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About: Deuterium
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endpoint"><i class="bi-box-arrow-up-right"></i> Sparql Endpoint </a> </li> </ul> </div> </div> </nav> <div style="margin-bottom: 60px"></div> <!-- /navbar --> <!-- page-header --> <section> <div class="container-xl"> <div class="row"> <div class="col"> <h1 id="title" class="display-6"><b>About:</b> <a href="http://dbpedia.org/resource/Deuterium">Deuterium</a> </h1> </div> </div> <div class="row"> <div class="col"> <div class="text-muted"> <span class="text-nowrap">An Entity of Type: <a href="http://dbpedia.org/class/yago/Part113809207">Part113809207</a>, </span> <span class="text-nowrap">from Named Graph: <a href="http://dbpedia.org">http://dbpedia.org</a>, </span> <span class="text-nowrap">within Data Space: <a href="http://dbpedia.org">dbpedia.org</a></span> </div> </div> </div> <div class="row pt-2"> <div class="col-xs-9 col-sm-10"> <p class="lead">Deuterium (or hydrogen-2, symbol 2H or deuterium, also known as heavy hydrogen) is one of two stable isotopes of hydrogen (the other being protium, or hydrogen-1). The nucleus of a deuterium atom, called a deuteron, contains one proton and one neutron, whereas the far more common protium has no neutrons in the nucleus. Deuterium has a natural abundance in Earth's oceans of about one atom in 6420 of hydrogen. Thus deuterium accounts for approximately 0.0156% (0.0312% by mass) of all the naturally occurring hydrogen in the oceans, while protium accounts for more than 99.98%. The abundance of deuterium changes slightly from one kind of natural water to another (see Vienna Standard Mean Ocean Water).</p> </div> <div class="col-xs-3 col-sm-2"> <a href="#" class="thumbnail"> <img src="http://commons.wikimedia.org/wiki/Special:FilePath/hydrogen-2.svg?width=300" alt="thumbnail" class="img-fluid" /> </a> </div> </div> </div> </section> <!-- page-header --> <!-- property-table --> <section> <div class="container-xl"> <div class="row"> <div class="table-responsive"> <table class="table table-hover table-sm table-light"> <thead> <tr> <th class="col-xs-3 ">Property</th> <th class="col-xs-9 px-3">Value</th> </tr> </thead> <tbody> <tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/abstract"><small>dbo:</small>abstract</a> </td><td class="col-10 text-break"><ul> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ca" >El deuteri, D o ²H és un dels isòtops estables de l'hidrogen. A diferència de la resta d'elements químics, els isòtops de l'hidrogen s'anomenen d'una manera específica: així, depenent de la composició del nucli atòmic, es parla de: * proti (H), fent referència a l'isòtop més comú, compost per un sol protó al nucli.; * de deuteri, isòtop que conté un protó i un neutró; * o de triti, que té un protó i dos neutrons (un neutró més que el deuteri). Té una massa d'uns dos dalton.</span><small> (ca)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="cs" >Jako deuterium se označuje atom s jádrem 2H, který má v jádře jeden proton a jeden neutron a od běžného vodíku se liší především atomovou hmotností, která činí 2,013 63 u. Často mu bývá přiřazována i chemická značka D, přestože se nejedná o jiný prvek. Jádro deuteria se označuje jako deuteron, což je částice s hmotností 2.013553212535(17) u a elektrickým nábojem + 1 e.</span><small> (cs)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ar" >الديوتيريوم (بالإنجليزية: Deuterium) (أو الهيدروجين -2، الرمز الكيميائي له D أو 2H، معروف أيضًا باسم الهيدروجين الثقيل) وهو الذرة التي تحتوي نواتها على بروتون واحد ونيوترون واحد وتسمى هذه الذرة بالهيدروجين الثقيل، وتسمى نواة الديوتريوم بالديوترون. وبذلك يعدّ الديوتريوم أحد النظائر الثلاثة الطبيعية للهيدروجين. حيث أن الشكل الشائع لذرة الهيدروجين هو ذرة مكونة من بروتون واحد فقط، وهذا هو النظير الأول للهيدروجين وأكثر تلك النظائر شهرة (يسمى أحياناً بالبروتيوم). وهناك نظير ثالث للهيدروجين يسمى التريشيوم (التريتيوم) وتكون نواة ذرة الهيدروجين في هذه الحالة مكونة من بروتون واحد ونيوترونين اثنين، والتريتيوم هو أثقل نظائر الهيدروجين الطبيعية وأكثرها ندرة. يوجد الديوتريوم في الطبيعة في مياه المحيطات والبحار، حيث أن هناك ذرة ديوتريوم واحدة من بين كل 6500 ذرة هيدروجين في الطبيعة (أي 154 لكل مليون). وبعبارة أخرى فإن نسبة الهيدوجين الثقيل إلى مجمل الهيدروجين الموجود في الطبيعة هي 0.015% (أو 0.030% بالنظر إلى الكتلة). ويعتقد أنه يمكن العثور على نسبة أكبر من الديوتريوم كلما توغلنا أكثر في عمق مياه المحيطات. من الناحية الفيزيائية فإن الديوتريوم هو غاز في درجة الحرارة العادية، وهو نظير مستقر إشعاعياً، أي أنه ليس له عمر نصف. كتلة هذا النظير هي 2.01355321270 وحدة كتل ذرية. يرمز للديوتريوم عادةً بالرمز D أو 2H، فمثلاً الرمز الكيميائي لجزيء الماء الثقيل هو D2O على خلاف جزيء الماء العادي والذي يرمز له بالرمز H2O. ومما يجدر ذكره أن الماء الثقيل أكثر لزوجة من الماء العادي وكثافته النسبية أعلى منه. الديوتيريوم هو أحد للهيدروجين (الآخر هو البروتيوم، أو الهيدروجين -1). على نواة من الديوتريوم ذرة، ودعا الديوترون، يحتوي على واحد بروتون واحد النيوترون، في حين أن البروتيوم أكثر شيوعا الآن لا يوجد لديه النيوترونات في النواة. يحتوي الديوتيريوم على وفرة طبيعية في محيطات الأرض تبلغ ذرة واحدة تقريبًا في 6420 من الهيدروجين. وهكذا يمثل الديوتيريوم حوالي 0.02٪ (0.03٪ بالكتلة) من كل الهيدروجين الطبيعي الموجود في المحيطات، بينما يمثل البروتيوم أكثر من 99.98٪. تتغير وفرة الديوتيريوم قليلاً من نوع واحد من المياه الطبيعية إلى نوع آخر (انظر معيار فيينا يعني مياه المحيط). اشتق اسم الديوتيريوم من الكلمة اليونانية deuteros، والتي تعني «الثانية»، للدلالة على الجسيمين اللذين يتألف منهما النواة. تم اكتشاف الديوتيريوم وتسميته في عام 1931 من قبل هارولد أوري. عندما تم اكتشاف النيوترون