Big Bang to Earth's Formation Concept Map

Slides:



Advertisements
Similar presentations
Life cycle of stars Nebulae to supernova.
Advertisements

A journey to the stars.
The Solar System and our Universe
Life Cycle of Stars 1st Step: Stars form from nebulas
Life Cycle of Stars. Omega / Swan Nebula (M17) Stars are born from great clouds of gas and dust called Stars are born from great clouds of gas and dust.
Star Life Cycle.
A star is born… A star is made up of a large amount of gas, in a relatively small volume. A nebula, on the other hand, is a large amount of gas and dust,
Star Life Cycle.
Life Cycle of Stars. Birth of a Star Born from interstellar matter (dust & gases) – Denser portions of the nebula Nebula begins to contract – Due to gravity.
The Life Cycle of a Star.
Solar System. What is the Solar System? Consists of a star, (like the sun) and all of the planets, moons and other bodies that travel around it. Planets.
View from the top of the Flatirons (Boulder, CO)
The Earth and Beyond.
1 Chapter 2 Creation of Oceans. 2 Supporting Evidence for the Big Bang Edwin Hubble discovered spreading of galaxies. Cosmic background radiation (the.
NOT THOSE TYPES OF STARS! LIFE CYCLE OF STARS WHAT IS A STAR? Star = ball of plasma undergoing nuclear fusion. Stars give off large amounts of energy.
How our Solar System (and Moon) came to be…. Learning Objectives Be able to explain – How our solar system and moon came to be.
Lives of stars.
Pictures for life death of solar system. Nebulas.
By Ryan and Mike. How stars are formed There are two main models of star formation. Gravitational collapse is a process when molecular clumps that are.
SOLAR SYSTEM AND STAR FORMATION. Solar System and Star Formation  Both happen at the same time, but we’ll look at the two events separately.
Stellar Life Stages Star Birth and Death.
Birth and Life of a Star What is a star? A star is a really hot ball of gas, with hydrogen fusing into helium at its core. Stars spend the majority of.
Earths Place in the Universe. Standard 2a and 2b Students know the solar system is located in an outer edge of the disc- shaped Milky Way Galaxy, which.
Formation of our solar system: The nebular hypothesis (Kant, 1755) Hydrogen (H), He (He) and “stardust” (heavier elements that were formed in previous.
1 Stellar Lifecycles The process by which stars are formed and use up their fuel. What exactly happens to a star as it uses up its fuel is strongly dependent.
What causes day and night? (Please get this right…) What causes day and night? (Please get this right…) Do you see different stars at night here than you.
THE BIG BANG This model suggests that somewhere around 13.7 billion years ago all matter in the Universe was contained in a hot, dense particle. The temperature.
THE BIG BANG Theory… How did the universe begin?.
Stars.
The Life Cycle of a Star The Horsehead Nebula – one of the most famous pictures in astronomy.
Life Cycle of Stars Birth Place of Stars:
Galaxies The basic structural unit of matter in the universe is the galaxy A galaxy is a collection of billions of _____________, gas, and dust held together.
The Sun-Earth-Moon System. What is the moon? The moon is a natural satellite of Earth This means that the moon orbits Earth.
Solar System Video: 1 How it Formed.
The Star Cycle. Birth Stars begin in a DARK NEBULA (cloud of gas and dust)… aka the STELLAR NURSERY The nebula begins to contract due to gravity in.
 At one time, the universe was a dense, hot, supermassive ball.  About 13.7 billion years ago, a violent explosion occurred sending material in all directions.
 There was nothing Billion Years Ago  Energy expanded out from a single point called a singularity.  Really HOT  No matter yet (no atoms)
The Life Cycle of Stars.
Stars Huge spheres of very hot gas that emit light and other radiation. They are formed from clouds of dust and gas, or nebulas, and go through different.
AQA Science © Nelson Thornes Ltd P3 4 Summary Stars and space Corel 768 (NT)
The Big Bang! ESCI 518 Fall Origins How and when did the: How and when did the: universe form? universe form? solar system / Earth form? solar system.
 How Stars Form: -The space around stars contains gas/dust  A nebula is a large cloud of dust/gas, some nebulas glow lit by other stars and some are.
The Life History of Stars How stars form and die.
THE LIFE CYCLE OF A STAR Objective: I will compare and contrast the life cycle of stars based on their mass.
12-2 Notes How Stars Shine Chapter 12, Lesson 2.
Life Cycle of Stars Objectives
The Sun, Formation of Elements, the Big Bang, and Black Holes
Astronomy-Part 4 Notes: The Life Cycle of Stars
8 Space physics Topic overview
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Astronomy-Part 4 Notes: The Life Cycle of Stars
The Star Lifecycle.
The Dramatic Birth, Life, and Death of a Star
The Life Cycle of a Star.
The Life Cycle of a Star.
Life Cycle of a Star.
There are millions of stars in our galaxy, the Milky Way
Stars form from nebulas Regions of concentrated dust and gas
A Solar system is born.
The Universe is HUGE Everything in the universe depends on the tiniest subatomic particles… But those particles can come together in some huge ways!
Life-Cycle of Stars.
Astronomy Mr. Coyle Earth Space Science Harwood Union H.S.
3A Objectives Describe the nebular theory in detail.
Life Cycles of Stars Where we’re going today…
Astronomy 2014 Study Guide.
The Life Cycle of a Star.
04/07/2019 The Earth and Beyond.
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Stars and Galaxies.
Presentation transcript:

