{"id":1317,"date":"2018-12-31T13:34:28","date_gmt":"2018-12-31T12:34:28","guid":{"rendered":"http:\/\/www.vulkanlandsternwarte.at\/?p=1317"},"modified":"2018-12-31T13:38:35","modified_gmt":"2018-12-31T12:38:35","slug":"ic-434","status":"publish","type":"post","link":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wordpress\/2018\/12\/31\/ic-434\/","title":{"rendered":"IC 434"},"content":{"rendered":"
\"\"<\/a>
IC 434<\/strong>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0 \u00a0\u00a0 \u00a0\u00a0 Siegfried Hold<\/figcaption><\/figure>\n

IC 434, wegen seiner Form wird er auch „Pferdekopfnebel“ genannt.
\nEin sehr beliebtes Objekt f\u00fcr Fotografen am Winterhimmel. Alnitak, der helle Stern, ist der linke untere vom „G\u00fcrtel des Orion“. Die Region wird von der „Sigma Orionis“ Gruppe, eingebettet in NGC 2030, zum leuchten angeregt.
\nIC 434 liegt in einer Entfernung von etwa 1500 Lichtjahren.<\/p>\n

Aufnahmedatum: <\/b>1.12.2018
\nTeleskop: <\/b>8″ Astrograph (Wuchtl)
\nKamera: <\/b>ASI 1600MC pro
\nFilter: <\/b>Astronomic L2
\nAufnahmedaten: <\/b>15X 300s
\nProzess:<\/b> PixInsight<\/p>\n

\"\"<\/a><\/p>\n

 <\/p>\n","protected":false},"excerpt":{"rendered":"

IC 434, wegen seiner Form wird er auch „Pferdekopfnebel“ genannt. Ein sehr beliebtes Objekt f\u00fcr Fotografen am Winterhimmel. Alnitak, der helle Stern, ist der linke untere vom „G\u00fcrtel des Orion“. Die Region wird von der „Sigma Orionis“ Gruppe, eingebettet in NGC 2030, zum leuchten angeregt. IC 434 liegt in einer Entfernung von etwa 1500 Lichtjahren. … <\/p>\n

Read more „IC 434“<\/span><\/a><\/p>\n","protected":false},"author":10,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6],"tags":[],"class_list":["post-1317","post","type-post","status-publish","format-standard","hentry","category-beobachtungen"],"_links":{"self":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/1317","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/users\/10"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/comments?post=1317"}],"version-history":[{"count":3,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/1317\/revisions"}],"predecessor-version":[{"id":1322,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/1317\/revisions\/1322"}],"wp:attachment":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/media?parent=1317"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/categories?post=1317"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/tags?post=1317"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}