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{{Kotak info karbon}}
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==Karakteristik==
[[File:Carbon
Perbendaan bentuk atau ''[[alotropi]]'' karbon (lihat di bawah) meliputi salah satu bahan yang dikenal palilng lunak, [[grafit]], dan juga bahan terkeras yang terbentuk secara alami, [[intan]]. Selain itu, karbon mempunyai afinitas membentuk [[ikatan kimia|ikatan]] dengan atom kecil lainnya, termasuk atom karbon lainnya, dan mampu membentuk ikatan [[kovalen]] multi-stabil dengan atom-atom ini. Alhasil, karbon dikenal membentuk hampir sepuluh juta senyawa yang berbeda; mayoritas dari seluruh [[senyawa kimia]].<ref name=lanl/> Karbon juga mempunyai titik [[sublimasi (kimia)|sublimasi]] tertinggi di antara unsur-unsur kimia. Pada [[tekanan atmosfer]], karbon tidak memiliki titik lebur karena [[titik tripel|titik tripelnya]] adalah 10,8 ± 0,2 MPa and 4.600 ± 300 K (~4.330 °C or 7.820 °F),<ref name=triple2/><ref name=triple3/> sehingga ia menyublim pada sekitar 3.900 K.<ref name="triple">{{cite journal|journal=Nature|volume=276|pages=695–696|date=1978|doi=10.1038/276695a0|title=The controversial carbon solid−liquid−vapour triple point|first=A.|last=Greenville Whittaker|issue=5689|bibcode=1978Natur.276..695W }}</ref><ref>{{cite news|url=http://lbruno.home.cern.ch/lbruno/documents/Bibliography/LHC_Note_78.pdf|title=On Graphite Transformations at High Temperature and Pressure Induced by Absorption of the LHC Beam|first=J. M.|last=Zazula|date=1997|accessdate=2009-06-06|publisher=CERN}}</ref>
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{{main|Alotrop karbon}}
[[Atom karbon]] adalah spesies dengan umur paling pendek dan, oleh sebab itu, karbon distabilkan dalam beragam struktur multi atom dengan konfigurasi molekul yang berbeda yang disebut [[alotrop]]. Tiga alotrop karbon yang relatif cukup dikenal adalah [[karbon amorf]], [[grafit]], dan [[intan]]. Setelah dianggap eksotis, [[fulerena]] yang saat ini sering disintesis dan digunakan dalam penelitian; mereka mulai mengungkap juga ''[[Bulkyball (molekul)|bulkyballs]]'',<ref name="buckyballs"/><ref name="nanotubes">{{cite book|editor=Ebbesen, T. W.|date=1997|title=Carbon nanotubes—preparation and properties|publisher=CRC Press|location=Boca Raton, Florida|isbn=0-8493-9602-6}}</ref> [[karbon nanotube]],<ref name="nanotubes2">{{cite journal|editor=Dresselhaus, M. S.|editor2= Dresselhaus, G.|editor3= Avouris, Ph.|date=2001|title=Carbon nanotubes: synthesis, structures, properties and applications|journal=Topics in Applied Physics|volume=80|isbn=3-540-41086-4|publisher=Springer|location=Berlin}}</ref> [[karbon nanobud]]<ref name="nanobuds">{{cite journal|date=2007|title=A novel hybrid carbon material|journal=Nature Nanotechnology|volume=2|pages=156–161|doi=10.1038/nnano.2007.37|last1=Nasibulin|first1=Albert G.|pmid=18654245|last2=Pikhitsa|first2=P.V.|last3=Jiang|first3=H.|last4=Brown|first4=D. P.|last5=Krasheninnikov|first5=A.V.|last6=Anisimov|first6=A. S.|last7=Queipo|first7=P.|last8=Moisala|first8=A.|last9=Gonzalez|first9=D.|issue=3|bibcode=2007NatNa...2..156N|display-authors=8 }}</ref> dan [[Karbon nanofiber|nanofiber]].