{"id":695,"date":"2025-02-25T00:12:24","date_gmt":"2025-02-25T00:12:24","guid":{"rendered":"https:\/\/www.lonepeak.space\/?p=695"},"modified":"2025-03-26T15:35:07","modified_gmt":"2025-03-26T15:35:07","slug":"m-82","status":"publish","type":"post","link":"https:\/\/www.lonepeak.space\/index.php\/2025\/02\/25\/m-82\/","title":{"rendered":"M 82"},"content":{"rendered":"\n<figure class=\"wp-block-gallery has-nested-images columns-default is-cropped wp-block-gallery-1 is-layout-flex wp-block-gallery-is-layout-flex\">\n<figure class=\"wp-block-image size-full\"><a href=\"https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z.webp\"><img loading=\"lazy\" decoding=\"async\" width=\"2517\" height=\"1729\" data-id=\"534\" src=\"https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z.webp\" alt=\"\" class=\"wp-image-534\" srcset=\"https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z.webp 2517w, https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z-300x206.webp 300w, https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z-1024x703.webp 1024w, https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z-768x528.webp 768w, https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z-1536x1055.webp 1536w, https:\/\/www.lonepeak.space\/wp-content\/uploads\/2025\/02\/M82Z-2048x1407.webp 2048w\" sizes=\"auto, (max-width: 2517px) 100vw, 2517px\" \/><\/a><\/figure>\n<\/figure>\n\n\n\n<p class=\"is-style-default\" style=\"padding-top:var(--wp--preset--spacing--30);font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.49), 19px);font-style:normal;font-weight:500\"><strong>Wikipedia Description:<\/strong><\/p>\n\n\n\n<p style=\"font-size:clamp(14.642px, 0.915rem + ((1vw - 3.2px) * 0.721), 22px);\"><strong>Messier 82<\/strong> (also known as <strong>NGC 3034<\/strong>, <strong>Cigar Galaxy<\/strong> or <strong>M82<\/strong>) is a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Starburst_galaxy\">starburst galaxy<\/a> approximately 12 million <a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">light-years<\/a> away in the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Constellation\">constellation<\/a> <a href=\"https:\/\/en.wikipedia.org\/wiki\/Ursa_Major\">Ursa Major<\/a>. It is the second-largest member of the <a href=\"https:\/\/en.wikipedia.org\/wiki\/M81_Group\">M81 Group<\/a>, with the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Galaxy#Isophotal_diameter\">D<sub>25<\/sub> isophotal diameter<\/a> of 12.52 <a href=\"https:\/\/en.wikipedia.org\/wiki\/Parsec#Parsecs_and_kiloparsecs\">kiloparsecs<\/a> (40,800 <a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">light-years<\/a>).<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-ned-1\">[1]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-RC3-5\">[5]<\/a><\/sup> It is about five times <a href=\"https:\/\/en.wikipedia.org\/wiki\/Luminosity#Astronomy\">more luminous<\/a> than the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Milky_Way\">Milky Way<\/a> and its central region is about one hundred times more luminous.<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-Barkeretal2008-7\">[7]<\/a><\/sup> The <a href=\"https:\/\/en.wikipedia.org\/wiki\/Starburst_region\">starburst activity<\/a> is thought to have been triggered by interaction with neighboring galaxy <a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_81\">M81<\/a>. As one of the closest starburst galaxies to Earth, M82 is the prototypical example of this galaxy type.<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-Barkeretal2008-7\">[7]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-Starburst-8\">[a]<\/a><\/sup> <a href=\"https:\/\/en.wikipedia.org\/wiki\/SN_2014J\">SN 2014J<\/a>, a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Type_Ia_supernova\">type Ia supernova<\/a>, was discovered in the galaxy on 21 January 2014.<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-astronomerstelegram.org-9\">[8]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-Huffington_Post-10\">[9]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-slate.com-11\">[10]<\/a><\/sup> In 2014, in studying M82, scientists discovered the brightest pulsar yet known, designated <a href=\"https:\/\/en.wikipedia.org\/wiki\/M82_X-2\">M82 X-2<\/a>.