{"id":18286,"date":"2018-09-25T10:49:20","date_gmt":"2018-09-25T13:49:20","guid":{"rendered":"http:\/\/www.astrofisicamas.cl\/?p=18286"},"modified":"2023-08-04T20:58:52","modified_gmt":"2023-08-04T20:58:52","slug":"la-controversia-de-canis-major-y-la-mision-gaia","status":"publish","type":"post","link":"https:\/\/astrofisicamas.cl\/en\/la-controversia-de-canis-major-y-la-mision-gaia\/","title":{"rendered":"Nuestra Investigaci\u00f3n: La controversia de Canis Major y la misi\u00f3n Gaia"},"content":{"rendered":"<h4><em><strong>Por Julio Carballo \u2013 Bello, investigador postdoctoral MAS y del Instituto de Astrof\u00edsica UC\u00a0<\/strong><\/em><\/h4>\n<p><!--more--><\/p>\n<p><strong>Hace casi 15 a\u00f1os, un grupo de astrof\u00edsicos descubri\u00f3 una sobredensidad de estrellas en la constelaci\u00f3n de Canis Major (Can Mayor), justo por debajo del disco de la V\u00eda L\u00e1ctea y a muy poca distancia de nosotros.<\/strong> Entre las posibles explicaciones a esta nueva estructura, el equipo cient\u00edfico a cargo de esta investigaci\u00f3n present\u00f3 como hip\u00f3tesis que esta sobredensidad representar\u00eda en realidad el n\u00facleo de una galaxia, devorada por la nuestra hace mucho tiempo. No ser\u00eda la primera vez que esto es observado, ya que hay otros muchos ejemplos en las regiones externas de la V\u00eda L\u00e1ctea, con restos de galaxias y peque\u00f1os sat\u00e9lites asimilados por nuestra hambrienta galaxia a lo largo de su historia.<\/p>\n<p><strong>Sin embargo, a diferencia de esos otros casos de galaxias acretadas, la hipot\u00e9tica galaxia de Canis Major presenta propiedades que bien podr\u00edan ser explicadas de manera diferente. El escenario alternativo que m\u00e1s fuerza ha tenido desde el descubrimiento de esta sobredensidad es que Canis Major, en realidad, es una parte de la propia V\u00eda L\u00e1ctea y un efecto de proyecci\u00f3n nos hace observarla como una gran nube en el cielo. Adem\u00e1s, se ha postulado que posiblemente uno de los brazos espirales de nuestra galaxia en una determinada proyecci\u00f3n dar\u00eda lugar a los efectos que observamos y que asociamos con Canis Major.<\/strong><\/p>\n<p>En la \u00faltima d\u00e9cada ha habido pocas novedades referentes a esta sobredensidad ya que otras subestructuras del halo gal\u00e1ctico han aparecido en los \u00faltimos tiempos, concentrando la mayor parte de la atenci\u00f3n de los nuevos instrumentos astron\u00f3micos. Entre ellos, la sonda espacial europea Gaia,\u00a0 lanzada en 2013, que tiene entre sus principales objetivos el estudio de la estructura y cinem\u00e1tica de la V\u00eda L\u00e1ctea. Los primeros datos se hicieron disponibles en 2016 y desde entonces, esta misi\u00f3n nos ha aportado datos de gran precisi\u00f3n, muy valiosos, acerca del movimiento de las estrellas y su distancia respecto a la Tierra.<\/p>\n<p><strong>Nuestro equipo de investigaci\u00f3n pretende ahora rescatar a la sobredensidad de Canis Major del olvido en el que ha ca\u00eddo los \u00faltimos a\u00f1os y aprovechar esta nueva oportunidad que nos brinda Gaia para desentra\u00f1ar las diferentes componentes de la V\u00eda L\u00e1ctea, incluso en regiones tan cercanas al plano como la ocupada por esta supuesta galaxia asimilada<\/strong>. Seleccionando una muestra de estrellas j\u00f3venes azules asociadas a Canis Major, y que no se observan en ninguna otra direcci\u00f3n del cielo, e intentando determinar cu\u00e1l es la velocidad y la \u00f3rbita de esta pol\u00e9mica galaxia incrustada en el plano gal\u00e1ctico. <strong>Con estos resultados en mano, seremos capaces de dar respuesta a una de las cuestiones abiertas de la Arqueolog\u00eda Gal\u00e1ctica, una rama relativamente reciente de la Astrof\u00edsica y que intenta comprender c\u00f3mo lleg\u00f3 nuestra galaxia a ser como la vemos hoy en d\u00eda.<\/strong><\/p>","protected":false},"excerpt":{"rendered":"<p>Por Julio Carballo \u2013 Bello, investigador postdoctoral MAS y del Instituto de Astrof\u00edsica UC\u00a0<\/p>","protected":false},"author":3,"featured_media":29143,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_coblocks_attr":"","_coblocks_dimensions":"","_coblocks_responsive_height":"","_coblocks_accordion_ie_support":"","_eb_attr":"","footnotes":""},"categories":[59],"tags":[],"class_list":["post-18286","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-columnas"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.2 - 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