{"title":"James Webb Collection","description":"\u003cp\u003eThe infrared universe as seen by NASA's James Webb Space Telescope, as museum-quality framed prints from Skylit Studio.\u003c\/p\u003e","products":[{"product_id":"pillars-of-creation-skylit-studio","title":"Pillars Of Creation | JAMES WEBB TELESCOPE | Skylit Studio","description":"\u003cstyle\u003e\n    .container-skylit {\n        max-width: 900px;\n        margin: 0 auto;\n        padding: 40px 20px;\n    }\n\n    .header-skylit {\n        text-align: center;\n        margin-bottom: 40px;\n        border-bottom: 2px solid #FFB503;\n        padding-bottom: 20px;\n    }\n\n    .logo-skylit {\n        font-size: 2.5em;\n        font-weight: 300;\n        background: linear-gradient(45deg, #0D0D1F, #FFB503, #FFDA73);\n        -webkit-background-clip: text;\n        -webkit-text-fill-color: transparent;\n        margin-bottom: 10px;\n    }\n\n    .subtitle-skylit {\n        color: #e5d9c5;\n        font-size: 1.1em;\n        font-weight: 300;\n    }\n\n    .main-title-skylit {\n            font-size: 2.2em;\n    color: #ffb503;\n    margin-bottom: 30px;\n    text-align: center;\n    text-shadow: 2px 2px 2px #be2119;\n    }\n\n    .content-skylit {\n        background: rgba(13, 13, 31, 0.55);\n        backdrop-filter: blur(12px);\n        border-radius: 16px;\n        padding: 38px;\n        box-shadow: 0 8px 34px rgba(0, 0, 0, 0.45);\n        border: 1px solid rgba(255, 255, 255, 0.06);\n    }\n\n    .paragraph-skylit {\n        margin-bottom: 22px;\n        font-size: 1.08em;\n        line-height: 1.62;\n        text-align: justify;\n        color: #EEE5D9;\n    }\n\n    .highlight-skylit {\n        color: #FFDA73;\n        font-weight: 600;\n        background: rgba(255, 181, 3, 0.18);\n        padding: 2px 6px;\n        border-radius: 4px;\n    }\n\n    .technical-term-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-style: italic;\n    }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003e\u003cspan\u003eThe Pillars of Creation\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe iconic \u003cspan class=\"highlight-skylit\"\u003ePillars of Creation\u003c\/span\u003e emerge in a breathtaking kaleidoscope of color through NASA's James Webb Space Telescope's near-infrared vision. These towering structures resemble ancient arches and spires rising from a celestial desert, yet they are composed of semi-transparent gas and dust in constant flux—a cosmic nursery where stellar birth unfolds before our eyes.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe true stars of this \u003cspan class=\"technical-term-skylit\"\u003eNear-Infrared Camera (NIRCam)\u003c\/span\u003e image are the newly formed celestial bodies themselves—brilliant red orbs adorned with characteristic eight-pointed diffraction spikes. When dense knots of material within the pillars accumulate sufficient mass, they collapse under their own gravitational pull, gradually heating up until they ignite in brilliant stellar fire.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAlong the pillar edges, undulating lines reminiscent of flowing lava mark the dramatic ejections from stars still in their formative stages. These young stellar objects periodically launch \u003cspan class=\"highlight-skylit\"\u003esupersonic jets\u003c\/span\u003e that collide with surrounding material clouds, creating bow shocks that ripple through space like the wake of a cosmic vessel. These stellar infants, merely hundreds of thousands of years old, will continue their formation process across millions of years.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWhile Webb's near-infrared capabilities might seem to pierce through cosmic veils to reveal distant galaxies, the \u003cspan class=\"technical-term-skylit\"\u003einterstellar medium\u003c\/span\u003e acts as a translucent curtain, blocking our view of the deeper universe. This gaseous veil, illuminated by the collective radiance of stars that have emerged from the pillars, creates a luminous barrier—much like standing in a well-lit room and looking through a window where interior light reflects on the glass, obscuring the outside world while highlighting the activity within.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's revolutionary perspective on the Pillars of Creation empowers researchers to refine their understanding of \u003cspan class=\"highlight-skylit\"\u003estellar formation\u003c\/span\u003e. By precisely cataloging star populations and measuring gas and dust quantities throughout the region, scientists are building a comprehensive picture of how stars emerge and escape from these cosmic clouds over millions of years.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe Pillars of Creation represent just a small fraction of the vast \u003cspan class=\"technical-term-skylit\"\u003eEagle Nebula\u003c\/span\u003e, located approximately \u003cspan class=\"highlight-skylit\"\u003e6,500 light-years\u003c\/span\u003e from Earth—a testament to the incredible scale and beauty of our universe.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb's NIRCam was developed through collaboration between the University of Arizona and Lockheed Martin's Advanced Technology Center.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Joseph DePasquale (STScI), Anton M. Koekemoer (STScI), Alyssa Pagan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":55250562384249,"sku":"DSP-POC-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40cm","offer_id":55250562417017,"sku":"DSP-POC-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 cm","offer_id":55250562449785,"sku":"DSP-POC-PRT-40X50-NOFRM","price":29.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 50 x 70 cm","offer_id":55250562482553,"sku":"DSP-POC-PRT-50X70-NOFRM","price":37.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 60 x 80 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{\n        color: #e5d9c5;\n        font-size: 1.1em;\n        font-weight: 300;\n    }\n\n    .main-title-skylit {\n            font-size: 2.2em;\n    color: #ffb503;\n    margin-bottom: 30px;\n    text-align: center;\n    text-shadow: 2px 2px 2px #be2119;\n    }\n\n    .content-skylit {\n        background: rgba(13, 13, 31, 0.55);\n        backdrop-filter: blur(12px);\n        border-radius: 16px;\n        padding: 38px;\n        box-shadow: 0 8px 34px rgba(0, 0, 0, 0.45);\n        border: 1px solid rgba(255, 255, 255, 0.06);\n    }\n\n    .paragraph-skylit {\n        margin-bottom: 22px;\n        font-size: 1.08em;\n        line-height: 1.62;\n        text-align: justify;\n        color: #EEE5D9;\n    }\n\n    .highlight-skylit {\n        color: #FFDA73;\n        font-weight: 600;\n        background: rgba(255, 181, 3, 0.18);\n        padding: 2px 6px;\n        border-radius: 4px;\n    }\n\n    .technical-term-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-style: italic;\n    }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003e\u003cspan\u003eThe Aftermath of Planetary Engulfment\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eNASA's James Webb Space Telescope has captured the extraordinary aftermath of what scientists believe to be the \u003cspan class=\"highlight-skylit\"\u003efirst directly observed planetary engulfment event\u003c\/span\u003e in astronomical history. This cosmic catastrophe reveals a complex system where a star has completely consumed its planetary companion, leaving behind a magnificent yet haunting celestial signature that tells the tale of this dramatic stellar meal.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIn the wake of this planetary destruction, Webb's unprecedented infrared vision reveals a \u003cspan class=\"technical-term-skylit\"\u003ehot accretion disk\u003c\/span\u003e of molecular gas spinning closely around the star—the superheated remains of the devoured world still clinging to its former host. This luminous disk, glowing with the thermal energy of the recent cosmic collision, serves as a blazing memorial to the planet that once called this star home.