"The halo primarily contains individual old stars and clusters of old stars ("globular clusters"). It may be over 130,000 light years across. The halo also contains "dark matter," which is material that we cannot see but whose gravitational force can be measured." to shorten the answer - individual stars, clusters, and dark matter.
The collection of ancient stars found in the center of the Local Group is called the Galactic Halo. The Galactic Halo is a spherical region of space that surrounds the disk of the Milky Way galaxy. It is made up of old, metal-poor stars that are thought to have formed very early in the history of the Milky Way. The Galactic Halo is also home to globular clusters, which are dense groups of hundreds of thousands of stars. The Galactic Halo is thought to be the remnant of a smaller galaxy that merged with the Milky Way billions of years ago. The merger caused the smaller galaxy to be torn apart, and its stars were scattered into the Galactic Halo. The Galactic Halo is a very sparsely populated region of space. The stars are so far apart that they are difficult to see individually with the naked eye. However, the Galactic Halo can be seen in the night sky as a faint glow of light.
Oh, that's a gentle question, friend! Stars aren't forming in the galactic halo mainly because the halo contains older stars and less of the materials needed for new stars to form compared to the galaxy's disk. Remember, even in the stillness of the halo, the universe twinkles with endless possibilities elsewhere!
Most Population II stars are found in the halo of the Milky Way galaxy, particularly in globular clusters and the surrounding stellar halo. These stars are typically older, metal-poor, and represent an early stage of star formation in the galaxy. While they can also be found in the bulge, the halo is their primary region, as it contains the remnants of ancient stellar populations formed before the galaxy's disc structure developed.
Scientists determine the Milky Way's mass outside the Sun's orbit by observing the motions of stars and gas in the galaxy and using gravitational models to calculate the total mass that is needed to hold these objects in their orbits. This method allows for estimating the mass of the Milky Way's dark matter halo, which makes up the majority of its mass.
The Milky Way galaxy is a spiral galaxy with a central bulge, a disk made up of arms of gas, dust, and stars, and a halo of globular clusters. The central bulge contains older stars, while the disk is where younger stars are formed. The galaxy is surrounded by a halo of dark matter that extends beyond the visible components.
In the Milky Way galactic halo, orbiting the galactic center in a long elliptical orbit around the galactic center
The collection of ancient stars found in the center of the Local Group is called the Galactic Halo. The Galactic Halo is a spherical region of space that surrounds the disk of the Milky Way galaxy. It is made up of old, metal-poor stars that are thought to have formed very early in the history of the Milky Way. The Galactic Halo is also home to globular clusters, which are dense groups of hundreds of thousands of stars. The Galactic Halo is thought to be the remnant of a smaller galaxy that merged with the Milky Way billions of years ago. The merger caused the smaller galaxy to be torn apart, and its stars were scattered into the Galactic Halo. The Galactic Halo is a very sparsely populated region of space. The stars are so far apart that they are difficult to see individually with the naked eye. However, the Galactic Halo can be seen in the night sky as a faint glow of light.
It is not. On the other hand, the Milky way sun creates the halo. When you see milky from above, it is diffucult to notice the halo. If you shift or rotate the view, you can see that the Milky way halo is a cicurference with the sun in the center and it covers all planets circling this sun. The term galactic halo is used to denote an extended, roughly spherical component of a galaxy, which extends beyond the main, visible component. It can refer to any of several distinct components which share these properties
the halo
Globular star clusters are members of the Milky Way galaxy. They are dense, spherical collections of stars that orbit the galactic center. These clusters contain thousands to millions of ancient stars and are typically found in the galactic halo.
A nebula is found in interstellar space.Globular cluster is the one found in a spherical halo that surrounds a spiral galaxy and open cluster is the one usually found along a galaxy's spiral disk.
Palomar 1 is located in the Milky Way galaxy's halo, not in the spiral arms. It is a globular cluster, which is a spherical collection of stars orbiting the galactic core.
ya my but hole
Oh, that's a gentle question, friend! Stars aren't forming in the galactic halo mainly because the halo contains older stars and less of the materials needed for new stars to form compared to the galaxy's disk. Remember, even in the stillness of the halo, the universe twinkles with endless possibilities elsewhere!
Most Population II stars are found in the halo of the Milky Way galaxy, particularly in globular clusters and the surrounding stellar halo. These stars are typically older, metal-poor, and represent an early stage of star formation in the galaxy. While they can also be found in the bulge, the halo is their primary region, as it contains the remnants of ancient stellar populations formed before the galaxy's disc structure developed.
study
The ones in the bulge or halo are older star, the ones in the disk are younger.