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In conjunction with data from the newly launched Euclid space satellite, scienti...

Piotr Kosek: "In conjunction with data from the newly launched Euclid space satellite, scientists expect to discover thousands of new gravitationally lens..." — Pending

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📅 12.06.2026 · Ciemna energia może jednak słabnąć? Nowe pomysły astrof... · 👁️ 18

Pending. The Euclid mission aims to study dark energy and dark matter using gravitational lensing. Due to its high resolution and wide-area survey capabilities, Euclid is expected to discover a large number of strong gravitationa...

"In conjunction with data from the newly launched Euclid space satellite, scientists expect to discover thousands of new gravitationally lensed quasars and hundreds of rare lensed supernovae. And such a statistical base will allow the measurement error of the Hubble constant to be reduced to below 1%." "W połączeniu z danymi z nowo wysłanego kosmicznego satelity Euklit, naukowcy spodziewają się odkryć tysiące nowych zsoczewkowanych grawitacyjnie kwazarów oraz setki rzadkich zsoczewkowanych supernowych. A taka baza statystyczna pozwoli zbić błąd pomiarowy stałej Habla do poziomu poniżej 1%."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
🔮 Forecast 🔹 Other Long timeframe (over 5 years) AI confidence (unresolved): 90% Resolves by: 31 Dec 2036 Assertiveness: high 🌍 Global Source on YouTube

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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

Ten przełom na szczęście dzieje się na naszych oczach. Obserwatorium Very Rubin, o którym był poprzedni Astroszort, do którego serdecznie was odsyłam, uruchomiło swój monumentalny przegląd nieba, w ramach którego zaawansowany teleskop będzie przez pełną dekadę, co kilka nocy, fotografował całe dostępne południowe niebo. I w połączeniu z danymi z nowo wysłanego kosmicznego satelity Euklit, naukowcy spodziewają się odkryć tysiące nowych zsoczewkowanych grawitacyjnie kwazarów oraz setki rzadkich zsoczewkowanych supernowych. A taka baza statystyczna pozwoli zbić błąd pomiarowy stałej Habla do poziomu poniżej 1%. A to uczyni napięcie HBla faktem bezdyskusyjnym i pozwoli na żywo obserwować jak ciemna energia zmieniała swoje oblicze na przestrzeni miliardów lat ewolucji wszechświata. Oczywiście wciąż nie odpowie nam to na pytanie czym ciemna energia jest, ale pokaże, że faktycznie jest jakiś parametr, który musimy uwzględniać i jest on zmienny w czasie. A to

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