out side technically it is not inside
the spiral galaxy is very bright because of its stars, that's why our galaxy is called the milky way because it looks milky and our galaxy(the milky way) is located in one of the arms of a spiral galaxy!
Our galaxy, the Milky Way, is a spiral galaxy. It consists of a central bulge surrounded by spiral arms that contain stars, gas, and dust. We are located on one of the outer arms of the galaxy.
A galaxy is a huge group of stars that form a spreading spiral. Our own Milky Way galaxy is an example of a spiral galaxy.
The Milky Way is a spiral galaxy, more specifically a "barred spiral galaxy" in which some stars are located in a horizontal band across the nucleus, rather than in the spiral arms.
Globular Cluster.
Globular Cluster.
Ionization nebulae in the galaxy M51 are predominantly located in the spiral arms of the galaxy. These regions are where massive, young stars are found, which emit high-energy ultraviolet radiation that ionizes the surrounding gas, creating the colorful nebulae. The ionization nebulae are often observed in regions of active star formation within the galaxy.
New stars are typically found in the spiral arms of a spiral galaxy. This is because the density of gas and dust is higher in the arms, creating the conditions necessary for star formation to occur. The gravitational forces within the spiral arms also play a role in triggering the collapse of gas clouds into new stars.
The Milky Way galaxy has spiral arms where a lot of new stars are being born, including the Orion Arm where our solar system is located. These spiral arms are regions of higher density that promote the formation of new stars due to gravitational interactions between gas and dust.
Nebulae are located within the spiral arms of spiral galaxies. These regions are areas of star formation where gas and dust clouds collide and condense, leading to the birth of new stars. The glowing gas and dust of nebulae can be seen as colorful patches within the spiral arms of galaxies like the Milky Way.
Ionization nebulae are predominantly located within spiral galaxies, often in regions of active star formation such as in the arms and central regions of the galaxy. They are also commonly found around hot, massive stars that emit enough energy to ionize the surrounding gas.
A flattened combination of matter containing stars, gas, and dust in a spiral galaxy is identified as the galaxy's disk. This disk is where most of the galaxy's star formation occurs and contains the majority of its stars and interstellar material. The spiral arms within the disk are regions of higher density that enhance star formation.