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eSurrounding this inner inferno, an enormous \u003cspan class=\"highlight-skylit\"\u003eexpanding cloud of cooler dust\u003c\/span\u003e envelops the entire scene like a cosmic shroud. This ethereal veil represents the final transformation of the engulfed planet—heavy elements that were once part of a Jupiter-sized world, now condensed into microscopic particles drifting through the void. The dust cloud continues to expand and cool, preserving the chemical fingerprints of the lost planet for millions of years to come.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's detailed observations, captured through its \u003cspan class=\"technical-term-skylit\"\u003eMIRI (Mid-Infrared Instrument)\u003c\/span\u003e and \u003cspan class=\"technical-term-skylit\"\u003eNIRSpec (Near-Infrared Spectrograph)\u003c\/span\u003e, have revolutionized our understanding of this engulfment process. Contrary to previous theories, the star did not dramatically swell to swallow its companion. Instead, the planet's orbit underwent a slow, inexorable decay over millions of years—a gradual death spiral that ended in complete assimilation.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe planetary victim in this cosmic drama was a \u003cspan class=\"highlight-skylit\"\u003eJupiter-sized giant\u003c\/span\u003e that orbited its star at a distance even closer than Mercury's relationship with our Sun. This extreme proximity sealed the planet's fate as gravitational forces and stellar radiation gradually eroded its orbital stability. Over eons, the planet spiraled ever closer until it began grazing the star's atmosphere, smearing its material around the stellar surface before being completely consumed.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis remarkable discovery offers scientists a rare glimpse into the violent processes that can reshape planetary systems. The event demonstrates how \u003cspan class=\"technical-term-skylit\"\u003eorbital decay\u003c\/span\u003e can lead to planetary destruction, while simultaneously creating new structures around the host star. The resulting dust cloud may eventually coalesce into new celestial bodies, suggesting that even in cosmic destruction, there exists the potential for rebirth and renewal.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe timing captured by Webb represents a cosmic moment frozen in astronomical time—the period approximately \u003cspan class=\"highlight-skylit\"\u003eone year after engulfment\u003c\/span\u003e when the expelled stellar material had sufficient time to cool and condense into the observed dust formations. This unique temporal window provides invaluable data about the immediate aftermath of planetary consumption and the rapid transformation of matter from planetary to circumstellar material.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eThis groundbreaking observation represents humanity's first direct evidence of a planetary engulfment event, opening new avenues for understanding stellar-planetary interactions and the dynamic evolution of exoplanetary systems.\n\u003cdiv class=\"image-feature-skylit\"\u003e\n\u003cimg src=\"https:\/\/cdn.shopify.com\/s\/files\/1\/0710\/5278\/7987\/files\/Planetary_Engulfment_Illustration-2.webp?v=1748618985\" alt=\"Infrared composite from NASA’s James Webb Space Telescope showing the aftermath of a planetary engulfment event — dust and gas encircling a star post-consumption.\" loading=\"lazy\"\u003e\n\u003cp class=\"caption-skylit\"\u003e📷 A NASA\/ESA\/CSA Webb composite image capturing the glowing aftermath of a planetary engulfment.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eIllustration:\u003c\/span\u003e NASA Scientific Visualization Studio\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eObservations:\u003c\/span\u003e Webb MIRI \u0026amp; NIRSpec Teams\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ 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   margin-bottom: 22px;\n        font-size: 1.08em;\n        line-height: 1.62;\n        text-align: justify;\n        color: #EEE5D9;\n    }\n\n    .highlight-skylit {\n        color: #FFDA73;\n        font-weight: 600;\n        background: rgba(255, 181, 3, 0.18);\n        padding: 2px 6px;\n        border-radius: 4px;\n    }\n\n    .technical-term-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-style: italic;\n    }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003e\u003cspan\u003eHerbig-Haro 49\/50: Where Stellar Birth Meets Cosmic Beauty\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eNASA's James Webb Space Telescope has captured one of the most spectacular examples of stellar birth in action through its observations of \u003cspan class=\"highlight-skylit\"\u003eHerbig-Haro 49\/50\u003c\/span\u003e—a breathtaking cosmic phenomenon where a young star's violent outbursts create an ethereal display of reddish-orange luminescence against the star-studded void. This extraordinary image showcases the raw power and beauty of stellar formation, revealing intricate details that illuminate how stars are born and how their energetic jets sculpt the surrounding interstellar environment.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe dramatic reddish-orange formations streaming through this image represent \u003cspan class=\"technical-term-skylit\"\u003eprotostellar jets\u003c\/span\u003e—narrow streams of superheated material launched by a \u003cspan class=\"highlight-skylit\"\u003estill-forming star\u003c\/span\u003e located just beyond the lower right corner of Webb's field of view. These jets, moving at incredible velocities through space, serve as cosmic sculptors, carving through the surrounding gas and dust with the force of stellar winds that can extend across vast interstellar distances, sometimes spanning light-years from their source.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eLike the wake generated by a high-speed vessel cutting through water, the graceful arcs and flowing structures visible in this image are created when the \u003cspan class=\"highlight-skylit\"\u003efast-moving stellar jets\u003c\/span\u003e collide with ambient interstellar material. This cosmic collision compresses and superheats the surrounding gas and dust, causing it to glow brilliantly as it cools and emits light across the electromagnetic spectrum. Webb's sensitive infrared detectors particularly excel at capturing the emission from \u003cspan class=\"technical-term-skylit\"\u003emolecular hydrogen and carbon monoxide\u003c\/span\u003e, revealing the chemical signatures of this stellar nursery.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIn a remarkable cosmic coincidence, this nearby Milky Way phenomenon is perfectly aligned with a \u003cspan class=\"highlight-skylit\"\u003edistant spiral galaxy\u003c\/span\u003e that appears at the very tip of the Herbig-Haro object's outflow. This background galaxy, located millions of times farther away than the stellar jet, displays a prominent blue central bulge indicating the presence of older stellar populations. The galaxy also exhibits subtle hints of \"side lobes,\" suggesting it may be a \u003cspan class=\"technical-term-skylit\"\u003ebarred-spiral galaxy\u003c\/span\u003e with distinctive structural features extending from its central region.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe spiral galaxy's arms are punctuated with reddish clumps that mark regions of \u003cspan class=\"highlight-skylit\"\u003ewarm dust and active star formation\u003c\/span\u003e—a beautiful reminder that stellar birth is occurring not just in our local cosmic neighbourhood, but throughout the universe. These distant star-forming regions, though appearing as mere points of light, represent entire stellar nurseries comparable to the dramatic scene playing out in Herbig-Haro 49\/50, but separated from us by the vast expanse of intergalactic space.