{"id":80,"date":"2015-02-27T06:00:00","date_gmt":"2015-02-27T06:00:00","guid":{"rendered":"http:\/\/localhost:4545\/guide-to-r-leonis\/"},"modified":"2025-03-22T16:21:33","modified_gmt":"2025-03-22T16:21:33","slug":"guide-to-r-leonis","status":"publish","type":"page","link":"https:\/\/www.popastro.com\/variablestar\/reference\/guides\/guide-to-r-leonis\/","title":{"rendered":"Guide to R Leonis"},"content":{"rendered":"<p>One of the brighter Mira type variables, located only 5 degrees from the bright star Regulus (Alpha Leonis).<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter size-full wp-image-2679\" src=\"https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2017\/11\/RLeo_LC_2014-2017jun.png\" alt=\"r leo\" width=\"647\" height=\"322\" srcset=\"https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2017\/11\/RLeo_LC_2014-2017jun.png 647w, https:\/\/www.popastro.com\/variablestar\/wp-content\/uploads\/sites\/3\/2017\/11\/RLeo_LC_2014-2017jun-300x149.png 300w\" sizes=\"auto, (max-width: 647px) 100vw, 647px\" \/><\/p>\n<p>R Leonis, like other Mira type variables, is a red giant star. The brightness variations were first recognised by J A Koch in 1782. The main cause of the brightness variations is pulsations in the star&#8217;s outer layers. However, there are also smaller scale changes that are related to the formation of very simple molecules when the pulsations cause the surface layers to cool and then split apart when the contraction phase causes the temperature to rise again.<\/p>\n<table class=\"spa_data_table\">\n<tbody>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Extreme brightness range<\/td>\n<td align=\"center\">4.8 &#8211; 11.0<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">More typical range<\/td>\n<td align=\"center\">5.4 &#8211; 10.5<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Period of variation<\/td>\n<td align=\"center\">310 days (approx 10months)<\/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 per month<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Observe using<\/td>\n<td align=\"center\">40mm or 50mm binoculars will suffice when near maximum, but 50-80mm binoculars will be required when fainter. A telescope is required to follow R Leo all the way down to minimum<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Visibility<\/td>\n<td align=\"center\">mid September to early June<\/td>\n<\/tr>\n<tr class=\"data\" align=\"left\">\n<td align=\"left\">Dates of maxima<\/td>\n<td align=\"center\">January 2025, November 2025<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>The following finder charts show the location of R Leonis. North is at the top of each chart.<\/p>\n<figure style=\"width: 667px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" src=\"\/images\/variablestar\/RLeo_wide_view.PNG\" alt=\"\" width=\"667\" height=\"377\" \/><figcaption class=\"wp-caption-text\">.<\/figcaption><\/figure>\n<p>The second chart, which is approx 9 degrees by 5 degrees, shows more detail around R Leo.<\/p>\n<p>You can follow the changes in R Leo by comparing its brightness with that of the comparison stars. These are labelled with their magnitudes (with the decimal point omitted). Thus, for example, &#8217;78&#8217; labels a comparison star of magnitude 7.8.<\/p>\n<figure style=\"width: 641px\" class=\"wp-caption alignnone\"><img loading=\"lazy\" decoding=\"async\" src=\"\/images\/variablestar\/RLeo_chart.PNG\" alt=\"\" width=\"641\" height=\"389\" \/><figcaption class=\"wp-caption-text\">.<\/figcaption><\/figure>\n","protected":false},"excerpt":{"rendered":"<p>A guide to the Mira type variable star R Leonis<\/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-80","page","type-page","status-publish","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=\"A guide to the Mira type variable star R Leonis\" \/>\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.popastro.com\/variablestar\/reference\/guides\/guide-to-r-leonis\/\" \/>\n\t<meta name=\"generator\" content=\"All in One SEO (AIOSEO) 5.0.0.1\" \/>\n\t\t<meta property=\"og:locale\" content=\"en_GB\" \/>\n\t\t<meta property=\"og:site_name\" content=\"Variable Star Section -\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"Guide to R Leonis - 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