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JADES-GS-z14-0 is 1,600 light years (ly) wide and very luminous. Spectroscopic a...

Piotr Kosek: "JADES-GS-z14-0 is 1,600 light years (ly) wide and very luminous. Spectroscopic analysis revealed the presence of strong ionized gas emission..." — True

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📅 06.02.2026 · To nie jest galaktyka? Czy patrzymy na obiekt zasilany... · 👁️ 4

True. The galaxy JADES-GS-z14-0, discovered by the James Webb Space Telescope, is a record-breaking high-redshift object (z ≈ 14.18-14.32), observed merely 290-300 million years after the Big Bang, during the "cosmic dawn". Th...

"JADES-GS-z14-0 is 1,600 light years (ly) wide and very luminous. Spectroscopic analysis revealed the presence of strong ionized gas emissions, including hydrogen and oxygen. [...] Its age, size, and luminosity added to a growing body of evidence that current theories of early star and galaxy formation are incomplete." "Jades GSZ140 jest prawdziwym problemem. Dlaczego? Bo jest za duży, jest za jasny. Według obowiązującego modelu Lambda CDM galaktyki w tamtym okresie, czyli w tak zwanym kosmicznym świcie, powinny być małe, słabe i dopiero raczkujące w procesie formowania gwiazd. Tymczasem ten obiekt wygląda na dojrzały, jakby formował gwiazdy szybciej i wydajniej niż jakikolwiek model na to pozwala."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

Teleskop Jamesa Weba dzięki swoim instrumentom Nearcam i Nearspierdził, że patrzymy na obiekt z przesunięciem ku czerwieni wynoszącym 14,32. A to oznacza, że widzimy go takim jakim był zaledwie 300 milionów lat po wielkim wybuchu. Dla kontekstu wcześniej rekordzistą był obiekt Z14, starszy o marne 10 milionów lat. Ale to Jades GSZ140 jest prawdziwym problemem. Dlaczego? Bo jest za duży, jest za jasny. Według obowiązującego modelu Lambda CDM galaktyki w tamtym okresie, czyli w tak zwanym kosmicznym świcie, powinny być małe, słabe i dopiero raczkujące w procesie formowania gwiazd. Tymczasem ten obiekt wygląda na dojrzały, jakby formował gwiazdy szybciej i wydajniej niż jakikolwiek model na to pozwala. Zanim przejdziemy do tego, czym ten obiekt może być, musimy zatrzymać się przy kluczowym pojęciu, bez którego nie zrozumiemy skali tego odkrycia. Chodzi o przesunięcie ku czerwieni, czyli tak zwany red shift. Kiedy patrzymy w niebo, patrzymy w przeszłość, no to oczywiście wiecie, ale światło podróżujące przez miliardy lat nie dociera do nas w taki

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