The models showed that the stars located near the center were traveling in quick...

📅 17.06.2026 · Czarna dziura 10x masywniejsza niż cała galaktyka. Jaki... · 👁️ 10

✓ True

True. Recent studies (published in 2025) on the dwarf galaxy Segue 1 indicate the presence of a central black hole with a mass significantly exceeding that of all the galaxy's stars. Dynamical models that best fit observations...

"The models showed that the stars located near the center were traveling in quick, tight circles, which is a tell-tale sign of an immense gravitational pull generated by a black hole. Additional support for a central black hole comes from a significant increase in the central rotation. Using individual velocities, we measure a rotation amplitude of 9.0 ± 2.4 km s−1." "Segułę 1 wykazuje gigantyczne anomalie w swojej wewnętrznej kinematyce, w tym jak porusza się wszystko w jej wnętrzu, które to bezpośrednio wspierają teorie o istnieniu centralnej czarnej dziury. Precyzyjne pomiary prędkości poszczególnych gwiazd pokazały bardzo gwałtowny wzrost rotacji w samym centrum tej galaktyki."

🌐 (Machine-translated — original in Polish) · Original in Polishuage

✅ Factual claim 🔹 Other AI assessment confidence: 90% Source on YouTube

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Oryginał w języku Polskim Open on YouTube

…laktyce SEG1 mogło dojść do gwałtownej, naddźwiękowej akrecji, która przekraczała tę barierę. Supermasowna czarna dziura mogła powstać niemal błyskawicznie, zanim galaktyka w ogóle zdołała wyprodukować większą populację gwiazd. No i tam sobie już po prostu zeżarła co zeżreć miała. Kolejnym niezwykle ważnym elementem tej układanki jest też fakt, że Segułę 1 wykazuje gigantyczne anomalie w swojej wewnętrznej kinematyce, w tym jak porusza się wszystko w jej wnętrzu, które to bezpośrednio wspierają teorie o istnieniu centralnej czarnej dziury. Precyzyjne pomiary prędkości poszczególnych gwiazd pokazały bardzo gwałtowny wzrost rotacji w samym centrum tej galaktyki. Amplituda tej rotacji w odległości no niespełna półtora minuty łuku od jądra, więc bardzo blisko w skali galaktycznej osiąga wartość aż 9 km/s, a w jeszcze ciaśniejszych obszarach wzrasta nawet do 14 km/s. I biorąc pod uwagę, że ogólna dyspersja prędkości dla całego tego układu wynosi zaledwie około 4 km/s, no to tak gigantyczny skok prędkości w c…

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Piotr Kosek: "The models showed that the stars located near the center were traveling in quick, tight circles, which is a tell-tale sign of an immense gra..." — True

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