NGC 3521
The presence of dark matter within NGC 3521 contributes to the overall mass distribution and stability of the galaxy. It is hypothesized that dark matter forms an invisible halo around the galaxy, providing additional gravitational force that holds the spiral arms together and maintains their flocculent appearance. The interplay between dark matter and visible components such as stars, gas, and dust may also contribute to the intermediate nature of NGC 3521's spiral structure.
SPECIFICATIONS
Telescope
..........................................................................................................................................................................................................................
Camera
..........................................................................................................................................................................................................................
Location
..........................................................................................................................................................................................................................
Date of observation
..........................................................................................................................................................................................................................
Date of observation
Between 24-01-12 and 24-02-09
Filters
..........................................................................................................................................................................................................................
Processing
..........................................................................................................................................................................................................................