في عام 1932، جعل هذا التركيب النووي للديوتيريوم واضحًا، وفاز أوري بجائزة نوبل عام 1934 «لاكتشافه الهيدروجين الثقيل». بعد فترة وجيزة من اكتشاف الديوتيريوم، أنتج يوري وآخرون عينات من «الماء الثقيل» الذي كان محتوى الديوتيريوم فيه شديد التركيز. يتم تدمير الديوتيريوم في الأجزاء الداخلية للنجوم بشكل أسرع مما يتم إنتاجه. يعتقد أن العمليات الطبيعية الأخرى تنتج كمية ضئيلة من الديوتيريوم. تم إنتاج كل الديوتيريوم الموجود في الطبيعة تقريبًا في الانفجار العظيم قبل 13.8 مليار سنة، حيث يرجع أصل النسبة الأساسية أو البدائية من الهيدروجين -1 إلى الديوتيريوم (حوالي 26 ذرة من الديوتيريوم لكل مليون ذرة هيدروجين) منذ ذلك الوقت. هذه هي النسبة الموجودة في الكواكب الغازية العملاقة، مثل كوكب المشتري. وجد تحليل نسب الديوتيريوم والبروتيوم في المذنبات نتائج مشابهة جدًا لمتوسط النسبة في محيطات الأرض (156 ذرة ديوتيريوم لكل مليون ذرة هيدروجين). هذا يعزز النظريات القائلة بأن معظم مياه المحيطات على الأرض هي من أصل مذنب. نسبة الديوتيريوم إلى البروتيوم للمذنب 67P / Churyumov-Gerasimenko، كما تم قياسها بواسطة مسبار الفضاء Rosetta، تبلغ حوالي ثلاثة أضعاف نسبة مياه الأرض. هذا الرقم هو أعلى رقم تم قياسه حتى الآن في مذنب. وهكذا تستمر نسب الديوتيريوم والبروتيوم في أن تكون موضوعًا نشطًا للبحث في كل من علم الفلك وعلم المناخ.</span><small> (ar)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="el" >Το δευτέριο ή υδρογόνο-2 (σύμβολο D ή ²H, επίσης γνωστό ως βαρύ υδρογόνο) είναι το ένα από δύο (2) σταθερά ισότοπα του υδρογόνου. Η φυσική του αφθονία στους ωκεανούς της Γης είναι περίπου 1 άτομο δευτερίου ανά 6.420 άτομα υδρογόνου-1 (που ονομάζεται και «πρώτιο»). Έτσι, το δευτέριο αντιπροσωπεύει περίπου το 0,0156% (ή 0,0312% κατά μάζα) του συνόλου του φυσικά υπάρχοντος υδρογόνου στους ωκεανούς, ενώ το πιο κοινό ισότοπο, το πρώτιο αντιπροσωπεύει μια αφθονία πάνω από 99,98%. Η αφθονία του δευτερίου αλλάζει ελαφρά από το ένα είδος φυσικού νερού σε άλλο. Ο πυρήνας του δευτερίου, που ονομάζεται «δευτερόνιο», περιέχει ένα πρωτόνιο και ένα νετρόνιο, ενώ ο αντίστοιχος του πολύ πιο άφθονου πρώτιου δεν περιέχει κανένα νετρόνιο. Το όνομα του δευτερίου σχηματίστηκε από την ελληνική λέξη «δεύτερος», που δηλώνει ότι ο πυρήνας του περιέχει δύο (2) σωματίδια. Το δευτέριο ανακαλύφθηκε το 1931 από τον (Harold Urey), που έτσι κέρδισε το Βραβείο Νόμπελ το 1934. Η ανακάλυψη αυτή ακολουθήθηκε από την ανακάλυψη του νετρονίου, το 1932, που έκανε την πυρηνική δομή του δευτερίου προφανή. Σύντομα μετά την ανακάλυψη του δευτερίου, ο Ούρευ και άλλοι παρασκεύασαν δείγματα του βαρέος ύδατος, στο οποίο το δευτέριο έχει υψηλότερη συγκέντρωση δευτερίου (ως και 100% στο «καθαρό βαρύ ύδωρ») από ότι στο φυσικό νερό. Επειδή το δευτέριο καταστρέφεται στο εσωτερικό των άστρων ταχύτερα απ' ό,τι παράγεται, και επειδή άλλες φυσικές διεργασίες παράγουν μόνο ασήμαντες (σχετικά) ποσότητες δευτερίου, θεωρείται ότι σχεδόν όλο το δευτέριο που βρίσκεται στη φύση παράχθηκε από τη Μεγάλη Έκρηξη, πριν περίπου 13,8 δισεκατομμύρια χρόνια. Επίσης θεωρείται ότι η βασική φυσική αναλογία ισοτόπων (περίπου 26 άτομα δευτερίου ανά εκατομμύριο ατόμων υδρογόνου), προέρχεται επίσης από εκείνη την εποχή. Η ίδια ισοτοπική αναλογία βρέθηκε και στους αεριώδεις γιγαντιαίους πλανήτες, όπως ο Δίας. Ωστόσο, διαφορετικά αστρονομικά σώματα βρέθηκαν να έχουν διαφορετικές ισοτοπικές αναλογίες, που αποδίδεται στο φυσικό ισοτοπικό διαχωρισμό που συμβαίνει όταν η ηλιακή θερμότητα λιώνει τους πάγους των κομητών. Ομοίως, ο κύκλος του νερού στη Γη, ίσως εμπλουτίζει (αργά και σταδιακά) το δευτέριο στους ωκεανούς του πλανήτη μας, σε βάρος του πρώτιου. Στην πραγματικότητα, η ισοτοπική αναλογία δευτερίου/πρωτίου σε έναν αριθμό κομητών είναι παρόμοιος με την αντίστοιχη μέση αναλογία στους ωκεανούς της Γης (156) άτομα δευτερίου ανά εκατομμύριο ατόμων υδρογόνου). Το γεγονός αυτό οδήγησε σε θεωρίες σύμφωνα με τις οποίες μεγάλο μέρος από το νερό των ωκεανών της Γης προήλθε από κομήτες (που έπεσαν πάνω της) . Οι ισοτοπικές αναλογίες δευτερίου/πρωτίου συνεχίζουν έτσι να αποτελούν πεδίο έρευνας τόσο για την Αστρονομία, όσο και για την Κλιματολογία.</span><small> (el)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="de" >Deuterium (von altgriechisch δεύτερος deúteros, „der Zweite“) ist ein natürliches Isotop des Wasserstoffs. Sein Atomkern wird auch Deuteron genannt, er besteht aus einem Proton und einem Neutron. Deuterium (2H) wird aufgrund seiner Masse auch als „schwerer Wasserstoff“ bezeichnet. Es wurde 1931 von den US-amerikanischen Chemikern Harold C. Urey und Ferdinand Brickwedde sowie George Murphy entdeckt. Urey erhielt dafür 1934 den Nobelpreis für Chemie. Die beiden anderen natürlichen Isotope des Wasserstoffs sind Protium (1H) und Tritium (3H). Aufgrund der großen Bedeutung der Isotope und weil die Massen sich stark unterscheiden, verwendet man für die Isotope Deuterium und Tritium auch eigene Symbole: D und T. Der Name Deuterium stammt von Gilbert Newton Lewis (der Lehrer von Urey), der auch als erster schweren Wasserstoff herstellte. Hinweise auf das Isotop gab es schon mit der Entwicklung der Massenspektrometrie in den 1920ern.</span><small> (de)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="eo" >Deŭterio (el la greka δευτερον: "la dua") estas krom procio kaj tricio, izotopo de hidrogeno. Ĝia atomkerno estas nomata ankaŭ deŭterono.