{"id":54,"date":"2015-02-12T06:00:00","date_gmt":"2015-02-12T06:00:00","guid":{"rendered":"http:\/\/localhost:4545\/guide-to-alpha-herculis\/"},"modified":"2018-01-23T11:14:39","modified_gmt":"2018-01-23T11:14:39","slug":"guide-to-alpha-herculis","status":"publish","type":"page","link":"https:\/\/www.popastro.com\/variablestar\/reference\/guides\/guide-to-alpha-herculis\/","title":{"rendered":"Guide to Alpha Herculis"},"content":{"rendered":"<p>A slowly changing variable star that is observable with the naked eye from reasonably dark observing sites.<\/p>\n<figure id=\"attachment_2820\" aria-describedby=\"caption-attachment-2820\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-2820\" src=\"https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2018\/01\/AlphaHer_LC_2014-2017_nomags.png\" alt=\"\" width=\"500\" height=\"251\" srcset=\"https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2018\/01\/AlphaHer_LC_2014-2017_nomags.png 660w, https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2018\/01\/AlphaHer_LC_2014-2017_nomags-300x150.png 300w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><figcaption id=\"caption-attachment-2820\" class=\"wp-caption-text\">Four year light curve for Alpha Herculis<\/figcaption><\/figure>\n<p>With Alpha Herculis being a quite red star, magnitude estimates can differ by a few tenths of a magnitude between observers. Hence, rather than plot this light curve with magnitude values on the vertical scale (and risk confusing observers whose magnitude values don&#8217;t exactly match those shown) , the scale has been left blank.\u00a0 Although some observers will routinely see Alpha Her brighter than will other observers, the hope is that each observer will see a similar pattern of rises and falls in brightness.<\/p>\n<p>Alpha Herculis is a red supergiant star. It doesn&#8217;t show huge changes in brightness but, with care, its brightness changes can be followed visually. The brightness changes are due to pulsations in the star&#8217;s cool outer layers.<\/p>\n<table border=\"1\" width=\"550\" cellspacing=\"0\" align=\"center\">\n<tbody>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Extreme brightness range<\/td>\n<td align=\"center\">3.0 &#8211; 4.0<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">More typical amplitude<\/td>\n<td align=\"center\">about 0.4 mag<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Period of variation<\/td>\n<td align=\"center\">Some sources suggest 100 days ; others suggest around 300 days<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Frequency of observation<\/td>\n<td align=\"center\">Worth checking a few times each month<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Observe using<\/td>\n<td align=\"center\">Naked eye from reasonably dark observing sites. May need to use 40mm or 50mm binoculars if light pollution is a problem.<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Visibility<\/td>\n<td align=\"center\">Can be observed all year round, but is not visible in the evening sky from December to April<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>The finder chart which follows show the location of Alpha Herculis.<\/p>\n<p>You can follow the brightness changes of Alpha Herculis by comparing it with the lettered comparison stars.<\/p>\n<p><img decoding=\"async\" src=\"\/images\/variablestar\/AlphaHer_chart.PNG\" alt=\"\" \/><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A guide to the semi-regular variable star Alpha Herculis<\/p>\n","protected":false},"author":4,"featured_media":0,"parent":81,"menu_order":0,"comment_status":"closed","ping_status":"open","template":"","meta":{"_monsterinsights_skip_tracking":false,"footnotes":""},"categories":[2],"tags":[],"class_list":["post-54","page","type-page","status-publish","hentry","category-variable-stars"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 5.0.0.1 - 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