{"id":279,"date":"2023-06-19T11:52:07","date_gmt":"2023-06-19T10:52:07","guid":{"rendered":"https:\/\/tithijagad.com\/?p=279"},"modified":"2024-06-30T10:15:13","modified_gmt":"2024-06-30T09:15:13","slug":"the-upcoming-supernova","status":"publish","type":"post","link":"https:\/\/tithijagad.com\/index.php\/2023\/06\/19\/the-upcoming-supernova\/","title":{"rendered":"The Upcoming Supernova"},"content":{"rendered":"\n<p class=\"has-medium-font-size\"><strong>Betelgeuse<\/strong>&nbsp;is a&nbsp;red supergiant&nbsp;star of&nbsp;spectral type&nbsp;M1-2 and one of the&nbsp;largest&nbsp;visible to the&nbsp;naked eye. It is usually the&nbsp;tenth-brightest&nbsp;star&nbsp;in the&nbsp;night sky&nbsp;and, after&nbsp;Rigel, the second-brightest in the&nbsp;constellation&nbsp;of&nbsp;Orion. It is a distinctly reddish,&nbsp;semiregular variable star&nbsp;whose&nbsp;apparent magnitude, varying between +0.0 and +1.6, has the widest range displayed by any&nbsp;first-magnitude star. At&nbsp;near-infrared&nbsp;wavelengths, Betelgeuse is the brightest star in the night sky. Its&nbsp;Bayer designation&nbsp;is&nbsp;<strong>\u03b1&nbsp;Orionis<\/strong>,&nbsp;Latinised&nbsp;to&nbsp;<strong>Alpha Orionis<\/strong>&nbsp;and abbreviated&nbsp;<strong>Alpha&nbsp;Ori<\/strong>&nbsp;or&nbsp;<strong>\u03b1&nbsp;Ori<\/strong>.<\/p>\n\n\n\n<p class=\"has-medium-font-size\">If it were at the center of our&nbsp;Solar System, its surface would lie beyond the&nbsp;asteroid belt&nbsp;and it would engulf the&nbsp;orbits&nbsp;of&nbsp;Mercury,&nbsp;Venus,&nbsp;Earth, and&nbsp;Mars. Calculations of Betelgeuse&#8217;s mass range from slightly under ten to a little over twenty times that of the&nbsp;Sun. For&nbsp;various reasons, its distance has been quite difficult to measure; current best estimates are on the order of 500\u2013600&nbsp;light-years&nbsp;from the Sun&nbsp;\u2013 a comparatively wide uncertainty for a relatively nearby star. Its&nbsp;absolute magnitude&nbsp;is about \u22126. Less than 10&nbsp;million years old, Betelgeuse has evolved rapidly because of its large mass and is expected to end its evolution with a&nbsp;supernova&nbsp;explosion, most likely within 100,000&nbsp;years. When Betelgeuse explodes, it will shine as bright as the&nbsp;half-Moon\u2014 for more than three months. Life on Earth will be unharmed.&nbsp;Having been ejected from its birthplace in the&nbsp;Orion OB1 association&nbsp;\u2013 which includes the stars in&nbsp;Orion&#8217;s Belt&nbsp;\u2013 this&nbsp;runaway star&nbsp;has been observed to be moving through the&nbsp;interstellar medium&nbsp;at a speed of&nbsp;30&nbsp;km\/s, creating a&nbsp;bow shock&nbsp;over four light-years wide.<\/p>\n\n\n\n<p class=\"has-medium-font-size\">In 1920, Betelgeuse became the first extrasolar star whose&nbsp;photospheres&#8217; angular size was measured. Subsequent studies have reported an&nbsp;angular diameter&nbsp;(i.e., apparent size) ranging from 0.042 to 0.056&nbsp;arcseconds; that range of determinations is ascribed to non-sphericity,&nbsp;limb darkening,&nbsp;pulsations&nbsp;and varying appearance at different&nbsp;wavelengths. It is also surrounded by a complex, asymmetric&nbsp;envelope, roughly 250&nbsp;times the size of the star, caused by&nbsp;mass loss&nbsp;from the star itself. The Earth-observed angular diameter of Betelgeuse is exceeded only by those of&nbsp;R Doradus&nbsp;and the Sun.<\/p>\n\n\n\n<p class=\"has-medium-font-size\">Starting in October&nbsp;2019, Betelgeuse began to dim noticeably, and by mid-February&nbsp;2020 its brightness had dropped by a factor of approximately 3, from magnitude 0.5 to 1.7. It then returned to a more normal brightness range, reaching a peak of 0.0 visual and 0.1 V-band magnitude in April 2023.&nbsp;Infrared observations found no significant change in&nbsp;luminosity&nbsp;over the last 50&nbsp;years, suggesting that the dimming was due to a change in&nbsp;extinction&nbsp;around the star rather than a more fundamental change. A study using the&nbsp;Hubble Space Telescope&nbsp;suggests that occluding dust was created by a surface mass ejection. This cast material millions of miles from the star that then cooled to form the dust that caused the star&#8217;s dimming.<\/p>\n\n\n\n<p class=\"has-medium-font-size\">Supernova of Betelgeuse is going to be unexpectable and also exiting. let&#8217;s see what the future upholds for us. <\/p>\n","protected":false},"excerpt":{"rendered":"<p>We should know what is coming in the future!!<\/p>\n","protected":false},"author":1,"featured_media":283,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_mi_skip_tracking":false},"categories":[5],"tags":[],"_links":{"self":[{"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/posts\/279"}],"collection":[{"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/comments?post=279"}],"version-history":[{"count":3,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/posts\/279\/revisions"}],"predecessor-version":[{"id":304,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/posts\/279\/revisions\/304"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/media\/283"}],"wp:attachment":[{"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/media?parent=279"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/categories?post=279"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/tithijagad.com\/index.php\/wp-json\/wp\/v2\/tags?post=279"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}