{"id":1608,"date":"2016-04-03T00:00:00","date_gmt":"2016-04-02T23:00:00","guid":{"rendered":"http:\/\/skymania.com\/spa_responsive\/eclipsing-binary-predictions-2016-apr-may\/"},"modified":"2017-12-07T17:31:46","modified_gmt":"2017-12-07T17:31:46","slug":"eclipsing-binary-predictions-2016-apr-may","status":"publish","type":"post","link":"https:\/\/www.popastro.com\/variablestar\/2016\/04\/03\/eclipsing-binary-predictions-2016-apr-may\/","title":{"rendered":"Eclipsing Binary Predictions : 2016 Apr-May"},"content":{"rendered":"<p>\n\tHere are predictions for eclipses that are reasonably favourable from the UK during April and May:<\/p>\n<p><!--more--><\/p>\n<p>\n\tTimes are in UT (same as GMT, 1 hour behind BST &#8211; so, for example, 20.6h UT is 21.6h BST)<\/p>\n<p>\n\t<u><strong>RZ Cassiopeiae<\/strong><\/u><\/p>\n<p>\n\tEclipses last 4.8h, with most of the brightness changes taking place during the middle 3 hours. The times shown below are for the mid-point of the eclipses<\/p>\n<p>\n\tApr: &nbsp; 3d&nbsp; 21.2h , 5d&nbsp; 1.9h , 9d&nbsp; 20.6h , 11d&nbsp; 1.3h , 17d&nbsp; 0.8h , 23d&nbsp; 0.2h , 28d&nbsp; 23.6h.<\/p>\n<p>\n\tMay:&nbsp; 4d&nbsp; 23.1h , 10d&nbsp; 22.5h , 16d&nbsp; 21.9h , 18d&nbsp; 2.6h , 22d&nbsp; 21.3h , 24d&nbsp; 2.0h , 30d&nbsp; 1.5h.<\/p>\n<p>\n\t<u><strong>U Cephei<\/strong><\/u><\/p>\n<p>\n\tEclipses last for approx 9 hours. The times shown below are for the eclipse mid-point. Eclipses are total, so there is a period of constant brightness around the middle of the eclipse.<\/p>\n<p>\n\tMay:&nbsp; 7d&nbsp; 3.2h , 12d&nbsp; 2.9h , 17d&nbsp; 2.6h , 22d&nbsp; 2.3h , 27d&nbsp; 2.0h.<\/p>\n<p>\n\t<u><strong>U Coronae Borealis<\/strong><\/u><\/p>\n<p>\n\tEclipses last for approx 12 hours. The times shown below are for the eclipse mid-point.<\/p>\n<p>\n\tApr: &nbsp; 2d&nbsp; 2.7h , 9d&nbsp; 0.3h , 15d&nbsp; 22.0h , 22d 19.7h.<\/p>\n<p>\n\tMay:&nbsp; 10d&nbsp; 2.0h , 16d&nbsp; 23.7h , 23d&nbsp; 21.4h , 30d 19.1h.<\/p>\n<p>\n\t<strong><u>beta Lyrae<\/u><\/strong><\/p>\n<p>\n\tBoth the deeper primary eclipse and less deep secondary eclipse can be followed visually. There is no period of constant brightness between eclipses.<\/p>\n<p>\n\tPrimary:&nbsp; Apr&nbsp; 13-15 , 26-28 ,&nbsp; May&nbsp; 8-10 , 21-23.<\/p>\n<p>\n\tSecondary:&nbsp; Apr&nbsp; 7-8 , 20-21 , May&nbsp; 2-3 , 15-16 , 28-29.<\/p>\n<p>\n\t<u><strong>beta Persei (<\/strong><\/u><u><strong>Algol)<\/strong><\/u><\/p>\n<p>\n\tEclipses last for approx 10 hours. The times shown below are for the eclipse mid-point. Eclipses are total, so there is a period of constant brightness around the middle of the eclipse.<\/p>\n<p>\n\tApr: &nbsp; 7d&nbsp; 23.5h , 10d&nbsp; 20.3h , 28d&nbsp; 1.2h , 30d&nbsp; 22.0h.<\/p>\n<p>\n\tMay:&nbsp; 20d&nbsp; 23.7h.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Here are predictions for eclipses that are reasonably favourable from the UK during April and May:<\/p>\n","protected":false},"author":4,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_monsterinsights_skip_tracking":false,"footnotes":""},"categories":[2],"tags":[],"class_list":["post-1608","post","type-post","status-publish","format-standard","hentry","category-variable-stars"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 5.0.0.1 - aioseo.com -->\n\t<meta name=\"description\" content=\"Here are predictions for eclipses that are reasonably favourable from the UK during April and May: Times are in UT (same as GMT, 1 hour behind BST - so, for example, 20.6h UT is 21.6h BST) RZ Cassiopeiae Eclipses last 4.8h, with most of the brightness changes taking place during the middle 3 hours. 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