{"id":40,"date":"2026-05-11T11:49:58","date_gmt":"2026-05-11T09:49:58","guid":{"rendered":"https:\/\/institucional.us.es\/astro21\/?page_id=40"},"modified":"2026-05-19T18:25:23","modified_gmt":"2026-05-19T16:25:23","slug":"que-es-ams","status":"publish","type":"page","link":"https:\/\/institucional.us.es\/astro21\/que-es-ams\/","title":{"rendered":"\u00bfQu\u00e9 es AMS?"},"content":{"rendered":"\t\t<div data-elementor-type=\"wp-page\" data-elementor-id=\"40\" class=\"elementor elementor-40\" data-elementor-post-type=\"page\">\n\t\t\t\t<div class=\"elementor-element elementor-element-a51a8c1 e-flex e-con-boxed e-con e-parent\" data-id=\"a51a8c1\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-5b61e7f elementor-icon-list--layout-inline elementor-align-center elementor-list-item-link-full_width elementor-widget elementor-widget-icon-list\" data-id=\"5b61e7f\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-list.default\">\n\t\t\t\t\t\t\t<ul class=\"elementor-icon-list-items elementor-inline-items\">\n\t\t\t\t\t\t\t<li class=\"elementor-icon-list-item elementor-inline-item\">\n\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/institucional.us.es\/astro21\/por-que-necesitamos-un-nuevo-inyector\/\">\n\n\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-icon-list-icon\">\n\t\t\t\t\t\t\t<svg aria-hidden=\"true\" class=\"e-font-icon-svg e-fas-info-circle\" viewBox=\"0 0 512 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><path d=\"M256 8C119.043 8 8 119.083 8 256c0 136.997 111.043 248 248 248s248-111.003 248-248C504 119.083 392.957 8 256 8zm0 110c23.196 0 42 18.804 42 42s-18.804 42-42 42-42-18.804-42-42 18.804-42 42-42zm56 254c0 6.627-5.373 12-12 12h-88c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h12v-64h-12c-6.627 0-12-5.373-12-12v-24c0-6.627 5.373-12 12-12h64c6.627 0 12 5.373 12 12v100h12c6.627 0 12 5.373 12 12v24z\"><\/path><\/svg>\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-icon-list-text\">\u00bfPor qu\u00e9 necesitamos un nuevo inyector?<\/span>\n\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t<\/li>\n\t\t\t\t\t\t\t\t<li class=\"elementor-icon-list-item elementor-inline-item\">\n\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/institucional.us.es\/astro21\/que-hace-el-inyector-en-un-sistema-ams\/\">\n\n\t\t\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-icon-list-icon\">\n\t\t\t\t\t\t\t<svg aria-hidden=\"true\" class=\"e-font-icon-svg e-fas-atom\" viewBox=\"0 0 448 512\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><path d=\"M223.99908,224a32,32,0,1,0,32.00782,32A32.06431,32.06431,0,0,0,223.99908,224Zm214.172-96c-10.877-19.5-40.50979-50.75-116.27544-41.875C300.39168,34.875,267.63386,0,223.99908,0s-76.39066,34.875-97.89653,86.125C50.3369,77.375,20.706,108.5,9.82907,128-6.54984,157.375-5.17484,201.125,34.958,256-5.17484,310.875-6.54984,354.625,9.82907,384c29.13087,52.375,101.64652,43.625,116.27348,41.875C147.60842,477.125,180.36429,512,223.99908,512s76.3926-34.875,97.89652-86.125c14.62891,1.75,87.14456,10.5,116.27544-41.875C454.55,354.625,453.175,310.875,413.04017,256,453.175,201.125,454.55,157.375,438.171,128ZM63.33886,352c-4-7.25-.125-24.75,15.00391-48.25,6.87695,6.5,14.12891,12.875,21.88087,19.125,1.625,13.75,4,27.125,6.75,40.125C82.34472,363.875,67.09081,358.625,63.33886,352Zm36.88478-162.875c-7.752,6.25-15.00392,12.625-21.88087,19.125-15.12891-23.5-19.00392-41-15.00391-48.25,3.377-6.125,16.37891-11.5,37.88478-11.5,1.75,0,3.875.375,5.75.375C104.09864,162.25,101.84864,175.625,100.22364,189.125ZM223.99908,64c9.50195,0,22.25586,13.5,33.88282,37.25-11.252,3.75-22.50391,8-33.88282,12.875-11.377-4.875-22.62892-9.125-33.88283-12.875C201.74516,77.5,214.49712,64,223.99908,64Zm0,384c-9.502,0-22.25392-13.5-33.88283-37.25,11.25391-3.75,22.50587-8,33.88283-12.875C235.378,402.75,246.62994,407,257.8819,410.75,246.25494,434.5,233.501,448,223.99908,448Zm0-112a80,80,0,1,1,80-80A80.00023,80.00023,0,0,1,223.99908,336ZM384.6593,352c-3.625,6.625-19.00392,11.875-43.63479,11,2.752-13,5.127-26.375,6.752-40.125,7.75195-6.25,15.00391-12.625,21.87891-19.125C384.7843,327.25,388.6593,344.75,384.6593,352ZM369.65538,208.25c-6.875-6.5-14.127-12.875-21.87891-19.125-1.625-13.5-3.875-26.875-6.752-40.25,1.875,0,4.002-.375,5.752-.375,21.50391,0,34.50782,5.375,37.88283,11.5C388.6593,167.25,384.7843,184.75,369.65538,208.25Z\"><\/path><\/svg>\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t<span class=\"elementor-icon-list-text\">\u00bfQu\u00e9 hace el inyector en un sistema AMS?