{"id":37,"date":"2004-10-04T21:30:00","date_gmt":"2004-10-04T21:30:00","guid":{"rendered":"http:\/\/perezmedia.net\/beltofvenus\/2004\/10\/04\/m71\/"},"modified":"2021-11-27T18:47:06","modified_gmt":"2021-11-27T18:47:06","slug":"m71","status":"publish","type":"post","link":"https:\/\/perezmedia.net\/beltofvenus\/2004\/10\/04\/m71\/","title":{"rendered":"Messier 71"},"content":{"rendered":"<p style=\"text-align: center\"><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2004\/img20041004_03_M71.jpg\" border=\"1\" color=\"ffffff\"><\/p>\n<p><b>Observation Notes:<\/b><\/p>\n<p>Through the 25 mm eyepiece, this globular cluster was dim and small, but still remarkably grainy. It was also elongated. In the 10 mm eyepiece a number of stars showed at the edges and a few across the face. The shape was irregular, and seemed to make a soft arrowhead pointing WSW. An asterism of 4 stars across the surface points WSW too and leads to another line of 3 stars outside, pointing in the same direction. Not sure, but it looks like there is a detached clump of stars to the north with 3 brighter stars involved.<\/p>\n<p><b>Factoids:<\/b><\/p>\n<p>There has been a lot of confusion as to whether M71 should be considered a loose globular, or a dense open cluster. Not just because it is pretty loose for a globular, but also because it has a high metal content (only M69 has more), and it is fairly small at 27 light years across. Currently, it is considered to be a globular. It is 13,000 light years away, and is approaching at roughly 23 km\/sec. M71 was first seen by De Ch\u00e9seaux in 1746, and then catalogued by Charles Messier in 1780, and then first resolved into stars by William Herschel in 1783.<\/p>\n<table width=\"470\" border=\"1\" cellspacing=\"0\" cellpadding-left=\"4\">\n<tbody>\n<tr>\n<td><b>Subject<\/b><\/td>\n<td>M71\/NGC 6838<\/td>\n<\/tr>\n<tr>\n<td><b>Classification<\/b><\/td>\n<td>Globular Cluster<\/td>\n<\/tr>\n<tr>\n<td><b>Position<\/b><\/td>\n<td>Sagitta [RA: 19:53.8 \/ Dec: +18:47]*<\/td>\n<\/tr>\n<tr>\n<td><b>Size*<\/b><\/td>\n<td>7.2&#8242;<\/td>\n<\/tr>\n<tr>\n<td><b>Brightness*<\/b><\/td>\n<td>8.2<\/td>\n<\/tr>\n<tr>\n<td><b>Date\/Time<\/b><\/td>\n<td>10\/4\/04 &#8211; 9:30 PM<\/td>\n<\/tr>\n<tr>\n<td><b>Observing Loc.<\/b><\/td>\n<td>Flagstaff, AZ &#8211; Home<\/td>\n<\/tr>\n<tr>\n<td><b>Instrument<\/b><\/td>\n<td>Orion SVP 6LT Reflector (150 mm dia.\/1200 mm F\/L)<\/td>\n<\/tr>\n<tr>\n<td><b>Eyepieces\/Mag.<\/b><\/td>\n<td>25 mm (48X); 10 mm (120X)<\/td>\n<\/tr>\n<tr>\n<td><b>Seeing<\/b><\/td>\n<td>4\/10<\/td>\n<\/tr>\n<tr>\n<td><b>Transparency<\/b><\/td>\n<td>Mag 5<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>* Based on published data.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>M071<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[16,17,18,19,20,21,22,27,15],"tags":[],"class_list":["post-37","post","type-post","status-publish","format-standard","hentry","category-deep-sky","category-globular-cluster","category-messier","category-sg-deep-sky","category-sg-globular-cluster","category-sg-messier","category-sg-star-cluster","category-sgc-sagitta","category-sketch-gallery"],"jetpack_featured_media_url":"","jetpack-related-posts":[{"id":36,"url":"https:\/\/perezmedia.net\/beltofvenus\/2004\/10\/03\/m54\/","url_meta":{"origin":37,"position":0},"title":"Messier 54","author":"jperez1690","date":"October 3, 2004","format":false,"excerpt":"M054","rel":"","context":"In &quot;Deep Sky&quot;","block_context":{"text":"Deep 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