Big Bang to Earth's Formation Concept Map By Hari Vellaipandian

Big Bang There was no time or space before the big bang. At first the universe was just energy. The universe expanded faster then the speed of light and was very, very hot. It cooled as it grew and began to form gas clouds and nebulas.

Matter and Anti-Matter When matter and anti-matter collide they annihilate each other. If the amount of both had been equal then the universe would have been pure energy, but there was 10,000,000,001 particle of matter for every 10,000,000,000 particles of anti matter. Because of this inequality, there was matter to form the universe we know.

Atomic Nucleus When they had cooled enough, the protons and neutrons were able to join to form atomic nuclei. The protons and neutrons made hydrogen and helium nuclei. The electrons were still too hot to join the neutrons and protons so there were still no full atoms.

Electrons make the first Atom It took billions of years(4.6) for the electrons to cool down enough to join with protons and neutrons. They joined to form the first hydrogen and helium atoms. When electrons joined the protons and neutrons it was like fog lifting and light could travel easier.

Proto-Star Formation First the nebulas grow with more atoms until they become unstable. The nebula collapses in on itself. The gravity of the cloud pulls in more and more gas. A proto-star hasn’t started nuclear fusion yet. Proto-stars are normally on the red spectrum

Nuclear Fusion in Star Nuclear fusion is what is what changes a proto-star to a star. It happens when the core gets hot enough and has enough energy that when the nuclei in the core hit each other they can combine. An example would be how hydrogen nuclei are turned into helium atoms.

Death of a Star - Supernova This happens when the nuclear fusion can no longer happen in the core. The heaviest element that can be formed in a star is iron. There is no enough energy for the iron atoms to combine Once this point is reached the core will contract and the outer parts will explode and send out a shockwave. That explosion is called a supernova. Supernovas can be a billion times as bright as the original star.

Fusion of Heavy Atoms When the stars core contracts violently during a supernova there is more energy and heat. This extra energy allows the heavier metals to form. Nuclear fusion is similar to how a car line works. It moves from one place to another adding another part.

Black Hole Structure The remaining contracted core of a supernova is called a neutron star. If the neutron star is twice the size of our sun then it will almost definitely collapse into a black hole. A black hole is so dense very little can escape its gravity. Light doesn’t illuminate black holes. Massive black holes are located in the center of galaxies. If matter is taken into a black hole it is super heated and turned into energy. The energy is sent out the black hole poles.

Formation of Proto-Sun to Star A proto-star becomes a star when nuclear fusion begins in the core. Nuclear fusions is started when the core is hot enough to push the nuclei together. The fusion in the proto-star normally occurs when heat in the core is at least 10,000,000 Kelvin.

Planet Tesimals to Proto-Planets Planet tesimals are on average a half mile across. Once the planet tesimals slow down enough and hit each other, static energy and friction will cause them to stick together. Another word for this is accretion. The gravity of the rocks would attract more matter and cause it to get bigger. It was a while before this could happen because at first the planet tesimals were moving to fast to stick. They would just destroy each other on contact.

Outer Planets The outer planets are Jupiter, Saturn, Uranus, and Neptune. They are all made up of primarily gas and are called the Gas Giants. The proto-planets would circle the sun on their orbits and their gravity would take in most gases and rocks.

Inner Planets The inner planets are Mercury, Venus, Earth, and Mars. The inner planets are made of mostly rock and metals. They formed after the outer planetes because they were in the rock line. In the rock line the rocks were moving to fast for the planet tesimals to move together, so they just broke each other if they collided.

Proto-Planets Collided and Earths Moon is Formed The proto-planets Earth and the Mars sized Theia collided. Magma was ejected into the air and Earth’s axis was tilted. The debris of impact was scatted and some was trapped in earths orbit. The debris slowly collected because of gravity. The gravitational force got stronger as the lump of collected debris grew. This  continued until all of the debris was collected and we were left with the Moon.

Earth's Bombardment and Extinctions The bombardment was 700 million years ago. It was a period when the inner 4 planets were hit with many asteroids and meteors. Most of Earth's water came from the late heavy bombardment in the form of hydrogen. There was another bombardment later. That was when the dinosaurs went extinct.