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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.
What else can I help you with?
Where did planets made mostly of gas and ice form within the protoplanetary disk?
Planets made mostly of gas and ice, known as gas giants and ice giants, typically formed in the outer regions of the protoplanetary disk. These areas were cooler, allowing volatile compounds like water, ammonia, and methane to condense into solids, which contributed to the formation of larger cores. As these cores grew, they could capture surrounding gas, leading to the development of massive atmospheres. In contrast, the inner regions of the disk, where temperatures were higher, favored the formation of rocky planets.
Are planets formed from the same clouds of gas and dust as stars?
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.
What is it called when planets are formed?
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.
What is the term that means planets in the making?
The term that refers to planets in the making is "protoplanets." Protoplanets are large bodies that form within a protoplanetary disk and can eventually collide and merge to create full-sized planets. They are a crucial stage in the process of planetary formation.
What is the compact gas and dust that became a planet?
A protoplanetary disk is a concentration of gas and dust around a young star that eventually comes together to form planets. As the material in the disk begins to clump together due to gravity, it forms planetesimals which then grow into planets through accretion and collisions.
How did Uranus form?
As best we know, the same way all the other planets did: accretion of objects in a protoplanetary disk.
Where did planets made mostly of gas and ice form within the protoplanetary disk?
Planets made mostly of gas and ice, known as gas giants and ice giants, typically formed in the outer regions of the protoplanetary disk. These areas were cooler, allowing volatile compounds like water, ammonia, and methane to condense into solids, which contributed to the formation of larger cores. As these cores grew, they could capture surrounding gas, leading to the development of massive atmospheres. In contrast, the inner regions of the disk, where temperatures were higher, favored the formation of rocky planets.
Collided to form planets?
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.
What will the protoplanetary disks eventually become?
That depends what the disk is forming round. If it is a large black hole it will form a quasar, if it is round a star, it will form planets (a solar system).
Are planets formed from the same clouds of gas and dust as stars?
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.
How do temperature differences in the protoplanetary disk the arrangement of the planets?
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.
What is it called when planets are formed?
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.
What is the term that means planets in the making?
The term that refers to planets in the making is "protoplanets." Protoplanets are large bodies that form within a protoplanetary disk and can eventually collide and merge to create full-sized planets. They are a crucial stage in the process of planetary formation.
What is the compact gas and dust that became a planet?
A protoplanetary disk is a concentration of gas and dust around a young star that eventually comes together to form planets. As the material in the disk begins to clump together due to gravity, it forms planetesimals which then grow into planets through accretion and collisions.
Explain why the material surrounding a young star forms a disk?
The prograde rotation of the collapsing cloud of gas and dust results in conservation of angular momentum, causing the material to flatten into a disk shape. This disk of material, known as a protoplanetary disk, is where planets are thought to form through the process of accretion and gravitational interactions.
Why are the inner planets closer to each other?
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.
What begins to take shape in the center of nebular?
In the center of a nebula, gas and dust begin to collapse due to gravitational forces, forming a swirling disc known as a protoplanetary disk. Within this disk, material gradually accumulates and clumps together to form planetesimals, which are the building blocks of planets.