<ref>{{cite journal|date=2007|title=Investigations of NanoBud formation|journal=Chemical Physics Letters|volume=446|pages=109–114|doi=10.1016/j.cplett.2007.08.050|last1=Nasibulin|first1=A|last2=Anisimov|first2=Anton S.|last3=Pikhitsa|first3=Peter V.|last4=Jiang|first4=Hua|last5=Brown|first5=David P.|last6=Choi|first6=Mansoo|last7=Kauppinen|first7=Esko I.|bibcode=2007CPL...446..109N }}</ref><ref>{{cite journal|date=2004|title=Synthesis and characterisation of carbon nanofibers with macroscopic shaping formed by catalytic decomposition of C{{sub|2}}H{{sub|6}}/H{{sub|2}} over nickel catalyst|journal=Applied Catalysis A|volume=274|pages=1–8|doi=10.1016/j.apcata.2004.04.008|author=Vieira, R|last2=Ledoux|first2=Marc-Jacques|last3=Pham-Huu|first3=Cuong}}</ref> Beberapa alotrop eksotis lainnya juga telah ditemukan, seperti [[lonsdaleit]],<ref name="lonsdaletite">{{cite journal|date=1967|title=Lonsdaleite, a new hexagonal polymorph of diamond|journal=Nature|volume=214|pages=587–589|doi=10.1038/214587a0|first=Frondel|last=Clifford|last2=Marvin|first2=Ursula B.|issue=5088|bibcode=1967Natur.214..587F }}</ref> ''[[glassy carbon]]'',<ref name="glassy carbon"/> [[karbon nanofoam]]<ref>{{cite journal|date=1999|title=Structural analysis of a carbon foam formed by high pulse-rate laser ablation|journal=Applied Physics A-Materials Science & Processing|volume=69|pages=S755–S758|doi=10.1007/s003390051522|author=Rode, A. V.|last2=Hyde|first2=S. T.|last3=Gamaly|first3=E. G.|last4=Elliman|first4=R. G.|last5=McKenzie|first5=D. R.|last6=Bulcock|first6=S.|issue=7}}</ref> dan [[karbon asetilen linear]] (karbin) ({{lang-en|carbyne}}).<ref name=LAC>{{cite book|author=Heimann, Robert Bertram|author2=Evsyukov, Sergey E.|author3=Kavan, Ladislav|last-author-amp=yes|title=Carbyne and carbynoid structures|url=http://books.google.com/books?id=swSQZcTmo_4C&pg=PA1|accessdate=2011-06-06|date=28 February 1999|publisher=Springer|isbn=978-0-7923-5323-2|pages=1–}}</ref>
[[File:Glassy carbon and a 1cm3 graphite cube HP68-79.jpg|thumb|left|Sampel
Bentuk [[amorf]] adalah campuran beragam atom karbon dalam bentuk non-kristal, iregular, kondisi glassy, yang secara esensi adalah [[grafit]] tetapi tidak mempertahankan struktur makro kristalnya. Karbon ini hadir dalam bentuk serbuk, dan merupakan konstituen utama dalam [[arang]], [[jelaga]], dan [[karbon aktif]]. Pada tekanan normal, karbon berada dalam bentuk [[grafit]], di mana masing-masing atom terikat secara trigonal dengan tiga atom karbon lainnya pada satu bidang cincin [[Heksagon|heksagonal]], seperti yang diperlihatkan oleh [[hidrokarbon aromatik]].<ref>{{cite book|title=The polymorphism of elements and compounds|last=Jenkins|first=Edgar|date=1973|publisher=Taylor & Francis|isbn=0-423-87500-0|page=30|url=http://books.google.com/books?id=XNYOAAAAQAAJ&pg=PA30|accessdate=2011-05-01}}</ref> Hasilnya adalah 2-dimensi datar yang tersusun dan terikat lemah melalui [[gaya van der Waals]].<!-- no evidence for upper case van der Waals; see [[Talk:Van der Waals#Van should be capitalized unless preceded by first name]] rebuttal -->Hal ini menyumbang sifat grafit yang lunak dan mudah patah.
