{"id":101,"date":"2005-02-04T01:45:00","date_gmt":"2005-02-04T01:45:00","guid":{"rendered":"http:\/\/perezmedia.net\/beltofvenus\/2005\/02\/04\/m96_m105_and_ng\/"},"modified":"2021-11-27T19:50:38","modified_gmt":"2021-11-27T19:50:38","slug":"m96_m105_and_ng","status":"publish","type":"post","link":"https:\/\/perezmedia.net\/beltofvenus\/2005\/02\/04\/m96_m105_and_ng\/","title":{"rendered":"Messier 96, Messier 105 and NGC 3384"},"content":{"rendered":"<p style=\"text-align: center\"><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2005\/img2005020402_M96M105.jpg\" border=\"1\" color=\"ffffff\"><\/p>\n<p><b>Observation Notes:<\/b><\/p>\n<p><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2005\/img2005020402_M96Finder.jpg\" border=\"1\" color=\"ffffff\" align=\"right\">These three galaxies were kind enough to fit in the field of view together. The two galaxies on the north side, M105 and NGC 3384 appeared about 10&#8242; apart, nucleus to nucleus. Their nucleii were softly stellar in appearance. M105 appeared basically circular and the brighter of the two, while NGC 3384 was elongated north-northeast to south-southwest. M96 was about 50&#8242; to the south. It was the largest and brightest of the three galaxies, elongated northwest to southeast. It didn&#8217;t have the same stellar nucleus as the other two, it was a bright nucleus, but not as concentrated. Observing all three galaxies at 120X didn&#8217;t expose more detail, mostly just verified what I had already seen at 37X.<\/p>\n<p><b>Factoids:<\/b><\/p>\n<p>M96 is a type Sa spiral galaxy that is the brightest of the Leo 1 group of galaxies, which includes M95 and M105 as well as other fainter galaxies. It lies about 38 million light years away and it&#8217;s bright inner portion extends about 66,000 light years in diameter. It has a fainter outer ring which extend that diameter to about 100,000 light years. The inner disk is composed of an old population of yellow stars. The galaxy contains a significant amount of dust and blue knots of star forming regions. It was discovered by Pierre M\u00e9chain in 1781 and thus cataloged by Charles Messier a few days later.<\/p>\n<p>M105 is an E1 elliptical galaxy that is a member of this same galaxy group and so is also about 38 million light years distant. It is often studied as a standard representative of elliptical galaxies. A Hubble Space Telescope survey of the galaxy has shown it to contain a massive central object weighing in at 50 million solar masses. M105 is moving away from us at 752 km\/sec. It was discovered by Pierre M\u00e9chan a few days after M96, but for some reason wasn&#8217;t included in Charles Messier&#8217;s catalog. It was added as M105 in 1947 by Helen Sawyer Hogg along with M106 and M107.<\/p>\n<p>NGC 3384 is an E7 elliptical galaxy that contains what appears to be a central bar. It also appears to be a member of the Leo 1 galaxy group.<\/p>\n<table width=\"470\" border=\"1\" cellspacing=\"0\" cellpadding-left=\"4\">\n<tbody>\n<tr>\n<td><b>Subject<\/b><\/td>\n<td>M96 (NGC 3368), M105 (NGC 3379), NGC 3384<\/td>\n<\/tr>\n<tr>\n<td><b>Classification<\/b><\/td>\n<td>Spiral and Eliptical Galaxies<\/td>\n<\/tr>\n<tr>\n<td><b>Position*<\/b><\/td>\n<td>Leo:<br \/>\nM96: [RA: 10:46.8 \/ Dec: +11:49]<br \/>\nM105: [RA: 10:47.8 \/ Dec: +12:35]<br \/>\nNGC 3384: [RA: 10:48.3 \/ Dec: +12:38]<\/td>\n<\/tr>\n<tr>\n<td><b>Size*<\/b><\/td>\n<td>M96: 7.1&#8242; x 5.1&#8242; \/ M105: 4.5&#8242; x 4.0&#8242; \/ NGC 3384: 5.9&#8242; x 2.6&#8242;<\/td>\n<\/tr>\n<tr>\n<td><b>Brightness*<\/b><\/td>\n<td>M96: 9.2 \/ M105: 9.3 \/ NGC 3384: 10.0<\/td>\n<\/tr>\n<tr>\n<td><b>Date\/Time<\/b><\/td>\n<td>February 4, 2005 &#8211; 1:45 AM<br \/>\n(February 4, 2005 &#8211; 08:45 UT)<\/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>32 mm (37X), 10 mm (120X)<\/td>\n<\/tr>\n<tr>\n<td><b>Conditions<\/b><\/td>\n<td>Clear, 25\u00b0F<\/td>\n<\/tr>\n<tr>\n<td><b>Seeing<\/b><\/td>\n<td>3\/10<\/td>\n<\/tr>\n<tr>\n<td><b>Transparency<\/b><\/td>\n<td>Mag 5.2<\/td>\n<\/tr>\n<tr>\n<td><b>Sources<\/b><\/td>\n<td><a href=\"http:\/\/www.seds.org\/\" target=\"_blank\" rel=\"noopener\">SEDS<\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>*Based on published data.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>M096<\/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":[16,28,18,19,29,21,53,15],"tags":[],"class_list":["post-101","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-leo","category-sketch-gallery"],"jetpack_featured_media_url":"","jetpack-related-posts":[{"id":77,"url":"https:\/\/perezmedia.net\/beltofvenus\/2005\/01\/15\/m65_and_m66\/","url_meta":{"origin":101,"position":0},"title":"Messier 65 and Messier 66","author":"jperez1690","date":"January 15, 2005","format":false,"excerpt":"M065","rel":"","context":"In &quot;Deep Sky&quot;","block_context":{"text":"Deep Sky","link":"https:\/\/perezmedia.net\/beltofvenus\/category\/deep-sky\/"},"img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":109,"url":"https:\/\/perezmedia.net\/beltofvenus\/2005\/02\/13\/m81_bodes_galax\/","url_meta":{"origin":101,"position":1},"title":"Messier 81 and Messier 82 &#8211; 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