Yoshihide Kozai oa 2009 Asian Science Camp August 3

Similar documents
Climate Regulation. - What stabilizes the climate - Greenhouse effect

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

Astron 104 Laboratory #10 Solar Energy and the Habitable Zone

Planetary Atmospheres (Chapter 10)

Today. Events. Terrestrial Planet Geology - Earth. Terrestrial Planet Atmospheres. Homework DUE next time

PTYS 214 Spring Announcements. Midterm 3 next Thursday!

Investigating Planets Name: Block: E1:R6

In-Class Question 1) Do you think that there are planets outside the solar which would be habitable for human life?

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Earth s Atmosphere About 10 km thick

The Atmosphere. Composition of the Atmosphere. Section 2

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Section 2: The Atmosphere

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Earth & Earthlike Planets. David Spergel

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Chapter 20 Earth: The Standard of Comparative Planetology

The Solar System. Earth as a Planet

CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1)

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Planetary Temperatures

anemometer a weather instrument that measures wind speed with wind-catching cups (SRB, IG)

The greenhouse effect

Clever Catch Weather Ball Question and Answer Sheets

General Comments about the Atmospheres of Terrestrial Planets

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

The Atmosphere Made up of mainly two gases: Nitrogen 78% Oxygen 21% Trace Gases 1%

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Unit 1: The Earth in the Universe

Our Sun. The centre of our solar system

PLANETARY ATMOSPHERES

FINAL EXAM (practice) ASTR Spring 2008 Instructor: Joel E. Tohline. 1. How many (real) planets are there in the solar system?

PRE-LAB FOR PLANETARY ATMOSPHERES

Grades 9-12: Earth Sciences

2010 Pearson Education, Inc.

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

4) Outline the major developments that allowed life to exist on Earth.

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am

Outline 9: Origin of the Earth: solids, liquids, and gases

Earth s Atmosphere. Atmospheric Composition 78% Nitrogen 21% Oxygen 1 % Argon, 0.03% Carbon dioxide, Water. Recall the Electro-Magnetic (EM) Spectrum

Scholarship 2015 Earth and Space Science

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

1. CLIMATOLOGY: 2. ATMOSPHERIC CHEMISTRY:

see disks around new stars in Orion nebula where planets are probably being formed 3

Today we will discuss global climate: how it has changed in the past, and how the current status and possible future look.

The History of the Earth

The Role of Biology in the Climate System: Long Term Climate Regulation. Earth History, Gaia and Human Perturbations of Biological Systems

Mars & Venus: Just Down the Street

CST Prep- 8 th Grade Astronomy

Chapter 4 Lesson 1: Describing Earth s Atmosphere

Module 4: Astronomy The Solar System Topic 3 Content: The Terrestrial Planets Notes Introduction

The Layered Atmosphere:

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings

Common Elements: Nitrogen, 78%

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

AST 105 Intro Astronomy The Solar System

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time.

Greenhouse Effect & Global Warming

NSCI 314 LIFE IN THE COSMOS 9 - SEARCHING FOR LIFE IN OUR SOLAR SYSTEM: EARTH'S MOON (CONTINUED), MERCURY, AND VENUS

Weather & Climate. Sanjay S. Limaye Space Science & Engineering Center University of Wisconsin-Madison

Plan. Questions? Syllabus; administrative details. Some Definitions. An Idea of Scale

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

The greenhouse effect

Object Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.

25-Nov-14. The Structure of Earth s Interior. What unique features of Earth are important for life as we know it?

ASTRONOMY 1010 Exam 2 October 19, 2007

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Earth. Interior Crust Hydrosphere Atmosphere Magnetosphere Tides

Announcements. Distances in the Solar System. The Main Point. Lecture #10: Solar System Survey II

2/22/ Atmospheric Characteristics

Meteorites. A Variety of Meteorite Types. Ages and Compositions of Meteorites. Meteorite Classification

The Sun and Planets Lecture Notes 6.

Planetary Atmospheres

Science Practice Astronomy (AstronomyJSuber)

0 questions at random and keep in order

Terrestrial Atmospheres

10/11/2010. Acceleration due to gravity, a. Bulk Properties Mass = 6 x kg Diameter = 12,756 km Density = 5515 kg/m 3 (mix of rock and iron)

Observing Habitable Environments Light & Radiation

In class quiz - nature of light. Moonbow with Sailboats (Matt BenDaniel)

3. Evolutionary change is random because gene mutations are random. A. True B. False

Ch 23 Touring Our Solar System 23.1 The Solar System 23.2 The Terrestrial Planet 23.3 The Outer Planets 23.4 Minor Members of the Solar System

Some Tips Before You Start:

AST 105 Intro Astronomy The Solar System

Chapter 2. Heating Earth's Surface & Atmosphere

Phys 214. Planets and Life

PLATO - 5. Planetary atmospheres

Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2

FCAT Review Space Science

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration

D] The Lunar eclipse; The shadow cast by the Earth on the moon during Lunar eclipse is always circular proving the Erath is a sphere.

