A typical rock formationib.berkeley.edu/courses/bio1b/evolutionfall11/pdfs/...A typical rock...
Transcript of A typical rock formationib.berkeley.edu/courses/bio1b/evolutionfall11/pdfs/...A typical rock...
A typical rock formation
Relative dating: some principles to follow...
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Principle of superposition
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Principle of original horizontality
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Principle of lateral continuity
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Principle of cross-cutting relationships
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Principle of inclusions
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Principles of unconformities (missing time)
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Radiometric Age Dating• Uses unstable isotopes of naturally
occurring elements. The isotopes decay: they change into different elements or different isotopes of the same element.
• The rate of decay is known (has been measured in the laboratory) for a variety of isotopes.
• When igneous rocks form, there is 100% parent and 0% daughter isotopes in the rock.
• The ratio of the parent and daughter isotopes can be measured using a mass spectrometer.
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Method Parent isotope
Daughter isotope Half life Dating range
Rubidium-strontium Rb-87 Sr-87 47 by 10m-4.6b
Uranium-lead U-238 Pb-206 4.5 by 10m-4.6b
Uranium-lead U-235 Pb-207 71.3 my 10m-4.6b
Thorium-lead Th-232 Pb-208 14.1 by 10m-4.6b
Potassium-argon K-40 Ar-40 1.3 by .1m-4.6b
Carbon-14 C-14 N-14 5730 y 100-100,000
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1999 GEOLOGIC TIME SCALECENOZOIC MESOZOIC PALEOZOIC
AGE(Ma)
EPOCH AGE PICKS(Ma)
MAGNETICPOLARITY PERIOD
HIST
.
ANO
M.
CHRO
N.
5
10
15
20
25
30
35
40
45
50
55
60
65
QUATER-NARY PLEISTOCENE
MIO
CENE
OLI
GO
CENE
TRIA
SSIC
JURA
SSIC
CRET
ACEO
US PERM
IAN
DEVO
NIAN
ORD
OVI
CIAN
SILU
RIAN
MIS
SISS
IPPI
ANPE
NNSY
LVAN
IAN
CAM
BRIA
N*CA
RBO
NIFE
ROUS
EOCE
NEPA
LEO
CENE
PLIOCENEPIACENZIANL
0.011.8
3.65.3
7.1
11.2
14.8
16.4
20.5
23.8
28.5
33.7
37.0
41.3
49.0
54.8
57.9
61.0
65.0
E
L
E
L
M
E
L
M
E
E
L
ZANCLEANMESSINIAN
TORTONIAN
SERRAVALLIAN
LANGHIAN
BURDIGALIAN
AQUITANIAN
CHATTIAN
RUPELIAN
PRIABONIAN
BARTONIAN
LUTETIAN
YPRESIAN
DANIAN
THANETIAN
SELANDIAN
CALABRIANHOLOCENE
TERT
IARY
PALE
OG
ENE
NEO
GEN
E1 C1
C2
C2A
C3
C3A
C4
C4A
C6
C6A
C6BC6C
C7
C8C9
C10
C11
C12
C13
C15C16
C17
C18
C19
C20
C21
C22
C23
C24
C25
C26
C27
C28
C29
C7A
C5
C5A
C5B
C5C
C5DC5E
22A
3
3A
44A
5
5B
5A
5C
66A
6B
7
8
910
1112
13
1516
17
18
19
20
21
22
23
24
25
28
29
26
27
7A
6C
5D5E
AGE(Ma)
EPOCH AGE PICKS(Ma)
UNCERT.(m.y.)
MAGNETICPOLARITY PERIOD
HIST
.
ANO
M.
CHRO
N.
AGE(Ma)
EPOCH AGE PICKS(Ma)PERIOD
70
260
280
300
320
340
380
360
400
420
440
460
480
500
520
540
80
90
100
110
120
130
140
150
160
170
180
190
210
200
220
230
240
NEO
COM
IAN
LATE
EARLY N.W
.S.
