Terraforming Mars and Venus. Reasons to Terraform Henceforth I spread confident wings to space I fear no barrier of crystal or of glass; I cleave the.

Slides:



Advertisements
Similar presentations
Terraforming Mars Wohoo, Star Trek! What is involved? Terraforming process Time Cost Colonization Worth the effort? Future interaction with space.
Advertisements

Terraforming Mars and Venus. Reasons to Terraform Henceforth I spread confident wings to space I fear no barrier of crystal or of glass; I cleave the.
Clicker Questions Chapter 6 The Terrestrial Planets Copyright © 2010 Pearson Education, Inc.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 16.
1.3 Extracting Energy from Biomass
Interiors of Terrestrial Planets. Mercury MEAN RADIUS: km MASS: (Earth=1) DENSITY: 5.43 (g/cm^3) GRAVITY: (Earth=1) ORBIT PERIOD:
Your Name Your Title Your Organization (Line #1) Your Organization (Line #2) Global warming.: Matthieu BERCHER, Master M.I.G.S., University of Burgundy,
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 11 : Earth’s Habitability Ty Robinson.
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Average distance from Sun =.39 AU Moonlike:
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Moonlike: Surface craters, no atmosphere.
Explaining the global warming theory Explaining the implications of science to contemporary public issues is an important part of our job. As an example.
Understanding Our Atmosphere
The inner planets What do the inner planets have in common? what are their characteristics?
The Solar System.
Space Exploration.
Planet Formation and the solar system REVIEW. The raw materials to form planets come most directly from what source?
Global Warming is the gradual increase in the temperature of earth’s atmosphere attributed to the greenhouse effect caused by increase levels of carbon.
Water, Water, Everywhere? Anuradha Koratkar, Susan Hoban, Albert Hill, and Brendan Shaughnessy.
Comparative Planetology I: Our Solar System Chapter Seven.
Habitable World. Requirements for life Every living thing has the same basic needs to survive on Earth: Water Moderate temperature Oxygen Nutrients Atmosphere.
Global Warming Global warming is the increase in the average measured temperature of the Earth's near-surface air and oceans since the mid-20th century,
Chapter 7e Earth is a living planet. 7.5 Earth as a Living Planet Our Goals for Learning What unique features on Earth are important for human life? How.
21st C ENTURY A STRONOMY T HIRD E DITION Hester | Smith | Blumenthal | Kay | Voss Chapter 8 Lecture Outline Atmospheres of the Terrestrial Planets.
Terrestrial Atmospheres Solar System Astronomy Chapter 8.
Sin’Kira Khan & Dane Fujinaka
Venus is named after the Roman goddess of love and beauty. Venus rotates on it’s axis every 243 earth days. Venus’ mean radius is 3,760.
The Mission to Colonize Mars A home away from home… (Yes, I know there aren’t oceans on Mars, but come on…the background looks cool)
PPT Lecture: Global Warming. Slide 2 - Greenhouse Effect The process of the atmosphere trapping heat from the sun. Without the atmosphere, heat would.
Feedback Loops. FEEDBACK LOOPS Change induces change What happens when you’re hot? What happens when you’re cold? These are examples of negative feedback.
Exam 2 Postponed Tuesday, November 12 Covers Chapters 7-10, & 14 One sheet of notes with writing on one side only.
Semester 2 Final Review Part 2 Carbohydrates, Photosynthesis & Respiration and Ecology.
(Terrestrial) Planetary Atmospheres II.  Atmospheres consist of exospheres only  Take either of their atmospheres, could “almost store them in a dorm.
Key Ideas Compare four methods used to study climate change.
Comparative Planetology I: Our Solar System. Guiding Questions 1.Are all the other planets similar to Earth, or are they very different? 2.Do other planets.
True or False Questions: 1. There are 687 days in a Martian year and 24 1/2 days in a Martian day. 2.There is some water on Mars. 3.The average temperature.
How much should it cost? Rank the following items in order of their importance to you. Then, next to each item, write down how much you would be willing.
1 Inner or Terrestrial Planets All the inner planets formed at the same time. Their composition is also very similar. They lack the huge atmospheres of.
Space Exploration. Space Travel Write down as many things as you can think of that a space explorer would need to survive in space.
Evolution of Earth’s Spheres
The Solar System. Solar System the sun and all things orbiting around it, including the eight major planets, their satellites, and all the smaller pieces.
Living on Mars! How do we plan to live on Mars The Pros and Cons of living on Mars.
ATMOSPHERE I Intro Layers of the Atmosphere Air Pressure
INNER PLANETS Terrestrial Planets are the Four planets closest to the sun. These planets have rocky terrain, and have higher temperatures due to receiving.
Life in our solar system
Life in our solar system
The atmosphere is a mixture of gases that surrounds a planet, such as Earth. Nitrogen, oxygen, carbon dioxide Gases can be added to and removed from the.
The Sun: Our star.
Planet Facts. Planet Size Vocabulary Surface Pressure (bars or atmospheres) - This is the atmospheric pressure (the weight of the atmosphere per.
Terraforming Mars Fact or Fiction By: Sarah Lee PHYS
THE INNER PLANETS. WHAT DO THEY ALL HAVE IN COMMON? Q : Which planet is largest? Q : Which planet has the most moons? Q : Which planet is most similar.
Copyright © 2010 Pearson Education, Inc. The Terrestrial Planets.
The Rare Earth: There aren’t too many places like our planet.. Everything is “just right” for life to exist.
Advanced Earth Science (Ch. 11) Atmospheric Basics.
Habitable Zone Notes “Life in the Goldilocks Zone”
Unit 6 By JOJO Frame of the article Part I: Why Part II: What Part III: How do scientists transform Mars? is Mars like? will the plan be carried out?
The greenhouse effect. How is the Earth warmed? Climate is affected by the conditions and components of the atmosphere. The Earth’s atmosphere acts like.
“Life in the Goldilocks Zone”
© 2017 Pearson Education, Inc.
Class Notes for Monday, Feb 20th
Mars The Red Planet.
Add to table of contents:
Global Warming Noadswood Science, 2016.
Habitable world.
How do we plan to live on Mars The Pros and Cons of living on Mars
Terraforming Mars 9 November 2016.
“Life in the Goldilocks Zone”
Are we alone in the universe?
Habitable world.
Atmosphere The atmosphere is a mixture of gases that surrounds a planet, such as Earth. Nitrogen, oxygen, carbon dioxide Gases can be added to and removed.
Why is Earth the Only Planet that Sustains Life?
Presentation transcript:

