{"id":564,"date":"2016-02-18T20:32:19","date_gmt":"2016-02-18T20:32:19","guid":{"rendered":"http:\/\/www.astronotas.org\/messier\/?p=564"},"modified":"2023-12-09T15:48:36","modified_gmt":"2023-12-09T19:48:36","slug":"m27","status":"publish","type":"post","link":"https:\/\/www.astronotas.org\/messier\/m27\/","title":{"rendered":"Messier 27"},"content":{"rendered":"\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\/11\/027.gif\"><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\/027.gif?resize=318%2C318\" alt=\"M27\" class=\"wp-image-1186\"\/><\/a><\/figure>\n\n\n\n<p><strong>Objeto: M27<\/strong><\/p>\n\n\n\n<p>Constelaci\u00f3n: Vulpecula<br>Fecha: 1994.05.08 | Hora: 7:19 UT<br>Lugar: Bo. Jauca, Santa Isabel, PR<\/p>\n\n\n\n<p>Tipo de objeto: Nebulosa planetaria<br>Nombre: Nebulosa de las Pesas, Dumbbell Nebula, NGC 6853<br>Magnitud: 8.1 | Tama\u00f1o: 350&#8243;<br>R.A. 19h59.6m | Dec. +22\u00b043&#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: filtro nebular (narrowband)<\/p>\n\n\n\n<p>Carta en Uranometr\u00eda 2000.0: 165<\/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\/11\/m27jp-20160220184541-b6713569.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"484\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27jp-20160220184541-b6713569.jpg?resize=640%2C484\" alt=\"M27\" class=\"wp-image-1896\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27jp-20160220184541-b6713569.jpg?w=640&amp;ssl=1 640w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27jp-20160220184541-b6713569.jpg?resize=300%2C227&amp;ssl=1 300w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption class=\"wp-element-caption\"> Jimmy P\u00e9rez <\/figcaption><\/figure>\n\n\n\n<h3 class=\"wp-block-heading\">Descripci\u00f3n<\/h3>\n\n\n\n<p><strong>Espa\u00f1ol:<\/strong> M27 result\u00f3 ser un objeto bien brillante y de gran tama\u00f1o. No se requer\u00eda filtro alguno para mejorar la visibilidad de este objeto, aunque con el filtro aumenta el contraste, y los espacios &#8220;vac\u00edos&#8221; (donde el material que compone la nube es menos denso) se llenan con un poco de nebulosidad. Sin el filtro, se pod\u00edan apreciar m\u00e1s estrellas en los alrededores de M27, lo que le an\u00e3de belleza al campo de visi\u00f3n. No se detect\u00f3 la estrella central (como era de esperarse).<\/p>\n\n\n\n<p><strong>English:<\/strong> M27 proved to be a very bright and large object. A filter is not required to improve its&nbsp;visibility, although it&nbsp;increases the contrast, and the &#8220;empty&#8221; spaces (where the material that makes up the cloud is less dense) are filled with some cloudiness. Without the filter, you can&nbsp;see more stars around M27, which adds richness&nbsp;to the field of view. The central star was not detected (as expected).<\/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\/11\/m27hw.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"1024\" src=\"https:\/\/i1.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?fit=640%2C640\" alt=\"M27\" class=\"wp-image-1898\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?resize=300%2C300&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?resize=150%2C150&amp;ssl=1 150w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?resize=768%2C768&amp;ssl=1 768w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hw.jpg?resize=50%2C50&amp;ssl=1 50w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption class=\"wp-element-caption\"> Hunter Wilson [<a href=\"http:\/\/hwilson.zenfolio.com\/messier\/h2ae83e38#h3a22caa8\">origen<\/a>] <\/figcaption><\/figure>\n\n\n\n<p><strong>Cometarios de Messier en 1771:<\/strong> El 12 de julio de 1764, trabaj\u00e9 en la b\u00fasqueda de nebulosas, descubr\u00ed una en la constelaci\u00f3n del Zorro, entre las dos patas de delante, y muy cerca de la estrella de quinta magnitud, d\u00e9cimo cuarta de esta constelaci\u00f3n, seg\u00fan el cat\u00e1logo de Flamsteed: se ve bien con un anteojo ordinario de 3 pies y medio. La examin\u00e9 con un telescopio gregoriano que aumentaba ciento cuatro&nbsp;veces: parec\u00eda de&nbsp;forma ovalada; no contiene ninguna&nbsp;estrella; su di\u00e1metro es de alrededor de 4 minutos de grado. Compar\u00e9 esta nebulosa con la estrella vecina que nombr\u00e9 aqu\u00ed arriba; su ascensi\u00f3n recta fue concluida de&nbsp;297\u00b0&nbsp;21&#8242; 41&#8243; y su declinaci\u00f3n de&nbsp;22\u00b0&nbsp;4&#8242; 0&#8243; boreal.