Geologic History of the Earth. Star Formation begins with a nudge…

Slides:



Advertisements
Similar presentations
Early atmosphere ~4.5 billion years ago Mostly Hydrogen and Helium Escaped into space Outgassing of water vapor and CO2 created a secondary atmosphere.
Advertisements

(Pflueger ). Today’s Objectives Students will be able to: 1. Discuss how we have arrived at the current atmosphere from the original atmosphere. 2. Compare.
Life Sustaining What’s needed of stars? Stablility.
Earth’s Atmosphere Noadswood Science, Earth’s Atmosphere To know how the Earth’s atmosphere has changed over time Tuesday, May 05, 2015.
From Fossils To Space Geology #1. What Do We Know?
(6) Earth in space and time. The student knows the evidence for how Earth's atmospheres, hydrosphere, and geosphere formed and changed through time. The.
Ch Formation of the Solar System
Click to listen Early atmosphere ~4.5 billion years ago Mostly Hydrogen and Helium Escaped into space Outgassing of water vapor and CO2 created a secondary.
The Hadean & Archean “It’s the Earth Jim, but not as we know it.”
Chapter 5: Earth and Its Moon. Goals Compare the Earth and the Moon and explain differences Describe the effects of gravity between the Earth and Moon.
How much can we change the Environment? n Locally – easy to see n Globally – do you believe it? –How many believe we, mere humans, can change the climate?
Average Composition of the Troposphere Gas Name Formula Abundance (%) Residence time (approx) Nitrogen N %42,000,000 years Oxygen O %5,000.
Evolution of the Early Earth
Planetary Atmospheres, the Environment and Life (ExCos2Y) Topic 1: Composition of Atmospheres Chris Parkes Rm 455 Kelvin Building.
Formation of the Solar System Chapter 27 page 684-
The History of the Earth. Origin of the Universe The universe began about 14.4 billion years ago The Big Bang Theory states that, in the beginning, the.
Early Earth’s Atmosphere. The First Atmosphere The early (first) atmosphere would have been similar to the Sun--mainly hydrogen and helium, but this atmosphere.
28 Sep 2000ASTR103, GMU, Dr. Correll1 Ch 05--Earth and Moon.
Earth and Other Planets Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great cloud of dust.
Geologic History and the Evolution of Life
The History of the Earth
Chapter 6 The Earth. Our Earth is a very special place.
Origins of the Atmosphere
Review 2 What was the solar nebula? What was it made of? How did gravitational collapse affect the Solar nebula? How does conservation of energy and angular.
EVOLUTION OF EARTH’S ATMOSPHERE Febrys Knolan L. Velasco 8- Mandela.
Objective: Explain the development of Earth’s atmosphere and the influence of early life on the atmosphere.
L.O: To know what the earth’s atmosphere was like in the past and what it is like now. Starter: What does the air we live in consist of?
Information n Class Website l n You are welcome to give your suggestions to improve the site!
Dr Mark Cresswell The Atmosphere 69EG5513 – Climate & Climate Change.
Origin, Evolution, and Composition of the Atmosphere
HOW DID WE GET HERE?? EARTH AND THE ORIGIN OF LIFE.
The Exam results …. Note: Ex1 score = (number correct)/49 You get one ‘bonus’ question due to boo-boo on a question in the 3PMer’s test.
Evolution of Earth’s Spheres
Copyright © 2014 All rights reserved, Government of Newfoundland and Labrador Earth Systems 3209 Unit: 1 Introduction to Earth Science – The Evolution.
1 Terrestrial World Atmospheres Some terrestrial worlds have atmospheres. Others don't. Venus and Mars have thick/thin atmospheres respectively made mostly.
How Earth Became Habitable Habitability. Obviously…… The planet has to form first….check your notes on planet formation.
The Origin of the Atmosphere
1 Photosynthesis (Process that changed history) Light energy + CO 2 + H 2 O  glucose + O 2 IMPORTANT POINTS:  Example of 1 st Law of Thermodynamics:
Chapter 22 The Precambrian Earth Precambrian Time: -includes everything before the ________ period of the Paleozoic era -length of about ___ billion.
(6) Earth in space and time. The student knows the evidence for how Earth's atmospheres, hydrosphere, and geosphere formed and changed through time. The.
1 UIUC ATMOS 397G Biogeochemical Cycles and Global Change Lecture 3: Origin of Earth’s Atmosphere Don Wuebbles Department of Atmospheric Sciences University.
Habitability: Making a habitable planet 26 January 2016.
Weather and the Atmosphere. Meteorology– Weather – Study of atmosphere at a given time and place, due to unequal heating of Earth’s surface Study of atmosphere.
P337\Section 4 Geologic Time Scale. 1a How long ago did the Earth form? 4.6 billion years ago.
22.3 – Formation of the Atmosphere and Oceans
Advanced Earth Science (Ch. 11) Atmospheric Basics.
Earth’s Atmosphere and Geologic Time Period
FORMATIONS: MOON, ATMOSPHERE, AND OCEAN Objective: I will describe the formation of Earth’s moon, atmosphere, and ocean. 12/2/15 PAGE 41.
The Earth’s Atmosphere
1) What is the approximate percentage of oxygen in Earth’s modern day atmosphere? . Answer 21 %
Earth Formation & Early History
Past and Present of the Earth’s Atmosphere
Atmospheric History of Venus
5.9 Chemistry of the atmosphere
Evolution of the Early Earth
Early Earth:.
The study of everything on and in the Earth (including the oceans and the atmosphere), and everything outside of it (the universe). - four major branches.
The earth takes shape.
Astronomy 04 The Solar System
Origin of the Atmosphere and Oceans
Chapter 1 Earth Science Review.
Earths Early History Looking into the past: Stars and rocks, both show what has been LAND ENVIRONMENTS Earth Formed approx. 4.6 Billion Years Ago (BYA)
A Quick Look at the History of Life on Earth
Composition And Origin
Primordial Atmosphere
Chapter 11 - Atmosphere.
Sci The Earth take Shapes
THE DEVELOPMENT OF EARTH.
Formation of the Atmosphere and Oceans
Life on Earth.
Presentation transcript:

