{"id":236345,"date":"2024-06-25T21:01:21","date_gmt":"2024-06-25T21:01:21","guid":{"rendered":"https:\/\/michigandigitalnews.com\/index.php\/2024\/06\/25\/how-big-is-the-universe-the-shape-of-space-time-could-tell-us\/"},"modified":"2025-06-25T17:16:11","modified_gmt":"2025-06-25T17:16:11","slug":"how-big-is-the-universe-the-shape-of-space-time-could-tell-us","status":"publish","type":"post","link":"https:\/\/michigandigitalnews.com\/index.php\/2024\/06\/25\/how-big-is-the-universe-the-shape-of-space-time-could-tell-us\/","title":{"rendered":"How big is the universe? The shape of space-time could tell us"},"content":{"rendered":"<p> [ad_1]<br \/>\n<\/p>\n<div id=\"\">\n<figure class=\"ArticleImage\">\n<div class=\"Image__Wrapper\"><img fetchpriority=\"high\" decoding=\"async\" class=\"Image\" width=\"1350\" height=\"900\" alt=\"https:\/\/www.esa.int\/ESA_Multimedia\/Images\/2022\/07\/Stephan_s_Quintet_NIRCam_and_MIRI_imaging Stephan?s Quintet ? NIRCam and MIRI imaging An enormous mosaic of Stephan?s Quintet is the largest image to date from the NASA\/ESA\/CSA James Webb Space Telescope, covering about one-fifth of the Moon?s diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The visual grouping of five galaxies was captured by Webb?s Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). With its powerful, infrared vision and extremely high spatial resolution, Webb shows never-before-seen details in this galaxy group. Sparkling clusters of millions of young stars and starburst regions of fresh star birth grace the image. Sweeping tails of gas, dust and stars are being pulled from several of the galaxies due to gravitational interactions. Most dramatically, Webb?s MIRI instrument captures huge shock waves as one of the galaxies, NGC 7318B, smashes through the cluster. These regions surrounding the central pair of galaxies are shown in the colours red and gold. This composite NIRCam-MIRI image uses two of the three MIRI filters to best show and differentiate the hot dust and structure within the galaxy. MIRI sees a distinct difference in colour between the dust in the galaxies versus the shock waves between the interacting galaxies. The image processing specialists at the Space Telescope Science Institute in Baltimore opted to highlight that difference by giving MIRI data the distinct yellow and orange colours, in contrast to the blue and white colours assigned to stars at NIRCam?s wavelengths.\" src=\"https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg\" sizes=\"(min-width: 1288px) 837px, (min-width: 1024px) calc(57.5vw + 55px), (min-width: 415px) calc(100vw - 40px), calc(70vw + 74px)\" srcset=\"https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=300 300w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=400 400w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=500 500w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=600 600w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=700 700w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=800 800w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=837 837w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=900 900w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1003 1003w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1100 1100w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1200 1200w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1300 1300w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1400 1400w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1500 1500w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1600 1600w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1674 1674w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1700 1700w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1800 1800w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=1900 1900w, https:\/\/images.newscientist.com\/wp-content\/uploads\/2024\/06\/24135020\/SEI_210189894.jpg?width=2006 2006w\" loading=\"eager\" fetchpriority=\"high\" data-image-context=\"Article\" data-image-id=\"2436718\" data-caption=\"\" data-credit=\"NASA, ESA, CSA, and STScI\"\/><\/div><figcaption class=\"ArticleImageCaption\">\n<div class=\"ArticleImageCaption__CaptionWrapper\">\n<p class=\"ArticleImageCaption__Credit ArticleImageCaption__Credit--NoTitle\">NASA, ESA, CSA, and STScI<\/p>\n<\/div>\n<\/figcaption><\/figure>\n<\/p>\n<p>In a sense, we are at the centre of the universe \u2013 but only because we can see the same distance in every direction, giving us the perfectly spherical observable universe. The speed limit of light combined with the inexorable expansion of the cosmos means that we can see about 46 billion light years in every direction. What lies beyond this horizon? That is a mystery we may never solve.<\/p>\n<p>But there are clues. Two competing effects govern the overall size of the universe: <a href=\"https:\/\/www.newscientist.com\/definition\/gravity\/\">gravity<\/a> and <a href=\"https:\/\/www.newscientist.com\/article\/2425253-there-are-hints-that-dark-energy-may-be-getting-weaker\/\">dark energy<\/a>. All matter has mass, which causes gravitational forces that pull everything towards everything else. To their surprise, however, cosmologists in the early 20th century found that distant galaxies seem to be hurtling away from us. The mysterious force causing this strange expansion of space was dubbed dark energy, and its nature remains elusive to this day.<\/p>\n<p>\u201cUp until the discovery of dark energy and the acceleration of expansion, the universe was simpler,\u201d says cosmologist <a href=\"https:\/\/astro.uchicago.edu\/people\/wendy-l-freedman.php\">Wendy Freedman<\/a> at the University of Chicago. Without dark energy, the universe would be much smaller and its size easier to predict.<\/p>\n<p>Even with dark energy, the universe may only be slightly larger than what is observable. In March, <a href=\"https:\/\/www.linkedin.com\/in\/jean-luc-lehners-a945b5132\">Jean-Luc Lehners<\/a>, then at the Max Planck Institute for Gravitational Physics in Germany, and <a href=\"https:\/\/uwaterloo.ca\/astrophysics-centre\/contacts\/jerome-quintin\">Jerome Quintin<\/a> at the University of Waterloo in Canada <a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0370269324000467?via%3Dihub\">published a model<\/a> that suggested the period of rapid expansion right after the big bang, called inflation, could have been even shorter than we thought. This would leave the universe smaller\u2026<\/p>\n<\/p><\/div>\n<p>[ad_2]<br \/>\n<br \/><a href=\"https:\/\/www.newscientist.com\/article\/mg26234970-500-how-big-is-the-universe-the-shape-of-space-time-could-tell-us\/?utm_campaign=RSS%7CNSNS&#038;utm_source=NSNS&#038;utm_medium=RSS&#038;utm_content=home\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>[ad_1] NASA, ESA, CSA, and STScI In a sense, we are at the centre of the universe \u2013 but only because we can see the<\/p>\n","protected":false},"author":1,"featured_media":236346,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[177],"tags":[],"_links":{"self":[{"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/posts\/236345"}],"collection":[{"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/comments?post=236345"}],"version-history":[{"count":0,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/posts\/236345\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/media\/236346"}],"wp:attachment":[{"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/media?parent=236345"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/categories?post=236345"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/michigandigitalnews.com\/index.php\/wp-json\/wp\/v2\/tags?post=236345"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}