Spiral Galaxy Messier 81, located on the northern constellation of Ursa Big, and has a mass of black holes about 68 million times the sun.
Scientists have relied on it to carry out new research and discover an unexpectedly strong connection between mass black holes and spiral branch geometry. At the same time, they also predict that lower mass black holes in the galaxy will have open spiral arms.
The power of this relationship makes it possible for anyone to assess how black the hole behind a large spiral galaxy looks at its image. This is a better method than any other method used to predict the previous black hole mass.
By looking at the different levels of tightness of the spiral arms, the masses of the central black hole and the corresponding galaxy in the mass units of the galaxy estimate the masses of black holes in the spiral galaxy.
This method also allows to predict the mass of black holes in pure galaxies with bulging segments filled with constellations.
Based on the relationship between black hole mass and spiral branch geometry, scientists can also study medium mass black hole communities (about 100 to 100,000 times larger than the sun), losing calculus at the present time. They have a much larger mass than any single star, but are smaller than huge black holes and billions of times heavier than our Sun.