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Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] [Venue; Date] Project B612 Goal: To significantly alter the orbit of an asteroid in a controlled manner by 2015

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Page 1: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA)

Rusty Schweickart

Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA)

Rusty Schweickart

[Venue; Date][Venue; Date][Venue; Date][Venue; Date]

Project B612Project B612Goal: To significantly alter the

orbit of an asteroid in a controlled manner by 2015

Goal: To significantly alter the orbit of an asteroid in a

controlled manner by 2015

Page 2: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Note: This is a draft presentation. It is incomplete. Things need to be checked. The last several slides were not constructed for this presentation but could be used as a basis for more in-depth treatment of certain issues. The Southwest Research Institute logo needs to be removed…I just haven’t

done it yet (because I don’t know how, off the top of my head).

Clark Chapman, October 21, 2002

Page 3: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

What is the Danger from Asteroids?

During your lifetime, there is a 1-in-3000 [ck] chance that an undiscovered asteroid (or comet) more than one kilometer wide will strike the Earth, threatening civilization.

During your lifetime, there is a few-percent chance that a 100-meter (or larger) asteroid will strike the Earth with the energy of 100 Megatons (5000 Hiroshima bombs)

The impact hazard is an extreme example of a natural disaster (a small chance of happening, but with huge consequences) that challenges a rational response by citizens and policy-makers.

Page 4: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

The Asteroid Belt, the Trojans, and the Near-Earth Asteroids

Page 5: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

The Range of Asteroid Impacts...

Meteorites hit regularly

Devastating events in our lifetime

Civilization destroyers

Dinosaur killers (mass extinctions)

Page 6: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

The 20th Century’s Biggest Impact was Very Destructive

This Siberian forest (the size of a major city) was felled in 1908 by a 15-Megaton asteroid explosion, “Tunguska”

Page 7: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

What are we Doing About the Threat?

The only thing we are doing right now is to search for asteroids (larger than 1 kilometer) that might strike

There are suggestions that we should be searching for smaller asteroids

We are only beginning to think about what we might do if an asteroid were found to be heading toward Earth

Project B612 has a more concrete suggestion!Project B612 has a more concrete suggestion!

Page 8: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

We Have a Goal:

Why is development of a deflection program important?Why is development of a deflection program important? An insurance policy.

Why do we need to test?Why do we need to test? We want to know that the technology will work before we have to use it for real.

Why by 2015?Why by 2015? Because we can, and we should not wait.

What kind of an asteroid will we move?What kind of an asteroid will we move? A small, repre-sentative one (whose orbit does not threaten Earth).

What is “a controlled manner”?What is “a controlled manner”? It is deflected far enough so that it would miss the Earth (had it been headed toward Earth) and it doesn’t break up into dangerous pieces.

Significantly alter the orbit of an asteroid in a controlled manner by 2015

Significantly alter the orbit of an asteroid in a controlled manner by 2015

Page 9: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

How Much Warning will we Have?

Asteroids found by Spaceguard:

Nearly all will be certified as “not going to hit”

If one is found headed to Earth, we’ll likely have decades of warning.

Extremely rarely, we might have short warning but time to evacuate

Asteroids NOT found before they hit:

Would hit with near-zero warning.

Page 10: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

How Can we Deflect an Asteroid?

Blowing it up is NOT a good option Uncontrolled shattering into spray of

dangerous fragments Not as effective as you might think,

especially for a “rubble pile” How would we PUSH it away from

collision course, and hold it together? Yarkovsky effect: “paint it white” Solar sail: use “light pressure” Mass driver: throw rocks off the

surface Ablation: evaporate a spot on the

surface Attach a rocket

Page 11: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Criteria for Evaluating Deflection Options

Should miss the Earth given a decade of warning: a few cm/sec change in velocity

Must move asteroids at least 100 meters in size, preferably many hundreds of meters

Must transport the device from Earth’s surface to speeding asteroid using available launch vehicle

Should work for a wide variety of asteroids (weak, metallic, icy, etc.)

Page 12: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Eros is NOT Like the Moon!

The Moon has craters.

Eros has rocks.

Page 13: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Some Salient Facts about the Impact Hazard

It is notnot a “Deep Impact” or “Armageddon” shoot-em-down just before they hit scenario

For asteroids, orbiting in the inner solar system, it is a case of finding them decades in advance of an impact…with long lead-times for mitigation: For every asteroid with <1 year warning time, there are 50 with 5 decades of lead-time (but comets are another matter)

It is one of the few big hazards for which it is technologically feasible, with some confidence, to stop the catastrophe from happening (by deflection)

Page 14: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Conclusions 1…

The impact hazard is REAL but it is VERY UNLIKELY to happen during our lifetimes

Its potential consequences are horrific… exceeding any other natural hazard and equalling all-out nuclear war

We could avert a threatened impact

In a post-September 11th world, it is difficult (for me) to predict how people might react to near-misses, huge-but-low-probability disasters, bombs in space, and other impact hazard issues

Page 15: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Conclusions 2...

Humans have the intelligence and capability toHumans have the intelligence and capability toprotect our civilization from this threat from theprotect our civilization from this threat from theskies.skies.

The dinosaurs failed.The dinosaurs failed.

Is society going to gamble and submit to fate orIs society going to gamble and submit to fate orwill it undertake a measured, rational response?will it undertake a measured, rational response?

Society must educate its leaders and publicSociety must educate its leaders and publicofficials to the facts of the impact hazard, decideofficials to the facts of the impact hazard, decidewhat should be done, then do it.what should be done, then do it.

Page 16: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Tsun

ami

Str

atos

pher

ic D

ust

Risk vs. Scale of Impact

Annual fatalities peak for events near the “threshold size”, about 2 km

Orange/yellow zone illustrates our range of uncertainties for agricultural disaster due to stratospheric dust

Page 17: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Chances from Dying from Selected Causes (for U.S.A.)

By terrorism (mostly due to Sept. 11th attacks)

Page 18: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

The Torino Scale

Events Having No Events Having No Likely ConsequencesLikely Consequences

Events MeritingEvents MeritingCareful MonitoringCareful Monitoring

Events MeritingEvents MeritingConcernConcern

ThreateningThreateningEventsEvents

CertainCertainCollisionsCollisions

Page 19: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

How the Torino Scale is Calculated: From the Probability of Impact and Size

Page 20: Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart Clark Chapman (SwRI) Piet Hut (IAS) Ed Lu (NASA) Rusty Schweickart [Venue; Date] Project

Why are the big/rare ones so much more important than Tunguskas?

Only asteroids larger than ~1 mile across can be globally destructive and threaten civilization

For every devastating 15-MT Tunguska blast, there are ~100 earthquakes, floods, and typhoons that are equally destructive

Cost-effectiveness drops sharply with size: the average annual fatalities drop while the costs of finding the objects and responding to them rises

But, there are contrary viewpoints and interests: On a politician’s But, there are contrary viewpoints and interests: On a politician’s “watch”, why would he/she care about what might happen decades “watch”, why would he/she care about what might happen decades from now? “Star Warriors” in the DOE and DOD who would like to from now? “Star Warriors” in the DOE and DOD who would like to test their inventions and try shooting down small asteroids. And test their inventions and try shooting down small asteroids. And astronomers who would love to have more and bigger telescopes.astronomers who would love to have more and bigger telescopes.