</span><small> (eo)</small></span></li> <li><span class="literal"><span property="dbo:abstract" lang="en" >Deuterium (or hydrogen-2, symbol 2H or deuterium, also known as heavy hydrogen) is one of two stable isotopes of hydrogen (the other being protium, or hydrogen-1). The nucleus of a deuterium atom, called a deuteron, contains one proton and one neutron, whereas the far more common protium has no neutrons in the nucleus. Deuterium has a natural abundance in Earth's oceans of about one atom in 6420 of hydrogen. Thus deuterium accounts for approximately 0.0156% (0.0312% by mass) of all the naturally occurring hydrogen in the oceans, while protium accounts for more than 99.98%. The abundance of deuterium changes slightly from one kind of natural water to another (see Vienna Standard Mean Ocean Water). The name deuterium is derived from the Greek deuteros, meaning "second", to denote the two particles composing the nucleus. Deuterium was discovered and named in 1931 by Harold Urey. When the neutron was discovered in 1932, this made the nuclear structure of deuterium obvious, and Urey won the Nobel Prize in 1934 "for his discovery of heavy hydrogen". Soon after deuterium's discovery, Urey and others produced samples of "heavy water" in which the deuterium content had been highly concentrated. Deuterium is destroyed in the interiors of stars faster than it is produced. Other natural processes are thought to produce only an insignificant amount of deuterium. Nearly all deuterium found in nature was produced in the Big Bang 13.8 billion years ago, as the basic or primordial ratio of hydrogen-1 to deuterium (about 26 atoms of deuterium per million hydrogen atoms) has its origin from that time. This is the ratio found in the gas giant planets, such as Jupiter. The analysis of deuterium–protium ratios in comets found results very similar to the mean ratio in Earth's oceans (156 atoms of deuterium per million hydrogen atoms). This reinforces theories that much of Earth's ocean water is of cometary origin. The deuterium–protium ratio of the comet 67P/Churyumov–Gerasimenko, as measured by the Rosetta space probe, is about three times that of Earth water. This figure is the highest yet measured in a comet. Deuterium–protium ratios thus continue to be an active topic of research in both astronomy and climatology.</span><small> (en)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="eu" >Deuterioa, isotopo zeinuaz ere ezaguna, naturan aurki dezakegun bigarren hidrogeno isotopo arruntena dugu. Protioa baino askoz eskasagoa da eta hidrogeno guztiaren %0,000115 osatzen du. Deuterio hitza isotopoak izendatzeko existitzen diren hitz gutxietako bat da, orohar isotopoek ez baitute izenik jasotzen zeinuaz besterik. 2H protioarekin batera hidrogenoaren isotopo egonkor bakarra dugu. izena egozten zaio, eta bi nukleoiz osatua du nukleoa, protoi batez eta neutroi batez. Ekilibrio elektrikoan elektroi bakarra izaten du. Lurreko hidrogenoaren %0,0026 eta %0,0184 artean deuterioa dugu. Isotopo honek ez du erradioaktibitaterik eta ez du giza osasunean eragin nabarmenik. atomo ugariz osaturiko urari `ur astun` izena egozten zaio deuterioa protioa baino astunagoa baita. Deuterioa eta deuterioak osatzen dituen substantziak marka ez-radioaktibo gixa erabili ohi dira saiakera kimikoetan baita 1H-NMR espektroskopiako solbente gixa. `Ur astuna` neutroi moderatzaile eta hozgarri gixa erabili ohi da erreaktore nuklearretan. Deuterioa fusio nuklearrerako erregai gixa erabili liteke, gaur egun frantzia egoaldean eraikitzen ari dira lehen fusio generadorea ITER proiektuaren baitan hain zuzen ere.</span><small> (eu)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="fr" >Le deutérium, noté 2H ou D, est l'isotope de l'hydrogène dont le nombre de masse est égal à 2 : son noyau atomique, appelé deuton ou deutéron, compte 1 proton et 1 neutron avec un spin 1+ pour une masse atomique de 2,014 101 777 8 g/mol. Il est caractérisé par un excès de masse de 13 135,722 9 keV et une énergie de liaison nucléaire par nucléon de 1 112 keV. Il s'agit d'un isotope stable découvert en 1931 par Harold Clayton Urey, chimiste à l'université Columbia ; cette découverte lui valut le prix Nobel de chimie en 1934.</span><small> (fr)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="es" >El deuterio (del griego Δεύτερος segundo), cuyo símbolo es ²H, es un isótopo estable del hidrógeno que se encuentra en la naturaleza con una abundancia del 0,015 % del total de átomos de hidrógeno (uno de cada 6500). El núcleo del deuterio está formado por un protón y un neutrón (el hidrógeno tiene solamente un protón). Cuando el isótopo pierde su electrón el ion resultante recibe el nombre de deuterón. El deuterio también recibe el nombre de hidrógeno pesado. Se puede nombrar como ²H o como D. Aunque no es un elemento diferenciado en el sentido estricto (es hidrógeno), la diferenciación entre las propiedades de los isótopos es tanto más acusada cuanto más ligero sea el elemento químico al que pertenecen. En el caso del deuterio las diferencias son máximas ya que tiene el doble de masa atómica que el hidrógeno. El deuterio fue detectado en 1931 por Harold Clayton Urey, un químico de la Universidad de Columbia. Urey ganó, en 1934, el Premio Nobel de química por este trabajo. La existencia del deuterio en la Tierra, otras partes del Sistema Solar (según lo confirmado por las sondas planetarias) y en los espectros de estrellas es un dato importante en cosmología. La fusión estelar destruye el deuterio y no hay procesos de creación naturales conocidos con excepción de la nucleosíntesis primordial, que pudo haber producido el deuterio en una abundancia cercana a la natural observada en este elemento. Esta abundancia parece ser una fracción muy similar a la del hidrógeno, dondequiera que se encuentre este. Así, la existencia del deuterio es una de las discusiones a favor de la teoría del Big Bang en vez de la teoría del estado estacionario del universo. El deuterio combinado con el oxígeno forma agua pesada.