<\/span>\n\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t<\/li>\n\t\t\t\t\t\t<\/ul>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-4dca7bc e-grid e-con-full e-con e-parent\" data-id=\"4dca7bc\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t<div class=\"elementor-element elementor-element-b8224e7 e-con-full e-flex e-con e-child\" data-id=\"b8224e7\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t<div class=\"elementor-element elementor-element-5bad0ee elementor-widget elementor-widget-text-editor\" data-id=\"5bad0ee\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>La Espectrometr\u00eda de Masas es una t\u00e9cnica que permite separar iones at\u00f3micos o moleculares que se mueven en funci\u00f3n de su masa, gracias a la aplicaci\u00f3n de campos magn\u00e9ticos y electrost\u00e1ticos.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-be3d23e e-con-full e-flex e-con e-child\" data-id=\"be3d23e\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t<div class=\"elementor-element elementor-element-4fe7a79 elementor-widget elementor-widget-text-editor\" data-id=\"4fe7a79\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>La Espectrometr\u00eda de Masas con Acelerador (AMS) a\u00f1ade a la Espectrometr\u00eda de Masas tradicional el uso de un acelerador electrost\u00e1tico. Esto permite incrementar de una manera extraordinaria la capacidad de distinguir los iones de inter\u00e9s de otros interferentes. Se aplica a la detecci\u00f3n de is\u00f3topos radiactivos de periodo de semidesintegraci\u00f3n muy grande, como el <sup>14<\/sup>C, el <sup>10<\/sup>Be, el <sup>129<\/sup>I, etc.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-d3dda4c e-con-full e-flex e-con e-child\" data-id=\"d3dda4c\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t<div class=\"elementor-element elementor-element-d38fe67 elementor-widget elementor-widget-text-editor\" data-id=\"d38fe67\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>AMS es como:<\/p><ul><li>Encontrar un guisante en mil campos de f\u00fatbol juntos.<\/li><li>Encontrar una gota de agua determinada en una piscina ol\u00edmpica.<\/li><li>Agrupar a toda la poblaci\u00f3n del planeta en el mismo sitio y encontrarte all\u00ed con tu \u00fanico hermano.<\/li><\/ul>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-71b66c4 e-flex e-con-boxed e-con e-parent\" data-id=\"71b66c4\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-1265431 elementor-widget elementor-widget-heading\" data-id=\"1265431\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t\t<h3 class=\"elementor-heading-title elementor-size-default\">\u00bfQu\u00e9 es un acelerador electrost\u00e1tico?<\/h3>\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-3e2b73a elementor-widget elementor-widget-text-editor\" data-id=\"3e2b73a\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>Un <strong>acelerador electrost\u00e1tico<\/strong> es un dispositivo que utiliza <strong>voltajes muy altos<\/strong> \u2014del orden de cientos de miles o incluso un mill\u00f3n de voltios\u2014 para acelerar iones (\u00e1tomos cargados) hasta energ\u00edas elevadas. Puedes imaginarlo como una \u201crampa el\u00e9ctrica\u201d muy empinada: cuanto mayor es el voltaje, m\u00e1s r\u00e1pido cae el ion por esa rampa.<\/p><p>En el caso del CNA, el sistema AMS utiliza un acelerador tipo <strong>Tandetron de 1<\/strong><strong>\u202fMV<\/strong>, que aplica un potencial de un mill\u00f3n de voltios para:<\/p><ul><li><strong>Acelerar<\/strong> los iones a velocidades suficientes para analizarlos con precisi\u00f3n.