{"id":634,"date":"2016-02-24T00:47:17","date_gmt":"2016-02-24T00:47:17","guid":{"rendered":"http:\/\/www.astronotas.org\/messier\/?p=634"},"modified":"2023-12-09T22:08:05","modified_gmt":"2023-12-10T02:08:05","slug":"m47","status":"publish","type":"post","link":"https:\/\/www.astronotas.org\/messier\/m47\/","title":{"rendered":"Messier 47"},"content":{"rendered":"\n<figure class=\"wp-block-image size-large is-style-default\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"318\" height=\"318\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/047.gif?resize=318%2C318\" alt=\"M47\" class=\"wp-image-1202\"\/><\/figure>\n\n\n\n<p><strong>Objeto: M47<\/strong><\/p>\n\n\n\n<p>Constelaci\u00f3n: Puppis<br>Fecha: 1994.02.16 | Hora: 1:15 UT<br>Lugar: Sumidero, Aguas Buenas, PR<\/p>\n\n\n\n<p>Tipo de objeto: C\u00famulo abierto, clase D<br>Nombre: NGC 2422<br>Magnitud: 4.4 | Tama\u00f1o: 30&#8242;<br>R.A. 7h36.6m | Dec. \u201314\u00b030&#8242;<br>\u00c9poca: 2000.0<\/p>\n\n\n\n<p>Instrumento: Meade MTS-SN 6<br>Ocular: 8.8 mm UWA | Aumento: 87x<br>Campo aparente: 84\u00b0 | Campo actual: 57&#8242;<br>Otros:<\/p>\n\n\n\n<p>Carta en Uranometr\u00eda 2000.0: 274<\/p>\n\n\n\n<figure class=\"wp-block-image size-large is-style-default\"><a href=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/M47.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"453\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/M47.jpg?resize=640%2C453\" alt=\"M47\" class=\"wp-image-1992\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/M47.jpg?w=730&amp;ssl=1 730w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/M47.jpg?resize=300%2C212&amp;ssl=1 300w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption> Juan Luis Mart\u00ednez <\/figcaption><\/figure>\n\n\n\n<h3 class=\"wp-block-heading\">Descripci\u00f3n<\/h3>\n\n\n\n<p><strong>Espa\u00f1ol:<\/strong> Es necesario mencionar que el dibujo que se incluye no hace justicia a la verdadera apariencia de M47, seg\u00fan se ve a trav\u00e9s de un telescopio. En efecto, es mejor observarlo con poco aumento; la mejor imagen fue obtenida a 30x, pues presentaba todo el c\u00famulo y sus inmediaciones dentro del mismo campo de visi\u00f3n. Sus componentes principles son considerablemente brillantes, y a mayor magnificaci\u00f3n, aumenta la cantidad de estrellas visibles en el c\u00famulo, la mayor\u00eda de ellas de poca magnitud (min\u00fasculas en apariencia). Semejantemente, resultan muy llamativas las varias estrellas dobles (o binarias) en M47, especialemente, una muy pr\u00f3xima a lo que se puede considerar como el centro del conglomerado.<\/p>\n\n\n\n<p><strong>English:<\/strong>&nbsp;It is necessary to say this sketch does no justice to the true appearance of M47 as seen through a telescope. The cluster&nbsp;looks&nbsp;better at low magnification; the best view&nbsp;was obtained at 30x, since it was possible to see all the cluster and its surroundings&nbsp;in the same field of view. Its principal components are considerably bright, and at higher magnification, the number of stars increase, most of them quite faint (tiny in appearance). Similarly, there are various double (or binary) stars in M47, especially near&nbsp;to what could be considered the cluster&#8217;s center.<\/p>\n\n\n\n<figure class=\"wp-block-image size-large is-style-default\"><a href=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"1024\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?fit=640%2C640\" alt=\"M47\" class=\"wp-image-1993\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?resize=300%2C300&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?resize=150%2C150&amp;ssl=1 150w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?resize=768%2C768&amp;ssl=1 768w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47.jpg?resize=50%2C50&amp;ssl=1 50w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption> NOAO\/AURA\/NSF [<a href=\"https:\/\/www.noao.edu\/image_gallery\/html\/im0789.html\">origen<\/a>] <\/figcaption><\/figure>\n\n\n\n<p><strong>Comentarios de Messier en 1784:<\/strong> C\u00famulo de estrellas poco alejado del precedente, las estrellas m\u00e1s grandes; el centro del c\u00famulo comparado con la misma estrella, la segunda del Nav\u00edo. El c\u00famulo no contiene ninguna&nbsp;nebulosidad.<\/p>\n\n\n\n<p class=\"has-text-align-center\"><strong>Mapa para localizar a M47<\/strong><\/p>\n\n\n\n<figure class=\"wp-block-image size-full is-style-default\"><a href=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s047.png\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"576\" height=\"792\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s047.png?resize=576%2C792\" alt=\"Mapa para localizar a M47\" class=\"wp-image-862\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s047.png?w=576&amp;ssl=1 576w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s047.png?resize=218%2C300&amp;ssl=1 218w\" sizes=\"auto, (max-width: 576px) 100vw, 576px\" \/><\/a><figcaption>Haga click para agrandar.<\/figcaption><\/figure>\n\n\n\n<figure class=\"wp-block-image size-large is-style-default\"><a href=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"638\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?resize=640%2C638\" alt=\"M47\" class=\"wp-image-1994\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?resize=300%2C300&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?resize=150%2C150&amp;ssl=1 150w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?resize=768%2C766&amp;ssl=1 768w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441c.jpg?resize=50%2C50&amp;ssl=1 50w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption> Credit: ESO\/Digitized Sky Survey 2. Acknowledgement: Davide De Martin [<a href=\"http:\/\/www.eso.org\/public\/images\/eso1441c\/\">origen<\/a>] <\/figcaption><\/figure>\n\n\n\n<figure class=\"wp-block-image size-large is-style-default\"><a href=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441a.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"618\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441a.jpg?resize=640%2C618\" alt=\"M47\" class=\"wp-image-1995\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441a.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441a.jpg?resize=300%2C289&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/12\/m47-eso1441a.jpg?resize=768%2C741&amp;ssl=1 768w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption> ESO [<a href=\"http:\/\/www.eso.org\/public\/images\/eso1441a\/\">origen<\/a>] <\/figcaption><\/figure>\n","protected":false},"excerpt":{"rendered":"<p>Objeto: M47 Constelaci\u00f3n: PuppisFecha: 1994.02.16 | Hora: 1:15 UTLugar: Sumidero, Aguas Buenas, PR Tipo de objeto: C\u00famulo abierto, clase DNombre: NGC 2422Magnitud: 4.4 | Tama\u00f1o: 30&#8242;R.A. 7h36.6m | Dec. \u201314\u00b030&#8242;\u00c9poca: 2000.0 Instrumento: Meade MTS-SN 6Ocular: 8.8 mm UWA | Aumento:&hellip; <a href=\"https:\/\/www.astronotas.org\/messier\/m47\/\" class=\"more-link\">Continue Reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jetpack_post_was_ever_published":false,"_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_publicize_message":"","jetpack_publicize_feature_enabled":true,"jetpack_social_post_already_shared":true,"jetpack_social_options":{"image_generator_settings":{"template":"highway","default_image_id":0,"font":"","enabled":false},"version":2}},"categories":[19],"tags":[216,217,212,213],"class_list":["post-634","post","type-post","status-publish","format-standard","hentry","category-cumulos-abiertos","tag-m47","tag-messier-47","tag-ngc-2422","tag-puppis"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.2 - 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