{"id":1047119,"date":"2026-09-06T15:25:25","date_gmt":"2026-09-06T15:25:25","guid":{"rendered":"https:\/\/www.europesays.com\/us\/1047119\/"},"modified":"2026-09-06T15:25:25","modified_gmt":"2026-09-06T15:25:25","slug":"astronomers-confirm-einsteins-gravity-by-viewing-light-from-behind-a-supermassive-black-hole","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/us\/1047119\/","title":{"rendered":"Astronomers confirm Einstein\u2019s gravity by viewing light from behind a supermassive black hole"},"content":{"rendered":"<ul class=\"mb-4\">\n<li class=\"ml-4 safari:ml-6 list-disc\">\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Astronomers detected delayed X-ray flashes consistent with light reflected from the far side of an accretion disk and bent around a supermassive black hole by its intense gravity.<\/p>\n<\/li>\n<li class=\"ml-4 safari:ml-6 list-disc\">\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The photons did not escape from inside the black hole. They originated outside the event horizon, where warped spacetime redirected normally hidden light into Earth&#8217;s line of sight.<\/p>\n<\/li>\n<li class=\"ml-4 safari:ml-6 list-disc\">\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The observation provided direct evidence for a long-predicted general-relativistic effect and gave researchers a new way to probe the mysterious X-ray corona surrounding actively feeding black holes.<\/p>\n<\/li>\n<\/ul>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">A black hole nearly 800 million light-years away briefly revealed something that should ordinarily have been hidden from view.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">While studying powerful X-ray flares from the center of the galaxy I Zwicky 1, astronomers detected smaller flashes arriving later and at different X-ray energies. Their timing and energy shifts matched a remarkable prediction: the photons had reflected from the far side of the black hole&#8217;s accretion disk before the black hole&#8217;s gravity bent their paths around it and toward Earth.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The discovery, published in <a data-ylk=\"slk:Nature;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.nature.com\/articles\/s41586-021-03667-0\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Nature<\/a>, provided direct observational evidence for X-rays re-emerging from behind a supermassive black hole. <a data-ylk=\"slk:Stanford University;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.stanford.edu\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Stanford University<\/a> and <a data-ylk=\"slk:SLAC National Accelerator Laboratory;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www6.slac.stanford.edu\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">SLAC National Accelerator Laboratory<\/a> researchers led the work using observations from ESA&#8217;s XMM-Newton and NASA&#8217;s NuSTAR observatories.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">&#8220;Any light that goes into that black hole doesn&#8217;t come out, so we shouldn&#8217;t be able to see anything that&#8217;s behind the black hole,&#8221; said Stanford astrophysicist Dan Wilkins.<\/p>\n<p><img alt=\"Light echoes from behind a black hole. (CREDIT: ESA)\" loading=\"lazy\" width=\"960\" height=\"540\" decoding=\"async\" data-nimg=\"1\" class=\"rounded-lg\" style=\"color:transparent\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2026\/09\/https:\/\/media.zenfs.com\/en\/the_brighter_side_of_news_articles_781\/5160319e1a8eafb4725e546fc090ccef.p.jpeg\"\/><\/p>\n<p>Light echoes from behind a black hole. (CREDIT: ESA)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The explanation lies in a distinction that sounds subtle but is crucial. The detected light did not escape from inside the event horizon. Instead, it traveled through the severely <a data-ylk=\"slk:curved spacetime;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/physicists-rewrite-einsteins-equations-to-define-spacetime-evolution\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">curved spacetime<\/a> surrounding the black hole, where gravity bent photons from otherwise hidden portions of the disk into the astronomers&#8217; line of sight.<\/p>\n<p>Two flares exposed the black hole&#8217;s hidden side<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">I Zwicky 1, commonly called I Zw 1, contains an actively feeding supermassive black hole surrounded by a brilliant accretion disk.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">NuSTAR watched the object continuously for 5.3 days in January 2020, while XMM-Newton observed it during two long intervals. About 150,000 seconds into the campaign, the X-ray emission erupted in two flares lasting roughly 10,000 seconds each. At their peaks, the X-ray count rate reached about 2.5 times its earlier average.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Those large flares were interesting but not unprecedented. What followed caught the researchers&#8217; attention.