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mersecske
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Are there any big difference of star distribution and H-atom distribution in the Milky Way on large scale (larger scale than starts)?
The Milky Way is a spiral galaxy that contains our Solar System. It is estimated to be around 13.51 billion years old and is home to about 200-400 billion stars.
The stars in the Milky Way are not evenly distributed. They are mostly concentrated in the galactic disk, with a smaller number in the central bulge and the outer halo. The distribution of stars is affected by the galaxy's rotation and gravitational forces.
The H-atom distribution in the Milky Way is used to map the galaxy's structure and measure its mass. It is estimated that about 70% of the galaxy's mass is made up of hydrogen atoms, which are mainly located in the spiral arms of the galaxy.
Scientists use various techniques such as radio telescopes, infrared imaging, and spectroscopy to study the distribution of stars and H-atoms in the Milky Way. They also use computer simulations to model the galaxy's structure and evolution.
The Milky Way is a typical spiral galaxy, and its star and H-atom distribution is similar to that of other spiral galaxies. However, it is unique in its size and mass, and it also has a relatively high rate of star formation compared to other galaxies.