{"id":834,"date":"2015-09-21T10:32:39","date_gmt":"2015-09-21T10:32:39","guid":{"rendered":"http:\/\/microastronomia.astroedu.net\/?page_id=834"},"modified":"2015-10-16T09:51:45","modified_gmt":"2015-10-16T09:51:45","slug":"zeptoscopi-12","status":"publish","type":"page","link":"https:\/\/microastronomia.cosmozoom.eu\/?page_id=834","title":{"rendered":"zeptoScopi 12"},"content":{"rendered":"<address><strong> <a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0660.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-902 alignleft\" style=\"border: 3px solid black;\" alt=\"zDSCN0660\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0660-300x229.jpg\" width=\"300\" height=\"229\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0660-300x229.jpg 300w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0660-196x150.jpg 196w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0660-150x114.jpg 150w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0660.jpg 872w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a><\/strong><a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0655.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright  wp-image-903\" style=\"border: 3px solid black;\" alt=\"zDSCN0655\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0655-300x216.jpg\" width=\"240\" height=\"173\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0655-300x216.jpg 300w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0655-207x150.jpg 207w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0655-150x108.jpg 150w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0655.jpg 900w\" sizes=\"(max-width: 240px) 100vw, 240px\" \/><\/a><strong>Tipo:<\/strong> monocular prisma techo Bak4-FC<\/address>\n<address><strong>Di\u00e1metro:<\/strong> 12 mm<\/address>\n<address><strong>Aumento: <\/strong>4x (fijo)<\/address>\n<address><strong>Pupila de salida:\u00a0<\/strong> 3mm<\/address>\n<address><strong>Campo m\u00e1ximo \u00fatil:<\/strong> 12.5\u00ba\u00a0<\/address>\n<address><strong>Peso:<\/strong> 60g<\/address>\n<address><strong>Dimensiones (L x D):<\/strong> 58mm x 30mm<\/address>\n<address>\u00a0<\/address>\n<address><span style=\"color: #ffffff;\">&#8230;..<\/span><\/address>\n<address><span style=\"color: #ffffff;\">&#8230;&#8230;<\/span><\/address>\n<address><span style=\"color: #ffffff;\">&#8230;&#8230;<\/span><\/address>\n<address class=\"mceTemp\">\n<dl class=\"wp-caption alignright\" id=\"attachment_1067\" style=\"width: 190px;\">\n<dt class=\"wp-caption-dt\"><a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0729.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1067\" alt=\"zDSCN0729\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0729-300x247.jpg\" width=\"180\" height=\"148\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0729-300x247.jpg 300w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0729-182x150.jpg 182w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0729-150x123.jpg 150w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0729.jpg 800w\" sizes=\"(max-width: 180px) 100vw, 180px\" \/><\/a><\/dt>\n<dd class=\"wp-caption-dd\">Micro familia. De izquierda a derecha: attoScopi, zeptoScopi y yoctoScopi. Los nombres responden a prefijos del Sistema Internacional.<\/dd>\n<\/dl>\n<\/address>\n<p style=\"text-align: justify;\">Despu\u00e9s de la observaci\u00f3n a simple vista, y de no existir el yoctoScopi, este monocular se puede considerar \u00abcasi\u00bb lo m\u00ednimo para la contemplaci\u00f3n del firmamento. De manufactura oriental, se distribuye bajo diferentes nombres a precios muy econ\u00f3micos. Concebido para uso diurno terrestre y tambi\u00e9n como lupa, su calidad no es nada del otro mundo, pero es mejor de lo que pudiera parecer. A pesar de estar limitado por su aumento y di\u00e1metro, tiene una razonable transmisi\u00f3n de luz y contraste, lo que lo hace \u00fatil para algunos objetos celestes, ya que permite llegar aproximadamente hasta magnitud 8.5. Con \u00e9l, se consigue ver Neptuno en visi\u00f3n directa.