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's unprecedented \u003cspan class=\"technical-term-skylit\"\u003enear- and mid-infrared capabilities\u003c\/span\u003e through its NIRCam and MIRI instruments have revealed layers of cosmic depth previously invisible to astronomical observation. Beyond the foreground stellar jet and the aligned spiral galaxy, countless additional galaxies populate the background, their ancient light shining through the diffuse infrared glow of the nearby Herbig-Haro object. This cosmic layering effect demonstrates the telescope's extraordinary ability to simultaneously observe multiple epochs of cosmic history within a single frame.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis image represents more than just aesthetic beauty—it provides crucial scientific insights into the \u003cspan class=\"highlight-skylit\"\u003emechanisms of stellar formation\u003c\/span\u003e and the ways young stars interact with their environment. The detailed structure of the jets, the shock fronts they create, and the resulting heating and cooling processes all contribute to our understanding of how protostars evolve and how their energetic activities influence the formation of planetary systems and the chemical enrichment of interstellar space.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eHerbig-Haro objects are named after astronomers George Herbig and Guillermo Haro, who first studied these remarkable phenomena in the 1950s. Webb's observations represent the most detailed view ever captured of such stellar outflows.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstruments:\u003c\/span\u003e Webb NIRCam \u0026amp; MIRI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e STScI Science Team\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed 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    font-size: 1.08em;\n        line-height: 1.62;\n        text-align: justify;\n        color: #EEE5D9;\n    }\n\n    .highlight-skylit {\n        color: #FFDA73;\n        font-weight: 600;\n        background: rgba(255, 181, 3, 0.18);\n        padding: 2px 6px;\n        border-radius: 4px;\n    }\n\n    .technical-term-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-style: italic;\n    }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    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Birth\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIn the constellation Serpens, approximately \u003cspan class=\"highlight-skylit\"\u003e650 light-years from Earth\u003c\/span\u003e, lies one of the most dramatic examples of stellar formation captured by modern astronomy. \u003cspan class=\"technical-term-skylit\"\u003eLynds 483 (L483)\u003c\/span\u003e presents itself as a striking hourglass-shaped nebula where two actively forming protostars are orchestrating a spectacular cosmic light show through their violent outbursts of gas and dust. This remarkable stellar nursery showcases the raw power of stellar birth in unprecedented detail.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eHidden within a single pixel at the center of this cosmic hourglass are \u003cspan class=\"highlight-skylit\"\u003etwo young protostars\u003c\/span\u003e that have been blasting out collimated energetic jets of material for tens of thousands of years. These stellar infants, embedded in an opaque horizontal disk of cold gas and dust, remain invisible to direct observation yet reveal their presence through the magnificent bipolar outflows that extend across the surrounding space like cosmic searchlights piercing the darkness.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's revolutionary \u003cspan class=\"technical-term-skylit\"\u003eNIRCam (Near-Infrared Camera)\u003c\/span\u003e has revealed the violence of star formation in dramatic detail, capturing shimmering ejections of gas and dust that gleam in brilliant orange, blue, and purple hues. The telescope's infrared vision shows how \u003cspan class=\"highlight-skylit\"\u003etwisting shock fronts\u003c\/span\u003e expand and collide with slower, denser material, creating asymmetrical lines and structures that appear to run into one another in a complex cosmic dance.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe intricate patterns visible throughout L483 tell the story of episodic stellar outbursts spanning millennia. \u003cspan class=\"highlight-skylit\"\u003eRecent ejections colliding with older ones\u003c\/span\u003e cause the material to crumple and twirl based on the varying densities of what is colliding. This cosmic archaeology preserved in gas and dust allows astronomers to reconstruct the evolutionary history of these young stars and understand the mechanisms driving their formation.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eBeyond its visual spectacle, Lynds 483 serves as a chemical laboratory where \u003cspan class=\"technical-term-skylit\"\u003eorganic molecules\u003c\/span\u003e are being forged in the cosmic furnace. Chemical reactions within the stellar ejections and surrounding cloud have produced a rich array of compounds including \u003cspan class=\"highlight-skylit\"\u003ecarbon monoxide, methanol, and several other organic molecules\u003c\/span\u003e—the building blocks that may one day contribute to the formation of planetary systems around these nascent stars.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe dark V-shaped regions visible in the image represent areas where the surrounding dust is so dense that not even Webb's powerful infrared capabilities can penetrate. These \u003cspan class=\"technical-term-skylit\"\u003eopacity zones\u003c\/span\u003e contrast dramatically with the brighter regions where starlight shines through thinner sections of dust, creating a complex interplay of light and shadow that reveals the three-dimensional structure of this stellar formation region.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eNamed after American astronomer \u003cspan class=\"highlight-skylit\"\u003eBeverly Turner Lynds\u003c\/span\u003e, who cataloged dark nebulae in the early 1960s, L483 represents one of the most fertile environments for star formation. Despite appearing as a dark void to earlier observations, these dense molecular clouds are actually cosmic nurseries where the next generation of stars will emerge over millions of years, eventually becoming stars similar in mass to our own Sun.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis image, spanning less than \u003cspan class=\"highlight-skylit\"\u003ehalf a light-year\u003c\/span\u003e within the larger dark nebula complex, offers astronomers crucial insights into calculating how much material the stars have expelled, understanding which molecules are created when materials collide, and mapping the varying densities throughout this dynamic stellar formation region. The observations contribute to our evolving understanding of how stars and potentially planetary systems are born from the cosmic dark.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb's 2024 observations of Lynds 483 represent the most detailed view ever captured of this stellar nursery, revealing structures and processes invisible to previous generations of telescopes.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003ePrincipal Investigator:\u003c\/span\u003e M. Garcia Marin\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Alyssa Pagan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":55246798750073,"sku":"DSP-LYNDS-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40 cm","offer_id":55246798848377,"sku":"DSP-LYNDS-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 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of astronomy's most celebrated supernova remnants—a cosmic graveyard where a massive star met its violent end nearly a millennium ago. \u003cspan class=\"technical-term-skylit\"\u003eThe Crab Nebula (M1)\u003c\/span\u003e represents the aftermath of a stellar explosion so brilliant that Chinese astronomers recorded its appearance in broad daylight during 1054 CE, creating a \"guest star\" visible for weeks before fading into the cosmic tapestry.