ess200a prof. jin-yi yu plate tectonics and climateyu/class/ess200a.2004/lecture.6... · 2005. 9....
TRANSCRIPT
1
ESS
200A
Pro
f. J
in-Y
i Yu
Lec
ture
6: S
olid
Ear
th (
Out
line)
Clim
ate
Rol
e of
the
Solid
Ear
th
Inte
rnal
Str
uctu
re o
f th
e So
lid E
arth
The
ory
of P
late
Tec
toni
cs
His
tory
of
Pla
te T
ecto
nics
Fro
mT
he B
lue
Pla
net
ESS
200A
Pro
f. J
in-Y
i Yu
Pla
te T
ecto
nics
and
Clim
ate
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
How
can
one
acc
ount
for
the
alte
rnat
ing
peri
ods
of c
limat
ic w
arm
th a
nd
cool
ness
obs
erve
d in
the
geol
ogic
rec
ord?
Par
t of
the
answ
er m
ust l
ie in
the
tect
onic
act
ivity
and
the
posi
tions
of
the
cont
inen
ts.
ESS
200A
Pro
f. J
in-Y
i Yu
Tec
toni
c-S
cale
Cli
mat
e C
hang
e
The
fai
nt y
oung
Sun
pa
rado
x an
d its
pos
sibl
e ex
plan
atio
n.
Why
was
Ear
th ic
e-fr
ee
even
at t
he p
oles
100
Myr
ag
o (t
he M
esoz
oic
Era
)?
Wha
t cau
sed
Ear
th’s
cl
imat
e to
coo
l ove
r th
e la
st 5
5 M
yr(t
he C
enoz
oic
Era
)?
Ice-
free
Ear
th
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
ESS
200A
Pro
f. J
in-Y
i Yu
Pla
te T
ecto
nics
Con
tine
ntal
Dri
ftin
g T
heor
yA
lfre
d W
egen
er p
ropo
sed
that
all
the
cont
inen
ts
wer
e on
ce a
ssem
bled
into
a s
uper
cont
inen
t (P
ange
a) a
nd th
en b
roke
and
slo
wly
dri
fted
to th
eir
curr
ent p
ositi
ons.
Pla
te T
ecto
nics
The
bra
nch
of te
cton
ics
that
dea
ls w
ith
the
proc
esse
s by
whi
ch th
e lit
hosp
here
pla
tes
mov
e an
d in
tera
ct w
ith e
ach
othe
r is
cal
led
plat
e te
cton
ics.
2
ESS
200A
Pro
f. J
in-Y
i Yu
Cir
cula
tion
of th
e So
lid E
arth
Col
d L
ithos
pher
e
Fro
mT
he B
lue
Pla
net
The
ris
ing
hot r
ocks
and
slid
-aw
ay f
low
s ar
e th
ough
t to
be th
e fa
ctor
th
at c
ontr
ol th
e po
sitio
ns o
f oc
ean
basi
ns a
nd c
ontin
ents
.
The
con
vect
ion
dete
rmin
es th
e sh
ape
of th
e E
arth
.E
SS20
0AP
rof.
Jin
-Yi Y
u
Tw
enty
Rig
id P
late
s
Wha
t can
hap
pen
to th
e co
ld b
ound
ary?
The
lith
osph
ere
has
brok
en in
to a
num
ber o
f ro
cky
piec
es, c
alle
dpl
ates
.
The
re a
re a
few
larg
e pl
ates
plu
s a
num
ber
of s
mal
ler
one
com
pris
e th
e E
arth
’s s
urfa
ce (
a to
tal o
f 20
pla
tes)
.
The
pla
tes
rang
e fr
om s
ever
al h
undr
ed to
sev
eral
thou
sand
kilo
met
ers
in
wid
th.
Fro
mT
he B
lue
Pla
net
ESS
200A
Pro
f. J
in-Y
i Yu
Con
tinen
tal a
nd O
cean
ic C
rust
s
Som
e lit
hosp
heri
cpl
ates
are
com
pose
d pr
imar
ily
of
ocea
nic
crus
tal m
ater
ial,
whe
reas
oth
ers
are
com
pose
d pr
imar
ily o
f co
ntin
enta
l mat
eria
ls.
The
con
tinen
ts s
tand
, on
aver
age,
abo
ut 4
.5 k
m
abov
e th
e fl
oor
of th
e oc
ean
basi
ns.
