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If we know the orbit and speed of an object, we can calculate the mass of what a...

Piotr Kosek: "If we know the orbit and speed of an object, we can calculate the mass of what attracts it. And these calculations clearly state: in this sm..." — True

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📅 06.03.2026 · Sagittarius A* to nie czarna dziura? Niepokojąca hipote... · 👁️ 3

True. The claim is true. Calculating the mass of a central object based on the orbit and speed of bodies orbiting it is a fundamental principle of celestial mechanics, derived from Kepler's laws and Newton's law of universal g...

"If we know the orbit and speed of an object, we can calculate the mass of what attracts it. And these calculations clearly state: in this small point, there must be something that weighs as much as 4 million of our suns." "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."
🌐 (Machine-translated — original in Polish) · Original in Polishuage
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Transcript excerpt

Oryginał w języku Polskim Open on YouTube

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 momencie na scenę wchodzi ogólna teoria względności. Jest ona naszą najlepszym drogowskazem po grawitacji we wszechświecie. I według tej teorii, jeśli upchamy tak wielką masę w tak małej objętości, to materia nie wytrzyma. Zapadnie się pod własną masą do punktu o niesk

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