</span><small> (es)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ga" >Iseatóp trom hidrigine ina bhfuil prótón is neodrón sa núicléas (mar mhalairt ar phrótón amháin, mar atá sa bhunhidrigin). Úsáidtear D nó 2H mar shiombail dó. Is deoitéiriam 0.015% den hidrigin nádúrtha. Tugtar uisce trom ar uisce atá déanta as (D2O), le dlús 1.1 g cm-3, agus úsáidtear é seo in imoibreoirí núicléacha áirithe. Tábhachtach i gcomhleá núicléach freisin.</span><small> (ga)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="in" >Deuterium disebut juga Hidrogen-2, atau hidrogen berat (simbol ditulis D atau 2H) merupakan salah satu daripada tiga bentuk isotop hidrogen yang terdiri daripada protium, deuterium, dan tritium. Deuterium merupakan isotop stabil dengan kelimpahan alami di samudra Bumi kira-kira satu dari 6500 atom hidrogen (~154 ppm). Dengan demikian deuterium merupakan 0.015% (0.030% berat) dari semua hidrogen yang terbentuk secara alami. Inti deuterium, disebut deuteron, mengandung satu proton dan satu netron, sementara inti hidrogen paling umum terdiri dari hanya satu proton dan tanpa netron. Nama isotop berasal dari bahasa Yunani, deuteros yang berarti "dua", untuk menunjukkan 2 partikel sub-atomik yang menyusun inti.</span><small> (in)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ja" >重水素（じゅうすいそ、英: heavy hydrogen）またはデューテリウム (英: deuterium) とは、水素の安定同位体のうち、原子核が陽子1つと中性子1つとで構成されるものをいう。重水素は 2H と表記するが、 D（deuteriumの頭文字）と表記することもある。例えば重水の分子式を D2O と表記することがある。 原子核が陽子1つと中性子2つとで構成される水素（3H）は三重水素またはトリチウムと呼ばれる。重水素、三重水素に対して普通の水素（原子核が陽子1つのもの）は軽水素（1H）と呼ばれる。</span><small> (ja)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ko" >( 중양성자는 여기로 연결됩니다. 양성자 2개가 결합한 핵종에 대해서는 헬륨-2 문서를 참고하십시오.) 중수소(重水素)는 수소의 동위 원소 중 하나로 2H 또는 D(Deuterium)로 표기한다. 삼중수소와 구별하기 위해 이중수소(二重水素)라고 부르기도 한다.</span><small> (ko)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="it" >Il deuterio (dal greco δεύτερος déuteros, il secondo) è un isotopo stabile dell'idrogeno il cui nucleo (chiamato deutone o deuterone) è composto da un protone e un neutrone. Fu scoperto nel 1931 da Harold Urey, che per questo vinse il Premio Nobel per la chimica nel 1934. La sua abbondanza isotopica è pari a 0,015% (0,030% in termini di massa). Nonostante non sia propriamente un elemento chimico a sé stante, si utilizza il simbolo 2H o D per indicarlo. Come l'isotopo dell'idrogeno più comune, il prozio, a temperatura e pressione ambiente il deuterio forma un gas di molecole biatomiche con formula 2H2 o D2. Sulla terra si trova in natura in minima percentuale nella molecola dell'acqua, da cui può essere prodotta artificialmente acqua arricchita in deuterio, l'acqua pesante.</span><small> (it)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="nl" >Deuterium of 2H (occasioneel waterstof-2 genoemd) is een stabiele isotoop van waterstof met in de atoomkern een proton en een neutron. In plaats van de gebruikelijke notatie voor isotopen 2H wordt meestal gebruikgemaakt van het symbool D. In tegenstelling tot tritium, een andere isotoop van waterstof, is deuterium stabiel. De abundantie op Aarde is laag: ongeveer 0,015% van alle waterstofatomen is deuterium. Het meest voorkomende isotoop van waterstof is protium (1H). Deuterium werd in 1932 door Harold Urey ontdekt; hiervoor werd hem in 1934 de Nobelprijs voor de Scheikunde toegekend.De waterstof-isotoop deuterium dankt zijn naam aan het het Griekse woord deuteros, dat tweede betekent en daarmee verwijst naar het tweede deeltje in de kern van het waterstofatoom naast een proton: een neutron.</span><small> (nl)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="pt" >O deutério (símbolo ²H ou informalmente D) também conhecido como hidrogênio pesado é um dos isótopos estáveis do hidrogênio. O núcleo atômico do deutério é formado por um próton e um nêutron e sua massa atômica é de 2.014102. Foi descoberto em 1931 por por Harold Clayton Urey e seus colaboradores, que o separaram do hidrogênio por destilação fracionada a -259 °C. Esta descoberta lhe rendeu o Nobel de Química em 1934. O nome provém do grego deuteros que significa "segundo" mostrando as duas partículas que compunham o núcleo. As chances de encontrarmos o deutério na água marinha em moléculas de óxido de deutério (²H2O) são de 0,0156%, mas a concentração nos oceanos varia de acordo com a localização e a profundidade. Encontra-se na natureza na proporção de 1 para cada cerca de 6.410 átomos de hidrogênio.</span><small> (pt)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="pl" >Deuter (2H, D) – stabilny izotop wodoru występujący naturalnie. W wodzie morskiej (SMOW) występuje w ilości około 1 atomu na 6420 atomów protu (wodoru zwykłego, 1H) (około 0,02 grama w 1 litrze wody). Jądro deuteru (deuteron) składa się z jednego protonu i jednego neutronu, podczas gdy jądrem protu jest jeden proton. Masa atomowa deuteru jest około dwukrotnie większa od izotopu 1H i wynosi 2,0140 u. Deuter został odkryty w 1931 roku przez Harolda Claytona Ureya, chemika z Columbia University, za co otrzymał on Nagrodę Nobla z chemii w 1934 roku. Ze względu na małą masę i mały przekrój czynny (0,11 σ/fm²) deuter jest dobrym moderatorem szybkich neutronów. Związki deuteru (np. ciężka woda) wykorzystywane są w reaktorach jądrowych. Deuter może zastępować zwykły wodór we wszystkich związkach, co skutkuje zwykle niewielkimi, lecz stosunkowo łatwymi do zmierzenia, zmianami ich właściwości fizycznych i chemicznych. Woda zawierająca atomy deuteru nosi nazwę ciężkiej wody. W zależności od