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