Terraforming Mars and Venus

Reasons to Terraform Henceforth I spread confident wings to space I fear no barrier of crystal or of glass; I cleave the heavens and soar to the infinite. And while I rise from my own globe to others And penetrate even further through the eternal field, That which others saw from afar, I leave far behind me. Giordano Bruno On the Infinite Universe and Worlds, 1584

Reasons to Terraform Extreme pollution of Earth Extreme crowding on Earth The imminent destruction of Earth by impact Scarcity of raw materials; creation of permanent mining operations Adventure; because it’s there

Conditions on the Sister Planets EarthMarsVenus Atmosphere % O % N % CO Pressure 1 atm0.006 atm 90 atm Temperature -15 C to 40 C-140 C to -15 C450 C Water liquid/frozenfrozennone Gravity 1.0 g0.38 g≈ 1.0 g Magnetic Field adequatenone Length of Day 1 day≈ 1 day117 days

Conditions on the Sister Planets EarthMarsVenus Atmospheric Chemistry % O % N % CO Pressure 1 atm0.006 atm 90 atm Temperature -15 C to 40 C-140 C to -15 C450 C Water liquid/frozenfrozennone Gravity 1.0 g0.38 g≈ 1.0 g Magnetic Field adequatenone Length of Day 1 day≈ 1 day117 days

Do We Need Earth-Like Conditions? Not necessarily Obtaining the right oxygen level might be very difficult With the right pressure and temperature, humans could grow food and mine without spacesuits (need oxygen masks) Different term? -- ecosynthesis (Macelroy, 1976)

Goals for Terraforming Mars Increase atmospheric pressure Warm terrain and atmosphere Prevent loss of atmosphere

Mars Ecosynthesis James Graham, Astrobiology, 4: (2004) 1000-year process Probably have several hundred thousand years before Earth is uninhabitable

Schemes for Atmospheric Warming Pollution: manufacture and release hydrocarbons to enhance greenhouse effect Melt CO at the poles through to use of space mirrors Steer ammonia-rich asteroids or comets to impact -- decades of delay

James Graham’s Model (2004)

“It is concluded that a drastic modification of Martian conditions can be achieved using 21st century technology. The Mars so produced will closely resemble the conditions existing on the primitive Mars. Humans operating on the surface of such a Mars would require breathing gear, but pressure suits would be unnecessary. With outside atmospheric pressures raised, it will be possible to create large dwelling areas by means of very large inflatable structures. Average temperatures could be above the freezing point of water for significant regions during portions of the year, enabling the growth of plant life in the open. The spread of plants could produce enough oxygen to make Mars habitable for animals in several millennia. More rapid oxygenation would require engineering efforts supported by multi-terrawatt power sources. It is speculated that the desire to speed the terraforming of Mars will be a driver for developing such technologies, which in turn will define a leap in human power over nature as dramatic as that which accompanied the creation of post-Renaissance industrial civilization.” Robert M.Zubrin and Christopher P. McKay, “Technological Requirements for Terraforming Mars,” date unknown but after

Goals for Terraforming Venus Reduce atmospheric temperature Eliminate most of dense CO atmosphere Add breathable oxygen (Establish magnetic field by spin-up) (Push Venus further from the Sun)

Venus Ecosynthesis Reduce temperature – Space-based solar shade (Paul Birch)

Venus Ecosynthesis Reduce CO 2 and reduce pressure – Microbes to turn excessive CO 2 into carbohydrates – Capture in carbonates by introduction of magnesium and calcium metals – Direct liquifaction – Introduction of hydrogen H 2 + CO 2 ⇒ C + H 2 O

Venus Ecosynthesis Establish magnetic field – Molten interior – Spin-up Mass drivers ? Rocket assist ?

An Interesting Alternative to Venus Ecosynthesis Floating colonies – 50 km altitude – Pressure about 1 atmosphere – Temperature: 0 – 50 C

Philosophical (Ethical?) Issues Do we have the right to alter a natural environment?

Philosophical (Ethical?) Issues Pros – Ecosynthesis would allow free movement with breathing masks – Colonists could live off local biomass – A unifying project for Earth’s people – Would provide a survival colony in the face of an Earth disaster – Stimulate technological developments – Better use of resources than building military stockpiles

Philosophical (Ethical?) Issues Cons – Enormous time scales – Very long-term economic payback – Less attention to important terrestrial problems – Legal and administrative roadblocks Who gets to live there? Who owns it? Who controls it? Earth or the other planet? – People’s physiology would evolve in different gravity of Mars Bone structure Muscle mass Internal organs?