składu izotopowego wodoru ciężka woda może mieć wzór: * HDO – jeden z dwóch atomów wodoru jest zastąpiony atomem deuteru * D2O – obydwa atomy wodoru są zastąpione atomami deuteru</span><small> (pl)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="sv" >Deuterium, av grekiska deuteros ("den andre"), vanligen kallat tungt väte, är en stabil isotop av väte, där atomkärnan innehåller en neutron utöver den proton som kännetecknar den vanliga väteisotopen protium. Deuterium utgör 0,0156 procent av vätet på jorden. Isotopen betecknas 2H eller D. Deuterium har vissa egenskaper, till exempel låg absorption av neutroner, som gör den användbar som moderator i kärnreaktorer som använder icke-anrikat uran, då i form av tungt vatten (D2O). Deuterium kan även användas som bränsle i fusionreaktorer, både rent och blandat med tritium. Eftersom deuteriumkärnor är bosoner finns andra tillämpningar inom kärnmagnetisk resonans än för protium. Deuterium upptäcktes av Harold Urey 1931, vilket gav honom Nobelpriset i kemi 1934. En deuteriumkärna kallas också för deuteron eller deutron.</span><small> (sv)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="uk" >Дейте́рій (позначення: ²H, D) — стійкий ізотоп гідрогену з масовим числом 2.</span><small> (uk)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="zh" >氘（dāo）（英語：Deuterium），又称重氢、氫-2，為氢的一种穩定同位素，元素符号一般为D或2H。它的原子核由一颗质子和一颗中子组成。在大自然的含量约为一般氢的7000分之一。</span><small> (zh)</small></span></li> <li style="display:none;"><span class="literal"><span property="dbo:abstract" lang="ru" >Дейте́рий (лат. deuterium, от др.-греч. δεύτερος «второй»), тяжёлый водород, обозначается символами D и 2H — стабильный изотоп водорода с атомной массой, равной 2. Ядро (дейтрон) состоит из одного протона и одного нейтрона. Открыт в 1932 году американским физико-химиком Гарольдом Юри. Природное содержание — 0,0115 ± 0,0070 %.</span><small> (ru)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/thumbnail"><small>dbo:</small>thumbnail</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="dbo:thumbnail" resource="http://commons.wikimedia.org/wiki/Special:FilePath/hydrogen-2.svg?width=300" href="http://commons.wikimedia.org/wiki/Special:FilePath/hydrogen-2.svg?width=300"><small>wiki-commons</small>:Special:FilePath/hydrogen-2.svg?width=300</a></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/ontology/wikiPageExternalLink"><small>dbo:</small>wikiPageExternalLink</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="dbo:wikiPageExternalLink nofollow" resource="http://atom.kaeri.re.kr/" href="http://atom.kaeri.re.kr/">http://atom.kaeri.re.kr/</a></span></li> <li><span 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href="http://dbpedia.org/property/after"><small>dbp:</small>after</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:after" lang="en" >Stable</span><small> (en)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/alternateNames"><small>dbp:</small>alternateNames</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:alternateNames" lang="en" >hydrogen-2, D</span><small> (en)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/before"><small>dbp:</small>before</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:before" lang="en" >—</span><small> (en)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/date"><small>dbp:</small>date</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:date" lang="en" >February 2014</span><small> (en)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/element"><small>dbp:</small>element</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:element" lang="en" >hydrogen</span><small> (en)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/heavier"><small>dbp:</small>heavier</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="dbp:heavier" resource="http://dbpedia.org/resource/Tritium" href="http://dbpedia.org/resource/Tritium"><small>dbr</small>:Tritium</a></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/imageCaption"><small>dbp:</small>imageCaption</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:imageCaption" lang="en" >Deuterium isotope highlighted on a truncated table of nuclides for atomic numbers 1 through 29. 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Stable isotopes in blue.</span><small> (en)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/lighter"><small>dbp:</small>lighter</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="dbp:lighter" resource="http://dbpedia.org/resource/Hydrogen_atom" href="http://dbpedia.org/resource/Hydrogen_atom"><small>dbr</small>:Hydrogen_atom</a></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/mass"><small>dbp:</small>mass</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:mass" datatype="xsd:double" >2.014102</span><small> (xsd:double)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/massNumber"><small>dbp:</small>massNumber</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:massNumber" datatype="xsd:integer" >2</span><small> (xsd:integer)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/name"><small>dbp:</small>name</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:name" lang="en" >Deuterium, hydrogen-2</span><small> (en)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/numNeutrons"><small>dbp:</small>numNeutrons</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:numNeutrons" datatype="xsd:integer" >1</span><small> (xsd:integer)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/numProtons"><small>dbp:</small>numProtons</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:numProtons" datatype="xsd:integer" >1</span><small> (xsd:integer)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/reason"><small>dbp:</small>reason</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:reason" lang="en" >why did they need heavy water to run a reactor?