertoire in Protein Biosynthesis|journal=Int. J. Mol. Sci.|date=24 September 2019|volume=20|issue=21|pages=5507|doi=10.3390/ijms20215507|pmid=31694194|pmc=6862034|doi-access=free}} The evolution of the genetic code ended with 20 proteinogenic amino acids. From a chemical point of view, most of them are Alanine-derivatives particularly suitable for the construction of α-helices and β-sheets{{snd}} basic secondary structural elements of modern proteins. Direct evidence of this is an experimental procedure in molecular biology known as alanine scanning.

A hypothetical "Proline World" would create a possible alternative life with the genetic code based on the proline chemical scaffold as the protein backbone. Similarly, a "Glycine World" and "Ornithine World" are also conceivable, but nature has chosen none of them.{{cite journal|last1=Kubyshkin|first1=Vladimir|last2=Budisa|first2=Nediljko|title=Anticipating alien cells with alternative genetic codes: away from the alanine world!|journal=Curr. Opin. Biotechnol.|date=3 July 2019|volume=60|pages=242–249|doi=10.1016/j.copbio.2019.05.006|pmid=31279217|doi-access=free}} Evolution of life with Proline, Glycine, or Ornithine as the basic structure for protein-like polymers (foldamers) would lead to parallel biological worlds. They would have morphologically radically different body plans and genetics from the living organisms of the known biosphere.{{cite journal|last1=Budisa|first1=Nediljko|last2=Kubyshkin|first2=Vladimir|last3=Schmidt|first3=Markus|title=Xenobiology: A Journey towards Parallel Life Forms|journal=ChemBioChem|date=22 April 2020|volume=21|issue=16|pages=2228–2231|doi=10.1002/cbic.202000141|pmid=32323410|doi-access=free}}

{{main|Non-planetary abiogenesis}}

{{See also|Dusty plasma}}

In 2007, Vadim N. Tsytovich and colleagues proposed that lifelike behaviors could be exhibited by dust particles suspended in a plasma, under conditions that might exist in space.{{cite press release |title=Physicists Discover Inorganic Dust With Lifelike Qualities |url=https://www.sciencedaily.com/releases/2007/08/070814150630.htm |work=ScienceDaily |publisher=Institute of Physics |date=15 August 2007 }}{{cite journal| title=From plasma crystals and helical structures towards inorganic living matter| journal= New J. Phys.| volume= 9| issue= 263| doi=10.1088/1367-2630/9/8/263|first=V N| last= Tsytovich| author2= G E Morfill, V E Fortov, N G Gusein-Zade, B A Klumov and S V Vladimirov| date=14 August 2007| page=263|bibcode = 2007NJPh....9..263T | last3=Fortov| first3=V E| last4=Gusein-Zade| first4=N G| last5=Klumov| first5=B A| last6=Vladimirov| first6=S V| doi-access=free}} Computer models showed that, when the dust became charged, the particles could self-organize into microscopic helical structures, and the authors offer "a rough sketch of a possible model of...helical grain structure reproduction".

In 2020, Luis A. Anchordoqu and Eugene M. Chudnovsky of the City University of New York hypothesized that cosmic necklace-based life composed of magnetic monopoles connected by cosmic strings could evolve inside stars.{{cite journal |last1=A. Anchordoqui |first1=Luis |last2=M. Chudnovsky |first2=Eugene |title=Can Self-Replicating Species Flourish in the Interior of a Star? |journal=Letters in High Energy Physics |date=31 March 2020 |volume=2020 |page=166 |doi=10.31526/lhep.2020.166 |bibcode=2020LHEP....3..166A }} This would be achieved by a stretching of cosmic strings due to the star's intense gravity, thus allowing it to take on more complex forms and potentially form structures similar to the RNA and DNA structures found within carbon-based life. As such, it is theoretically possible that such beings could eventually become intelligent and construct a civilization using the power generated by the star's nuclear fusion. Because such use would use up part of the star's energy output, the luminosity would also fall. For this reason, it is thought that such life might exist inside stars observed to be cooling faster or dimmer than current cosmological models predict.