Con
tine
ntal
cru
st is
rel
ativ
ely
ligh
t (de
nsit
y 2.
7
g/cm
3), w
here
as o
cean
ic c
rust
is r
elat
ivel
y he
avy
(den
sity
clo
se to
3.2
g/c
m3)
.E
SS20
0AP
rof.
Jin
-Yi Y
u
Tem
pera
ture
Str
uctu
res
in th
e So
lid E
arth
Fro
mT
he B
lue
Pla
net
The
lith
osph
eric
pla
tes
are
ridi
ng o
n to
p of
a la
yer
of h
ot, d
uctil
e, e
asily
de
form
ed m
ater
ial c
alle
d th
e as
then
osph
ere,
or
“wea
k la
yer”
.
Hea
t mov
es b
y co
nduc
tion
abov
e 10
0 km
and
by
conv
ectio
n be
low
100
km
.
Tem
pera
ture
at t
he c
ente
r of
the
eart
h is
bel
ieve
d to
clo
se to
500
0ºC
.
3
ESS
200A
Pro
f. J
in-Y
i Yu
Hea
t In
Ear
th’s
Int
erio
r
The
re a
re tw
o m
ajor
sou
rces
of
the
heat
in E
arth
’s
inte
rior
:
(1)
Rad
ioac
tive
deca
y: o
f po
tass
ium
, ura
nium
, and
th
oriu
m.
(2)
Res
idua
l hea
t fro
m E
arth
’s f
orm
atio
n: A
tr
emen
dous
am
ount
of
ener
gy w
as tr
ansf
erre
d to
Ear
th
duri
ng th
e ac
cret
ion
of th
e pl
anet
by
colli
sion
s w
ith
plan
etes
imal
s.
ESS
200A
Pro
f. J
in-Y
i Yu
The
The
ory
of P
late
Tec
toni
cs
A m
ajor
pro
blem
of
the
cont
inen
t dri
ftin
g th
eory
is: H
ow c
ould
the
cont
inen
ts d
rift
th
roug
h th
e ri
gid
sea
floo
r?
Thi
s pr
oble
m is
ans
wer
ed b
y th
e se
aflo
or
spre
adin
g hy
poth
esis
: Con
tine
nts
do n
ot p
low
th
roug
h th
e se
a fl
oor.
Con
tine
nts
and
segm
ents
of
oce
an fl
oor
are
conn
ecte
d in
to p
late
s th
at
cont
inuo
usly
mov
e aw
ay fr
om o
ne a
noth
er a
t m
id-o
cean
rid
ges.
ESS
200A
Pro
f. J
in-Y
i Yu
Sea
floo
r S
prea
ding
(fro
mT
he e
arth
Sys
tem
)
ESS
200A
Pro
f. J
in-Y
i Yu
Pla
te M
argi
nsIn
tera
ctio
ns b
etw
een
plat
es o
ccur
alo
ng
thei
r ed
ges.
The
re a
re th
ree
type
s of
pla
te
mar
gins
:
(1)
Div
erge
nt m
argi
ns
form
mid
-oce
an r
idge
s (o
ver
ocea
ns)
and
rift
val
leys
(ov
er la
nds)
(2)
Con
verg
ent m
argi
ns
form
dee
p-se
a tr
ench
es (
two
ocea
nic
plat
es
or o
cean
+con
tinen
tal p
late
s) o
r hi
gh
mou
ntai
ns (
such
as
Tib
etan
Pla
teau
) (t
wo
cont
inen
tal p
late
s).
(3)
Tra
nsfo
rm f
ault
mar
gins
form
ear
thqu
ake
faul
ts
Fro
mT
he B
lue
Pla
net
4
ESS
200A
Pro
f. J
in-Y
i Yu
Thr
ee W
ays
for
Solid
Ear
th to
Aff
ect C
lim
ate
Pol
ar p
osit
ion
hypo
thes
is
Che
mic
al W
eath
erin
g H
ypot
hesi
s
Seaf
loor
Spr
eadi
ng H
ypot
hesi
s
ESS
200A
Pro
f. J
in-Y
i Yu
The
Pol
ar P
ositi
on H
ypot
hesi
s
The
pol
ar p
ositi
on h
ypot
hesi
s fo
cuse
d on
la
titu
dina
l pos
ition
as
a ca
use
of g
laci
atio
n of
co
ntin
ents
.