</span><small> (en)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/spin"><small>dbp:</small>spin</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:spin" datatype="xsd:integer" >1</span><small> (xsd:integer)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://dbpedia.org/property/symbol"><small>dbp:</small>symbol</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><span property="dbp:symbol" lang="en" >H</span><small> (en)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a 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resource="http://dbpedia.org/class/yago/WikicatIsotopesOfHydrogen" href="http://dbpedia.org/class/yago/WikicatIsotopesOfHydrogen"><small>yago</small>:WikicatIsotopesOfHydrogen</a></span></li> <li><span class="literal"><a class="uri" rel="rdf:type" resource="http://dbpedia.org/class/yago/Substance100019613" href="http://dbpedia.org/class/yago/Substance100019613"><small>yago</small>:Substance100019613</a></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://www.w3.org/2000/01/rdf-schema#comment"><small>rdfs:</small>comment</a> </td><td class="col-10 text-break"><ul> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ca" >El deuteri, D o ²H és un dels isòtops estables de l'hidrogen. A diferència de la resta d'elements químics, els isòtops de l'hidrogen s'anomenen d'una manera específica: així, depenent de la composició del nucli atòmic, es parla de: * proti (H), fent referència a l'isòtop més comú, compost per un sol protó al nucli.; * de deuteri, isòtop que conté un protó i un neutró; * o de triti, que té un protó i dos neutrons (un neutró més que el deuteri). Té una massa d'uns dos dalton.</span><small> (ca)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="cs" >Jako deuterium se označuje atom s jádrem 2H, který má v jádře jeden proton a jeden neutron a od běžného vodíku se liší především atomovou hmotností, která činí 2,013 63 u. Často mu bývá přiřazována i chemická značka D, přestože se nejedná o jiný prvek. Jádro deuteria se označuje jako deuteron, což je částice s hmotností 2.013553212535(17) u a elektrickým nábojem + 1 e.</span><small> (cs)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="eo" >Deŭterio (el la greka δευτερον: "la dua") estas krom procio kaj tricio, izotopo de hidrogeno. Ĝia atomkerno estas nomata ankaŭ deŭterono.</span><small> (eo)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="fr" >Le deutérium, noté 2H ou D, est l'isotope de l'hydrogène dont le nombre de masse est égal à 2 : son noyau atomique, appelé deuton ou deutéron, compte 1 proton et 1 neutron avec un spin 1+ pour une masse atomique de 2,014 101 777 8 g/mol. Il est caractérisé par un excès de masse de 13 135,722 9 keV et une énergie de liaison nucléaire par nucléon de 1 112 keV. Il s'agit d'un isotope stable découvert en 1931 par Harold Clayton Urey, chimiste à l'université Columbia ; cette découverte lui valut le prix Nobel de chimie en 1934.</span><small> (fr)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ga" >Iseatóp trom hidrigine ina bhfuil prótón is neodrón sa núicléas (mar mhalairt ar phrótón amháin, mar atá sa bhunhidrigin). Úsáidtear D nó 2H mar shiombail dó. Is deoitéiriam 0.015% den hidrigin nádúrtha. Tugtar uisce trom ar uisce atá déanta as (D2O), le dlús 1.1 g cm-3, agus úsáidtear é seo in imoibreoirí núicléacha áirithe. Tábhachtach i gcomhleá núicléach freisin.</span><small> (ga)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="in" >Deuterium disebut juga Hidrogen-2, atau hidrogen berat (simbol ditulis D atau 2H) merupakan salah satu daripada tiga bentuk isotop hidrogen yang terdiri daripada protium, deuterium, dan tritium. Deuterium merupakan isotop stabil dengan kelimpahan alami di samudra Bumi kira-kira satu dari 6500 atom hidrogen (~154 ppm). Dengan demikian deuterium merupakan 0.015% (0.030% berat) dari semua hidrogen yang terbentuk secara alami. Inti deuterium, disebut deuteron, mengandung satu proton dan satu netron, sementara inti hidrogen paling umum terdiri dari hanya satu proton dan tanpa netron. Nama isotop berasal dari bahasa Yunani, deuteros yang berarti "dua", untuk menunjukkan 2 partikel sub-atomik yang menyusun inti.</span><small> (in)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ja" >重水素（じゅうすいそ、英: heavy hydrogen）またはデューテリウム (英: deuterium) とは、水素の安定同位体のうち、原子核が陽子1つと中性子1つとで構成されるものをいう。重水素は 2H と表記するが、 D（deuteriumの頭文字）と表記することもある。例えば重水の分子式を D2O と表記することがある。 原子核が陽子1つと中性子2つとで構成される水素（3H）は三重水素またはトリチウムと呼ばれる。重水素、三重水素に対して普通の水素（原子核が陽子1つのもの）は軽水素（1H）と呼ばれる。</span><small> (ja)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ko" >( 중양성자는 여기로 연결됩니다. 양성자 2개가 결합한 핵종에 대해서는 헬륨-2 문서를 참고하십시오.) 중수소(重水素)는 수소의 동위 원소 중 하나로 2H 또는 D(Deuterium)로 표기한다. 삼중수소와 구별하기 위해 이중수소(二重水素)라고 부르기도 한다.</span><small> (ko)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="uk" >Дейте́рій (позначення: ²H, D) — стійкий ізотоп гідрогену з масовим числом 2.</span><small> (uk)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="zh" >氘（dāo）（英語：Deuterium），又称重氢、氫-2，為氢的一种穩定同位素，元素符号一般为D或2H。它的原子核由一颗质子和一颗中子组成。在大自然的含量约为一般氢的7000分之一。</span><small> (zh)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ru" >Дейте́рий (лат. deuterium, от др.-греч. δεύτερος «второй»), тяжёлый водород, обозначается символами D и 2H — стабильный изотоп водорода с атомной массой, равной 2. Ядро (дейтрон) состоит из одного протона и одного нейтрона. Открыт в 1932 году американским физико-химиком Гарольдом Юри. Природное содержание — 0,0115 ± 0,0070 %.