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The Vera C. Rubin Observatory is just weeks, maybe even just days, away from off...

Piotr Kosek: "The Vera C. Rubin Observatory is just weeks, maybe even just days, away from officially beginning its landmark 10-year sky survey, according..." — Misleading

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📅 12.06.2026 · Ciemna energia może jednak słabnąć? Nowe pomysły astrof... · 👁️ 2

Misleading. The Vera C. Rubin Observatory is indeed set to conduct a monumental, decade-long Legacy Survey of Space and Time (LSST) of the southern sky using its advanced Simonyi Survey Telescope. However, as of June 12, 2026, the d...

"The Vera C. Rubin Observatory is just weeks, maybe even just days, away from officially beginning its landmark 10-year sky survey, according to officials at the 248th American Astronomical Society (AAS) meeting in Pasadena this week." "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."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
Factual claim 🔹 Other AI assessment confidence: 90% 🌍 Global Source on YouTube

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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

zić ostatecznie to jakby nie patrzeć epokowe odkrycie, żeby precyzyjnie prześledzić proces słabnięcia ciemnej energii, astronomowie potrzebują jednak gigantycznej bazy danych, która zredukuje wszelkie niepewności pomiarowe do absolutnego minimum, bo w tym momencie wciąż jest ich całkiem sporo. 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 pozwo

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