{"id":484,"date":"2009-09-07T01:17:37","date_gmt":"2009-09-07T01:17:37","guid":{"rendered":"http:\/\/perezmedia.net\/beltofvenus\/2009\/09\/07\/m85_ngc_4382_an\/"},"modified":"2009-09-07T01:17:37","modified_gmt":"2009-09-07T01:17:37","slug":"m85_ngc_4382_an","status":"publish","type":"post","link":"https:\/\/perezmedia.net\/beltofvenus\/2009\/09\/07\/m85_ngc_4382_an\/","title":{"rendered":"Messier 85 (NGC 4382) and NGC 4394"},"content":{"rendered":"<div class=\"imageblock\"><a href=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2009\/img2009042603_M85lg.jpg\" target=\"_blank\" rel=\"noopener\"><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2009\/img2009042603_M85.jpg\" alt=\"Sketch of Messier 85 (M85 \/ NGC 4382) and NGC 4394\"><\/a><\/p>\n<p class=\"caption\">Sketch of Messier 85 (NGC 4382) and NGC 4394<\/p>\n<p><i>Click image to view larger version.<\/i><\/p>\n<\/div>\n<p><b>Observation Notes:<\/b><\/p>\n<p>This was a great pair to observe. M85 had a stellar core and was mildly elongated at a PA of about 25 degrees and appeared to be about 4 x 3 arc minutes in size. A star was embedded just northeast of its core. NGC 4394 was about 7 arc minutes to the east-northeast and also had a stellar core. Its circular profile was adorned with a bar positioned at a PA of 140 degrees. It appeared to be about 2.5 arc minutes in diameter.<\/p>\n<p>A cursory look at the DSS image shows M85&#8217;s outer profile to be aligned almost exactly north-south. However, examining this and <a href=\"http:\/\/www.supernovae.net\/snimages\/reference\/n4382.jpg\" target=\"_blank\" rel=\"noopener\">other images<\/a> further suggests that the brighter, inner portion of the galaxy is elongated to the northeast as I noticed in this observation.<\/p>\n<div class=\"imageblock\"><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2009\/img2009042603_M85dss.jpg\" alt=\"Sketch\/DSS Photo Comparison of Messier 85 (M85 \/ NGC 4382) and NGC 4394\"><\/p>\n<p class=\"caption\">Sketch\/DSS Photo Comparison of Messier 85 (NGC 4382) and NGC 4394<\/p>\n<\/div>\n<p><b>Object Information:<\/b><\/p>\n<p>Galaxy M85 is about 125,000 light years in diameter and 60 million light years away. Although originally classified as a lenticular S0 galaxy, deep exposures show indications of spiral structure. Apparently, the foreground star northeast of the core has repeatedly been mistaken for a supernova. M85 is paired with barred spiral NGC 4394 about 8 arc minutes to the east. Both galaxies are receding at 700 m\/sec which suggests that they are physically paired.<\/p>\n<p>M85 was discovered in 1781 by Pierre M&eacute;chain, and is also cataloged as UGC 7508, MCG+03-32-029, VCC 798, PGC 40515, h 1242, GC 2946, CGCG 099.045, KCPG 334A.<\/p>\n<p>NGC 4394 was discovered by F.W. Herschel in 1784 and is also catalogued as UGC 7523, MCG+03-32-035, VCC 857, PGC 40614, H II-55, h 1251, GC 2957, CGCG 099.047, KCPG 334B, IRAS 12234+1829.<\/p>\n<table class=\"objectdata\">\n<tr>\n<td><b>Subject<\/b><\/td>\n<td class=\"subject\">M85 (NGC 4382) and NGC 4394<\/td>\n<\/tr>\n<tr>\n<td><b>Classification<\/b><\/td>\n<td>M85: Lenticular or Spiral Galaxy (Type SA(s)+P)<br \/>NGC 4394: Spiral Galaxy (Type (R)SB(r)b II)<\/td>\n<\/tr>\n<tr>\n<td><b>Position*<\/b><\/td>\n<td>M85: Coma Berenices [RA: 12:25:24.2 \/ Dec: +18:11:27]<br \/>NGC 4394: [RA: 12:25:55.6 \/ Dec: 18:12:50]<\/td>\n<\/tr>\n<tr>\n<td><b>Size*<\/b><\/td>\n<td>M85: 7.1&#8242; x 5.5&#8242;<br \/>NGC 4394: 3.6&#8242; x 3.2&#8242;<\/td>\n<\/tr>\n<tr>\n<td><b>Brightness*<\/b><\/td>\n<td>M85: 9.2 vMag; 10.1 bMag; 13.1 Surface Brightness<br \/>NGC 4394: 10.9 vMag; 11.5 bMag; 13.4 Surface Brightness<\/td>\n<\/tr>\n<tr>\n<td><b>Date\/Time<\/b><\/td>\n<td>APR 26, 2009 &#8211; 10:20 PM (APR 27, 2009 &#8211; 05:20 UT)<\/td>\n<\/tr>\n<tr>\n<td><b>Observing Loc.<\/b><\/td>\n<td>Flagstaff, Arizona &#8211;  Home<\/td>\n<\/tr>\n<tr>\n<td><b>Instrument<\/b><\/td>\n<td>Orion SkyQuest XT8 Dobsonian (203 mm dia.\/1200 mm F\/L)<\/td>\n<\/tr>\n<tr>\n<td><b>Eyepieces\/Mag.<\/b><\/td>\n<td>Pentax XW10 (120X)<\/td>\n<\/tr>\n<tr>\n<td><b>Conditions<\/b><\/td>\n<td>Clear, breezy, porch lights<\/td>\n<\/tr>\n<tr>\n<td><b>Seeing<\/b><\/td>\n<td>5\/10<\/td>\n<\/tr>\n<tr>\n<td><b>Transparency<\/b><\/td>\n<td>Mag 5.5 NELM<\/td>\n<\/tr>\n<tr>\n<td><b>*Sources<\/b><\/td>\n<td><a href=\"http:\/\/seds.org\/messier\/m\/m085.html\" target=\"_blank\" rel=\"noopener\">SEDS; <a href=\"http:\/\/www.ngcicproject.org\" target=\"_blank\" rel=\"noopener\">NGC\/IC Project<\/a>; <a href=\"http:\/\/archive.stsci.edu\/dss\/acknowledging.html\" target=\"_blank\" rel=\"noopener\">DSS<\/a>; Starry Night Pro Plus 5; <i>Atlas of the Messier Objects<\/i> &#8211; Ronald Stoyan<\/a><\/td>\n<\/tr>\n<\/table>\n","protected":false},"excerpt":{"rendered":"<p>M085<\/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":[16,28,18,19,29,21,89,15],"tags":[],"class_list":["post-484","post","type-post","status-publish","format-standard","hentry","category-deep-sky","category-galaxy","category-messier","category-sg-deep-sky","category-sg-galaxy","category-sg-messier","category-sgc-coma-berenices","category-sketch-gallery"],"jetpack_featured_media_url":"","jetpack-related-posts":[{"id":469,"url":"https:\/\/perezmedia.net\/beltofvenus\/2009\/05\/01\/messier_49_ngc\/","url_meta":{"origin":484,"position":0},"title":"Messier 49 (NGC 4472)","author":"jperez1690","date":"May 1, 2009","format":false,"excerpt":"M049","rel":"","context":"In &quot;Deep Sky&quot;","block_context":{"text":"Deep 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