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAt the heart of this expanding shell of gas and dust beats the remnant of the exploded star: \u003cspan class=\"highlight-skylit\"\u003ea rapidly spinning neutron star called a pulsar\u003c\/span\u003e. This dense stellar corpse, no larger than a city yet containing more mass than our Sun, rotates at incredible speeds while generating powerful magnetic fields that accelerate particles to near light-speed. The pulsar's relentless energy drives the nebula's ongoing expansion and creates the mesmerizing structures visible today.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's revolutionary \u003cspan class=\"technical-term-skylit\"\u003eNIRCam and MIRI instruments\u003c\/span\u003e have dissected the Crab's complex anatomy in unprecedented detail, revealing a cage-like structure of \u003cspan class=\"highlight-skylit\"\u003efluffy red-orange filaments\u003c\/span\u003e composed of doubly ionized sulfur that form the nebula's outer shell. For the first time, astronomers have mapped the warm dust emission throughout the remnant, represented as fluffy magenta material that creates intricate patterns most apparent in the nebula's lower left and upper right regions.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe most striking feature captured by Webb is the \u003cspan class=\"technical-term-skylit\"\u003esynchrotron radiation\u003c\/span\u003e—emission produced by charged particles spiraling around magnetic field lines at relativistic speeds. This phenomenon appears as \u003cspan class=\"highlight-skylit\"\u003emilky, smoke-like wisps\u003c\/span\u003e that trace the invisible magnetic field structure emanating from the central pulsar. The thin white ribbons and curvy wisps follow ripple-like patterns that reveal the three-dimensional architecture of the pulsar's powerful magnetic field.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's infrared vision has revealed an unexpected dust distribution that challenges previous understanding of supernova remnants. Unlike other stellar explosions where dust congregates at the center, \u003cspan class=\"highlight-skylit\"\u003ethe Crab's dust resides in dense filaments of the outer shell\u003c\/span\u003e, with warmer grains in the outermost regions and cooler dust prevalent near the center. This unusual arrangement adds to the Crab's reputation as one of astronomy's most peculiar supernova remnants.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe nebula's yellow-white and green mottled regions represent areas where \u003cspan class=\"technical-term-skylit\"\u003edust particles and ionized sulfur coincide\u003c\/span\u003e, forming large loop-like structures throughout the interior. Meanwhile, blue-tinted filaments reveal the presence of singly ionized iron, providing crucial clues about the chemical composition and explosion mechanism that created this cosmic monument to stellar death.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eBeyond its visual spectacle, the Crab Nebula serves as a cosmic laboratory for understanding supernova physics. Webb's spectroscopic analysis has refined measurements of the \u003cspan class=\"highlight-skylit\"\u003enickel-to-iron abundance ratio\u003c\/span\u003e, helping astronomers determine whether this explosion resulted from an electron-capture supernova—a rare type of stellar death—or a conventional core-collapse event from a star with eight to ten times our Sun's mass.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis expanding shell of stellar debris, now spanning several light-years across, continues to evolve as \u003cspan class=\"technical-term-skylit\"\u003eshockwaves from the original explosion\u003c\/span\u003e interact with surrounding interstellar material. The Crab Nebula stands as both a testament to the violent forces that shape our universe and a preview of the eventual fate awaiting massive stars throughout the cosmos—a cycle of stellar birth, death, and rebirth that has continued for billions of years.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb's 2023-2024 observations of the Crab Nebula represent the highest-resolution infrared study ever conducted of this iconic supernova remnant, revealing structural details invisible to previous generations of telescopes.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003ePrincipal Investigator:\u003c\/span\u003e T. Temim (Princeton University)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Joseph DePasquale (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam and MIRI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":55251183337849,"sku":"DSP-CRAB-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40 cm","offer_id":55251183370617,"sku":"DSP-CRAB-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 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4px;\n    }\n\n    .technical-term-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-style: italic;\n    }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003e\u003cspan\u003eSerpens Nebula: Cosmic Choreography of Stellar Birth Revealed\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIn the constellation Serpens, approximately \u003cspan class=\"highlight-skylit\"\u003e1,300 light-years from Earth\u003c\/span\u003e, lies a cosmic nursery where the secrets of stellar formation have finally been unveiled. \u003cspan class=\"technical-term-skylit\"\u003eThe Serpens Nebula\u003c\/span\u003e represents one of astronomy's youngest star-forming regions at just one to two million years old—a cosmic infant where Webb's unprecedented infrared vision has captured a phenomenon astronomers have theorized about for decades but never directly observed.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAt the heart of this discovery lies a groundbreaking revelation: \u003cspan class=\"highlight-skylit\"\u003eperfectly aligned protostellar outflows\u003c\/span\u003e streaming from newborn stars in synchronized formation. Unlike the typically chaotic orientations found in other star-forming regions, these jets of gas erupting from stellar embryos all flow in the same direction with the same degree of inclination, resembling \"sleet pouring down during a storm\" as they pierce through the cosmic darkness.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's revolutionary \u003cspan class=\"technical-term-skylit\"\u003eNIRCam (Near-Infrared Camera)\u003c\/span\u003e has revealed these spectacular outflows as \u003cspan class=\"highlight-skylit\"\u003ebright red clumpy streaks\u003c\/span\u003e visible in the nebula's upper left region. These crimson signatures represent shockwaves created when jets of molecular hydrogen and carbon monoxide, expelled at tremendous velocities from newborn protostars, collide with surrounding gas and dust. The infrared detection marks the first time these extremely young stellar phenomena have been observed with such clarity.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe synchronized nature of these outflows provides crucial evidence supporting long-held theories about stellar formation. As \u003cspan class=\"technical-term-skylit\"\u003einterstellar gas clouds collapse\u003c\/span\u003e to form stars, they spin faster due to conservation of angular momentum, creating swirling magnetic fields that launch material into twin jets perpendicular to forming protostellar disks. The remarkable alignment suggests that \u003cspan class=\"highlight-skylit\"\u003estars born in the same region inherit similar rotational orientations\u003c\/span\u003e from their parent molecular cloud.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eBeyond the aligned outflows, the Serpens Nebula hosts a particularly dense cluster of \u003cspan class=\"highlight-skylit\"\u003enewly forming stars approximately 100,000 years old\u003c\/span\u003e, some destined to grow to the mass of our Sun. This stellar nursery also features the enigmatic \"Bat Shadow\"—a planet-forming disk first observed by Hubble in 2020 that appears to flap or shift, creating one of astronomy's most intriguing dynamic phenomena visible at the image center.