After a nebula, the next stage in the life cycle of a star is usually a protostar, where gravity causes the gas and dust within the nebula to begin collapsing and forming a dense core. Following this stage, the protostar may evolve into a main sequence star, where nuclear fusion begins in its core and it enters a stable period of energy production.
Gravity is the force responsible for pulling particles within a nebula together. As particles within the nebula are attracted to each other by gravity, they gradually collapse and become more compact, eventually leading to the formation of stars and planets.
A nebula develops into a solar system through the process of gravitational collapse. As the nebula contracts due to gravity, it starts to spin and flatten into a spinning disk. Within this disk, the material begins to clump together and form planetesimals, which eventually coalesce to form planets, moons, and other objects in the solar system.
A nebula is a cloud of gas and dust in outer space. These formations can be the birthplaces of stars or remnants of dying stars. Nebulae are commonly observed by astronomers and can come in various shapes and sizes.
This describes a nebula, which is a vast cloud of gas and dust in space where stars are born. The gases and dust within a nebula are the raw materials that eventually come together under gravity to form new stars.
A nebula typically consists of gas, dust, and plasma. These elements come together in space to form vast clouds of various shapes and sizes. Nebulae are often where new stars are born.
the sky
Which Nebula? Astronomically speaking, no it does not. In our lifetime, we will not come anywhere near to a nebula. If your thinking of the Andromeda Galaxy then - well expect galactic fireworks - but not for about 3 billion years. [See related question]
Yes, Nebula's die. They die when they get to close to Black Holes.
Musa comes from the Harmonic Nebula.
It condensed from the interstellar nebula form which our star, the Sun, was formed.
The Crab Nebula is a nebula.
nebula
Gravity is the force responsible for pulling particles within a nebula together. As particles within the nebula are attracted to each other by gravity, they gradually collapse and become more compact, eventually leading to the formation of stars and planets.
A nebula develops into a solar system through the process of gravitational collapse. As the nebula contracts due to gravity, it starts to spin and flatten into a spinning disk. Within this disk, the material begins to clump together and form planetesimals, which eventually coalesce to form planets, moons, and other objects in the solar system.
The Stingray Nebula (Hen 3-1357) is a planetary nebula. (The youngest known).
There isn't 'an' Eagle Nebula. There is 'the' Eagle Nebula. This is just the familiar name for a large cloud surrounding the Open Cluster M16. Nebulae come in all conceivable shapes and sizes, so they are all different from each other!
A nebula is a cloud of gas and dust in outer space. These formations can be the birthplaces of stars or remnants of dying stars. Nebulae are commonly observed by astronomers and can come in various shapes and sizes.