<\/p>\n<dl class=\"wp-caption alignright\" id=\"attachment_911\" style=\"width: 166px;\">\n<dt class=\"wp-caption-dt\"><\/dt>\n<\/dl>\n<figure id=\"attachment_914\" aria-describedby=\"caption-attachment-914\" style=\"width: 158px\" class=\"wp-caption alignleft\"><a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0675.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-914 \" style=\"border: 3px solid black;\" alt=\"zDSCN0675\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0675-225x300.jpg\" width=\"158\" height=\"210\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0675-225x300.jpg 225w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0675-112x150.jpg 112w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0675.jpg 675w\" sizes=\"(max-width: 158px) 100vw, 158px\" \/><\/a><figcaption id=\"caption-attachment-914\" class=\"wp-caption-text\">Adaptador casero a tr\u00edpode o monopi\u00e9.<\/figcaption><\/figure>\n<figure id=\"attachment_918\" aria-describedby=\"caption-attachment-918\" style=\"width: 180px\" class=\"wp-caption alignright\"><a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0664.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-918 \" alt=\"Parte trasera: ocular.\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0664-300x231.jpg\" width=\"180\" height=\"139\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0664-300x231.jpg 300w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0664-194x150.jpg 194w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0664-150x115.jpg 150w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0664.jpg 900w\" sizes=\"(max-width: 180px) 100vw, 180px\" \/><\/a><figcaption id=\"caption-attachment-918\" class=\"wp-caption-text\">Parte trasera: ocular.<\/figcaption><\/figure>\n<figure id=\"attachment_909\" aria-describedby=\"caption-attachment-909\" style=\"width: 180px\" class=\"wp-caption alignright\"><a href=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0656.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\" wp-image-909  \" alt=\"Parte delantera: objetivo de 12mm.\" src=\"http:\/\/microastronomia.astroedu.net\/wp-content\/uploads\/2015\/09\/zDSCN0656-300x209.jpg\" width=\"180\" height=\"125\" srcset=\"https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0656-300x209.jpg 300w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0656-214x150.jpg 214w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0656-150x104.jpg 150w, https:\/\/microastronomia.cosmozoom.eu\/wp-content\/uploads\/2015\/09\/zDSCN0656.jpg 900w\" sizes=\"(max-width: 180px) 100vw, 180px\" \/><\/a><figcaption id=\"caption-attachment-909\" class=\"wp-caption-text\">Parte delantera: objetivo de 12mm.<\/figcaption><\/figure>\n<h2><\/h2>\n<h2><\/h2>\n<h2><\/h2>\n<address>\u00a0<\/address>\n<address>\n<h2><\/h2>\n<h2><\/h2>\n<h2><\/h2>\n<p><span style=\"color: #ffffff;\">&#8230;&#8230;&#8230;.<\/span><\/p>\n<p><span style=\"color: #ffffff;\">&#8230;&#8230;&#8230;.<\/span><\/p>\n<p><span style=\"color: #ffffff;\">&#8230;&#8230;&#8230;.<\/span><\/p>\n<h2><span style=\"color: #ffffff;\">\u00a0<\/span><\/h2>\n<p><span style=\"color: #ffffff;\">&#8230;&#8230;&#8230;.<\/span><\/p>\n<h2><\/h2>\n<h2><span style=\"text-decoration: underline;\"><strong>OBJETOS OBSERVADOS CON EL zeptoScopi<\/strong><\/span><\/h2>\n<p><em>Se listan objetos observados por el autor bajo un cielo de magnitud l\u00edmite 6.5-6.7, entre 3 y 4 en la escala de Bortle, con la zona Sur con algo de contaminaci\u00f3n lum\u00ednica. <\/em>Seg\u00fan su nivel de dificultad: en <em>letra <strong>oscura<\/strong> para objetos f\u00e1ciles de percibir, en <span style=\"color: #ffcc00;\">\u00e1mbar<\/span> para los de dificultad media y en <span style=\"color: #ff0000;\">rojo<\/span> para los dif\u00edciles pero a\u00fan accesibles. Acr\u00f3nimos usados: VD: Visi\u00f3n Directa, VL: Visi\u00f3n Lateral.