{"id":2181,"date":"2026-04-01T20:49:15","date_gmt":"2026-04-01T18:49:15","guid":{"rendered":"https:\/\/voyage-astrophoto.fr\/index.php\/messier\/m14\/"},"modified":"2026-04-01T20:49:15","modified_gmt":"2026-04-01T18:49:15","slug":"m14","status":"publish","type":"messier_object","link":"https:\/\/voyage-astrophoto.fr\/index.php\/messier\/m14\/","title":{"rendered":"M14 &#8211; M14"},"content":{"rendered":"<p>\u00c0 30 300 ann\u00e9es-lumi\u00e8re, il poss\u00e8de une luminosit\u00e9 absolue \u00e9quivalente \u00e0 400 000 Soleils.[10, 12] En 1938, une nova y a \u00e9t\u00e9 observ\u00e9e, \u00e9v\u00e9nement extr\u00eamement rare au sein d\\&rsquo;un amas globulaire. Contrairement \u00e0 M10 ou M12, il reste difficile \u00e0 r\u00e9soudre en \u00e9toiles individuelles sans un t\u00e9lescope d\\&rsquo;au moins 200 mm en raison de sa concentration et de la poussi\u00e8re interstellaire sur le trajet lumineux.[4, 2]<\/p>\n","protected":false},"featured_media":0,"template":"","meta":[],"class_list":["post-2181","messier_object","type-messier_object","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/voyage-astrophoto.fr\/index.php\/wp-json\/wp\/v2\/messier_object\/2181","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/voyage-astrophoto.fr\/index.php\/wp-json\/wp\/v2\/messier_object"}],"about":[{"href":"https:\/\/voyage-astrophoto.fr\/index.php\/wp-json\/wp\/v2\/types\/messier_object"}],"wp:attachment":[{"href":"https:\/\/voyage-astrophoto.fr\/index.php\/wp-json\/wp\/v2\/media?parent=2181"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}