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== Characteristics == [[File:Solid and liquid xenon.jpg|left|thumb|A layer of solid xenon floating on top of liquid xenon inside a high voltage apparatus]] [[File:Xe nanoparticles in Al.jpg|thumb|left|Liquid (featureless) and crystalline solid Xe nanoparticles produced by implanting Xe<sup>+</sup> ions into aluminium at room temperature]] Xenon has [[atomic number]] 54; that is, its nucleus contains 54 [[proton]]s. At [[standard temperature and pressure]], pure xenon gas has a density of 5.894 kg/m<sup>3</sup>, about 4.5 times the density of the Earth's atmosphere at sea level, 1.217 kg/m<sup>3</sup>.<ref>{{cite web | last = Williams | first = David R. | date = April 19, 2007 | url = http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html | title = Earth Fact Sheet | publisher = NASA | access-date = October 4, 2007 }}</ref> As a liquid, xenon has a density of up to 3.100 g/mL, with the density maximum occurring at the triple point.<ref name="detectors">{{cite book | first1 = Elena | last1 = Aprile | author2 = Bolotnikov, Aleksey E. | author3 = Doke, Tadayoshi | title = Noble Gas Detectors | publisher = [[Wiley-VCH]] | date = 2006 | isbn = 3-527-60963-6 | url = https://books.google.com/books?id=tsnHM8x6cHAC&pg=PT1 | pages = 8–9 }}</ref> Liquid xenon has a high polarizability due to its large atomic volume, and thus is an excellent solvent. It can dissolve hydrocarbons, biological molecules, and even water.<ref>{{Cite journal | title = Xenon as a solvent | journal = Nature | date = September 10, 1981 | pages = 165–166 | volume = 293 | issue = 5828 | doi = 10.1038/293165a0 | author-link1 = Peter M. Rentzepis | first1 = P. M. | last1 = Rentzepis | first2 = D. C. | last2 = Douglass | s2cid = 4237285 | bibcode = 1981Natur.293..165R }}</ref> Under the same conditions, the density of solid xenon, 3.640 g/cm<sup>3</sup>, is greater than the average density of [[granite]], 2.75 g/cm<sup>3</sup>.<ref name="detectors" /> Under [[pascal (unit)|gigapascals]] of [[pressure]], xenon forms a metallic phase.<ref>{{cite journal | last1 = Caldwell | first1 = W. A. | author2 = Nguyen, J. | author3 = Pfrommer, B. | author4 = Louie, S. | author5 = Jeanloz, R. | author-link5 = Raymond Jeanloz | date = 1997 | title = Structure, bonding and geochemistry of xenon at high pressures | journal = [[Science (journal)|Science]] | volume = 277 | issue = 5328 | pages = 930–933 | doi = 10.1126/science.277.5328.930 }}</ref> Solid xenon changes from [[Face-centered cubic]] (fcc) to [[Close-packing of spheres|hexagonal close packed]] (hcp) crystal phase under pressure and begins to turn metallic at about 140 GPa, with no noticeable volume change in the hcp phase.<ref name=":0"> {{cite web|first=E.|last=Fontes |title=Golden Anniversary for Founder of High-pressure Program at CHESS|publisher=Cornell University |url=http://news.chess.cornell.edu/articles/2006/RuoffAnnv.html|access-date=May 30, 2009 }}</ref> It is completely metallic at 155 GPa.<ref>{{cite journal | author1 = Eremets, Mikhail I. | author-link = Mikhail Eremets | author2 = Gregoryanz, Eugene A. | author3 = Struzhkin, Victor V. | author4 = Mao, Ho-Kwang | author5 = Hemley, Russell J. | author6 = Mulders, Norbert | author7 = Zimmerman, Neil M. | year = 2000 | title = Electrical Conductivity of Xenon at Megabar Pressures | journal = Physical Review Letters | volume = 85 | issue = 13 | pages = 2797–800 | bibcode = 2000PhRvL..85.2797E | doi = 10.1103/PhysRevLett.85.2797 | pmid = 10991236 | s2cid = 19937739 }}</ref> When metallized, xenon appears sky blue because it absorbs red light and transmits other visible frequencies. Such behavior is unusual for a metal and is explained by the relatively small width of the electron bands in that state.<ref name="Fontes">{{cite web | first = E. | last = Fontes | title = Golden Anniversary for Founder of High-pressure Program at CHESS | publisher = Cornell University | url = http://news.chess.cornell.edu/articles/2006/RuoffAnnv.html | access-date = May 30, 2009 }}</ref>{{Better citation needed|reason=The current source is self-published (by a university) and not primarily scientific|date=May 2024}} [[File:Xenon-flash.gif|thumb|200px|Xenon flashing inside a [[flashtube]] frame by frame]] Liquid or solid xenon [[nanoparticle]]s can be formed at room temperature by implanting Xe<sup>+</sup> ions into a solid matrix. Many solids have lattice constants smaller than solid Xe. This results in compression of the implanted Xe to pressures that may be sufficient for its liquefaction or solidification.<ref>{{cite journal | last1 = Iakoubovskii | first1 = Konstantin | last2 = Mitsuishi | first2 = Kazutaka | last3 = Furuya | first3 = Kazuo | title = Structure and pressure inside Xe nanoparticles embedded in Al | journal = Physical Review B | volume = 78 | issue = 6 | pages = 064105 | year = 2008 | doi = 10.1103/PhysRevB.78.064105 | s2cid = 29156048 | bibcode = 2008PhRvB..78f4105I | url = https://mdr.nims.go.jp/pid/0e7dcc69-b57a-41e3-8c29-470317925117 }}</ref> Xenon is a member of the zero-[[Valence (chemistry)|valence]] elements that are called [[noble gas|noble]] or [[inert gas]]es. It is inert to most common chemical reactions (such as combustion, for example) because the outer [[valence shell]] contains eight electrons. This produces a stable, minimum energy configuration in which the outer electrons are tightly bound.<ref>{{cite web | last = Bader | first = Richard F. W. | url = http://miranda.chemistry.mcmaster.ca/esam/ | title = An Introduction to the Electronic Structure of Atoms and Molecules | publisher = [[McMaster University]] | access-date = September 27, 2007 }}</ref> In a [[gas-filled tube]], xenon emits a [[blue]] or [[lavender (color)|lavenderish]] glow when excited by [[Electric arc|electrical discharge]]. Xenon emits a band of [[Spectral line|emission lines]] that span the visual spectrum,<ref>{{cite web | last = Talbot | first = John | url = http://web.physik.rwth-aachen.de/~harm/aixphysik/atom/discharge/index1.html | title = Spectra of Gas Discharges | publisher = Rheinisch-Westfälische Technische Hochschule Aachen | access-date = August 10, 2006 | url-status = dead | archive-url = https://web.archive.org/web/20070718115616/http://web.physik.rwth-aachen.de/~harm/aixphysik/atom/discharge/index1.html | archive-date = July 18, 2007 }}</ref> but the most intense lines occur in the region of blue light, producing the coloration.<ref>{{cite book | first = William Marshall | last = Watts | date = 1904 | title = An Introduction to the Study of Spectrum Analysis | url = https://archive.org/details/anintroductiont00hugggoog | publisher = [[Longmans, Green, and Co.]] | location = London }}</ref>
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