Thi
s hy
poth
esis
sug
gest
ed th
at ic
e sh
eets
sh
ould
app
ear
on c
ontin
ents
whe
n th
ey a
re
loca
ted
at p
olar
or
near
-pol
ar la
titu
des.
To
expl
ain
the
occu
rren
ce o
f ice
hous
e in
terv
als,
this
hyp
othe
sis
call
s no
t on
wor
ldw
ide
clim
ate
chan
ges
but s
impl
y on
the
mov
emen
ts o
f con
tinen
ts o
n te
cton
ic p
late
s.
Thi
s hy
poth
esis
can
not
exp
lain
the
clim
ate
of th
e L
ate
Prot
eroz
oic
Era
, whe
n bo
th
cont
inen
ts a
nd g
laci
ers
appe
ar to
hav
e be
en
situ
ated
at r
elat
ivel
y lo
w la
titu
des.
It c
an n
ot e
xpla
in th
e w
arm
Mes
ozoi
c E
ra
whe
n hi
gh-l
atitu
de c
ontin
ents
wer
e pr
esen
t bu
t wer
e al
mos
t com
plet
ely
ice-
free
.(f
rom
Ear
th’s
Cli
mat
e: P
ast a
nd F
utur
e)
ESS
200A
Pro
f. J
in-Y
i Yu
Clim
ate
Cha
nges
in th
e L
ast 5
00 M
yr
Clim
ate
in th
e pa
st 5
00 m
illio
n ye
ars
have
alte
rnat
ed b
etw
een
long
pe
riod
s of
war
m c
limat
e an
d sh
ort p
erio
ds o
f co
ld c
limat
e.
Dur
ing
the
last
500
mill
ion
year
s, m
ajor
con
tinen
t-si
ze ic
e sh
eets
ex
iste
d on
Ear
th d
urin
g th
ree
iceh
ouse
ear
: (1)
a b
rief
inte
rval
near
430
M
yr a
go, (
2) a
muc
h lo
nger
inte
rval
fro
m 3
25 to
240
Myr
ago
, and
(3)
th
e cu
rren
t ice
hous
e er
a of
the
last
35
mill
ion
year
.
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
ESS
200A
Pro
f. J
in-Y
i Yu
Che
mic
al W
eath
erin
gT
he p
reci
pita
tion
proc
ess
in th
e at
mos
pher
e di
ssol
ve a
nd r
emov
e C
O2
from
the
atm
osph
ere.
Roc
ks e
xpos
ed a
t Ear
th’s
sur
face
un
derg
o ch
emic
al a
ttac
k fr
om th
is
rain
of
dilu
te a
cid.
Thi
s w
hole
pro
cess
is k
now
n as
ch
emic
al w
eath
erin
g.
The
rat
e of
che
mic
al w
eath
erin
g te
nd
to in
crea
se a
s te
mpe
ratu
re in
crea
ses.
Wea
ther
ing
requ
ires
wat
er a
s a
med
ium
bot
h fo
r th
e di
ssol
utio
n of
m
iner
als
and
for
the
tran
spor
t of
the
diss
olve
d m
ater
ials
to th
e oc
ean
The
rat
e of
che
mic
al w
eath
erin
g in
crea
ses
as p
reci
pita
tion
incr
ease
s.
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
5
ESS
200A
Pro
f. J
in-Y
i Yu
Neg
ativ
e Fe
edba
ck F
rom
Che
mic
al W
eath
erin
g
The
che
mic
al w
eath
erin
g w
orks
as
a ne
gati
ve
feed
back
that
mod
erat
es
long
-ter
m c
limat
e ch
ange
.
Thi
s ne
gati
ve f
eedb
ack
mec
hani
sm li
nks
CO
2le
vel i
n th
e at
mos
pher
e to
the
tem
pera
ture
and
pr
ecip
itatio
n of
the
atm
osph
ere.
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
ESS
200A
Pro
f. J
in-Y
i Yu
Ear
th’s
The
rmos
tat –
Che
mic
al W
eath
erin
g
Che
mic
al w
eath
erin
g ac
ts a
s E
arth
’s th
erm
osta
t an
d re
gula
te it
s lo
ng-t
erm
clim
ate.