<\/li><li><strong>Romper mol\u00e9culas indeseadas<\/strong> que podr\u00edan confundirse con los is\u00f3topos buscados.<\/li><li><strong>Seleccionar la carga<\/strong> del ion final, ayudando a separar especies distintas.<\/li><\/ul><p><strong><br \/>Por qu\u00e9 esto es importante:<\/strong><br \/>En espectrometr\u00eda de masas con aceleradores, necesitamos que el ion \u201cviaje limpio\u201d, sin compa\u00f1eros molestos que puedan confundirse con \u00e9l. El acelerador desempe\u00f1a este papel clave: elimina interferencias moleculares y prepara el haz para las etapas de separaci\u00f3n final.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-b431bee elementor-widget elementor-widget-image\" data-id=\"b431bee\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"image.default\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<img fetchpriority=\"high\" decoding=\"async\" width=\"800\" height=\"499\" src=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-b.jpg\" class=\"attachment-large size-large wp-image-93\" alt=\"\" srcset=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-b.jpg 1014w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-b-300x187.jpg 300w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-b-768x479.jpg 768w\" sizes=\"(max-width: 800px) 100vw, 800px\" \/>\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-d856cd1 e-flex e-con-boxed e-con e-parent\" data-id=\"d856cd1\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-1683c2e elementor-widget elementor-widget-heading\" data-id=\"1683c2e\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t\t<h3 class=\"elementor-heading-title elementor-size-default\">\u00bfQu\u00e9 son los radionucleidos raros?<\/h3>\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-84206c2 e-con-full e-flex e-con e-child\" data-id=\"84206c2\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t<div class=\"elementor-element elementor-element-e16fb6e elementor-widget__width-initial elementor-widget elementor-widget-image\" data-id=\"e16fb6e\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"image.default\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<img decoding=\"async\" width=\"800\" height=\"534\" src=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-1-1024x683.jpg\" class=\"attachment-large size-large wp-image-94\" alt=\"\" srcset=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-1-1024x683.jpg 1024w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-1-300x200.jpg 300w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-1-768x512.jpg 768w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-1.jpg 1300w\" sizes=\"(max-width: 800px) 100vw, 800px\" \/>\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-2e421b6 elementor-widget elementor-widget-text-editor\" data-id=\"2e421b6\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>Los <strong>radionucleidos raros<\/strong> son is\u00f3topos que existen en cantidades extremadamente peque\u00f1as en la naturaleza o que se producen en procesos muy limitados (cosmogenia, fisi\u00f3n, actividad humana). Algunos ejemplos comunes en AMS son <strong>\u00b9\u2074C, \u00b9\u2070Be, \u00b3\u2076Cl, \u00b9\u00b2\u2079I, \u00b2\u2076Al<\/strong>, y varios <strong>act\u00ednidos<\/strong>.<\/p><p>Estos radionucleidos suelen tener dos caracter\u00edsticas importantes:<\/p><p><strong>1. Est\u00e1n en concentraciones baj\u00edsimas<\/strong><\/p><p>Pueden aparecer en muestras en proporciones del tipo <strong>1 \u00e1tomo entre 10\u00b9\u00b2\u201310\u00b9\u2075<\/strong>, lo que hace que las t\u00e9cnicas anal\u00edticas convencionales no puedan detectarlos.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-3ab35c9 elementor-widget elementor-widget-text-editor\" data-id=\"3ab35c9\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p><strong>2. Contienen informaci\u00f3n valios\u00edsima<\/strong><\/p><ul><li>El <strong>\u00b9\u00b2\u2079I<\/strong> puede revelar contaminaci\u00f3n nuclear o reconstruir procesos oce\u00e1nicos.