{"id":1267,"date":"2019-11-24T15:01:00","date_gmt":"2019-11-24T19:01:00","guid":{"rendered":"http:\/\/www.astronotas.org\/messier\/?p=1267"},"modified":"2023-12-09T22:09:18","modified_gmt":"2023-12-10T02:09:18","slug":"m50","status":"publish","type":"post","link":"https:\/\/www.astronotas.org\/messier\/m50\/","title":{"rendered":"Messier 50"},"content":{"rendered":"\n
\"M50\"<\/a><\/figure>\n\n\n\n

Objeto: M50<\/strong><\/p>\n\n\n\n

Constelaci\u00f3n: Monoceros
Fecha: 1995.01.07 | Hora: 5:17 UT
Lugar de observaci\u00f3n: Jauca, Santa Isabel, PR<\/p>\n\n\n\n

Tipo de objeto: C\u00famulo abierto
Nombre: (NGC 2323)
Magnitud: 5.9 | Tama\u00f1o: 16′
R.A. 7h03.2m | Dec. \u20138\u00b020′
\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: 40′
Otros: lente Barlow 2x<\/p>\n\n\n\n

Carta en Uranometr\u00eda 2000.0: 273<\/p>\n\n\n\n

\"M50\"<\/a>
John Mirtle [origen<\/a>]<\/figcaption><\/figure>\n\n\n\n

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

Espa\u00f1ol:<\/strong> M50 luce bastante grande. Muchas de sus estrellas son brillantes, la mayor\u00eda de ellas color blanco, aunque se detectan, con facilidad, estrellas amarillas.<\/p>\n\n\n\n

English:<\/strong> M50 looks pretty large. Many of its stars are bright, most of them are white, even though there are some yellow stars easily detectable.<\/p>\n\n\n\n

\"M50\"<\/a>
NOAO\/AURA\/NSF [origen<\/a>]<\/figcaption><\/figure>\n\n\n\n

Comentarios de Messier en 1784:<\/strong>  C\u00famulo de peque\u00f1as estrellas m\u00e1s o menos brillantes, debajo del muslo derecho del Monoceros, arriba de la estrella \u03b8 de la oreja del gran Can, y cerca de una estrella de 7.ma magnitud. Fue observando el cometa de 1772 que M. Messier observ\u00f3 este c\u00famulo. Fue reportado en la carta de este cometa, que \u00e9l la traz\u00f3. Mem. Acad. 1772.<\/p>\n\n\n\n

Mapa para localizar a M50<\/strong><\/p>\n\n\n\n

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

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