Spiral galaxy.
Clouds of gas and dust in which stars form are called nebulae. These regions of space are where the raw materials for star formation gather and eventually collapse under their own gravity to give birth to new stars.
This disk of dust and gas that formed the sun and planets is called the solar nebula. It is a rotating cloud of gas and dust left over from the formation of a star. Over time, the particles in the nebula began to clump together and form planetesimals, eventually leading to the formation of planets.
The dust and gas located between stars in a galaxy is called the interstellar medium (ISM). This material plays a crucial role in the formation of new stars and planets within the galaxy.
Stars. That is how stars are formed. They form from nebulae.
The birthplace for stars is called a stellar nursery. These nurseries are regions within galaxies where gas and dust condense to form new stars.
No. The clouds of gas and dust are called nebulae. A quasar is a disk of superheated matter falling into an enormous black hole.
Yes, the solar system including our Sun and planets is believed to have formed from a large disk of gas and dust called a proto-disk or proto-solar disk, due to gravitational effects. It is currently thought that several stars formed from the same cloud as our Sun.
Molecular clouds
Yes, planets are formed from the same clouds of gas and dust as stars. These clouds are called molecular clouds, and they consist mostly of hydrogen and helium along with other elements. As the cloud collapses under gravity to form a star, leftover material congregates to form planets and other smaller bodies in the newly formed solar system.
The gases and dust from which stars condense are called cosmic dust or particles.
A galaxy contains stars, gas and dust. In a spiral galaxy like the Milky Way, the stars, gas, and dust are organized into a "bulge," a "disk" containing "spiral arms," and a "halo." Elliptical galaxies have a bulge-like central region and a halo, but do not have a disk.
It is called a stellar nebula.
Clouds of gas and dust in which stars form are called nebulae. These regions of space are where the raw materials for star formation gather and eventually collapse under their own gravity to give birth to new stars.
Which of the following statements correctly summarize key differences between the disk and the halo?Answer:Clusters of young stars are found only in the disk.Stars in the disk all orbit in the same direction and nearly the same plane, while halo stars have more randomly oriented orbits.Gas and dust are abundant in the disk but not in the halo.Disk stars come in a broad range of masses and colors, while halo stars are mostly of low mass and red.
Stars in the disk all orbit in the same direction and nearly the same plane, while halo stars have more randomly oriented orbits.Clusters of young stars are found only in the disk.Disk stars come in a broad range of masses and colors, while halo stars are mostly of low mass and red.Gas and dust are abundant in the disk but not in the halo.
They get enegry by giant clouds of dust called nebulae.
This disk of dust and gas that formed the sun and planets is called the solar nebula. It is a rotating cloud of gas and dust left over from the formation of a star. Over time, the particles in the nebula began to clump together and form planetesimals, eventually leading to the formation of planets.