<br \/>\n<\/em><\/p>\n<address>\u00a0<\/address>\n<p><span style=\"text-decoration: underline;\">LUNA<\/span><br \/>\n&#8211; <strong>Mares, cr\u00e1teres y otras estructuras.<\/strong><\/p>\n<p><span style=\"text-decoration: underline;\">PLANETAS<\/span><br \/>\n&#8211;<strong>Venus<\/strong>: apariencia estelar.<br \/>\n&#8211;<strong>Marte<\/strong>: apariencia estelar.<br \/>\n&#8211;<strong>J\u00fapiter<\/strong>: apariencia estelar.<br \/>\n&#8211;<strong>Saturno<\/strong>: apariencia estelar.<br \/>\n&#8211;<strong>Urano<\/strong>:\u00a0 apariencia estelar en VD.<br \/>\n&#8211;<strong>Neptuno<\/strong>: apariencia estelar en VD.<\/p>\n<p><span style=\"text-decoration: underline;\">ESTRELLAS DOBLES, M\u00daLTIPLES Y PECULIARES<\/span><br \/>\n&#8211;<strong>16-17 Draconis<\/strong>: se resuelve f\u00e1cil en VD.<br \/>\n&#8211;<strong>56 Andromedae<\/strong>: muy f\u00e1cil, al lado de NGC752.<br \/>\n&#8211;<strong>Beta Capricorni<\/strong>: la secundaria a medio camino entre VD y VL, como un d\u00e9bil y peque\u00f1o punto de luz.<br \/>\n&#8211;<strong>Nu Draconis<\/strong>: se divide con bastante facilidad.<br \/>\n&#8211;<strong>Zeta Lyrae<\/strong>: se desdobla relativamente f\u00e1cil en VD.<\/p>\n<p><span style=\"text-decoration: underline;\">ASTERISMOS<\/span><br \/>\n&#8211;<strong>La Cascada de Kemble<\/strong>: se resuelve en estrellas en VD.<\/p>\n<p><span style=\"text-decoration: underline;\">C\u00daMULOS ABIERTOS<\/span><br \/>\n&#8211;<strong>M11<\/strong>: aspecto nebular, relativamente grande en VD.<br \/>\n&#8211;<strong>M36-37-38<\/strong>: juntos en el mismo campo y visibles en VD.<br \/>\n&#8211;<span style=\"color: #ffcc00;\">NGC752<\/span>: visible con relativa comodidad en VL.<br \/>\n&#8211;<strong>NGC1502<\/strong>: se observa en VD con aspecto de estrella brillante.<\/p>\n<p><span style=\"text-decoration: underline;\">C\u00daMULOS GLOBULARES<\/span><br \/>\n&#8211;<strong>M13<\/strong>: nebulosidad peque\u00f1a en VD.<br \/>\n&#8211;<strong>M22<\/strong>: nebulosidad relativamente d\u00e9bil y grande en VD, que muestra cierto gradiente n\u00facleo-periferia en VL.<\/p>\n<p><span style=\"text-decoration: underline;\">NEBULOSAS<\/span><br \/>\n&#8211;<strong>M17<\/strong>: f\u00e1cil en VD, se ve su t\u00edpica forma alargada.<br \/>\n&#8211;<span style=\"color: #ffcc00;\">M27<\/span>: en VL, peque\u00f1a nuubecilla.<\/p>\n<p><span style=\"text-decoration: underline;\">GALAXIAS<\/span><br \/>\n&#8211;<strong>M33<\/strong>: F\u00e1cil en VD.<\/p>\n<\/address>\n","protected":false},"excerpt":{"rendered":"<p>Tipo: monocular prisma techo Bak4-FC Di\u00e1metro: 12 mm Aumento: 4x (fijo) Pupila de salida:\u00a0 3mm Campo m\u00e1ximo \u00fatil: 12.5\u00ba\u00a0 Peso:<\/p>\n<p><a href=\"https:\/\/microastronomia.cosmozoom.eu\/?page_id=834\" class=\"more-link\">Seguir leyendo<span class=\"screen-reader-text\">zeptoScopi 12<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":823,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/pages\/834"}],"collection":[{"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=834"}],"version-history":[{"count":41,"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/pages\/834\/revisions"}],"predecessor-version":[{"id":1125,"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/pages\/834\/revisions\/1125"}],"up":[{"embeddable":true,"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=\/wp\/v2\/pages\/823"}],"wp:attachment":[{"href":"https:\/\/microastronomia.cosmozoom.eu\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=834"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}