The theory that explains the formation of planets through the condensing of a solar nebula is known as the Solar Nebula Theory. According to this theory, the solar system originated from a rotating cloud of gas and dust, known as the solar nebula. As the nebula collapsed under its gravity, it spun faster and flattened into a disk, allowing particles to collide and stick together, eventually forming larger bodies that became the planets. This process highlights the role of gravity and angular momentum in the formation of celestial bodies.
The Nebular Theory suggests that celestial objects, such as stars and planets, formed from a rotating cloud of gas and dust, known as a nebula. As the nebula cooled and contracted under gravity, it began to clump together, leading to the formation of solid particles, which eventually coalesced into larger bodies. This process explains the formation of solar systems and the arrangement of planets around stars.
B. The young sun's solar winds pushed gases outward to the outer solar system.
The nebular hypothesis is a widely-accepted theory that explains the formation of the solar system. It suggests that the Sun and planets formed from a spinning disk of gas and dust called a solar nebula. As the nebula contracted due to gravity, it flattened into a disk and the Sun formed at the center, while planets and other celestial bodies formed from material in the disk.
The nebular model explains how our solar system formed from a rotating cloud of gas and dust called a solar nebula. Gravity caused the nebula to collapse, forming a central protostar surrounded by a spinning disk. Over time, the material in the disk clumped together to form planets and other solar system bodies.
A meteorite is a piece of rock that is similar to the material formed into planets. Meteorites are remnants from the early solar system that can provide insights into the processes that formed the planets.
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The Nebular Theory suggests that celestial objects, such as stars and planets, formed from a rotating cloud of gas and dust, known as a nebula. As the nebula cooled and contracted under gravity, it began to clump together, leading to the formation of solid particles, which eventually coalesced into larger bodies. This process explains the formation of solar systems and the arrangement of planets around stars.
A dipeptide is the molecule formed by condensing only two amino acids together.
B. The young sun's solar winds pushed gases outward to the outer solar system.
the sun was bigger and brghter then gave birth to four gas planets then rocky ones and probable give birth again our system is getting larger the planets lining up just might do that 26000 104000 104000000 anamate solar system in reverse its possibe
The nebular hypothesis is a widely-accepted theory that explains the formation of the solar system. It suggests that the Sun and planets formed from a spinning disk of gas and dust called a solar nebula. As the nebula contracted due to gravity, it flattened into a disk and the Sun formed at the center, while planets and other celestial bodies formed from material in the disk.
The planets formed by ice would be Jupiter and Saturn!!......I think.............;)
A condensing agent is a substance or reagent that promotes a condensation reaction, where two molecules combine to form a larger molecule with the elimination of a smaller molecule. It accelerates the reaction by aiding in the removal of the byproduct formed during the reaction. Common condensing agents include dehydrating agents like sulfuric acid or acetic anhydride.
Planets in the solar system are thought to have formed from a giant rotating disk of gas and dust around the young Sun, known as the solar nebula. Small particles in this disk collided and stuck together, gradually growing into planetesimals and eventually forming protoplanets and then fully-fledged planets through accretion and gravitational interactions.
The protoplanet nebular model explains the differences between terrestrial and giant planets primarily through their formation regions within the solar nebula. Terrestrial planets formed closer to the Sun, where higher temperatures allowed only metals and silicates to condense, resulting in smaller, rocky bodies. In contrast, giant planets formed farther out, where cooler temperatures enabled the accumulation of ices and gases, leading to the formation of large, gaseous envelopes around solid cores. This gradient in temperature and composition during the solar system's formation accounts for the distinct characteristics of the two types of planets.
The planets formed out of the solar nebular there is no concept of the "first" they all formed slowly at the same time.
The nebular model explains how our solar system formed from a rotating cloud of gas and dust called a solar nebula. Gravity caused the nebula to collapse, forming a central protostar surrounded by a spinning disk. Over time, the material in the disk clumped together to form planets and other solar system bodies.