Geologic History of the Earth

Star Formation begins with a nudge…

Formation of the Solar System

Planetary accretion

Why terrestrials and Jovians?

Terrestrial Composition

Jovian Composition

Leftover Debris

Kuiper Belt

Oort Cometary Cloud

Formation of the Moon (4.5 BYA)

Structure of the Earth’s Interior

Heaviest impacts lasted 100 million years Tapered off 3.5 billion years ago Evidence? Impacts still occur today Early Bombardments

Cratered Worlds

Earth was not formed with atmosphere Gasses brought by planetesimals Outgassing and impacts released gasses H 2 0 CO 2 N 2 H 2 S SO 2 Water vapor condensed to form oceans Oceans were in place 4.3 – 4.4 BYA Formation of the Oceans and Atmosphere

Earth’s Primitive Atmosphere Produced by outgassing Formed 4.3 – 4.4 billion years ago? Rich in hydrogen, carbon, nitrogen, oxygen CO CO 2 N 2 H 2 O some H H 2 Contained complex molecules from ISM Hydrogen lingered for a few million years

Atmospheric Retention Molecular velocity Planetary Escape Velocity photodissociation

Evolution of the Earth’s Atmosphere Oxygen Levels [Currently ~21%] billion years ago Photosynthesis Originally oxidation kept pace with oxygen production (CO  CO 2, rust) Evolution of large plants, trees, flowers, grasses (600 MYA)

Creation of Ozone (O 3 ) O 2 + UV  O + O O + O 2  O 3 Requires the absence of hydrogen Significantly increased 600 MYA Ozone allowed life to venture onto land

Nitrogen Levels [Currently ~ 78%] Liberated by outgassing Significance of denitrifying bacteria Atmospheric nitric oxide (N+O)  rain  soil/oceans  bacteria  atmosphere Evolution of the Earth’s Atmosphere

Argon [Currently ~ 1%] Inert: formed by radioactive decay of potassium Liberated by outgassing Evolution of the Earth’s Atmosphere

Carbon dioxide [Currently ~0.01%] Dominated early atmosphere “locked up” in calcium carbonates (limestone, chalks) Evolution of the Earth’s Atmosphere

Carbon cycle Accelerated by living sea creatures

Does the geologic history of the Earth lead to the formation of life? Does this make life unique to the Earth? Atmosphere has been altered by life Existence of extrasolar planets has been confirmed

Chapter 11: 260 – 278 (Q: 1, 2, 3) Chapter 8: 189 – 196 (Q: 2, 3, 4)