<\/p>\n\n\n\n<p><strong>Comentarios de Messier en 1784:<\/strong> Nebulosa sin estrella, descubierta en el Zorro, entre las dos patas delanteras y muy cerca de la estrella 14.<sup>ta<\/sup> de esta constelaci\u00f3n, de 5.<sup>ta<\/sup> magnitud seg\u00fan Flamsteed; se ve bien con un anteojo ordinario de tres pies y medio: parece de forma ovalada y no contiene ninguna&nbsp;estrella. M. Messier refiere su posici\u00f3n en la carta del cometa de 1779, que ser\u00e1 grabada para el volumen de la Academia del mismo a\u00f1o. Vuelta a ver el 31 de enero de 1781.<\/p>\n\n\n\n<p class=\"has-text-align-center\"><strong>Mapa para localizar a M27<\/strong><\/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\/11\/s027.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\/s027.png?resize=576%2C792\" alt=\"Mapa para localizar a M27\" class=\"wp-image-842\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s027.png?w=576&amp;ssl=1 576w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/s027.png?resize=218%2C300&amp;ssl=1 218w\" sizes=\"auto, (max-width: 576px) 100vw, 576px\" \/><\/a><figcaption class=\"wp-element-caption\">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\/11\/m27.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"538\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27.jpg?resize=640%2C538\" alt=\"M27\" class=\"wp-image-1899\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27.jpg?resize=300%2C252&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27.jpg?resize=768%2C645&amp;ssl=1 768w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption class=\"wp-element-caption\"> T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOAO\/AURA\/NSF) [<a href=\"https:\/\/noirlab.edu\/public\/es\/images\/noao-m27-kpno-mayall-4-m\/?nocache=true\">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\/11\/m27hst.jpg\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"377\" src=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hst.jpg?resize=640%2C377\" alt=\"M27\" class=\"wp-image-1900\" srcset=\"https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hst.jpg?w=1024&amp;ssl=1 1024w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hst.jpg?resize=300%2C177&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.astronotas.org\/messier\/wp-content\/uploads\/2019\/11\/m27hst.jpg?resize=768%2C452&amp;ssl=1 768w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><figcaption class=\"wp-element-caption\"> NASA and The Hubble Heritage Team (STScI\/AURA) [<a href=\"https:\/\/science.nasa.gov\/mission\/hubble\/science\/explore-the-night-sky\/hubble-messier-catalog\/messier-27\/\">origen<\/a>] <\/figcaption><\/figure>\n","protected":false},"excerpt":{"rendered":"<p>Objeto: M27 Constelaci\u00f3n: VulpeculaFecha: 1994.05.08 | Hora: 7:19 UTLugar: Bo. Jauca, Santa Isabel, PR Tipo de objeto: Nebulosa planetariaNombre: Nebulosa de las Pesas, Dumbbell Nebula, NGC 6853Magnitud: 8.1 | Tama\u00f1o: 350&#8243;R.A. 19h59.6m | Dec. +22\u00b043&#8242;\u00c9poca: 2000.0 Instrumento: Meade MTS-SN 6Ocular:&hellip; <a href=\"https:\/\/www.astronotas.org\/messier\/m27\/\" 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":[127],"tags":[472,124,123,129,131,473],"class_list":["post-564","post","type-post","status-publish","format-standard","hentry","category-nebulosas-planetarias","tag-dumbbell-nebula","tag-m27","tag-messier-27","tag-nebulosa-de-las-pesas","tag-ngc-6853","tag-vulpecula"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.2 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Messier 27 - Cat\u00e1logo Messier<\/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:\/\/www.astronotas.org\/messier\/m27\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Messier 27 - Cat\u00e1logo Messier\" \/>\n<meta property=\"og:description\" content=\"Objeto: M27 Constelaci\u00f3n: VulpeculaFecha: 1994.05.08 | Hora: 7:19 UTLugar: Bo. 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