{"id":563,"date":"2016-02-18T20:32:13","date_gmt":"2016-02-18T20:32:13","guid":{"rendered":"http:\/\/www.astronotas.org\/messier\/?p=563"},"modified":"2023-12-09T15:46:56","modified_gmt":"2023-12-09T19:46:56","slug":"m26","status":"publish","type":"post","link":"https:\/\/www.astronotas.org\/messier\/m26\/","title":{"rendered":"Messier 26"},"content":{"rendered":"\n
\"M26\"<\/a><\/figure>\n\n\n\n

Objeto: M26<\/strong><\/p>\n\n\n\n

Constelaci\u00f3n: Scutum
Fecha: 1994.08.28 | Hora: 1:56 UT
Lugar: Jauca, Santa Isabel, PR<\/p>\n\n\n\n

Tipo de objeto: C\u00famulo abierto, clase F
Nombre: NGC 6694
Magnitud: 8.0 | Tama\u00f1o: 15′
R.A. 18h45.2m | Dec. \u20139\u00b024′
\u00c9poca: 2000.0<\/p>\n\n\n\n

Instrumento: Meade MTS-SN 6
Ocular: 8.8 mm UWA | Aumento: 173x
Campo aparente: 84\u00b0 | Campo actual: 28′
Otros: lente Barlow 2x<\/p>\n\n\n\n

Carta en Uranometr\u00eda 2000.0: 295<\/p>\n\n\n\n

\"M26\"<\/a>
Hunter Wilson [origen<\/a>] <\/figcaption><\/figure>\n\n\n\n

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

Espa\u00f1ol:<\/strong> M26, aunque interesante, luce menos atractivo de lo que se puede apreciar en astrofotograf\u00edas. Exhib\u00eda menos cantidad de estrellas, algunas de las cuales eran bien tenues. Tampoco se detectan colores en sus componentes, pues todas se ven blancas.<\/p>\n\n\n\n

English:<\/strong> Although it is interesting, M26 looks less attractive than it can be seen in pictures. It exhibited fewer stars, some of which were quite faint. No colors were detected in any of its components because all of them looked white.<\/p>\n\n\n\n

\"M26\"<\/a>
Hillary Mathis, Vanessa Harvey, REU program\/NOAO\/AURA\/NSF [origen<\/a>] <\/figcaption><\/figure>\n\n\n\n

Cometarios de Messier en 1771:<\/strong> La misma noche, descubr\u00ed otro c\u00famulo de estrellas cerca de \u03b7 y \u03bf de Ant\u00ednoo, entre las cuales se halla una que es m\u00e1s brillante que las otras: con un anteojo de tres pies, no es posible distinguirlas, hace falta emplear un buen instrumento: las vi muy bien con un telescopio gregoriano que aumentaba ciento cuatro veces; entre ellas no se ve ninguna nebulosidad, pero con un anteojo de 3 pies y medio estas estrellas parecen formar una sola, bajo la forma de una nebulosa; el di\u00e1metro de este c\u00famulo puede tener 2 minutos de grado. Determin\u00e9 su posici\u00f3n como igual que la de la estrella \u03bf de Ant\u00ednoo, su ascensi\u00f3n recta es de 278\u00b0 5′ 25″ y su declinaci\u00f3n de 9\u00b0 38′ 14″ meridional.<\/p>\n\n\n\n

Comentarios de Messier en 1784:<\/strong> C\u00famulo de estrellas cerca de las estrellas \u03b7 y \u03bf de Ant\u00ednoo, entre las cuales hay una que tiene m\u00e1s luz: con un anteojo de tres pies no se puede distinguir, hace falta emplear un buen instrumento. Este c\u00famulo no contiene ninguna nebulosidad.<\/p>\n\n\n\n

Mapa para localizar a M26<\/strong><\/p>\n\n\n\n

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

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