{"product_id":"m3-overlayed-with-in-christ-alone-3730-2077","title":"M3 Overlayed with \"In Christ Alone\"","description":"\u003cp data-rte-preserve-empty=\"true\"\u003eMessier 3 (M3; also NGC 5272) is a \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Globular_cluster\"\u003eglobular cluster\u003c\/a\u003e located 33.9 thousand light years from Earth in the northern \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Constellation\"\u003econstellation\u003c\/a\u003e of \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Canes_Venatici\"\u003eCanes Venatici\u003c\/a\u003e. It is one of the largest and brightest globular clusters discovered with around 500,000 stars.\u003c\/p\u003e\n\u003cp data-rte-preserve-empty=\"true\"\u003eIt was discovered on May 3, 1764, and was the first Messier object to be discovered by \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Charles_Messier\"\u003eCharles Messier\u003c\/a\u003e himself. Messier originally mistook the object for a nebula without stars. This mistake was corrected after the stars were resolved by \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/William_Herschel\"\u003eWilliam Herschel\u003c\/a\u003e around 1784. Since then, it has become one of the best-studied globular clusters. Identification of the cluster's unusually large \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Variable_star\"\u003evariable star\u003c\/a\u003e population was begun in 1913 by American astronomer \u003ca href=\"https:\/\/en.wikipedia.org\/wiki\/Solon_Irving_Bailey\"\u003eSolon Irving Bailey\u003c\/a\u003e and new variable members continue to be identified up through 2004.\u003c\/p\u003e","brand":"FLM Astro","offers":[{"title":"Default Title","offer_id":43215329755213,"sku":null,"price":5.0,"currency_code":"USD","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0716\/2662\/1005\/files\/InChristAlone.M3.jpg?v=1783381034","url":"https:\/\/flm3dastro.com\/products\/m3-overlayed-with-in-christ-alone-3730-2077","provider":"FLM","version":"1.0","type":"link"}