Frank Drake suggested in 1973 that intelligent life could inhabit neutron stars.{{cite journal|last=Drake|first=F.D.|date=December 1973|title=Life on a Neutron Star: An Interview with Frank Drake|journal=Astronomy|pages=5–8|url=https://www.gwern.net/docs/science/1973-drake.pdf |archive-url=https://web.archive.org/web/20210315021022/https://www.gwern.net/docs/science/1973-drake.pdf |archive-date=2021-03-15 |url-status=live}} Physical models in 1973 implied that Drake's creatures would be microscopic.{{citation needed|date=April 2024}}

Scientists who have considered possible alternatives to carbon-water biochemistry include:

• J. B. S. Haldane (1892–1964), a geneticist noted for his work on abiogenesis.
• V. Axel Firsoff (1910–1981), British astronomer.{{Cite journal|author=V. Axel Firsoff|date=January 1962|title=An Ammonia-Based Life|journal=Discovery|volume=23|pages=36–42}} cited in {{cite web|url=http://www.daviddarling.info/encyclopedia/A/ammonialife.html/|title=ammonia-based life|last=Darling|first=David|archive-url=https://web.archive.org/web/20121018095038/http://www.daviddarling.info/encyclopedia/A/ammonialife.html|archive-date=2012-10-18|url-status=dead|access-date=2012-10-01}}
• Isaac Asimov (1920–1992), biochemist and science fiction writer.{{Cite journal| journal=Cosmic Search|title=Not as We Know it – the Chemistry of Life|date=Winter 1981|issue= 9 (Vol 3 No 1)|author=Isaac Asimov|publisher=North American AstroPhysical Observatory|url=http://www.bigear.org/CSMO/HTML/CS09/cs09all.htm}}
• Fred Hoyle (1915–2001), astronomer and science fiction writer.
• Norman Horowitz (1915–2005), Caltech geneticist who devised the first experiments carried out to detect life on Mars.
• George C. Pimentel (1922–1989), American chemist, University of California, Berkeley.{{cite book|title=Intelligent Life in the Universe|last=Shklovskii|first=I.S.|author2=Carl Sagan|date=1977|publisher=Picador|page=229}}
• Peter Sneath (1923–2011), microbiologist, author of the book Planets and Life.
• Gerald Feinberg (1933–1992), physicist and Robert Shapiro (1935–2011), chemist, co-authors of the book Life Beyond Earth.{{cite book|title=Life Beyond Earth|url=https://archive.org/details/lifebeyondearthi0000fein|url-access=registration|last=Feinberg|first=Gerald|author2=Robert Shapiro|date=1980|publisher=Morrow|isbn=978-0-688-03642-3}}{{pn|date=June 2024}}A detailed review of this book is: {{Cite journal|author=John Gribbin|date=2 Oct 1980|title=Life beyond Earth|journal=New Scientist|page=xvii}}
• Carl Sagan (1934–1996), astronomer, science popularizer, and SETI proponent.
• Jonathan Lunine (born 1959), American planetary scientist and physicist.
• Robert Freitas (born 1952), specialist in nano-technology and nano-medicine.{{cite book|url=http://www.xenology.info/Xeno.htm|title=Xenology: An Introduction to the Scientific Study of Extraterrestrial Life, Intelligence, and Civilization|last=Freitas|first=Robert A.|date=1979|publisher=Xenology Research Institute|location=Sacramento, CA}}This work is acknowledged the partial basis of the article {{cite web|url=http://www.daviddarling.info/encyclopedia/A/ammonialife.html/|title=ammonia-based life|last=Darling|first=David|archive-url=https://web.archive.org/web/20121018095038/http://www.daviddarling.info/encyclopedia/A/ammonialife.html|archive-date=2012-10-18|url-status=dead|access-date=2012-10-01}}
• John Baross (born 1940), oceanographer and astrobiologist, who chaired a committee of scientists under the United States National Research Council that published a report on life's limiting conditions in 2007.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007.Committee on the Limits of Organic Life in Planetary Systems, Committee on the Origins and Evolution of Life, National Research Council; [http://books.nap.edu/openbook.php?record_id=11919&page=R10 The Limits of Organic Life in Planetary Systems]; The National Academies Press, 2007; page 5

{{div col|colwidth=30em}}

• Abiogenesis
• Astrobiology
• Carbon chauvinism
• Carbon-based life
• Earliest known life forms
• Extraterrestrial life
• Hachimoji DNA
• Iron–sulfur world hypothesis
• Life origination beyond planets
• Mirror life
• Nexus for Exoplanet System Science
• Non-cellular life
• Non-proteinogenic amino acids
• Nucleic acid analogues
• Planetary habitability
• Shadow biosphere

{{div col end}}

{{reflist|30em}}

• {{Cite journal| journal=Astrobiology |title=Many Chemistries Could Be Used to Build Living Systems | date=2004 |volume=4 |pages= 137–167 |first=William |last=Bains |s2cid=27477952 | doi = 10.1089/153110704323175124| pmid=15253836| issue=2 |bibcode = 2004AsBio...4..137B }}

• [http://www.faqs.org/faqs/astronomy/faq/part6/section-16.html Astronomy FAQ]
• [http://www.daviddarling.info/encyclopedia/A/ammonialife.html Ammonia-based life]
• [http://www.daviddarling.info/encyclopedia/S/siliconlife.html Silicon-based life]

{{Astrobiology}}

{{Extraterrestrial life}}

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