earth history, ch. 191 cenozoic tectonics final break-up of pangaea destruction of tethys ocean...

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Earth History, Ch. 19 1 Cenozoic tectonics • Final break-up of Pangaea • Destruction of Tethys ocean – Alpine—Himalaya orogenic belt

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Page 1: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 1

Cenozoic tectonics

• Final break-up of Pangaea

• Destruction of Tethys ocean– Alpine—Himalaya orogenic belt

Page 2: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 2

Page 3: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 3

Page 4: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 4

Page 5: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 5

Page 6: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 6

Page 7: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 7

Page 8: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 8

Destruction of the Tethyan Seaway

• In Neogene time, Indian Subcontinent and several smaller continental fragments of Gondwanaland collided with Eurasia

• Result was Himalaya Mountains, mountains of the “Near East”, and Alps

• Today, only the Mediterranean Sea, Black Sea, Caspian Sea, and Aral Sea are vestiges of the former Tethyan Seaway

Page 9: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 9

Final driftof IndianSubcontinent

Page 10: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 10

Closure ofTethys Seaway

Page 11: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 11

Continental glaciation

• Early Neogene climate was relatively mild

• In mid-Pliocene time, ~3.2 million years ago, modern ice age began

• Ice age continues today, although glacial maxima and minima are cyclical, and we are now in an “interglacial” episode

Page 12: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 12

NorthernHemispherecontinentalglaciers

Maximum extent ofPleistocene icecap

Page 13: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 13

Continental glaciationBering Land Bridge was largely ice-free and a corridor for faunal interchange between North America and Asia

Page 14: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 14

Waxing and waning of glaciers

• High frequency glacial and interglacial cycles:– Periodic changes in the tilt of Earth’s axis relative to

plane of orbit

– Periodic changes in the orbit itself, due to gravitational pull of other planets

• Cycles can be documented through oxygen isotope records

• Waxing and waning has displaced plant ecosystems by up to 20° latitude

Page 15: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 15

Oxygenisotoperecord

(these should bepositive numbers)

Page 16: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 16

Displacement of floral ecosystems

Page 17: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 17

Origin of the Great Lakes and Lake Bonneville

• Retreat of glaciers after the most recent glacial interval left behind large basins that eventually filled with water– Great Lakes formed within the past 10,000 to

15,000 years– Lake Bonneville covered much of Utah; now

the Great Salt Lake is a “tiny” remnant

Page 18: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 18

Great Lakes and Lake Bonneville

Page 19: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 19

Finals

• 4th lecture exam is Wed. @ 10:00am

• Copy of last year’s test is on the web

Page 20: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 20

Maximum extent ofPleistocene icecap

Page 21: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 21

What was the ultimate cause of Pliocene-Pleistocene glaciation?

• Probably related to creation of Isthmus of Panama– Modification of global ocean currents– Separation of Atlantic and Pacific oceans

resulted in dramatic cooling of Arctic Ocean water

Page 22: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 22

Page 23: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 23

Page 24: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 24

Human Evolution:Superfamily Hominoideaincludes gibbons, man,and apes.

Homo is the only genusin Family Hominidae;sapiens is the only speciesin the genus Homo.

Page 25: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 25

Early origins

• Earliest “hominoid” fossils are from Africa, ~20 Ma (early Miocene)

• These early “hominoids” are probably ancestral to both modern hominids and pongiids, but fossil record is spotty

• mid- to late-Miocene was a time of “hominoid” radiation throughout Africa and Eurasia (more “apes” then than now!)

• By latest Miocene time, only one genus had survived: Gigantopithecus

Page 26: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 26

Gigantopithecus

Page 27: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 27

Australopithecines • Earliest true hominids appeared at Miocene-

Pliocene transition, ~5.3 Ma*, the australopithecines– Australopithecus, Paranthropus, et al.

• Australopithecus (4.0-2.3 Ma) was somewhat intermediate in appearance between modern apes and humans (but not an evolutionary intermediate):– Males larger than females (4.5 ft vs. 3.5 ft)– Brain size barely larger than modern chimp– Bi-pedal, but spent much time in trees

Page 28: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 28

Australopithecus

“Lucy”, a female of thespecies A. afarensis,found in 3.2 Ma bedsIn Ethiopia

Page 29: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 29

Bi-pedalAustralopithecustracks preservedin volcanic ash,~3.0 Ma, fromTanzania

Page 30: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 30

Reconstruction ofAustralopithecus

Shoulder joint typical ofarborescent apes:long arms, strong wrists, long curved fingers

Page 31: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 31

Early Homo

• Australopithecus branched into at least two species (A. afarensis and A. africanus)

• earliest Homo originated from Australopithecus approximately 2.4 Ma

• By 2.0 Ma, at least two species of early Homo were in existence

Page 32: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 32

Hominidstratigraphy

Page 33: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 33

Early Homo

• Characteristics of early Homo:– Large brain (800 cm3 vs only 450 cm3 for

Australopithecus)– Smaller teeth– Ability to make and use stone tools

• Meat in diet

– Spent most of the time on the ground (not in trees)

Page 34: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 34

Skull of Homo habilis

Page 35: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 35

Brain size vs. mode of life• Brain of all newborn primates = ~10% of body

weight– Brain growth stops shortly after birth in monkeys and

apes– Brain growth continues for ~1 year in Homo

• Homo development is delayed relative to chimps and apes

• Delayed maturation of Homo requires significant parental care– Parents must hold babies, thus arms not free to hold tree

branches

Page 36: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 36

Brain size vs. mode of life

• Development of large brain may be related to climate change in Africa (~2.5 Ma):– Drying out of climate reduced forests– Life on ground may have paved the way for

prolonged parental care– “Obligatory” bipedalism probably preceeded

increase in brain size

Page 37: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 37

Homo erectus

• Homo erectus evolved from early Homo approximately 1.6 Ma

• First hominid to migrate beyond Africa– “Peking Man”, “Java Man”

• Looked similar to modern humans, but:– Slightly smaller brain (1000 cm3 vs 1400 cm3)– Narrower pelvis

Page 38: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 38

Homo erectus

Bones of an 11 or 12 yearold boy (1.6 Ma)

Page 39: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 39

Homo neanderthalensis

• Neanderthal fossils are known in Eurasia in beds ranging from 100,000 to 35,000 years old– Probably originated from a European or Asian

population of H. erectus or related species

• Fossils commonly found in cave deposits– Probably practiced some form of religion– Buried dead family members with food and

tools

Page 40: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 40

Neanderthalburial

Page 41: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 41

Homo sapiens

• Homo sapiens (modern humans) originated in Africa ~150,000 ybp (presumably from an African popolation of H. erectus or related species)

• DNA from H. sapiens and H. neanderthalensis indicates that ancestral populations may have diverged by 500,000 ybp

Page 42: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 42

Homo sapiens

• Homo sapiens seemingly stayed in Africa for several tens of thousands of years before migrating to Europe

• Oldest European fossils of H. sapiens are ~33,000 ybp—about the same time H. neanderthalensis vanished

Page 43: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 43

Postscript: New discovery (2002)

Earliest hominid:Sahelanthropus tchadensis,6 to 7 Ma fossils fromChad

Much earlier origin and wider dispersal ofhuman lineage thanpreviously thought

Michel Brunet

Page 44: Earth History, Ch. 191 Cenozoic tectonics Final break-up of Pangaea Destruction of Tethys ocean –Alpine—Himalaya orogenic belt

Earth History, Ch. 19 44

bipedalism

climate change

increase in brain capacity

1st widespread hominidEurasian hominid

African emmigrant

(widespread early hominids prior to 5.3 Ma)