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Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

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Page 1: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Theme 10 – Leftovers: Impacts and Mass Extinctions

ASTR 101Prof. Dave Hanes

Page 2: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

The Effect of Impacts

Page 3: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Two Competing Hypotheses

Page 4: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

The Disappearance of the Dinosaurs

Page 5: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Just How Abrupt Was It?

Page 6: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

First Evidence Suggesting a Catastrophic Event

Discovery of the thin KT Layer [K = Cretaceous]

relatively high in Iridium

contains lots of ash and soot

is seen world-wide, typically several cm thick

is considerably thicker in southern parts of North America

Page 7: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Different fossils (includingmicro-organisms) are seenabove and below the layer.

Much more Iridium in the layer than you would

expect (but still just a few parts per billion!)

Page 8: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

A Helpful Analogy

The Crime Scene

At a murder scene, we find a tiny trace of my DNA (perhaps from a drop of sweat) although I claim never to have been there

It’s not the dominant material present, but it is surprising to find it at all.

The KT Boundary

Earth has its fair share of Iridium, but most of it is in the core, thanks to differentiation: there’s very little in crustal material.

So where did the extra Iridium in the KT layer come from?

Page 9: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Three Obvious Possibilities

Perhaps a period of enhanced volcanic activity dredged Iridium up from deeper layers (and the volcanism killed off many species, including the dinosaurs); or

Perhaps a big impact (by an asteroid, say) blasted out a lot of material from deep within the Earth, including Ir; or

Perhaps an incoming object, with its own share of Iridium, broke up on impact, and sprinkled its own material (and additional material from the Earth’s crust) all over the planet.

Page 10: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Other Important Evidence

1. Evidence of extensive fires

2. Impact site found, surrounded by ‘ejecta blanket’

3. Near the site, “shocked” quartz crystals (which are evidence of direct impact)

4. Evidence of huge tsunamis

5. The impact site has the right age!

Page 11: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Evidencefor Huge Fires

- lots of soot and organic material inthe KT layer

Page 12: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

The Impact Site(the 100-km diameter crater suggest an impact by

a 10-km body

Page 13: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Ejecta and Tsunamis

Page 14: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

The Chicxulub Story… Alan Hildebrand

Page 15: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Before and After(but much overgrown and eroded today)

Page 16: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

One Question:

Would There Be Global Damage?

Would the impact rupture the Earth as a whole, or knock it out of its orbit?

A 10 km comet would have about 1 trillionth of the mass of the Earth. If it is brought to a halt on impact, the Earth itself will pick up about one trillionth of the comet’s original speed in that new direction (thanks to the Conservation of Linear Momentum) – obviously negligible.

So the Earth’s orbital motion would be utterly unaffected.

Page 17: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

But a Lot of Energy is Pumped into the Biosphere!

The incoming object (10 km diameter) will have a mass of at least a trillion tons

It is coming in at perhaps 50 km/sec

On impact, it releases as much kinetic energy as about 100 trillion tons of TNT

Page 18: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

A Large Hydrogen Bombequivalent to ~10 megatons

Chicxulub is equivalent to about ten million such hydrogen bombs!

Page 19: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Does the Atmosphere Protect Us?

No. At its velocity,the object meetsthe atmosphere just afraction of a secondbefore impact withthe solid surface.

(Does your skin protect you from a bullet?)

Page 20: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Immediate Consequences

The compression of the air causes enormous heating. Animals and plants in the vicinity crumple up “…like cellophane in a fire” (B. Bryson)

There are atmospheric shock waves from the supersonic flight of the asteroid. (Remember Chelyabinsk?)

The impact causes tsunamis and a big ‘ejecta blanket,’ and vaporizes a lot of sea water.

Page 21: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Hollywood’s Treatment

Deep Impact

http://www.astro.queensu.ca/~hanes/ASTR101-Fall2015/ANIMS/Deep-Impact.mp4

Page 22: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Subsequently

Pulverized material (from the asteroid and the crustal rocks) is thrown into the air – many billions of tons

If falls back in pieces like uncountable numbers of meteors, glowing red hot

On continent-wide scales, the whole sky lights up like a blast furnace

Grasslands and forests over much of the Americas erupt in flame (hence the soot)

Page 23: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Long-Term Consequences

‘Nuclear Winter’ : the foreseeable consequences of a nuclear war. Smokeand soot fills the air, blocking the sun; we entera long ‘deep freeze.’

Page 24: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Can It Happen Again?

Yes. We are in a ‘cosmic shooting gallery’

Because asteroids are low-mass, their orbits are constantly being perturbed by the gravity of Jupiter and the other planets

So we cannot safely predict their orbits into the remote future, even if we could find all the dangerous objects now

Page 25: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

There are Recent Examplesby objects of various sizes

We have already considered:Tunguska – 1908Shoemaker-Levy – 1994Chelyabinsk - 2013

Near-miss captured in home movie (1950s):

http://www.astro.queensu.ca/~hanes/ASTR101-Fall2015/ANIMS/Meteor-Skim.mp4

Toutatis - 2004

Page 26: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Fortunately:For every big asteroid, there are millions of mid-sized ones

and trillions of pebbles. So big impacts are relatively rare.

Page 27: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Don’t be Complacent!

An event on the KT scale is likely to happen, on average, once every 100 million years (My)

The most recent was 65 My ago

This does not mean that we are safe for the next 35 MY!

Page 28: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

Other Mass Extinctions?

The Permian-Triassic event (the “Great Dying”) 252 million years ago was (in the words of Wikipedia):

“…the Earth's most severe known extinction event, with up to 96% of all marine species and 70% of terrestrial vetebrate species becoming extinct. It is the only known mass extinction of insects … Because so much biodiversity was lost, the recovery of life on Earth took significantly longer than after any other extinction event, possibly up to 10 million years.”

It has been suggested that this extinction was also the immediate consequence of an impact, but the evidence is inconclusive (partly because seafloor rocks are completely recycled on 200-million-year timescales).

Page 29: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

How Can We Protect Ourselves?

The critical point is early discovery.

Hence NEO (‘Near Earth Orbiter’) surveys and programs, to identify all the potential problem objects!

Page 30: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

‘Nudge’ it Out of its Current Path

Page 31: Theme 10 – Leftovers: Impacts and Mass Extinctions ASTR 101 Prof. Dave Hanes

…or Use Gravity