
Dust Obscured Black Hole Mass: JWST Recalibration
JWST observations reveal dust obscured a black hole (LID-568), leading to overestimation of its mass and accretion rate. Recalculation using infrared light provides a more accurate mass estimation.
JWST observations reveal dust obscured a black hole (LID-568), leading to overestimation of its mass and accretion rate. Recalculation using infrared light provides a more accurate mass estimation.
For instance, a surface covered in the black rock basalt would hint at the presence of volcanoes, like on many planets in our solar system.