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">As each flare declined, small peaks appeared at different times in separate X-ray energy bands. The pattern appeared first among blueshifted iron-line photons and later among <a data-ylk=\"slk:redshifted photons;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/upenn-physicists-make-light-work-of-computing\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">redshifted photons<\/a>. Statistical testing found less than a 0.01% probability that the pattern resulted from random Poisson or unrelated red-noise variations.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The sequence matched theoretical calculations for an X-ray flare echoing across an accretion disk.<\/p>\n<p><img alt=\"Delayed X-ray flashes showed light from a hidden accretion disk bending around a black hole, revealing relativity in action. (CREDIT: ESA)\" loading=\"lazy\" width=\"945\" height=\"945\" decoding=\"async\" data-nimg=\"1\" class=\"rounded-lg\" style=\"color:transparent\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2026\/09\/https:\/\/media.zenfs.com\/en\/the_brighter_side_of_news_articles_781\/5670c91fd9313ff2175b883ef687fc3a.g.gif\"\/><\/p>\n<p>Delayed X-ray flashes showed light from a hidden accretion disk bending around a black hole, revealing relativity in action. (CREDIT: ESA)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">&#8220;I&#8217;d already seen them in the theory I&#8217;ve been developing, so once I saw them in the telescope observations, I could figure out the connection,&#8221; Wilkins said.<\/p>\n<p>A black hole can bend light around itself<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Albert Einstein&#8217;s general theory of relativity describes gravity not simply as a force but as a curvature of spacetime produced by mass and energy.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Near a black hole, that curvature becomes extreme. Light normally travels along the straightest available path through spacetime, but when spacetime itself is curved, those paths can appear dramatically bent to a distant observer.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">That effect allowed X-rays from the hidden far side of I Zw 1&#8217;s accretion disk to travel around the black hole rather than disappear behind it. The <a data-ylk=\"slk:black hole&#039;s gravitational field;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/the-physics-of-no-return-what-actually-happens-if-you-get-pulled-into-a-black-hole\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">black hole&#8217;s gravitational field<\/a> also magnified some of the radiation through gravitational lensing.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Models had predicted such a signature decades earlier. A 1999 study of iron-line reverberation calculated how X-rays reflected from different regions of an accretion disk should arrive at different times and energies in the curved spacetime around a spinning black hole.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The I Zw 1 observations finally exposed that behavior in actual flare data.<\/p>\n<p><img alt=\"Schematic of the X-ray reverberation model. (CREDIT: Dan Wilkins et al, Nature)\" loading=\"lazy\" width=\"798\" height=\"520\" decoding=\"async\" data-nimg=\"1\" class=\"rounded-lg\" style=\"color:transparent\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2026\/09\/https:\/\/media.zenfs.com\/en\/the_brighter_side_of_news_articles_781\/66d850f5f503779d7fad4f8bf675b465.jpeg\"\/><\/p>\n<p>Schematic of the X-ray reverberation model. (CREDIT: Dan Wilkins et al, Nature)<\/p>\n<p>The X-ray &#8216;colors&#8217; mapped different parts of the disk<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The different energies of the delayed flashes were just as important as their timing.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Material in the accretion disk races around the black hole at tremendous speeds. X-rays from the approaching side become blueshifted toward higher energies, while light from the receding side shifts lower. Gravity also stretches photons to lower energies, producing a gravitational redshift that becomes stronger closer to the black hole.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">These effects distort the normally narrow iron K fluorescence line emitted around 6.4 kiloelectronvolts. By following how that line changed with time, astronomers could identify which regions of the disk were responding to a flare.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">During the events, <a data-ylk=\"slk:blueshifted emission;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/galaxy-killing-wind-may-explain-why-giant-galaxies-died-so-early\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">blueshifted emission<\/a> arrived first. More redshifted photons followed later, matching light reflected from the rear portion of the disk and forced onto longer curved routes around the black hole.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The team also measured an average iron K reverberation delay of 746 plus or minus 157 seconds.