<\/li><li>Los <strong>act\u00ednidos<\/strong> permiten estudiar residuos nucleares y transporte de materiales radiactivos.<\/li><li>Los is\u00f3topos <strong>cosmog\u00e9nicos<\/strong> permiten datar rocas, glaciares o sedimentos.<\/li><li>Algunos <strong>radionucleidos estelares<\/strong> ayudan a entender la formaci\u00f3n de elementos en el cosmos.<\/li><\/ul><p>En otras palabras: aunque estos is\u00f3topos sean extraordinariamente escasos, contienen informaci\u00f3n clave para reconstruir historias geol\u00f3gicas, ambientales, nucleares e incluso astrof\u00edsicas.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-149d721 elementor-widget elementor-widget-image\" data-id=\"149d721\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"image.default\">\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<img decoding=\"async\" width=\"800\" height=\"534\" src=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-2-1024x683.jpg\" class=\"attachment-large size-large wp-image-95\" alt=\"\" srcset=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-2-1024x683.jpg 1024w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-2-300x200.jpg 300w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-2-768x512.jpg 768w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-2.jpg 1300w\" sizes=\"(max-width: 800px) 100vw, 800px\" \/>\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-ddf9cbf e-flex e-con-boxed e-con e-parent\" data-id=\"ddf9cbf\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-ccae006 elementor-widget elementor-widget-heading\" data-id=\"ccae006\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t\t<h3 class=\"elementor-heading-title elementor-size-default\">\u00bfPor qu\u00e9 medir cantidades del orden de 10\u207b\u00b9\u2075?<\/h3>\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-58144ce elementor-widget elementor-widget-text-editor\" data-id=\"58144ce\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t\t\t\t\t\t<p>Medir concentraciones tan peque\u00f1as como <strong>10<\/strong><strong>\u207b<\/strong><strong>\u00b9\u2075<\/strong> \u2014equivalente a un \u00e1tomo entre <strong>un cuatrill\u00f3n<\/strong>\u2014 es necesario porque:<\/p><p><strong>1. La naturaleza trabaja con cantidades min\u00fasculas<\/strong><\/p><p>Muchos procesos dejan \u00abhuellas\u00bb infinitamente peque\u00f1as, pero muy significativas. Por ejemplo:<\/p><ul><li>El \u00b9\u00b2\u2079I producido por actividades nucleares humanas puede dispersarse tanto que s\u00f3lo queden rastros ultratraza.<\/li><li>Los radionucleidos cosmog\u00e9nicos generados por rayos c\u00f3smicos se acumulan lentamente en rocas durante miles de a\u00f1os, produciendo cantidades \u00ednfimas.<\/li><\/ul><p><strong>2. Necesitamos distinguir entre interferencias y se\u00f1al verdadera<\/strong><\/p><p>Cuando buscamos is\u00f3topos extremadamente raros, cualquier interferencia \u2014una mol\u00e9cula, un is\u00f3topo vecino, una impureza del material\u2014 puede falsear el resultado.<\/p><p>Por eso la AMS:<\/p><ul><li><strong>Elimina mol\u00e9culas<\/strong> en el acelerador.<\/li><li><strong>Separa masas<\/strong> con imanes de alta resoluci\u00f3n (como el nuevo inyector de 120\u00b0).<\/li><li><strong>Detecta iones individuales<\/strong>, contando literalmente cada \u00e1tomo de inter\u00e9s.<\/li><\/ul><p><strong><br \/>3. Comprender procesos lentos, antiguos o muy diluidos<\/strong><\/p><p>Si algo ocurre muy despacio o muy lejos en el tiempo, deja muy poca se\u00f1al:<\/p><ul><li>Tasas de erosi\u00f3n milim\u00e9tricas por milenios<\/li><li>Transporte oce\u00e1nico a escala planetaria<\/li><li>Contaminantes radiactivos diluidos en ecosistemas<\/li><li>Producci\u00f3n estelar de elementos pesados<\/li><\/ul><p>Medir 10\u207b\u00b9\u2075 es la \u00fanica manera de acceder a ese nivel de detalle.