</span><small> (ru)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="ar" >الديوتيريوم (بالإنجليزية: Deuterium) (أو الهيدروجين -2، الرمز الكيميائي له D أو 2H، معروف أيضًا باسم الهيدروجين الثقيل) وهو الذرة التي تحتوي نواتها على بروتون واحد ونيوترون واحد وتسمى هذه الذرة بالهيدروجين الثقيل، وتسمى نواة الديوتريوم بالديوترون. وبذلك يعدّ الديوتريوم أحد النظائر الثلاثة الطبيعية للهيدروجين. حيث أن الشكل الشائع لذرة الهيدروجين هو ذرة مكونة من بروتون واحد فقط، وهذا هو النظير الأول للهيدروجين وأكثر تلك النظائر شهرة (يسمى أحياناً بالبروتيوم). وهناك نظير ثالث للهيدروجين يسمى التريشيوم (التريتيوم) وتكون نواة ذرة الهيدروجين في هذه الحالة مكونة من بروتون واحد ونيوترونين اثنين، والتريتيوم هو أثقل نظائر الهيدروجين الطبيعية وأكثرها ندرة.</span><small> (ar)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="el" >Το δευτέριο ή υδρογόνο-2 (σύμβολο D ή ²H, επίσης γνωστό ως βαρύ υδρογόνο) είναι το ένα από δύο (2) σταθερά ισότοπα του υδρογόνου. Η φυσική του αφθονία στους ωκεανούς της Γης είναι περίπου 1 άτομο δευτερίου ανά 6.420 άτομα υδρογόνου-1 (που ονομάζεται και «πρώτιο»). Έτσι, το δευτέριο αντιπροσωπεύει περίπου το 0,0156% (ή 0,0312% κατά μάζα) του συνόλου του φυσικά υπάρχοντος υδρογόνου στους ωκεανούς, ενώ το πιο κοινό ισότοπο, το πρώτιο αντιπροσωπεύει μια αφθονία πάνω από 99,98%. Η αφθονία του δευτερίου αλλάζει ελαφρά από το ένα είδος φυσικού νερού σε άλλο.</span><small> (el)</small></span></li> <li><span class="literal"><span property="rdfs:comment" lang="en" >Deuterium (or hydrogen-2, symbol 2H or deuterium, also known as heavy hydrogen) is one of two stable isotopes of hydrogen (the other being protium, or hydrogen-1). The nucleus of a deuterium atom, called a deuteron, contains one proton and one neutron, whereas the far more common protium has no neutrons in the nucleus. Deuterium has a natural abundance in Earth's oceans of about one atom in 6420 of hydrogen. Thus deuterium accounts for approximately 0.0156% (0.0312% by mass) of all the naturally occurring hydrogen in the oceans, while protium accounts for more than 99.98%. The abundance of deuterium changes slightly from one kind of natural water to another (see Vienna Standard Mean Ocean Water).</span><small> (en)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="de" >Deuterium (von altgriechisch δεύτερος deúteros, „der Zweite“) ist ein natürliches Isotop des Wasserstoffs. Sein Atomkern wird auch Deuteron genannt, er besteht aus einem Proton und einem Neutron. Deuterium (2H) wird aufgrund seiner Masse auch als „schwerer Wasserstoff“ bezeichnet. Es wurde 1931 von den US-amerikanischen Chemikern Harold C. Urey und Ferdinand Brickwedde sowie George Murphy entdeckt. Urey erhielt dafür 1934 den Nobelpreis für Chemie.</span><small> (de)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="eu" >Deuterioa, isotopo zeinuaz ere ezaguna, naturan aurki dezakegun bigarren hidrogeno isotopo arruntena dugu. Protioa baino askoz eskasagoa da eta hidrogeno guztiaren %0,000115 osatzen du. Deuterio hitza isotopoak izendatzeko existitzen diren hitz gutxietako bat da, orohar isotopoek ez baitute izenik jasotzen zeinuaz besterik. 2H protioarekin batera hidrogenoaren isotopo egonkor bakarra dugu. izena egozten zaio, eta bi nukleoiz osatua du nukleoa, protoi batez eta neutroi batez. Ekilibrio elektrikoan elektroi bakarra izaten du. Lurreko hidrogenoaren %0,0026 eta %0,0184 artean deuterioa dugu. Isotopo honek ez du erradioaktibitaterik eta ez du giza osasunean eragin nabarmenik. atomo ugariz osaturiko urari `ur astun` izena egozten zaio deuterioa protioa baino astunagoa baita. Deuterioa eta deu</span><small> (eu)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="es" >El deuterio (del griego Δεύτερος segundo), cuyo símbolo es ²H, es un isótopo estable del hidrógeno que se encuentra en la naturaleza con una abundancia del 0,015 % del total de átomos de hidrógeno (uno de cada 6500). El núcleo del deuterio está formado por un protón y un neutrón (el hidrógeno tiene solamente un protón). Cuando el isótopo pierde su electrón el ion resultante recibe el nombre de deuterón. El deuterio fue detectado en 1931 por Harold Clayton Urey, un químico de la Universidad de Columbia. Urey ganó, en 1934, el Premio Nobel de química por este trabajo.</span><small> (es)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="it" >Il deuterio (dal greco δεύτερος déuteros, il secondo) è un isotopo stabile dell'idrogeno il cui nucleo (chiamato deutone o deuterone) è composto da un protone e un neutrone. Fu scoperto nel 1931 da Harold Urey, che per questo vinse il Premio Nobel per la chimica nel 1934.</span><small> (it)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="pl" >Deuter (2H, D) – stabilny izotop wodoru występujący naturalnie. W wodzie morskiej (SMOW) występuje w ilości około 1 atomu na 6420 atomów protu (wodoru zwykłego, 1H) (około 0,02 grama w 1 litrze wody). Jądro deuteru (deuteron) składa się z jednego protonu i jednego neutronu, podczas gdy jądrem protu jest jeden proton. Masa atomowa deuteru jest około dwukrotnie większa od izotopu 1H i wynosi 2,0140 u. Deuter został odkryty w 1931 roku przez Harolda Claytona Ureya, chemika z Columbia University, za co otrzymał on Nagrodę Nobla z chemii w 1934 roku.