LATE
EARLY
MIDDLE
LATE
EARLY
MIDDLE
MAASTRICHTIAN65
248252256260
269
282
296303
290
323327
342
354
364370
380
391
400
412417419423428
443449
458464470
485490
500506512516
495
520
543
71.3 1
83.585.889.093.5
99.0
112
121
127
132
137
144
151154
164
159
CAMPANIAN
TATARIANUFIMIAN-KAZANIAN
KUNGURIAN
ARTINSKIAN
SAKMARIAN
ASSELIANGZELIAN
KASIMOVIANMOSCOVIAN
BASHKIRIANSERPUKHOVIAN
VISEAN
TOURNAISIAN
FAMENNIANFRASNIANGIVETIAN
EIFELIAN
EMSIANPRAGHIAN
LOCKHOVIANPRIDOLIANLUDLOVIAN
WENLOCKIAN
LLANDOVERIAN
ASHGILLIANCARADOCIANLLANDEILIANLLANVIRNIAN
ARENIGIAN
TREMADOCIANSUNWAPTAN*STEPTOEAN*MARJUMAN*
DELAMARAN*DYERAN*
MONTEZUMAN*
SANTONIANCONIACIANTURONIAN
CENOMANIAN
ALBIAN
APTIAN
BARREMIAN
HAUTERIVIAN
VALANGINIAN
BERRIASIAN
TITHONIAN
KIMMERIDGIANOXFORDIANCALLOVIAN
BATHONIAN
BAJOCIAN
AALENIAN
TOARCIAN
PLIENSBACHIAN
SINEMURIAN
HETTANGIAN
NORIAN
RHAETIAN
CARNIAN
LADINIAN
ANISIAN
OLENEKIANINDUAN
C31
C32
C33
31
3233
M0M1
M5
M10M12M14M16
M18M20M22
M25
M29
M3
169
176180
195
190
202206210
221
234
227
248245242
111
4
4
4
5
67
7
8
8
88
8
8
888
9
9
9
9910
1
2
3
3
.2
311
RAPI
D PO
LARI
TY C
HANG
ES
PRECAMBRIAN
PRO
TERO
ZOIC
ARCH
EAN
AGE(Ma)
EON ERABDY.AGES(Ma)
750
900
1600
2500
3000
3400
3800?
1000
1250
1500
1750
2000
2250
2500
2750
3000
3250
3500
3750
LATE
EARLY
MIDDLE
LATE
EARLY
MIDDLE
L
L
M
E
E
E
E
D
C
B
A
L
L
L
M
30 C30
30 C30
C3434
543
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Paleomagnetics
Earth has a dipole magnetic field, with the direction in line with the axis of spin.
When rocks form, they are permanently magnetized in the direction of the current magnetic latitude.
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Plate Tectonics
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Fossils
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A fossil is any recognizable evidence of preexisting life.
Types of fossils: (1) Trace fossils (2) Preserved material
Fossils are our only direct evidence ofwhat organisms looked like in the past.
The fossil record is a biased one.
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Where is the time?
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Taphonomy: The study of the process of fossilization, from death of the organismto discovery by the paleontologist.
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Types of biases in the fossil record
• Fossils with no hard parts are rarely preserved. Fossil record is mostly a record of shells and bones.
• Organisms that lived in areas where they are likely to be preserved.
• Time averaging of fossil beds.
• Post-mortem transport, scavenging,
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Diatoms Foraminifera
Microfossils
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“Invertebrates”
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Vertebrates
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Stromatolites
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TransitionalForms
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Basilosaurus hind leg
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Ankle bones of the archaeocetes Rodhocetus (Eocene)on the left, a pronghorn (middle) and Artiocetus (right).Note the double-pulleyed astragalus. Other features in common are a notched cuboid and a prominent fibular facet.
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Tiktaalik roseae (late Devonian)Wednesday, October 26, 11
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Microfossils from the Apex Chert, North Pole, Australia
About 3.465 billion years old, resembling filamentous cyanobacteria
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Stromatolite, North Pole deposits, Western Australia
about 3.5 billion years old
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Extant stromatolite showing closeup of cyanobacteria
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Proterozoic (2.5 bya to 544 mya). Evolution of organisms with oxygenic photosynthesis caused an increase in oxygen levels. Rising oxygen levels in the world’s oceans caused the formation of iron oxide, often preserved in the banded iron formation.
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Eukaryotic milestones
• 2.7 bya: chemical traces of eukaryotic-type lipids in fossil organic matter (controversial).
• 2.1 bya: Grypania spiralis, the first fairly well-accepted fossil eukaryote
• 1.6-1.8 bya: origin of single-celled algae of unknown type, known as acritarchs
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Grypania spiralis from Michigan
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acritarch
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