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-1caf04a e-flex e-con-boxed e-con e-parent\" data-id=\"1caf04a\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-38868a5 elementor-widget elementor-widget-heading\" data-id=\"38868a5\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t\t<h4 class=\"elementor-heading-title elementor-size-default\">Bloques visuales:<\/h4>\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-08d6b80 e-flex e-con-boxed e-con e-parent\" data-id=\"08d6b80\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-5a250e6 e-con-full e-flex e-con e-child\" data-id=\"5a250e6\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t<div class=\"elementor-element elementor-element-9d8f3e4 elementor-position-top elementor-widget elementor-widget-image-box\" data-id=\"9d8f3e4\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"image-box.default\">\n\t\t\t\t\t<div class=\"elementor-image-box-wrapper\"><figure class=\"elementor-image-box-img\"><img loading=\"lazy\" decoding=\"async\" width=\"1536\" height=\"1024\" src=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-3.jpg\" class=\"attachment-full size-full wp-image-91\" alt=\"Ion source \u2192 Low energy line \u2192 Accelerator \u2192 High energy line\" srcset=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-3.jpg 1536w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-3-300x200.jpg 300w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-3-1024x683.jpg 1024w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-3-768x512.jpg 768w\" sizes=\"(max-width: 1536px) 100vw, 1536px\" \/><\/figure><div class=\"elementor-image-box-content\"><p class=\"elementor-image-box-description\">Ion source \u2192 Low energy line \u2192 Accelerator \u2192 High energy line<\/p><\/div><\/div>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-d0dcb6f e-con-full e-flex e-con e-child\" data-id=\"d0dcb6f\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t<div class=\"elementor-element elementor-element-d8767bb elementor-position-top elementor-widget elementor-widget-image-box\" data-id=\"d8767bb\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"image-box.default\">\n\t\t\t\t\t<div class=\"elementor-image-box-wrapper\"><figure class=\"elementor-image-box-img\"><img loading=\"lazy\" decoding=\"async\" width=\"602\" height=\"606\" src=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-4.webp\" class=\"attachment-full size-full wp-image-92\" alt=\"\" srcset=\"https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-4.webp 602w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-4-298x300.webp 298w, https:\/\/institucional.us.es\/astro21\/wp-content\/uploads\/2026\/05\/Figura-4-150x150.webp 150w\" sizes=\"(max-width: 602px) 100vw, 602px\" \/><\/figure><div class=\"elementor-image-box-content\"><p class=\"elementor-image-box-description\">Gr\u00e1fico de una separaci\u00f3n de masas<\/p><\/div><\/div>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t","protected":false},"excerpt":{"rendered":"<p>\u00bfPor qu\u00e9 necesitamos un nuevo inyector? \u00bfQu\u00e9 hace el inyector en un sistema AMS? La Espectrometr\u00eda de Masas es una t\u00e9cnica que permite separar iones at\u00f3micos o moleculares que se mueven en funci\u00f3n de su masa, gracias a la aplicaci\u00f3n de campos magn\u00e9ticos y electrost\u00e1ticos. La Espectrometr\u00eda de Masas con Acelerador (AMS) a\u00f1ade a la [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-40","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.6 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>\u00bfQu\u00e9 es AMS? - ASTROAMS \u2013 Accelerator Mass Spectrometry for Astrophysics<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/institucional.us.es\/astro21\/que-es-ams\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"\u00bfQu\u00e9 es AMS? - ASTROAMS \u2013 Accelerator Mass Spectrometry for Astrophysics\" \/>\n<meta property=\"og:description\" content=\"\u00bfPor qu\u00e9 necesitamos un nuevo inyector? \u00bfQu\u00e9 hace el inyector en un sistema AMS? 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