{"id":586,"date":"2016-02-21T11:37:56","date_gmt":"2016-02-21T11:37:56","guid":{"rendered":"http:\/\/www.astronotas.org\/messier\/?p=586"},"modified":"2019-12-01T20:16:33","modified_gmt":"2019-12-02T00:16:33","slug":"m37","status":"publish","type":"post","link":"https:\/\/www.astronotas.org\/messier\/m37\/","title":{"rendered":"Messier 37"},"content":{"rendered":"\n
\"M37\"<\/a>
NOAO\/AURA\/NSF [origen<\/a>] <\/figcaption><\/figure>\n\n\n\n

Objeto: M37<\/strong><\/p>\n\n\n\n

Constelaci\u00f3n: Auriga
Fecha: 1992.12.28 | Hora: 23:50 UT
Lugar: Sumidero, Aguas Buenas, PR<\/p>\n\n\n\n

Tipo de objeto: C\u00famulo abierto, clase F
Nombre: NGC 2099
Magnitud: 6.2 | Tama\u00f1o: 24′
A.R. 5h52.3m | Dec. +32\u00b033′
\u00c9poca: 2000.0<\/p>\n\n\n\n

Instrumento: Meade MTS-SN 6
Ocular: 25 mm MA | Aumento: 60x
Campo aparente: 40\u00b0 | Campo actual: 1\u00b020′
Otros: lente Barlow 2x<\/p>\n\n\n\n

Carta en Uranometr\u00eda 2000.0: 97<\/p>\n\n\n\n

\"M37\"<\/a>
DSS2 @ Wikisky.org<\/figcaption><\/figure>\n\n\n\n

Descripci\u00f3n<\/h3>\n\n\n\n

Espa\u00f1ol:<\/strong> M37 es un c\u00famulo abierto en la constelaci\u00f3n de Auriga; uno de los tres que se \u201cal\u00ednean\u201d en el centro de la misma: M36, M37 y M38. Visualmente, M37 est\u00e1 densamente poblado de estrellas, ninguna de ellas sobresaliente de entre las otras. En cierto sentido, este c\u00famulo se asemeja un poco a un c\u00famulo globular con pocas estrellas. Sus estrellas tambi\u00e9n son de un color blanco o blanco azulado.<\/p>\n\n\n\n

English:<\/strong> M37 is an open cluster in Auriga; one of three that line up in the middle of this constellation: M36, M37 and M38. Visually, M37 is densely populated, and none of its stars stand out from the others. In a sense, this cluster –somewhat– resembles a globular cluster with few stars. Its stars are also a white or blue-white.<\/p>\n\n\n\n

\"M37\"<\/a>
DSS2 @ Wikisky.org <\/figcaption><\/figure>\n\n\n\n

Cometarios de Messier en 1771:<\/strong> La misma noche, observ\u00e9 un segundo c\u00famulo de peque\u00f1as estrellas que no estaba lejos del precedente, cerca de la pierna derecha del Cochero y sobre el paralelo de la estrella \u03c7 de esta constelaci\u00f3n: las estrellas son m\u00e1s peque\u00f1as que aquellas del c\u00famulo precedente: son tambi\u00e9n m\u00e1s cercanas unas de otras, y contienen una nebulosidad. Con un anteojo ordinario de 3 pies y medio, apenas se ven las estrellas; pero se distinguen con un instrumento de m\u00e1s grande efecto. Determin\u00e9 la posici\u00f3n del centro de este c\u00famulo, que puede tener de extensi\u00f3n 8 a 9 minutos de grado: su ascensi\u00f3n recta fue de 84\u00b0 15′ 12″, y su declinaci\u00f3n de 32\u00b0 11′ 51″ boreal.<\/p>\n\n\n\n

Comentarios de Messier en 1784:<\/strong> C\u00famulo de peque\u00f1as estrellas, un poco alejada del precedente, sobre el paralelo de \u03c7 del Cochero; las estrellas son m\u00e1s peque\u00f1as, m\u00e1s pr\u00f3ximas y contenidas en la nebulosidad; con un anteojo ordinario de 3 pies y medio, apenas se ven las estrellas. Este c\u00famulo es reportado en la carta del segundo cometa de 1771. Mem. Acad. 1777.<\/em><\/p>\n\n\n\n

Mapa para localizar a M37<\/strong><\/p>\n\n\n\n

\"Mapa<\/a>
Haga click para agrandar.<\/figcaption><\/figure>\n","protected":false},"excerpt":{"rendered":"

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