2.1 Solar nebular model Flashcards
When was the Big Bang?
14 billion years ago (14 Ga)
When was the solar system formed?
4.6 billion years ago (4.6 Ga)
What is a nebula?
A giant cloud of molecular hydrogen and dust.
What happened to the nebula to begin the creation of the solar system?
It collapsed, possibly due to the shockwave from a nearby exploding star) and became denser.
What is a protoplanetary disc?
A rotating flat gaseous cloud that was created due to the collapse of the solar nebula.
What occurred as a result of the heat and high density occurring at the centre of the protoplanetary disc?
It triggered nuclear fusion, increasing the temperature of the surface of the star at the centre of the protoplanetary disc.
What is meant by the term accretion?
An increase in mass by the addition of material e.g. by rocky particles colliding.
What is a planetesimal?
A small body of rocky material that has been created by gravitational and electrostatic forces. They are around 1 km in diameter.
What is a protoplanet?
It forms when planetesimals accrete (join together). They are approximately the size of the moon.
Approximately how long did it take for protoplanets to collide and form the terrestrial planets?
Up to 1 billion years.
Why did giant gas planets form in the outer reaches of the solar system?
They formed from the less dense elements that was sent further away from the sun when it collapsed and produced a shockwave.
What are asteroids?
The left over planetesimals that did not form planets.
What are meteorites?
Fragments of asteroids.
How did the moon form?
A protoplanet impacted the young Earth between 30 and 50 million years after the formation of the Solar System.
What assumption do we have to make in order to use meteorites as evidence for the Earth’s composition and structure?
All the material in the Solar System originated from the same source.