Thousands of years ago, a star in our galaxy violently exploded and created a glowing supernova remnant called Cassiopeia A that has intrigued scientists for decades. <\/p>\n
Now, a new image captured by the James Webb Space Telescope has revealed the closest and most detailed look inside the exploded star, according to astronomers. Analyzing the image could help researchers better understand the processes that fuel these massive incendiary events. <\/p>\n
The space observatory has also allowed astronomers to glimpse mysterious features that haven\u2019t appeared in images taken of the remnant using telescopes like Hubble, Chandra or Spitzer or Webb\u2019s other instruments. <\/p>\n
The new image was shared on Monday by first lady Dr. Jill Biden as she debuted the first-ever digital White House Advent Calendar, which includes Webb\u2019s new perspective of Cassiopeia A that seems to shine like a Christmas ornament. <\/p>\n
\u201cWe\u2019ve never had this kind of look at an exploded star before,\u201d said astronomer Dan Milisavljevic, assistant professor of physics and astronomy at Purdue University, in a statement. \u201cSupernovae are primary drivers of cosmological evolution. The energies, their chemical abundances \u2014 there is so much that depends on our understanding of supernovae. This is the closest look we\u2019ve had at a supernova in our galaxy.\u201d <\/p>\n
Swirls of gas and dust are all that remain of the star that went supernova 10,000 years ago. Cassiopeia A is located 11,000 light-years away in the Cassiopeia constellation. A light-year, equivalent to 5.88 trillion miles (9.46 trillion kilometers), is how far a beam of light travels in one year. <\/p>\n
The light from Cassiopeia A first reached Earth about 340 years ago. As the youngest known supernova remnant in our galaxy, the celestial object has been studied by a multitude of ground- and space-based telescopes. The remnant stretches for about 10 light-years across, or 60 trillion miles (96.6 trillion kilometers). <\/p>\n
Insights from Cas A, as the remnant is also known, allow scientists to learn more about the life cycle of stars. <\/p>\n
Astronomers used Webb\u2019s Near-Infrared Camera, called NIRCam, to see the supernova remnant at different wavelengths of light than those used in previous observations. The image shows unprecedented details of the interaction between the expanding shell of material created by the supernova as it collides with the gas released by the star prior to the explosion. <\/p>\n
But the image looks completely different from one taken by Webb in April using the telescope\u2019s Mid-Infrared Instrument, or MIRI. In each image, certain features stand out that are invisible in the other. <\/p>\n
Webb observes the universe in wavelengths of infrared light, which is invisible to the human eye. As scientists process Webb\u2019s data, the light captured by the telescope is translated into a spectrum of colors visible to humans. <\/p>\n
The new NIRCam image is dominated by orange and light pink flashes of color within the supernova remnant\u2019s inner shell. The colors correspond to gaseous knots of elements shed by the star, including oxygen, argon, neon and sulfur. Mixed within the gas are dust and molecules. Eventually, all of these ingredients will combine to form new stars and planets. <\/p>\n
Studying the remnant allows scientists to reconstruct what happened during the supernova. <\/p>\n
\u201cWith NIRCam\u2019s resolution, we can now see how the dying star absolutely shattered when it exploded, leaving filaments akin to tiny shards of glass behind,\u201d Milisavljevic said. \u201cIt\u2019s really unbelievable after all these years studying Cas A to now resolve those details, which are providing us with transformational insight into how this star exploded.\u201d <\/p>\n
When comparing the NIRCam image with the MIRI image taken in April, the new perspective seems less colorful. The bright swirls of orange and red from the April image look smokier through NIRCam\u2019s eyes, showing where the shock wave from the supernova crashed into surrounding material. <\/p>\n
The white light in the NIRCam image is due to synchrotron radiation, which is created when charged particles accelerate and travel around magnetic field lines. <\/p>\n
A key feature missing from the NIRCam view is the \u201cGreen Monster\u201d from the MIRI image, or a circle of green light in the remnant\u2019s center, that has puzzled and challenged astronomers. <\/p>\n
But new details can be seen in the near-infrared image that point to circular holes wreathed in white and purple, designating charged particles of debris that shape the gas shed by the star before it exploded. <\/p>\n
Another new feature in the NIRCam image is a blob nicknamed Baby Cas A that can be seen in the bottom right corner, which looks like an offspring of the larger supernova remnant and is located 170 light-years behind Cassiopeia A. <\/p>\n
Baby Cas A is actually a feature called a light echo, where the supernova\u2019s light interacted with dust and caused it to heat up. The dust continues to glow as it cools over time. <\/p>\n
\u201cIt\u2019s staggering,\u201d said Milisavljevic, who led a project team that contributed to the new image. \u201cSome features have popped up that are completely new \u2014 that will change the way we think about stellar life cycles.\u201d <\/p>\n\n
Thousands of years ago, a star in our galaxy violently exploded and created a glowing supernova remnant called Cassiopeia A that has intrigued scientists for decades. Now, a new image captured by the James Webb Space Telescope has revealed the closest and most detailed look inside the exploded star, according to astronomers. Analyzing the image <\/p>\n","protected":false},"author":0,"featured_media":12823,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[],"class_list":{"0":"post-12822","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-world"},"_links":{"self":[{"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/posts\/12822","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"replies":[{"embeddable":true,"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/comments?post=12822"}],"version-history":[{"count":0,"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/posts\/12822\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/media\/12823"}],"wp:attachment":[{"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/media?parent=12822"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/categories?post=12822"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/shareperformanceinsight.com\/index.php\/wp-json\/wp\/v2\/tags?post=12822"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}