K/T Extinction

ssealey 5,569 views 23 slides Oct 18, 2013
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CRETACEOUS-TERTIARY
EXTINCTION
GLY 5020 EARTH HISTORY – DR. FARLEY
UNIVERSITY OF NORTH CAROLINA
PEMBROKE
FALL 2009
SARAH SEALEY


Occurs when the last representative of a
taxon dies.

For Earth History, extinction is the last, or
most recent, occurrence of an identifiable
fossil.

MASS EXTINCTION

Greater than 50% of all species die at similar
time

Geologically short intervals of intense
species extinction

Mass Extinction Events of Greatest Severity
60% Terrestrial 90%
Marine

Patterns during Mass Extinction
Occurs in both terrestrial and marine
environments
On land, animals suffer yet plants seem highly
resistant
Disappearance of tropical life forms
Tendency of certain animal groups to experience
and survive (trilobites and ammonoids)
Periodicity in geological time (occurring about
every 26 million years)

Extinction Agents

Catastrophic

Extraterrestrial impacts such as meteorites
or comet showers

Geologic

Volcanism, glaciation, sea levelvariations,
global climactic changes, oxygen/salinity
level changes in ocean

K/T Extinction 65 MYA

Victims

Many species of coccolithophorid: never recover diversity

Many species of foram

All ammonoids

All belemnoids

All rudists

All plesiosaurs

All mosasaurs

All pterosaurs

All non-flying dinosaurs

Several clades of birds

Many mammal groups (only monotreme prototheres, multituberculate allotheres, the ancestors
and closest relatives of the marsupials among the metatheres, and the ancestors and closest
relatives of the placentals among the eutheres)

Proposed Causes: The Maastrichtian
Regression
Draining of epeiric seas would alter terrestrial
climate

Increased Maastrichtian volcanism,
especially the Deccan Traps

Decrease insolation (incoming sunlight) by presence
of fine particles in high atmosphere

Also change Earth's albedo, although not as
dramatically

Would operate on the scale of a few tens of
thousands to hundreds of thousands of years

The Chicxulub Impact

1980 – Walter Alvarez

Hypothesized: an asteroid impacted Earth at
the K/T boundary

Evidence:

Iridium

Shocked Quartz

Tektites

Chicxulub Crater
10-15 km diameter
(size of Manhattan)

IridiumGGGGG LY 502EARY0THGAH5 YIG
SOAAO2G02GAH5 YY0SG
–5HDO0.–GFE5GUHDNGD DHG02G
V D5CP–GSDE–5M
Platinum-like metal,
common in metallic
asteroids but very rare in
Earth's crust.

Shocked Quartz

Tektites

Tektites

Probable EffectsGLY 5052 EA0
G
GLYL 5L0Y2E502A0LRLTHI0RL T0SO– DE.0A2TO0
FUHL0DT ELTN0VCP0M0VB
P
0OLH E2R5KK0
G
9UT5E02A0YSHFE02UY0 –2TS L0O ELTS Y0A2T0
!SY2OLELT50 T2UR.0"U5E0YS!L0EFLTO2RUDYL T0
L –2R50
G
9Y 5E0 L02UY0L 5E EL0RL T#I0TLHS2R$0SE0
2UY0#L0ALYE0 T2UR0EFL02TY.0#UE0LDTL 5L0
SEF0S5E RDL0
G
%F2D! L50AT2O0SO– DE02UY0HLRLT EL0
FUHL0E5UR OS50&'ES Y'0 L5(0
Short term:

Release lots of energy near impact, form
huge crater: 1.8 x 10
8
megatons!!

Burst of light would vaporize material for
kilometers around, just like thermonuclear
weapons

Blast wave would devastate nearby region; it
would be felt around the world, but decrease
with distance

Shockwaves from impact would generate
huge tsunamis ("tidal" waves)

Longer term:

Material vaporized by impact kicked high up in
atmosphere: reduced amount of incoming sunlight

Observations on Mars showed big temperature
drops due to high-level particles

In human history, eruption of Tambora in
Indonesia in 1815 produced chilling effects
worldwide for more than a year later

Dust and ash would block out sunlight, reducing
photosynthesis and killing off plants on land and
surface algae in water; herbivores feeding on these
would die; carnivores feeding on these would starve
(after a brief feast)

Collapse of foodwebs would require long term to
recover, as many parts of each foodchain might be
lost

Additional possible effects include:

Superacid rain

Global firestorms

Global tsunami

Tsunami

Crater Animation
BOOM!
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