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's infrared capabilities have unveiled additional mysterious features throughout the region, including an \u003cspan class=\"technical-term-skylit\"\u003eeye-shaped crevice\u003c\/span\u003e that appears as if a star is bursting through cosmic material, and extremely dark patches where dense concentrations of gas and dust completely block near-infrared light. These layered structures of varying densities create complex three-dimensional architectures reminiscent of the famous Pillars of Creation.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe nebula also harbors remarkable stellar objects including \u003cspan class=\"highlight-skylit\"\u003eSMM 1, a binary protostar system\u003c\/span\u003e where two forming stars orbit each other while producing separate but overlapping outflows, and OO Serpentis—a young star that erupted violently in 1995, providing astronomers with a rare glimpse of extreme stellar outbursts that typically last only brief periods in cosmic time.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis discovery represents just the beginning of an ambitious scientific program to understand \u003cspan class=\"technical-term-skylit\"\u003evolatile chemical survival\u003c\/span\u003e during star and planet formation. Future observations will use Webb's NIRSpec spectrograph to investigate how compounds like water and carbon monoxide—materials essential for planetary development—persist through the violent processes of stellar birth, potentially illuminating the chemical foundations necessary for life itself.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb's 2024 observations of the Serpens Nebula mark the first direct imaging of aligned protostellar outflows, providing unprecedented evidence for theoretical models of how stars form in cosmic nurseries.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003ePrincipal Investigator:\u003c\/span\u003e K. Pontoppidan (NASA-JPL)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eLead Author:\u003c\/span\u003e J. Green (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Alyssa Pagan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":55251268272505,"sku":"DSP-SERP-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40cm","offer_id":55251268305273,"sku":"DSP-SERP-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 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  display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003e\u003cspan\u003eNGC 604: A Star-Forming Symphony in the Triangulum Galaxy\u003c\/span\u003e\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eLocated approximately \u003cspan class=\"highlight-skylit\"\u003e2.73 million light-years away\u003c\/span\u003e in the Triangulum Galaxy (M33), \u003cspan class=\"technical-term-skylit\"\u003eNGC 604\u003c\/span\u003e stands as one of the largest and most luminous star-forming regions in our local galactic neighbourhood. Captured by the \u003cspan class=\"technical-term-skylit\"\u003eJames Webb Space Telescope’s NIRCam\u003c\/span\u003e, this celestial marvel reveals the breathtaking scale and complexity of cosmic birth on a scale spanning over 1,700 light-years across.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIn this image, brilliant stellar winds from \u003cspan class=\"highlight-skylit\"\u003ehot, young stars\u003c\/span\u003e have carved dramatic cavities into the surrounding gas and dust. These violent outbursts shape the architecture of the nebula, generating pressure waves that both destroy and trigger further star formation across the region. It’s a galactic symphony of destruction and renewal, conducted by gravity and radiation.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe vibrant \u003cspan class=\"highlight-skylit\"\u003eorange-red filaments\u003c\/span\u003e seen here signify the presence of \u003cspan class=\"technical-term-skylit\"\u003epolycyclic aromatic hydrocarbons (PAHs)\u003c\/span\u003e—carbon-rich molecules that float through interstellar space. These organic compounds are often linked with the very building blocks of life. Further out, the deeper crimson tones mark cold, dense molecular hydrogen—prime real estate for the next generation of stars to emerge.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAmidst these colourful clouds, Webb’s NIRCam reveals cooler gas illuminated by energetic starlight. The ghostly hues of \u003cspan class=\"highlight-skylit\"\u003eblue and white\u003c\/span\u003e represent ionised hydrogen, glowing from ultraviolet light emitted by the youngest, most massive stars. These regions burn with the fierce brightness of formation and are key to understanding stellar evolution across the cosmos.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eNGC 604’s proximity and sheer scale offer astronomers a rare chance to study an extreme concentration of newly forming stars in exquisite detail. In contrast to distant, barely resolved nebulae, this galactic nursery is close enough to observe intricate features—twisting gas arcs, radiation-blasted cavities, and sprawling clouds dense with potential for future suns.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe colours in this image are not visible to the naked eye—they’re constructed using multiple filters from Webb’s \u003cspan class=\"technical-term-skylit\"\u003einfrared camera\u003c\/span\u003e. Each colour represents a different wavelength of light: blue (F090W), cyan (F187N), green (F335M), and red (F444W + F470N). Together, they unveil a previously hidden world of stellar creation in one of the universe’s most captivating galactic nurseries.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWhether displayed in your home or studio, this visual story of NGC 604 offers a humbling reminder of the scale and beauty of our universe. It speaks to the eternal dance of birth and transformation unfolding in silence, light-years away from Earth—and yet, now, within reach through art and science.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eCaptured on 28 January 2024 and rendered with scientific precision by NASA, ESA, CSA, and STScI, this Webb image represents one of the most detailed observations of a star-forming region ever made.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003ePrincipal Investigator:\u003c\/span\u003e M. Marin\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Alyssa Pagan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eFilters Used:\u003c\/span\u003e F090W, F187N, F200W, F335M, F444W, F470N\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":55281784652153,"sku":"DSP-NGC604-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 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\u003cspan class=\"highlight-skylit\"\u003ePismis 24\u003c\/span\u003e, an energetic cluster of newly formed stars located at the heart of the \u003cspan class=\"technical-term-skylit\"\u003eLobster Nebula (NGC 6357)\u003c\/span\u003e, around 5,500 light-years away in \u003cspan class=\"highlight-skylit\"\u003eScorpius\u003c\/span\u003e. One of the Milky Way’s closest sites of massive star birth, this region allows astronomers to observe the formation of some of the galaxy’s heaviest, brightest stars.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe towering “mountains” in the scene are not rock but \u003cspan class=\"technical-term-skylit\"\u003evast, sculpted walls of gas and dust\u003c\/span\u003e, carved away by intense ultraviolet radiation and powerful stellar winds. Webb’s NIRCam reveals the dramatic interaction between these newly formed stars and the material from which they were born—illuminated clouds, evaporating ridges, and turbulent flows shaped by extreme energy.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eSome stars in Pismis 24 are among the most massive known, with masses exceeding \u003cspan class=\"highlight-skylit\"\u003e100 times that of the Sun\u003c\/span\u003e. Their radiation ionises the nebula, creating the glowing, sculpted structures visible here. The bright stellar field above the dust ridge reveals dozens of young hot stars in early stages of evolution.