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

Clicker Questions Chapter 6 The Terrestrial Planets Copyright © 2010 Pearson Education, Inc.
Space Colonization Terra-forming
1.3 Extracting Energy from Biomass
11/15/99Norm Herr (sample file) SOLAR SYSTEM The Sun Nine Planets Sixty-one satellites of the planets Many Comets and asteroids.
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
Human Impact on Ecosystems
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.
The Solar System.
The Solar System. The Sun  Temperature: 6,000c (11,000 F)  Made mostly of hydrogen and helium.
Space Exploration.
Our Solar System. Our solar system in order from the sun 1.Mercury 2.Venus 3.Earth 4.Mars 5.Asteroid Belt 6.Jupiter 7.Saturn 8.Uranus 9.Neptune 10.Kuiper.
Water, Water, Everywhere? Anuradha Koratkar, Susan Hoban, Albert Hill, and Brendan Shaughnessy.
Our solar system Chapter 2 By Mrs. Shaw.
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,
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.
JUPITER.
Sin’Kira Khan & Dane Fujinaka
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.
Ticket A 99 percent of the solar system’s mass is in the what. Click here for answer.
A yellow star made of HYDROGEN AND HELIUM GAS. The sun gives off ENERGY!
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.
Bell work Create a new mnemonic device to help you remember the order of the planets: My Very Excited Mother Just Served Us Nectarines. Mercury, Venus,
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.
Exploring the Solar System GCSE Astronomy – Lesson 26.
Space Exploration. Space Travel Write down as many things as you can think of that a space explorer would need to survive in space.
Image Courtesy of NASA/JPL-Caltech.  Known to Babylonians 3,600 years ago as “Star that Wandered”  The Greeks referred to it as “Ares” the god of War.
THE SOLAR SYSTEM. UNITS OF MEASURMENT IN ASTRONOMY ASTRONOMICAL UNIT, AU = 93,000,000 MILES = 150,000,000 km = AVERAGE DISTANCE FROM EARTH TO THE SUN.
Comparative Planetology I: Our Solar System Chapter Seven.
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.
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
How’s it going to end? Climate evolution on Mars and Venus and its bearing on the very long term fate of the Earth’s climate system.
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
PLANETS What is an AU? An astronomical unit (AU) is the average distance of the Earth from the sun. 1 AU = 150 million kilometers.
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.
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 Universe … is everything What is the… The largest objects in the universe are galaxies… …there are different types, categorised by their shape.
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
Global Warming Noadswood Science, 2016.
Planet Facts.
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.
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

Terraforming in Literature 1898, H. G. Wells, The War of the Worlds, terraforming of Earth by alien invaders 1910, Octave Beliard, La Journee d’un Parisien au XXI siecle, turn the Moon into a sanctuary for endangered species 1930, Olaf Stapeldon, Last and First Men, terraforming of Venus by Earth conquerors 1950, Robert A. Heinlein, Farmer in the Sky, family emigrating to Ganymeade which is undergoing terraforming 1952, Isaac Asimov, The Martian Way, terraforming Mars using ice from Saturn’s rings 1965+, Frank Herbert, Dune (and sequels), converting desert-world, Arra’kis, to Earth-like conditions and vice-versa 1984, James Lovelock and Michael Allaby, Greening of Mars, first realistic proposals , Kim Stanley Robinson, Mars Trilogy, centuries-long terraforming of Mars using contemporary scientific developments

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 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

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 2 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

Conditions on the Sister Planets EarthMarsVenus Atmosphere 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

Goals for Terraforming Venus Reduce atmospheric temperature Eliminate most of dense CO 2 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

Technological Benefits of Space Exploration Programs solar panels implantable heart monitors cancer therapies light-weight materials water purification systems improved computing capabilities global search-and-rescue systems Etcetera, etcetera (Yul Brynner, “The King and I”)

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?