▲[[File:Glassy carbon and a 1cm3 graphite cube HP68-79.jpg|thumb|left|Sampel besar ''glassy carbon''.]]
Karena delokalisasi salah satu elektron terluar masing-masing atom untuk membentuk [[Elektron terdelokalisasi|awan-π]], grafit menghantarkan [[listrik]], tetapi hanya pada bidang masing-masing lembar [[ikatan kovalen]]. Hal ini yang menyebabkan karbon mempunyai [[konduktivitas listrik]] massal yang rendah dibandingkan kebanyakan [[logam]]. Delokalisasi juga menyebabkan stabilitas energik grafit lebih besar daripada berlian pada suhu kamar.
[[File:Eight Allotropes of Carbon.png|thumb|300px|Some allotropes of carbon: a) [[diamond]]; b) [[graphite]]; c) [[lonsdaleite]]; d–f) [[fullerene]]s (C{{sub|60}}, C{{sub|540}}, C{{sub|70}}); g) [[amorphous carbon]]; h) [[carbon nanotube]].]]▼
▲[[File:Eight Allotropes of Carbon.png|thumb|300px|
[[Fullerene]]s have a graphite-like structure, but instead of purely [[hexagonal crystal system|hexagonal]] packing, they also contain pentagons (or even heptagons) of carbon atoms, which bend the sheet into spheres, ellipses or cylinders. The properties of fullerenes (split into [[Buckyball (molecule)|buckyball]]s, [[carbon nanotube|buckytubes]] and [[nanobud]]s) have not yet been fully analyzed and represent an intense area of research in [[nanomaterials]]. The names ''"fullerene"'' and ''"buckyball"'' are given after [[Buckminster Fuller|Richard Buckminster Fuller]], popularizer of [[geodesic dome]]s, which resemble the structure of fullerenes. The buckyballs are fairly large molecules formed completely of carbon bonded trigonally, forming [[spheroid]]s (the best-known and simplest is the soccerball-shaped C{{sub|60}} [[buckminsterfullerene]]).<ref name="buckyballs" /> Carbon nanotubes are structurally similar to buckyballs, except that each atom is bonded trigonally in a curved sheet that forms a hollow [[cylinder (geometry)|cylinder]].<ref name="nanotubes" /><ref name="nanotubes2" /> Nanobuds were first reported in 2007 and are hybrid bucky tube/buckyball materials (buckyballs are covalently bonded to the outer wall of a nanotube) that combine the properties of both in a single structure.<ref name="nanobuds" />
Of the other discovered allotropes, [[carbon nanofoam]] is a [[ferromagnetic]] allotrope discovered in 1997. It consists of a low-density cluster-assembly of carbon atoms strung together in a loose three-dimensional web, in which the atoms are bonded trigonally in six- and seven-membered rings. It is among the lightest known solids, with a density of about 2 kg/m{{sup|3}}.<ref>{{cite journal|url=http://www.aip.org/pnu/2004/split/678-1.html|title=Carbon Nanofoam is the World's First Pure Carbon Magnet|volume=678|issue=1|date=March 26, 2004|author=Schewe, Phil|author2=Stein, Ben|last-author-amp=yes|journal=Physics News Update}}</ref> Similarly, [[glassy carbon]] contains a high proportion of closed [[porosity]],<ref name="glassy carbon"/> but contrary to normal graphite, the graphitic layers are not stacked like pages in a book, but have a more random arrangement. [[Linear acetylenic carbon]]<ref name=LAC/> has the chemical structure<ref name="LAC"/> -(C:::C){{sub|n}}-. Carbon in this modification is linear with ''sp'' [[orbital hybridization]], and is a [[polymer]] with alternating single and triple bonds. This type of carbyne is of considerable interest to [[nanotechnology]] as its [[Young's modulus]] is forty times that of the hardest known material – diamond.<ref>{{cite journal|title=Harder than Diamond: Determining the Cross-Sectional Area and Young's Modulus of Molecular Rods|author=Itzhaki, Lior|doi=10.1002/anie.200502448|journal=Angew. Chem. Int. Ed.|date=2005|volume=44|last2=Altus|first2=Eli|last3=Basch|first3=Harold|last4=Hoz|first4=Shmaryahu|pmid=16240306|issue=45|pages=7432–5}}</ref>