</span><small> (pl)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="nl" >Deuterium of 2H (occasioneel waterstof-2 genoemd) is een stabiele isotoop van waterstof met in de atoomkern een proton en een neutron. In plaats van de gebruikelijke notatie voor isotopen 2H wordt meestal gebruikgemaakt van het symbool D. In tegenstelling tot tritium, een andere isotoop van waterstof, is deuterium stabiel. De abundantie op Aarde is laag: ongeveer 0,015% van alle waterstofatomen is deuterium. Het meest voorkomende isotoop van waterstof is protium (1H). Deuterium werd in 1932 door Harold Urey ontdekt; hiervoor werd hem in 1934 de Nobelprijs voor de Scheikunde toegekend.De waterstof-isotoop deuterium dankt zijn naam aan het het Griekse woord deuteros, dat tweede betekent en daarmee verwijst naar het tweede deeltje in de kern van het waterstofatoom naast een proton: een neutro</span><small> (nl)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="pt" >O deutério (símbolo ²H ou informalmente D) também conhecido como hidrogênio pesado é um dos isótopos estáveis do hidrogênio. O núcleo atômico do deutério é formado por um próton e um nêutron e sua massa atômica é de 2.014102. Foi descoberto em 1931 por por Harold Clayton Urey e seus colaboradores, que o separaram do hidrogênio por destilação fracionada a -259 °C. Esta descoberta lhe rendeu o Nobel de Química em 1934. O nome provém do grego deuteros que significa "segundo" mostrando as duas partículas que compunham o núcleo.</span><small> (pt)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:comment" lang="sv" >Deuterium, av grekiska deuteros ("den andre"), vanligen kallat tungt väte, är en stabil isotop av väte, där atomkärnan innehåller en neutron utöver den proton som kännetecknar den vanliga väteisotopen protium. Deuterium utgör 0,0156 procent av vätet på jorden. Deuterium upptäcktes av Harold Urey 1931, vilket gav honom Nobelpriset i kemi 1934. En deuteriumkärna kallas också för deuteron eller deutron.</span><small> (sv)</small></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://www.w3.org/2000/01/rdf-schema#label"><small>rdfs:</small>label</a> </td><td class="col-10 text-break"><ul> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ar" >ديوتيريوم</span><small> (ar)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ca" >Deuteri</span><small> (ca)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="cs" >Deuterium</span><small> (cs)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="de" >Deuterium</span><small> (de)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="el" >Δευτέριο</span><small> (el)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="eo" >Deŭterio</span><small> (eo)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="es" >Deuterio</span><small> (es)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="eu" >Deuterio</span><small> (eu)</small></span></li> <li><span class="literal"><span property="rdfs:label" lang="en" >Deuterium</span><small> (en)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ga" >Deoitéiriam</span><small> (ga)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="fr" >Deutérium</span><small> (fr)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="in" >Deuterium</span><small> (in)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="it" >Deuterio</span><small> (it)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ko" >중수소</span><small> (ko)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ja" >重水素</span><small> (ja)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="nl" >Deuterium</span><small> (nl)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="pl" >Deuter</span><small> (pl)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="pt" >Deutério</span><small> (pt)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="sv" >Deuterium</span><small> (sv)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="ru" >Дейтерий</span><small> (ru)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="uk" >Дейтерій</span><small> (uk)</small></span></li> <li style="display:none;"><span class="literal"><span property="rdfs:label" lang="zh" >氘</span><small> (zh)</small></span></li> </ul></td></tr><tr class="odd"><td class="col-2"><a class="uri" href="http://www.w3.org/2000/01/rdf-schema#seeAlso"><small>rdfs:</small>seeAlso</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="rdfs:seeAlso" resource="http://dbpedia.org/resource/Proton_radius_puzzle" href="http://dbpedia.org/resource/Proton_radius_puzzle"><small>dbr</small>:Proton_radius_puzzle</a></span></li> <li><span class="literal"><a class="uri" rel="rdfs:seeAlso" resource="http://dbpedia.org/resource/Proton_NMR" href="http://dbpedia.org/resource/Proton_NMR"><small>dbr</small>:Proton_NMR</a></span></li> </ul></td></tr><tr class="even"><td class="col-2"><a class="uri" href="http://www.w3.org/2002/07/owl#sameAs"><small>owl:</small>sameAs</a> </td><td class="col-10 text-break"><ul> <li><span class="literal"><a class="uri" rel="owl:sameAs" resource="http://rdf.freebase.com/ns/m.02clk" href="http://rdf.freebase.com/ns/m.02clk"><small>freebase</small>:Deuterium</a></span></li> <li><span class="literal"><a class="uri" rel="owl:sameAs" resource="http://d-nb.info/gnd/4149226-2" href="http://d-nb.info/gnd/4149226-2">http://d-nb.info/gnd/4149226-2</a></span></li> <li><span class="literal"><a class="uri" rel="owl:sameAs" resource="http://www.wikidata.org/entity/Q102296" href="http://www.wikidata.org/entity/Q102296"><small>wikidata</small>:Deuterium</a></span></li> <li><span class="literal"><a class="uri" rel="owl:sameAs" resource="http://af.dbpedia.org/resource/Deuterium" href="http://af.dbpedia.org/resource/Deuterium"><small>dbpedia-af</small>:Deuterium</a></span></li> <li><span class="literal"><a class="uri" rel="owl:sameAs" 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