Far enough from the new Sun that they did not "evaporate". In other words, towards the outer rim of the main part of the disk.
Most of the material from the protoplanetary disk that formed our solar system ended up in the Sun and the eight planets, along with various moons, asteroids, and comets. The inner planets are made mostly of rock and metal, while the outer planets are composed mostly of gases and ice.
Planets are formed from a disk of gas and dust surrounding a young star known as a protoplanetary disk. Over time, the particles within the disk collide and stick together, gradually forming larger and larger objects. Eventually, these objects grow into planetesimals, which further accrete material to become planets.
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.
Planets are formed through a process called accretion, where dust and gas in a planetary disk gradually come together to form larger and larger bodies. Gravitational forces eventually cause these bodies to collide and merge, leading to the formation of planets.
By "accretion" of "planetesimals" from the "protoplanetary disk".
Far enough from the new Sun that they did not "evaporate". In other words, towards the outer rim of the main part of the disk.
Most of the material from the protoplanetary disk that formed our solar system ended up in the Sun and the eight planets, along with various moons, asteroids, and comets. The inner planets are made mostly of rock and metal, while the outer planets are composed mostly of gases and ice.
Dust and gas particles in a protoplanetary disk collided and stuck together to form planetesimals, which then collided and accreted to form planets. The process of gravitational attraction and collisions led to the formation of larger bodies within the disk, eventually forming planets.
As best we know, the same way all the other planets did: accretion of objects in a protoplanetary disk.
Jupiter is the biggest simply because it got the most stuff out of the "protoplanetary" disk from which the planets formed.
The protostellar disk is very hot and only rocks and metal can combine together in that heat, so that makes the inner planets. In the outer disk it is very cold, so there are only ice and dust particles able to combine together, there are though rock centers in the outer planets but ice and gas make up the majority: that makes the outer planets.
it is exactly protoplanetary disk.
Temperature differences in the protoplanetary disk can lead to variations in the composition and distribution of materials, impacting the formation of different types of planets. For instance, inner, hotter regions may favor the formation of rocky planets, while outer, colder regions may support the formation of gas giants. These temperature variations can influence the presence of volatile elements and compounds in different parts of the disk, which in turn affects the types of planets that can form.
Planets are formed from a disk of gas and dust surrounding a young star known as a protoplanetary disk. Over time, the particles within the disk collide and stick together, gradually forming larger and larger objects. Eventually, these objects grow into planetesimals, which further accrete material to become planets.
A disk of gas ad dust that forms round a proto-star as the star coalesces at the center and from which planets accurate. The related links below give more information.
The inner planets (Mercury, Venus, Earth, and Mars) are closer to each other because they formed from a protoplanetary disk closer to the Sun. The gravitational forces and interactions within the disk caused these planets to form in closer proximity compared to the outer planets.