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Carbon is the [[Abundance of the chemical elements|fourth most abundant chemical element]] in the universe by mass after hydrogen, helium, and oxygen. Carbon is abundant in the [[Sun]], [[star]]s, [[comet]]s, and in the [[celestial body's atmosphere|atmospheres]] of most [[planet]]s.<ref name="NASA-20140221" /> Some [[meteorite]]s contain microscopic diamonds that were formed when the [[solar system]] was still a [[protoplanetary disk]]. Microscopic diamonds may also be formed by the intense pressure and high temperature at the sites of meteorite impacts.<ref>{{cite book|author=Mark, Kathleen|date=1987|title=Meteorite Craters|publisher=University of Arizona Press|isbn=0-8165-0902-6}}</ref>
In 2014 [[NASA]] announced a [http://www.astrochem.org/pahdb/ greatly upgraded database] for tracking [[polycyclic aromatic hydrocarbons]] (PAHs) in the [[universe]]. More than 20% of the carbon in the universe may be associated with PAHs, complex compounds of carbon and hydrogen without oxygen.<ref>{{cite news
It has been estimated that the solid earth as a whole contains 730 [[parts per million|ppm]] of carbon, with 2000 ppm in the core and 120 ppm in the combined mantle and crust.<ref>William F McDonough [http://quake.mit.edu/hilstgroup/CoreMantle/EarthCompo.pdf The composition of the Earth] in {{cite book|title=Earthquake Thermodynamics and Phase Transformation in the Earth's Interior|date=2000|isbn=978-0126851854}}</ref> Since the mass of the earth is {{val|5.972|e=24|u=kg}}, this would imply 4360 million [[gigatonne]]s of carbon. This is much more than the amounts in the oceans or atmosphere (below).
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[[Isotope]]s of carbon are [[atomic nucleus|atomic nuclei]] that contain six [[proton]]s plus a number of [[neutron]]s (varying from 2 to 16). Carbon has two stable, naturally occurring [[isotope]]s.<ref name="isotopes"/> The isotope [[carbon-12]] ({{sup|12}}C) forms 98.93% of the carbon on Earth, while [[carbon-13]] ({{sup|13}}C) forms the remaining 1.07%.<ref name="isotopes"/> The concentration of {{sup|12}}C is further increased in biological materials because biochemical reactions discriminate against {{sup|13}}C.<ref>{{cite journal|last=Gannes|first=Leonard Z.|last2=Del Rio|first2=Carlos Martı́nez|last3=Koch|first3=Paul|title=Natural Abundance Variations in Stable Isotopes and their Potential Uses in Animal Physiological Ecology|journal=Comparative Biochemistry and Physiology – Part A: Molecular & Integrative Physiology|volume=119|issue=3|pages=725–737|date=1998|doi=10.1016/S1095-6433(98)01016-2}}</ref> In 1961, the [[International Union of Pure and Applied Chemistry]] (IUPAC) adopted the isotope [[carbon-12]] as the basis for [[atomic weight]]s.<ref>{{cite web|url=http://www.bipm.org/en/si/base_units/|title=Official SI Unit definitions|accessdate=2007-12-21}}</ref> Identification of carbon in [[NMR]] experiments is done with the isotope {{sup|13}}C.