<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-12\">[11]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-13\">[12]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-14\">[13]<\/a><\/sup><\/p>\n\n\n\n<p style=\"font-size:clamp(14.642px, 0.915rem + ((1vw - 3.2px) * 0.721), 22px);\">In November 2023, a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Gamma-ray_burst\">gamma-ray burst<\/a> was observed in M82, which was determined to have come from a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Magnetar\">magnetar<\/a>, the first such event detected outside the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Milky_Way\">Milky Way<\/a> (and only the fourth such event ever detected).<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-15\">[14]<\/a><\/sup><sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-16\">[15]<\/a><\/sup><\/p>\n\n\n\n<h2 class=\"wp-block-heading\" id=\"Discovery\" style=\"font-size:clamp(14.642px, 0.915rem + ((1vw - 3.2px) * 0.721), 22px);\">Discovery<\/h2>\n\n\n\n<p style=\"font-size:clamp(14.642px, 0.915rem + ((1vw - 3.2px) * 0.721), 22px);\">M82, with <a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_81\">M81<\/a>, was discovered by <a href=\"https:\/\/en.wikipedia.org\/wiki\/Johann_Elert_Bode\">Johann Elert Bode<\/a> in 1774; he described it as a &#8220;nebulous patch&#8221;, this one about 3\u20444 degree away from the other, &#8220;very pale and of elongated shape&#8221;. In 1779, <a href=\"https:\/\/en.wikipedia.org\/wiki\/Pierre_M%C3%A9chain\">Pierre M\u00e9chain<\/a> independently rediscovered both objects and reported them to <a href=\"https:\/\/en.wikipedia.org\/wiki\/Charles_Messier\">Charles Messier<\/a>, who added them to his catalog.<sup><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82#cite_note-seds-17\">[16]<\/a><\/sup><\/p>\n\n\n\n<p style=\"padding-top:var(--wp--preset--spacing--30);font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.49), 19px);\"><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_82\">Wikipedia: M82<\/a><\/p>\n\n\n\n<div style=\"height:39px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<p style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.49), 19px);font-style:normal;font-weight:500\">Acquisition Details:<\/p>\n\n\n\n<figure class=\"wp-block-table is-style-regular\" style=\"font-size:clamp(14px, 0.875rem + ((1vw - 3.2px) * 0.49), 19px);\"><table class=\"has-fixed-layout\" style=\"border-top-style:none;border-top-width:0px;border-right-style:none;border-right-width:0px;border-bottom-style:none;border-bottom-width:0px;border-left-width:1px\"><tbody><tr><td>Telescope<\/td><td>Takahashi TOA-130<\/td><\/tr><tr><td>Optics<\/td><td>Takahashi TOA-645 Flattener<\/td><\/tr><tr><td>Filter<\/td><td>None<\/td><\/tr><tr><td>Camera<\/td><td>ASI2600MC Pro OSC<\/td><\/tr><tr><td>Integration Time<\/td><td>3.6 Hours<\/td><\/tr><tr><td>Subframes<\/td><td>109 x 120 Seconds<\/td><\/tr><tr><td>Date<\/td><td>January 30, 2025<\/td><\/tr><tr><td>Location<\/td><td>Carlsbad, California<\/td><\/tr><\/tbody><\/table><\/figure>\n","protected":false},"excerpt":{"rendered":"<p>Wikipedia Description: Messier 82 (also known as NGC 3034, Cigar Galaxy or M82) is a starburst galaxy approximately 12 million light-years away in the constellation Ursa Major. It is the second-largest member of the M81 Group, with the D25 isophotal diameter of 12.52 kiloparsecs (40,800 light-years).[1][5] It is about five times more luminous than the [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":534,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-695","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/posts\/695","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/comments?post=695"}],"version-history":[{"count":4,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/posts\/695\/revisions"}],"predecessor-version":[{"id":716,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/posts\/695\/revisions\/716"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/media\/534"}],"wp:attachment":[{"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/media?parent=695"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/categories?post=695"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.lonepeak.space\/index.php\/wp-json\/wp\/v2\/tags?post=695"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}