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The spectrum of this galaxy shows no characteristic lines for heavy elements. Th...

Piotr Kosek: "The spectrum of this galaxy shows no characteristic lines for heavy elements. There is no trace of carbon or oxygen. Instead, the James Webb..." — True

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📅 06.05.2026 · Webb odkrył gwiazdy III populacji? Wszystko na to wskaz... · 👁️ 2

True. The claim is true. The James Webb Telescope indeed discovered the galaxy JADES-GS-z14-0, which shows a lack of heavy elements like carbon and oxygen, and instead a strong signature of ionized helium. This is consistent w...

"The spectrum of this galaxy shows no characteristic lines for heavy elements. There is no trace of carbon or oxygen. Instead, the James Webb Telescope recorded something very rare, a signature of ionized Helium." "Widmo tej galaktyki pokazuje brak jakichkolwiek linii charakterystycznych dla ciężkich pierwiastków. Nie ma tam śladu po węglu czy tlenie. Zamiast tego teleskop Jamesa Weba zarejestrował coś bardzo rzadkiego, sygnaturę zjonizowanego Helu."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

h miejscach, to wiemy dokładnie, co znajduje się w badanym obiekcie. Nawet jeśli dzieli nas od niego 13 miliardów lat świetlnych. To troszeczkę tak, jakbyśmy badali skład chemiczny odległego ogniska, analizując jedynie kolor dymu, który z niego wylatuje. W przypadku Hebe naukowcy szukali czegoś, czego tam nie ma. I to jest najbardziej ekscytujące. Widmo tej galaktyki pokazuje brak jakichkolwiek linii charakterystycznych dla ciężkich pierwiastków. Nie ma tam śladu po węglu czy tlenie. Zamiast tego teleskop Jamesa Weba zarejestrował coś bardzo rzadkiego, sygnaturę zjonizowanego Helu. Iizacja to sytuacja, w której atom przyjmuje tak dużą dawkę energii, jakieś fotony, że traci on swoje elektrony. Jeśli dostarczymy wystarczająco dużo energii, na przykład w postaci ekstremalnie silnego promieniowania ultrafioletowego, to wyrwiemy te elektrony z ich orbit. Do zjonizowania helu potrzeba niewyobrażalnej energii, znacznie większej niż

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