Inner Planets (Part II)

AT 350 EXAM #1 February 21, 2008

28-Aug-17. A Tour of Our Solar System and Beyond. The Sun

Transcription:

Atmosphere of Venus, Mars and Earth Yoshihide Kozai oa 2009 Asian Science Camp August 3

The Earth from the Moon

Venus

Mars

Jupiter

Orion Nebula Where stars are born Distance 1500light Years 50 light year Wide(3 million AU) Stars are born where Density of interstellar t Matter is high.

Chemical Composition of Atmosphere Chemical composition of atmosphere(%) N 2 O 2 CO 2 H 2 O H 2 He Venus 34 3.4 0.007007 96 0.019019 Earth 78 21 0.037 1~2.8 Mars 2.7 0.13 95 0.03 Jupiter 89 11 Surface pressure Temperature Solar distance Venus 90 atm. 460 C 0.72 AU Earth 1 20 C 100 1.00 Mars 0.006 60 C 1.52

Greenhouse Effect High temperature of Venus is caused by greenhouse effect due to thick atmosphere. When the sky is very clear (without clouds and greenhouse gases), thetemperature temperature comes down because of no blanket against infrared radiation from the surface. Carbon dioxide makes a greenhouse and if its abundance is much lower, the mean temperature of theearthearth should be lower.

Greenhouse effect Infrared radiation is absorbed/scattered in the atmosphere. SUN Cloud CO 2 Infrared Light Cloud CO CO 2 2 H H 2 O 2 O Visible ibl Light Surface

Mars Earth Venus

Comparison of the Atmospheres Venus Thick CO 2 Strong Greenhouse 460 C >> 50 C (no greenhouse) Water unstable Mars Very thin CO 2 Very weak Greenhous 60 C Water frozen Earth N 2 O 2 little CO 2 Moderate Greenhouse 20 C > 5 C (no greenhouse) Water stable = Ocean

Evolution of the atmosphere: How the Earth decreased CO 2? Carbon dioxide (CO 2 ) was first absorbed by huge sea covering the earth. In the sea, several plants were born and by their photosynthesis effect the plants absorbed carbon dioxide do deand made oxygen oyge (O 2 ).

Photosynthesis Organic matters

Stromatolite Modern stromatolites in Shark Bay, Western Australia Stromatolites are layered accretionary structures formed in shallow water by the trapping, binding and cementation of sedimentary grains by biofilms of microorganisms, i especially cyanobacteria (commonly known as blue-green algae). They include some of the most ancient records of life on Earth.

Fossile Stromatolite Microfossils 3.5x10 9 yr before present (Australia) that resemble filamentous cyanobacteria

Increase in oxygen In the sea, chlorophyta produced oxygen by photosynthesis and oxygen amount increased to be 1/100 of the present. Then, multicellular organism appeared on the Earth. It was 800 million years ago that crustacean and mollusk appeared, when oxygen amount was 1/10 of the present. Accordingly ozone (fromthree oxygen atoms) started increasing and the ozone layer in the upper atmosphere stopped solar UV and X ray, which are poisonous for the life. Formation of the ozone layer promote the life on the land.

Chlorophyta multicellular organism crustacean mollusk

Global Warming Organic materials containing carbon produced by photosynthesis were stored underground; oil was produced from organic materials. Coral reefs formation in the ocean capture carbon dioxide. (Limestone is composed of fossils of coral.) In recent 300 years as industrial activity has been very active by using oil and coral. Then much carbon dioxide was again produced. In the recent 50 years or so, global warming has become a serious problem.

Coral Reef Oil Field

Global Warming Increase in carbon dioxide in the atmosphere enhanced the greenhouse effect that delays the escape of energy obtained from solar radiation. That results in the global temperature increase, i.e., global warming. Melting of glaciers by the global warming should raise the sea level, which would be fatal for lowelevation islands. Japan is now in temperature zone. As proceeds the global warming, Japan will enter subtropical zone with hotter and more humid climate.

Light pollution Astronomical observation is strongly affected by light pollution, excessive obtrusive artificial lights. Especially in and around the large city, artificial lights brighten the night sky and prevent star observation. Under the sky glow of artificial lights which affect long exposure photographing, it is very difficult to observe dark stars. From the beginning of 20th century, astronomical observatories moved from cities to remote places with dark sky.

Dark sky Light pollution

Looking down the night earth from the space, we realize too much light have escaped to the sky. This amount is much greater than the least necessary illumination for lands. Light Environment Ordinance (Outdoor Lighting Ordinance) In order to decrease light pollution, Bisei town, Takayama village, Hamamatsu city, Tucson city (US) enacted Light EnvironmentOrdinance. For example, streetlights should be covered not to emit light upward to the sky. This would also decrease the power consumption.

Earth at night from a Satellite

Habitable planet (habitable zone) Liquid id water is stable on the surface of a planet.

Factors controlling habitability Distance from the sun (main star). Atmosphere (Greenhouse effect). Gravity Too small planets do not have atmosphere. Composition (presence of water). Luminosity of the sun (main star).

Mars was habitable. River delta Sedimentary rocks

Why was Mars habitable? Thick CO 2 atmosphere 4.0 billion yr ago. (3 5 atm. P CO2 ) Strong greenhouse effect. Thick atmosphere escaped?