[[Carbon-14]] ({{sup|14}}C) is a naturally occurring [[radioisotope]] which occurs in trace amounts on Earth of up to 1 part per [[10^12|trillion]] (0.0000000001%), mostly confined to the atmosphere and superficial deposits, particularly of [[peat]] and other organic materials.<ref>{{cite web|last=Brown|first=Tom|date=March 1, 2006|url=http://www.llnl.gov/str/March06/Brown.html|title=Carbon Goes Full Circle in the Amazon|publisher=Lawrence Livermore National Laboratory|accessdate=2007-11-25}}</ref> This isotope decays by 0.158 MeV [[beta decay|β{{sup|−}} emission]]. Because of its relatively short [[half-life]] of 5730 years, {{sup|14}}C is virtually absent in ancient rocks, but is created in the [[upper atmosphere]] (lower [[stratosphere]] and upper [[troposphere]]) by interaction of [[nitrogen]] with [[cosmic ray]]s.<ref>{{cite book|first=S.|last=Bowman|date=1990|title=Interpreting the past: Radiocarbon dating|publisher=British Museum Press|isbn=0-7141-2047-2}}</ref> The abundance of {{sup|14}}C in the [[atmosphere]] and in living organisms is almost constant, but decreases predictably in their bodies after death. This principle is used in [[radiocarbon dating]], invented in 1949, which has been used extensively to determine the age of carbonaceous materials with ages up to about 40,000 years.<ref>{{cite book
There are 15 known isotopes of carbon and the shortest-lived of these is {{sup|8}}C which decays through [[proton emission]] and [[alpha decay]] and has a half-life of 1.98739x10{{sup|−21}} [[Second|s]].<ref>{{cite web|url=http://barwinski.net/isotopes/query_select.php|title=Use query for carbon-8|accessdate=2007-12-21|publisher=barwinski.net}}</ref> The exotic {{sup|19}}C exhibits a [[nuclear halo]], which means its [[radius]] is appreciably larger than would be expected if the [[Atomic nucleus|nucleus]] were a [[sphere]] of constant [[density]].<ref>{{cite journal|url=http://www.sciencemag.org/cgi/content/full/286/5437/28?ck=nck|title=Beaming Into the Dark Corners of the Nuclear Kitchen|doi=10.1126/science.286.5437.28|pages=28–31|date=1999|last1=Watson|first1=A.|journal=Science|volume=286|issue=5437}}</ref>
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===Formation in stars===
{{main|Triple-alpha process|CNO cycle}}
Formation of the carbon atomic nucleus requires a nearly simultaneous triple collision of [[alpha particle]]s ([[helium]] nuclei) within the core of a [[giant star|giant]] or [[supergiant]] star which is known as the [[triple-alpha process]], as the products of further nuclear fusion reactions of helium with hydrogen or another helium nucleus produce [[isotopes of lithium|lithium-5]] and [[isotopes of beryllium|beryllium-8]] respectively, both of which are highly unstable and decay almost instantly back into smaller nuclei.<ref name="Audi">{{cite journal|last1=Audi|first1=G|doi=10.1016/S0375-9474(97)00482-X|title=The Nubase evaluation of nuclear and decay properties|date=1997|pages=1–124|volume=624|journal=Nuclear Physics A|url=http://amdc.in2p3.fr/nubase/nubase97.pdf|bibcode=1997NuPhA.624....1A|last2=Bersillon|first2=O.|last3=Blachot|first3=J.|last4=Wapstra|first4=A.H.}}</ref> This happens in conditions of temperatures over 100 megakelvin and helium concentration that the rapid expansion and cooling of the early universe prohibited, and therefore no significant carbon was created during the [[Big Bang]]. Instead, the interiors of stars in the [[H-R diagram|horizontal branch]] transform three helium nuclei into carbon by means of this process.<ref name=" Ostlie" >{{cite book|author=Ostlie, D.A.|author2=Carroll, B.W.|last-author-amp=yes
Rotational transitions of various isotopic forms of carbon monoxide (for example, {{sup|12}}CO, {{sup|13}}CO, and C{{sup|18}}O) are detectable in the [[submillimetre astronomy|submillimeter]] wavelength range, and are used in the study of [[Star formation|newly forming stars]] in [[molecular clouds]].<ref>{{cite book|author=Pikelʹner, Solomon Borisovich|title=Star formation|url=http://books.google.com/books?id=qbGLgcxnfpIC&pg=PA38|accessdate=2011-06-06|date=1977|publisher=Springer|isbn=978-90-277-0796-3|pages=38–}}</ref>
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