{"id":319,"date":"2007-02-22T21:11:30","date_gmt":"2007-02-22T21:11:30","guid":{"rendered":"http:\/\/perezmedia.net\/beltofvenus\/2007\/02\/22\/struve_1669\/"},"modified":"2007-02-22T21:11:30","modified_gmt":"2007-02-22T21:11:30","slug":"struve_1669","status":"publish","type":"post","link":"https:\/\/perezmedia.net\/beltofvenus\/2007\/02\/22\/struve_1669\/","title":{"rendered":"Struve 1669"},"content":{"rendered":"<p style=\"text-align: center\"><img decoding=\"async\" src=\"http:\/\/www.perezmedia.net\/beltofvenus\/archives\/images\/2007\/img2007011802_STF1669.jpg\" border=\"1\" color=\"ffffff\"><\/p>\n<p><b>Observation Notes:<\/b><\/p>\n<p>About a degree and a half south of the Sombrero Galaxy, M104, you&#8217;ll find the multiple star, Struve 1669. The main attraction here is a pair of 6th magnitude F class stars. When observing them, don&#8217;t forget to take in a third, tenth-magnitude star 1 arc minute to the southwest. The two brighter stars appeared to be separated by about 4 arc seconds, and resting at a PA of 315 degrees. Values in the Washington Double Star Catalog list 5.4&#8243; from 1828 and 312 degrees from 1991. Color was tough to nail down, and I eventually settled for pale yellow for the northwest star and white for the southeast companion. Give it a look the next time you&#8217;re dancing around that nearby galactic hat and see what colors you perceive.<\/p>\n<table color=\"ffffff\" width=\"470\" border=\"0\" cellspacing=\"2\" cellpadding=\"4\" style=\"line-height: 150%\">\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Subject<\/b><\/td>\n<td bgcolor=\"#3f4d6d\"><b style=\"color: white\">Struve 1669<\/b><\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Classification<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">Multiple Star<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Position (J2000)<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">Corvus [RA: 12:41:15.8 \/ Dec: -13:00:49]*<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Position Angle*<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">AB: 312\u00c2\u00b0 (1991); AC: 235\u00c2\u00b0 (1900)<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Separation*<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">AB: 5.4&#8243; (1828); AC: 59&#8243; (1900)<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Magnitudes*<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">A: 6.0; B: 6.1; C: 10.5<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Spectral Types*<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">F5V; F5V; &#8211;<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Date\/Time<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">JAN 18, 2007 &#8211; 06:40 AM MST (JAN 18, 2007 &#8211; 13:40 UT)<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Observing Loc.<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">Flagstaff, AZ &#8211; Home<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Instrument<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">Orion SVP 6LT Reflector (150 mm dia.\/1200 mm F\/L)<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Eyepieces\/Mag.<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">10 mm + 2X Barlow (240X)<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Conditions<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">Clear, calm, 11\u00c2\u00b0 F<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Seeing<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">4\/10 Pickering<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>Transparency<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">NELM Mag ~5.0<\/td>\n<\/tr>\n<tr>\n<td bgcolor=\"#3f4d6d\"><b>References<\/b><\/td>\n<td bgcolor=\"#3f4d6d\">The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)<\/td>\n<\/tr>\n<\/table>\n<p>*Based on published data.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Struve 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