<\/p>\n<p>The flares also revealed the black hole&#8217;s corona<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The researchers had originally set out to understand something else: the black hole&#8217;s corona.<\/p>\n<p><img alt=\"Features of the reverberation response function detected during the X-ray flares. (CREDIT: Dan Wilkins et al, Nature)\" loading=\"lazy\" width=\"960\" height=\"410\" decoding=\"async\" data-nimg=\"1\" class=\"rounded-lg\" style=\"color:transparent\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2026\/09\/https:\/\/media.zenfs.com\/en\/the_brighter_side_of_news_articles_781\/5b90e03a75e7b239c83851282bba5aed.jpeg\"\/><\/p>\n<p>Features of the reverberation response function detected during the X-ray flares. (CREDIT: Dan Wilkins et al, Nature)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">A corona is an extremely hot region of energetic particles close to a feeding black hole. Although its detailed structure remains uncertain, magnetic fields rising from the <a data-ylk=\"slk:accretion disk;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/strange-red-object-from-the-early-universe-could-be-the-first-black-hole-star\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">accretion disk<\/a> are thought to accelerate particles and produce powerful X-rays.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Earlier observations of I Zw 1 had suggested that its corona contains a broader component spread across the inner disk and a compact, vertically extended core responsible for faster changes in brightness.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">When the corona flares, some X-rays travel directly toward Earth. Others strike the accretion disk first and are reflected, creating delayed echoes. The time between direct and reflected radiation provides a way to measure structures only a few gravitational radii from the event horizon.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The 2020 observations showed that the brightest flares could illuminate the disk sharply enough for astronomers to resolve the unusual far-side echoes.<\/p>\n<p>General relativity became visible in the data<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The observations do not mean scientists literally photographed the back of a <a data-ylk=\"slk:black hole;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/jwst-finds-three-feeding-black-holes-packed-into-one-early-galaxy\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">black hole<\/a>. They detected a time-dependent X-ray signature that matched relativistic ray-tracing predictions for radiation coming from the disk&#8217;s hidden side.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Alternative explanations involving changing absorption, disk ionization or ordinary continuum fluctuations had difficulty reproducing the shifting iron-line pattern.<\/p>\n<p><img alt=\"The soft and hard X-ray spectra of I Zw 1 obtained by XMM-Newton and NuSTAR during the 2020 observations. (CREDIT: Dan Wilkins et al, Nature)\" loading=\"lazy\" width=\"960\" height=\"401\" decoding=\"async\" data-nimg=\"1\" class=\"rounded-lg\" style=\"color:transparent\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2026\/09\/https:\/\/media.zenfs.com\/en\/the_brighter_side_of_news_articles_781\/c7530f21d4ed0f6968cba18597ab1630.jpeg\"\/><\/p>\n<p>The soft and hard X-ray spectra of I Zw 1 obtained by XMM-Newton and NuSTAR during the 2020 observations. (CREDIT: Dan Wilkins et al, Nature)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The result offered an unusually direct demonstration of how strongly a black hole can reshape the paths of nearby photons.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">&#8220;Fifty years ago, when astrophysicists started speculating about how the magnetic field might behave close to a black hole, they had no idea that one day we might have the techniques to observe this directly and see <a data-ylk=\"slk:Einstein&#039;s general theory of relativity;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/groundbreaking-study-reaffirms-einstein-s-general-theory-of-relativity\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Einstein&#8217;s general theory of relativity<\/a> in action,&#8221; said study co-author Roger Blandford.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Black holes remain dark by definition. But the light surrounding them, bent, delayed and shifted by extreme gravity, can expose structures that would otherwise remain invisible.<\/p>\n<p>Dig deeper into black hole X-ray echoes<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">These resources explore the X-ray reverberation, accretion-disk reflection and coronal physics behind observations of light bent around black holes.