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S2 needs only 16 years to orbit the Galactic Center. In comparison, our Sun need...

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Piotr Kosek: "S2 needs only 16 years to orbit the Galactic Center. In comparison, our Sun needs over 200 million years for this. S2 approaches the center..." — True

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Piotr Kosek

📅 06.03.2026 · Sagittarius A* to nie czarna dziura? Niepokojąca hipote... · 👁️ 2

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True. The star S2 indeed orbits the supermassive black hole Sagittarius A* at the center of the Milky Way in approximately 16 years. Its orbit is highly elliptical, meaning it approaches the center at an extremely small distan...

"S2 needs only 16 years to orbit the Galactic Center. In comparison, our Sun needs over 200 million years for this. S2 approaches the center at an extremely small distance and accelerates to speeds that are difficult to imagine in earthly conditions." "S2 potrzebuje zaledwie 16 lat, by okrążyć Centrum Galaktyki. Dla porównania nasze słońce potrzebuje na to ponad 200 milionów lat. S2 zbliża się do centrum na ekstremalnie małą odległość i rozpędza się do prędkości, które trudno sobie wyobrazić w ziemskich warunkach."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
✅ Factual claim 🔹 Other AI assessment confidence: 100% Source on YouTube

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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

…Nie widzimy samej czarnej dziury, no bo jak sama nazwa wskazuje jest czarna. Ale widzimy co robi z otoczeniem. Obserwujemy gwiazdy, które krążą wokół tego punktu z zawrotnymi prędkościami. Najsłynniejszą z nich jest gwiazda oznaczona symbolem S2. To ona jest naszym głównym świadkiem koronnym w procesie przeciwko Sagittariusowi az gwiazdką. S2 potrzebuje zaledwie 16 lat, by okrążyć Centrum Galaktyki. Dla porównania nasze słońce potrzebuje na to ponad 200 milionów lat. S2 zbliża się do centrum na ekstremalnie małą odległość i rozpędza się do prędkości, które trudno sobie wyobrazić w ziemskich warunkach. Z ruchu gwiazdy S2 i jej towarzyszek możemy wyciągnąć twarde dane. Jeśli znamy orbitę i prędkość obiektu, to możemy wyliczyć masę tego, co go przyciąga. I te wyliczenia mówią jasno: w tym małym punkcie musi siedzieć coś, co waży tyle, co 4 miliony naszych słońc. Mamy więc obiekt, który jest bardzo masywny, bardzo mały i bardzo ciemny. W tym momenc…

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