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb captured this region using several infrared wavelengths, including \u003cspan class=\"technical-term-skylit\"\u003e0.9 μm, 1.87 μm, 2.0 μm, 3.35 μm (PAH emission), and 4.7 μm (molecular hydrogen)\u003c\/span\u003e. These wavelengths pierce deeply into dusty star-forming clouds, revealing structures and processes invisible to optical telescopes.\u003c\/div\u003e\n\u003cdiv class=\"science-box\"\u003e\n\u003ch3\u003eScience Highlights\u003c\/h3\u003e\n\u003cul style=\"margin: 0; padding-left: 18px;\"\u003e\n\u003cli\u003ePismis 24 sits within an active \u003cstrong\u003eH II region\u003c\/strong\u003e rich in newborn stars.\u003c\/li\u003e\n\u003cli\u003eThe nebula’s sculpted “peaks” are shaped by intense stellar radiation.\u003c\/li\u003e\n\u003cli\u003eField of view: \u003cstrong\u003e4.22 × 5.83 arcminutes\u003c\/strong\u003e (spanning several light-years).\u003c\/li\u003e\n\u003cli\u003eOrientation: \u003cstrong\u003eNorth is 182.7° right of vertical\u003c\/strong\u003e.\u003c\/li\u003e\n\u003c\/ul\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eBoth visually breathtaking and scientifically invaluable, this Webb image offers a rare glimpse into the beauty—and chaos—of star birth on a monumental scale.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eCaptured by Webb's NIRCam instrument across multiple infrared bands, revealing hidden details of dust, hydrogen, and newly formed stars within Pismis 24 and the wider Lobster Nebula.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstruments:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eRegion:\u003c\/span\u003e Pismis 24, NGC 6357 (Lobster Nebula)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e STScI Science Team\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":56290724807033,"sku":"DSP-PIS24-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40cm","offer_id":56290724839801,"sku":"DSP-PIS24-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 cm","offer_id":56290724872569,"sku":"DSP-PIS24-PRT-40X50-NOFRM","price":29.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 50 x 70 cm","offer_id":56290724905337,"sku":"DSP-PIS24-PRT-50X70-NOFRM","price":37.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 60 x 80 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.science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eNGC 6072: The Beautiful Chaos of a Dying Star\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe James Webb Space Telescope has captured a hauntingly beautiful moment in the lifecycle of a star with its latest image of \u003cspan class=\"highlight-skylit\"\u003eNGC 6072\u003c\/span\u003e, a planetary nebula in the southern constellation \u003cspan class=\"highlight-skylit\"\u003eScorpius\u003c\/span\u003e. What you see here is the spectacular final breath of a dying star — expanding clouds of gas and dust illuminated from within by its glowing core.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eRather than a simple spherical shell, NGC 6072 reveals a complex, multipolar structure: multiple outflows jet outward at different angles, forming lobes of glowing gas that push material into an equatorial disc. This unusual shape suggests the presence of at least one companion star interacting with the dying star — a celestial dance that dramatically shapes the nebula’s final form.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe colours in this print are more than just eye-catching — they encode real astrophysical detail. The red and orange hues trace cooler molecular gas (likely molecular hydrogen), while the brighter central glow marks the intensely heated, ionised gas surrounding the nebula’s core. The structures span several light-years, offering a window into the turbulent, transformative processes that follow a star’s death.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis NGC 6072 print is a tribute to cosmic impermanence — a vivid reminder that even in death, stars can shape the universe with breath-taking beauty. It brings to your home or workspace a moment of real astronomical drama and wonder, rendered in museum-grade detail and carefully framed by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eImage captured by Webb’s NIRCam \u0026amp; MIRI instruments. Colours represent emissions from molecular gas and ionised material, revealing the late-life transformations of a Sun-like star.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e NGC 6072, Planetary Nebula (Scorpius)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstruments:\u003c\/span\u003e Webb NIRCam \u0026amp; MIRI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit 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Studio","description":"\u003cstyle\u003e\n    .container-skylit {\n        max-width: 900px;\n        margin: 0 auto;\n        padding: 40px 20px;\n    }\n\n    .header-skylit {\n        text-align: center;\n        margin-bottom: 40px;\n        border-bottom: 2px solid #FFB503;\n        padding-bottom: 20px;\n    }\n\n    .logo-skylit {\n        font-size: 2.5em;\n        font-weight: 300;\n        background: linear-gradient(45deg, #0D0D1F, #FFB503, #FFDA73);\n        -webkit-background-clip: text;\n        -webkit-text-fill-color: transparent;\n        margin-bottom: 10px;\n    }\n\n    .subtitle-skylit {\n        color: #e5d9c5;\n        font-size: 1.1em;\n        font-weight: 300;\n    }\n\n    .main-title-skylit {\n            font-size: 2.2em;\n    color: #ffb503;\n    margin-bottom: 30px;\n    text-align: center;\n    text-shadow: 2px 2px 2px #be2119;\n    }\n\n    .content-skylit {\n        background: rgba(13, 13, 31, 0.55);\n        backdrop-filter: blur(12px);\n        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.paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eNGC 1333: A Stellar Nursery in the Perseus Molecular Cloud\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAbout \u003cspan class=\"highlight-skylit\"\u003e1,000 light-years\u003c\/span\u003e away, in the constellation Perseus, sits one of the nearest places where stars are being born right now. \u003cspan class=\"highlight-skylit\"\u003eNGC 1333\u003c\/span\u003e is a knot of gas and dust inside the Perseus Molecular Cloud, and the James Webb Space Telescope's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e sees straight through the murk that hides it from ordinary telescopes.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe result is a landscape of colour. Reflection nebulae glow blue and orange where starlight scatters off dust, dark lanes cut across the cloud, and the eight-pointed stars are the brightest young suns, only a few million years old. Between them Webb picks out dozens of \u003cspan class=\"highlight-skylit\"\u003ebrown dwarfs\u003c\/span\u003e and free-floating planetary-mass objects, too small to ignite as stars.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eJets and outflows from the infant stars punch through the cloud in red and pink, the \u003cspan class=\"technical-term-skylit\"\u003eHerbig-Haro\u003c\/span\u003e shock fronts that mark where new stars are still gathering material. Astronomers use fields like this one to ask how small an object can form the way a star does.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThis is what our own neighbourhood looked like 4.6 billion years ago. Printed on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released as ESA\/Webb Picture of the Month, August 2024. Near-infrared light mapped to visible colour.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e ESA\/Webb, NASA, CSA, A. Scholz, K. Muzic, A. Langeveld, R. Jayawardhana\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e NGC 1333, Reflection Nebula (Perseus)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":64487939309945,"sku":"DSP-NGC1333-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40cm","offer_id":64487939342713,"sku":"DSP-NGC1333-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 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#FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eRho Ophiuchi: Webb's First Anniversary Portrait of Star Birth\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eTo celebrate its first year of science, the James Webb Space Telescope pointed at the closest star-forming region to Earth: the \u003cspan 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Because it is so near, this small patch of sky holds no distant galaxies, only the dust, gas and roughly 50 young stars of a single nursery.