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><a data-ylk=\"slk:X-ray reverberation around accreting black holes;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/doi.org\/10.1007\/s00159-014-0072-0\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">X-ray reverberation around accreting black holes<\/a>: Reviews how time delays between direct coronal X-rays and disk-reflected radiation can map regions only a few gravitational radii from black holes. (The Astronomy and Astrophysics Review, 2014)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><a data-ylk=\"slk:X-Ray Iron Line Reverberation from Black Hole Accretion Disks;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/doi.org\/10.1086\/306913\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">X-Ray Iron Line Reverberation from Black Hole Accretion Disks<\/a>: Developed early theoretical predictions for the changing time and energy signatures of iron-line echoes around spinning black holes. (The Astrophysical Journal, 1999)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><a data-ylk=\"slk:Revealing structure and evolution within the corona of the Seyfert galaxy I Zw 1;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/doi.org\/10.1093\/mnras\/stx1814\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Revealing structure and evolution within the corona of the Seyfert galaxy I Zw 1<\/a>: Earlier observations of I Zw 1 revealed evidence for multiple coronal components and established the system as a target for X-ray reverberation studies. (Monthly Notices of the Royal Astronomical Society, 2017)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><a data-ylk=\"slk:Understanding X-ray reflection emissivity profiles in AGN: locating the X-ray source;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/doi.org\/10.1111\/j.1365-2966.2012.21308.x\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Understanding X-ray reflection emissivity profiles in AGN: locating the X-ray source<\/a>: Uses general-relativistic ray tracing to show how reflected X-rays can constrain the position and geometry of a black hole&#8217;s corona. (Monthly Notices of the Royal Astronomical Society, 2012)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><a data-ylk=\"slk:The origin of the lag spectra observed in AGN: Reverberation and the propagation of X-ray source fluctuations;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/doi.org\/10.1093\/mnras\/sts591\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">The origin of the lag spectra observed in AGN: Reverberation and the propagation of X-ray source fluctuations<\/a>: Models how gravitational delays, disk reflection and changes moving through a corona shape the observed timing of X-rays from active galaxies. (Monthly Notices of the Royal Astronomical Society, 2013)<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">Research findings are available online in the journal <a data-ylk=\"slk:Nature;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.nature.com\/articles\/s41586-021-03667-0\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Nature<\/a>.<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\">The original story &#8220;<a data-ylk=\"slk:Astronomers confirm Einstein&#039;s gravity by viewing light from behind a supermassive black hole;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"https:\/\/www.thebrighterside.news\/post\/astronomers-confirm-einsteins-gravity-by-viewing-light-from-behind-a-supermassive-black-hole\/\" rel=\"noopener noreferrer nofollow\" target=\"_blank\">Astronomers confirm Einstein&#8217;s gravity by viewing light from behind a supermassive black hole<\/a>&#8221; is published in The Brighter Side of News.<\/p>\n<p>Related Stories<\/p>\n<p class=\"mb-4 text-lg md:leading-8 break-words\"><strong>Like these kind of feel good stories? Get <\/strong><a data-ylk=\"slk:The Brighter Side of News&#039; newsletter;elm:context_link;itc:0;sec:content-canvas;\" data-yga=\"{&quot;yLinkElement&quot;:&quot;link&quot;,&quot;yLinkElementType&quot;:&quot;article_link&quot;}\" href=\"http:\/\/www.thebrighterside.news\/subscribe\" rel=\"noopener noreferrer nofollow\" target=\"_blank\"><strong>The Brighter Side of News&#8217; newsletter<\/strong><\/a><strong>.<\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"Astronomers detected delayed X-ray flashes consistent with light reflected from the far side of an accretion disk and&hellip;\n","protected":false},"author":3,"featured_media":1047120,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_share_on_mastodon":"0"},"categories":[25],"tags":[419161,419162,890,419163,492,159,63443,3972,67,132,68,419164,205022],"class_list":["post-1047119","post","type-post","status-publish","format-standard","has-post-thumbnail","category-physics","tag-dan-wilkins","tag-dan-wilkins-et-al","tag-esa","tag-nustar","tag-physics","tag-science","tag-stanford","tag-stanford-university","tag-united-states","tag-unitedstates","tag-us","tag-wilkins","tag-xmm-newton"],"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@us\/117224799157244004","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/1047119","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/comments?post=1047119"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/1047119\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media\/1047120"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media?parent=1047119"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/categories?post=1047119"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/tags?post=1047119"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}