Thi
s th
erm
osta
t mec
hani
sm
lies
in tw
o fa
cts:
(1
) th
e av
erag
e gl
obal
rat
e of
ch
emic
al w
eath
erin
g de
pend
s on
the
stat
e of
Ear
th’s
clim
ate,
(2
) w
eath
erin
g al
so h
as th
e ca
paci
ty to
alte
r th
at s
tate
by
regu
latin
g th
e ra
te w
hich
CO
2is
rem
oved
fro
m th
e at
mos
pher
e.(f
rom
Ear
th’s
Cli
mat
e: P
ast a
nd F
utur
e)
ESS
200A
Pro
f. J
in-Y
i Yu
Fain
t You
ng S
un P
arad
ox
Sola
r lu
min
osit
y w
as m
uch
wea
ker
(~30
%)
in th
e ea
rly
part
of
Ear
th’s
his
tory
(a
fain
t you
ng
Sun)
.
If E
arth
’s a
lbed
o an
d gr
eenh
ouse
ef
fect
rem
aine
d un
chan
ged
at th
at
time,
Ear
th’s
mea
n su
rfac
e te
mpe
ratu
re w
ould
be
wel
l bel
ow
the
free
zing
poi
nt o
f w
ater
dur
ing
a la
rge
port
ion
of it
s 4.
5 B
yrhi
stor
y.
Tha
t wou
ld r
esul
t in
a “s
now
ball”
Ear
th, w
hich
was
not
evi
dent
in
geol
ogic
rec
ord.
(fro
m T
he E
arth
Sys
tem
)E
SS20
0AP
rof.
Jin
-Yi Y
u
Tec
toni
c C
ontr
ol o
f C
O2
Inpu
t–T
he S
eafl
oor
Spre
adin
g R
ate
Hyp
othe
sis
Dur
ing
activ
e pl
ate
tect
onic
pro
cess
es, c
arbo
n cy
cles
con
stan
tly
betw
een
Ear
th’s
inte
rior
and
its
surf
ace.
The
car
bon
mov
es f
rom
dee
p ro
ck r
eser
voir
s to
th
e su
rfac
e m
ainl
y as
CO
2ga
s as
soci
ated
with
vo
lcan
ic a
ctiv
ity a
long
the
mar
gins
of
Ear
th’s
te
cton
ic p
late
s.
The
cen
terp
iece
of
the
seaf
loor
spr
eadi
ng
hypo
thes
is is
the
conc
ept t
hat c
hang
es in
the
rate
of
sea
floo
r sp
read
ing
over
mill
ions
of
year
s co
ntro
l the
rat
e of
del
iver
y of
CO
2to
the
atm
osph
ere
from
the
larg
e ro
ck r
eser
voir
of
carb
on, w
ith th
e re
sulti
ng c
hang
es in
atm
osph
eric
C
O2
conc
entr
atio
ns c
ontr
ollin
g E
arth
’s c
lim
ate.
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
6
ESS
200A
Pro
f. J
in-Y
i Yu
Tec
toni
c C
ontr
ol o
f C
O2
Rem
oval
–T
he
Upl
ift W
eath
erin
g H
ypot
hesi
s
The
upl
iftin
g w
eath
erin
g hy
poth
esis
as
sert
s th
at th
e gl
obal
mea
n ra
te o
f ch
emic
al w
eath
erin
g is
hea
vily
aff
ecte
d by
the
avai
labi
lity
of f
resh
roc
k an
d m
iner
al s
urfa
ces
that
the
wea
ther
ing
proc
ess
can
atta
ck.
Thi
s hy
poth
esis
sug
gest
s th
at te
cton
ic
uplif
ting
enha
nces
the
expo
sure
of
fres
hly
frag
men
ted
rock
whi
ch is
an
impo
rtan
t fac
tor
in th
e in
tens
ity
of
chem
ical
wea
ther
ing.
Thi
s hy
poth
esis
look
s at
che
mic
al
wea
ther
ing
as th
e ac
tive
driv
er o
f cl
imat
e ch
ange
, rat
her
than
as
a ne
gativ
e fe
edba
ck th
at m
oder
ates
clim
ate
chan
ges.
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)
ESS
200A
Pro
f. J
in-Y
i Yu
Can
The
se T
wo
Hyp
othe
ses
Exp
lain
T
ecto
nic-
Scal
e C
limat
e C
hang
es?
(fro
m E
arth
’s C
lim
ate:
Pas
t and
Fut
ure)