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe dark cloud at the centre and bottom is dense enough to block even Webb's infrared eyes; the stars forming inside it are still wrapped in their birth cocoons. Around them, the brilliant star \u003cspan class=\"technical-term-skylit\"\u003eS1\u003c\/span\u003e at the lower half of the frame has carved a glowing cave out of the dust, and the \u003cspan class=\"highlight-skylit\"\u003ered jets\u003c\/span\u003e shooting across the top are molecular hydrogen lit by outflows from newborn stars.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eSome of the young stars show tell-tale shadows: disks of gas and dust seen edge-on, the raw material of future planets. Webb's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e resolves them all at a level of detail no telescope had managed before.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eIt is a picture of a beginning, of the kind of place our own Sun was born in. Printed on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released 12 July 2023 for the telescope's first anniversary of science operations.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI, Klaus Pontoppidan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e Alyssa Pagan (STScI)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e Rho Ophiuchi cloud complex (Ophiuchus)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan 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margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eThe Cosmic Cliffs: Webb's First Look at a Stellar Nursery\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eOn 12 July 2022 the James Webb Space Telescope released its first full-colour images, and this was the one that stopped people. The \u003cspan class=\"highlight-skylit\"\u003eCosmic Cliffs\u003c\/span\u003e are the edge of a cavity in the nebula NGC 3324, at the northern rim of the Carina Nebula, about \u003cspan class=\"highlight-skylit\"\u003e7,600 light-years\u003c\/span\u003e away.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWhat looks like a mountain range at dusk is a wall of gas and dust; the tallest peaks are about seven light-years high. The cavity above it was hollowed out by ultraviolet light and winds from hot young stars just out of frame, and the \u003cspan class=\"highlight-skylit\"\u003esteam\u003c\/span\u003e rising off the ridge is gas boiling away from the cloud's surface.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e sees in infrared, which passes through the dust that hides this scene from visible-light telescopes. Hundreds of stars that Hubble could not see appear here, including newborn ones still buried in the cliffs and the jets they fire into space.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003ePrinted on 260gsm photo lustre paper and framed in the UK by Skylit Studio, from a portrait crop of the full Webb mosaic.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released 12 July 2022 among the telescope's first images.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e NGC 3324, Carina Nebula (Carina)\u003c\/div\u003e\n\u003cdiv 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margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eThe Southern Ring: A Star's Final Act\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe \u003cspan class=\"highlight-skylit\"\u003eSouthern Ring Nebula\u003c\/span\u003e, NGC 3132, is what a star like the Sun leaves behind. About \u003cspan class=\"highlight-skylit\"\u003e2,500 light-years\u003c\/span\u003e away in Vela, a dying star has been shedding its outer layers for thousands of years, and the shells of gas it threw off now glow in the light of the hot core left at the centre.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e shows those shells with a texture no telescope had seen: the foamy orange rim is molecular hydrogen, the blue interior is hotter ionised gas, and the streaks radiating outward are the shadows of dense knots of dust closer in. The nebula is nearly half a light-year across.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThere are two stars at the centre. The brighter one is an ordinary star still in its prime; the fainter one beside it is the dying star that made the nebula, and Webb's infrared view was the first to show it clearly cloaked in dust.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eOne of Webb's first images, released the day the telescope opened for science. Printed on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released 12 July 2022 among the telescope's first images.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e NGC 3132, Planetary Nebula (Vela)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit 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}\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eStephan's Quintet: Five Galaxies, One Collision\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003e\n\u003cspan class=\"highlight-skylit\"\u003eStephan's Quintet\u003c\/span\u003e was the first compact galaxy group ever discovered, in 1877, and Webb's image of it in July 2022 was the largest the telescope had made: a mosaic of nearly a thousand separate frames covering a patch of sky a fifth the width of the Moon.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eFour of the five galaxies are bound together about \u003cspan class=\"highlight-skylit\"\u003e290 million light-years\u003c\/span\u003e away in Pegasus, pulling one another apart. The sweeping tails of gas and stars between them are the debris of repeated close passes, and the shock front where one galaxy ploughs through the group is lit up across Webb's infrared view.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe fifth galaxy, \u003cspan class=\"technical-term-skylit\"\u003eNGC 7320\u003c\/span\u003e, at the left, is a bystander: it sits only 40 million light-years away, seven times closer, and simply happens to lie along the same line of sight. Webb resolves its individual stars while the distant four appear as glowing spirals.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003ePrinted on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam and MIRI composite released 12 July 2022 among the telescope's first images.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e Stephan's Quintet, HCG 92 (Pegasus)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstruments:\u003c\/span\u003e Webb 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   }\n\n    .science-box {\n        margin: 35px 0 25px;\n        padding: 22px;\n        background: rgba(255, 181, 3, 0.06);\n        border-left: 4px solid #FFB503;\n        border-radius: 10px;\n        color: #EFE5D8;\n    }\n\n    .science-box h3 {\n        color: #FFDA73;\n        margin-top: 0;\n        font-size: 1.25em;\n        margin-bottom: 10px;\n    }\n\n    .credits-skylit {\n        margin-top: 40px;\n        padding: 20px;\n        background: #4A434A;\n        border-radius: 10px;\n        border-left: 4px solid #FFB503;\n        color: #EEE5D9;\n    }\n\n    .credits-title-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        font-size: 1.25em;\n        margin-bottom: 15px;\n    }\n\n    .credit-section-skylit {\n        margin-bottom: 10px;\n    }\n\n    .credit-label-skylit {\n        color: #FFB503;\n        font-weight: 600;\n        display: inline-block;\n        min-width: 135px;\n    }\n\n    .footer-note-skylit {\n        margin-top: 30px;\n        padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eCassiopeia A: The Youngest Supernova Remnant in the Milky Way\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAbout 340 years ago the light from an exploding star reached Earth from the constellation Cassiopeia. Nobody seems to have recorded it, but the debris is still expanding today: \u003cspan class=\"highlight-skylit\"\u003eCassiopeia A\u003c\/span\u003e, roughly \u003cspan class=\"highlight-skylit\"\u003e11,000 light-years\u003c\/span\u003e away and ten light-years across, the youngest supernova remnant known in our galaxy.