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What percentage of the mass of the solar nebula consisted of elements other than hydrogen and helium?
Roughly 2% of the mass of the solar nebula consisted of elements other than hydrogen and helium. These elements include heavier elements like carbon, oxygen, and iron that were essential for the formation of planets and other celestial bodies.
The solar nebula was 98?
The solar nebula was a rotating cloud of gas and dust that formed our solar system about 4.6 billion years ago. It consisted mostly of hydrogen and helium, with traces of other elements. Over time, gravity caused the nebula to collapse and form the Sun and the planets.
What are the three major components of the solar nebula?
The three major components of the solar nebula are hydrogen, helium, and heavier elements or compounds. Hydrogen and helium account for the majority of the nebula's mass, while heavier elements, often referred to as "metals" in astrophysics, contribute to the formation of solid materials such as dust and ice. These components played a crucial role in the formation of the Sun and the planets in our solar system.
What were the three most common substances present in the solar nebula?
The three most common substances present in the solar nebula were hydrogen, helium, and small amounts of heavier elements such as carbon, oxygen, and nitrogen. Hydrogen and helium comprised the majority of the nebula's mass, accounting for about 98% of it. These elements formed the primordial gas from which the Sun and the solar system developed. The heavier elements, produced in earlier generations of stars, contributed to the formation of planets and other celestial bodies.
Is the solar nebular made up of mostly carbon and iron?
No, the solar nebula was primarily composed of hydrogen and helium, with trace amounts of other elements like carbon and iron. The solar system formed from the gravitational collapse of this nebula, leading to the formation of the Sun and planets.
What percentage of the mass of the solar nebula consisted of elements other than hydrogen and helium?
Roughly 2% of the mass of the solar nebula consisted of elements other than hydrogen and helium. These elements include heavier elements like carbon, oxygen, and iron that were essential for the formation of planets and other celestial bodies.
The solar nebula was 98?
The solar nebula was a rotating cloud of gas and dust that formed our solar system about 4.6 billion years ago. It consisted mostly of hydrogen and helium, with traces of other elements. Over time, gravity caused the nebula to collapse and form the Sun and the planets.
What is the difference in between nebula and solar nebula?
A solar nebula is related to the formation of our Solar System, any other nebula is just a nebula.
What are the three major components of the solar nebula?
The three major components of the solar nebula are hydrogen, helium, and heavier elements or compounds. Hydrogen and helium account for the majority of the nebula's mass, while heavier elements, often referred to as "metals" in astrophysics, contribute to the formation of solid materials such as dust and ice. These components played a crucial role in the formation of the Sun and the planets in our solar system.
What were the three most common substances present in the solar nebula?
The three most common substances present in the solar nebula were hydrogen, helium, and small amounts of heavier elements such as carbon, oxygen, and nitrogen. Hydrogen and helium comprised the majority of the nebula's mass, accounting for about 98% of it. These elements formed the primordial gas from which the Sun and the solar system developed. The heavier elements, produced in earlier generations of stars, contributed to the formation of planets and other celestial bodies.
Is the solar nebular made up of mostly carbon and iron?
No, the solar nebula was primarily composed of hydrogen and helium, with trace amounts of other elements like carbon and iron. The solar system formed from the gravitational collapse of this nebula, leading to the formation of the Sun and planets.
How was your solar system produced?
The solar system was produced by solar nebula. The nebula was disrupted by an unknow substance in the air.
What is the first step in building a solar system from solar nebula?
an explosion disturbs the dust in the nebula
What causes a solar nebula initially begin to form a solar system?
An explosion from outside the nebula
Percentage of the solar nebula's mass consisted of rocky material?
Roughly 1-2% of the solar nebula's mass consisted of rocky material. The majority of the nebula's mass was composed of hydrogen and helium, with smaller amounts of other elements like carbon, oxygen, and nitrogen. These rocky materials eventually accumulated to form the terrestrial planets in our solar system.
What percentage of the solar nebula's mass consisted of hydrogen and helium gases?
Roughly 98% of the solar nebula's mass consisted of hydrogen and helium gases. These two elements are the most abundant in the universe and are the primary components of stars like our sun.
What nebula was the sun created in?
The Solar Nebula, which does not exist anymore.