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eWebb's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e shows the explosion in unprecedented detail. The orange and pink knots are the star's own shredded interior, rich in oxygen, argon and neon, thrown outward at thousands of miles per second. The fine white filaments are the blast wave tearing through the gas the star shed before it died.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eAstronomers are using this image to trace what the star was made of and how it came apart, layer by layer. Supernovae like this one are where most of the heavy elements in the universe, including the calcium in bones and the iron in blood, were forged.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003ePrinted on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released 10 December 2023.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, STScI, Danny Milisavljevic (Purdue University), Ilse De Looze (UGent), Tea Temim (Princeton University)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e Cassiopeia A, Supernova Remnant (Cassiopeia)\u003c\/div\u003e\n\u003cdiv 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padding: 16px;\n        background: rgba(255, 255, 255, 0.02);\n        border-radius: 8px;\n        font-style: italic;\n        color: #d3c7b2;\n        text-align: center;\n        font-size: 0.96em;\n    }\n\n    @media (max-width: 768px) {\n        .main-title-skylit { font-size: 1.9em; }\n        .content-skylit { padding: 25px; }\n        .paragraph-skylit { text-align: left; }\n    }\n\u003c\/style\u003e\n\u003cdiv class=\"container-skylit\"\u003e\n\u003ch1 class=\"main-title-skylit\"\u003eNGC 346: Star Birth in a Neighbouring Galaxy\u003c\/h1\u003e\n\u003cdiv class=\"content-skylit\"\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003e\n\u003cspan class=\"highlight-skylit\"\u003eNGC 346\u003c\/span\u003e is the brightest and most active star-forming region in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way about \u003cspan class=\"highlight-skylit\"\u003e200,000 light-years\u003c\/span\u003e away in the southern constellation Tucana. Webb's \u003cspan class=\"technical-term-skylit\"\u003eNIRCam\u003c\/span\u003e image from January 2023 shows it as a glowing pink cloud laced with ribbons of dust.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe Small Magellanic Cloud has far fewer heavy elements than our galaxy, which makes it a stand-in for the early universe, when stars formed from gas that had not yet been enriched. Astronomers expected little dust here. Webb found plenty, along with thousands of newborn stars and protostars still gathering material.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003eThe dust ribbons are streams of gas feeding the young cluster at the centre, and the pink glow is hydrogen lit by the hottest of the new stars. It is a picture of how the first galaxies may have built their stars.\u003c\/div\u003e\n\u003cdiv class=\"paragraph-skylit\"\u003ePrinted on 260gsm photo lustre paper and framed in the UK by Skylit Studio.\u003c\/div\u003e\n\u003cdiv class=\"footer-note-skylit\"\u003eWebb NIRCam image released 11 January 2023.\u003c\/div\u003e\n\u003c\/div\u003e\n\u003cdiv class=\"credits-skylit\"\u003e\n\u003cdiv class=\"credits-title-skylit\"\u003eImage Credits\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eScience:\u003c\/span\u003e NASA, ESA, CSA, O. Jones (UK ATC), G. De Marchi (ESTEC), M. Meixner (USRA)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eImage Processing:\u003c\/span\u003e A. Pagan (STScI), N. Habel (USRA), L. Lenkic (USRA), L. Chu (NASA\/Ames)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eField:\u003c\/span\u003e NGC 346, Small Magellanic Cloud (Tucana)\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eInstrument:\u003c\/span\u003e Webb NIRCam\u003c\/div\u003e\n\u003cdiv class=\"credit-section-skylit\"\u003e\n\u003cspan class=\"credit-label-skylit\"\u003eAdaptation:\u003c\/span\u003e Skylit Studio\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"Skylit Studio","offers":[{"title":"Unframed Print \/ A4","offer_id":64488463073657,"sku":"DSP-NGC346-PRT-A4-NOFRM","price":19.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 30 x 40cm","offer_id":64488463106425,"sku":"DSP-NGC346-PRT-30X40-NOFRM","price":25.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 40 x 50 cm","offer_id":64488463139193,"sku":"DSP-NGC346-PRT-40X50-NOFRM","price":29.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 50 x 70 cm","offer_id":64488463171961,"sku":"DSP-NGC346-PRT-50X70-NOFRM","price":37.79,"currency_code":"GBP","in_stock":true},{"title":"Unframed Print \/ 60 x 80 cm","offer_id":64488463204729,"sku":"DSP-NGC346-PRT-60X80-NOFRM","price":59.79,"currency_code":"GBP","in_stock":true},{"title":"Classic Black Frame \/ A4","offer_id":64488463237497,"sku":"DSP-NGC346-BLK-A4","price":34.99,"currency_code":"GBP","in_stock":true},{"title":"Classic Black Frame \/ 30 x 40cm","offer_id":64488463270265,"sku":"DSP-NGC346-BLK-30X40","price":44.99,"currency_code":"GBP","in_stock":true},{"title":"Classic Black Frame \/ 40 x 50 cm","offer_id":64488463303033,"sku":"DSP-NGC346-BLK-40X50","price":54.99,"currency_code":"GBP","in_stock":true},{"title":"Classic Black Frame \/ 50 x 70 cm","offer_id":64488463335801,"sku":"DSP-NGC346-BLK-50X70","price":71.99,"currency_code":"GBP","in_stock":true},{"title":"Classic Black Frame \/ 60 x 80 cm","offer_id":64488463368569,"sku":"DSP-NGC346-BLK-60X80","price":107.99,"currency_code":"GBP","in_stock":false},{"title":"Elegant White Frame \/ A4","offer_id":64488463401337,"sku":"DSP-NGC346-WHT-A4","price":34.99,"currency_code":"GBP","in_stock":false},{"title":"Elegant White Frame \/ 30 x 40cm","offer_id":64488463434105,"sku":"DSP-NGC346-WHT-30X40","price":44.99,"currency_code":"GBP","in_stock":true},{"title":"Elegant White Frame \/ 40 x 50 cm","offer_id":64488463466873,"sku":"DSP-NGC346-WHT-40X50","price":54.99,"currency_code":"GBP","in_stock":false},{"title":"Elegant White Frame \/ 50 x 70 cm","offer_id":64488463499641,"sku":"DSP-NGC346-WHT-50X70","price":71.99,"currency_code":"GBP","in_stock":true},{"title":"Elegant White Frame \/ 60 x 80 cm","offer_id":64488463532409,"sku":"DSP-NGC346-WHT-60X80","price":107.99,"currency_code":"GBP","in_stock":false},{"title":"Natural Brown Frame \/ A4","offer_id":64488463565177,"sku":"DSP-NGC346-NAT-A4","price":34.99,"currency_code":"GBP","in_stock":false},{"title":"Natural Brown Frame \/ 30 x 40cm","offer_id":64488463597945,"sku":"DSP-NGC346-NAT-30X40","price":44.99,"currency_code":"GBP","in_stock":true},{"title":"Natural Brown Frame \/ 40 x 50 cm","offer_id":64488463630713,"sku":"DSP-NGC346-NAT-40X50","price":54.99,"currency_code":"GBP","in_stock":true},{"title":"Natural Brown Frame \/ 50 x 70 cm","offer_id":64488463663481,"sku":"DSP-NGC346-NAT-50X70","price":71.99,"currency_code":"GBP","in_stock":true},{"title":"Natural Brown Frame \/ 60 x 80 cm","offer_id":64488463696249,"sku":"DSP-NGC346-NAT-60X80","price":107.99,"currency_code":"GBP","in_stock":false},{"title":"Dark Brown Frame \/ A4","offer_id":64488463729017,"sku":"DSP-NGC346-DBR-A4","price":34.99,"currency_code":"GBP","in_stock":true},{"title":"Dark Brown Frame \/ 30 x 40cm","offer_id":64488463761785,"sku":"DSP-NGC346-DBR-30X40","price":44.99,"currency_code":"GBP","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0710\/5278\/7987\/files\/BLACKFRAME-skylitstudio-NGC346.jpg?v=1788629580"}],"url":"https:\/\/skylitstudio.co.uk\/collections\/james-webb-collection.oembed?page=2","provider":"Skylit Studio","version":"1.0","type":"link"}