Download - Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Transcript
Page 1: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Ast

rono

my

210

Sect

ion

1–M

WF

150

0-15

5013

4 A

stro

nom

y B

uild

ing

Thi

s C

lass

(L

ectu

re 2

5):

Deb

ris

Nex

t Cla

ss:

Bir

th o

f th

e So

lar

Syst

em

Mus

ic: A

my

Hit

the

Atm

osph

ere

–C

ount

ing

Cro

ws

2ndH

our

Exa

m in

2 w

eeks

!

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Out

line

•Pl

uto–

Plan

et o

r L

arge

st K

uipe

r B

elt O

bjec

t?

•L

ife

in o

ur S

olar

Sys

tem

?

•C

omet

s–Y

ou D

irty

Ice

ball

•A

ster

oids

–Sp

acec

raft

haz

ard?

•M

eter

oids

–w

atch

you

r he

ad

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

No

luna

r la

ndsc

ape,

no

Mar

tian

dese

rt c

anco

mpa

re to

the

terr

ifyin

g so

litud

e of

Plu

to.

Pat

rick

Moo

re a

nd D

avid

A. H

ardy

Cha

lleng

e of

the

Sta

rs(1

972)

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Cly

de T

omba

ugh

(190

6 –

1997

)

The

Dis

cove

ry o

f P

luto

•A

stro

nom

ers

calc

ulat

ed th

at th

ere

mus

t be

anot

her

body

per

turb

ing

the

orbi

ts o

f U

ranu

s an

d N

eptu

ne•

Perc

ival

Low

ell c

alcu

late

d th

at

“Pla

net X

” m

ust h

ave

a m

ass

7 tim

es

that

of

the

Ear

th•

Cly

de T

omba

ugh

was

hir

ed to

look

fo

r it

•In

193

0, h

e fo

und

a pl

anet

•In

hon

or o

f L

owel

l, it

was

nam

ed

Plut

o (P

.L.)

Page 2: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

For

tuna

te M

ista

ke

•It

turn

ed o

ut th

at

Plut

o w

as n

ot

Low

ell’

s “P

lane

t X”

•Pl

uto

has

only

0.

2% th

e m

ass

of

Ear

th, n

ot 7

tim

es

the

mas

s•

Too

sm

all t

o in

flue

nce

Ura

nus

& N

eptu

ne’s

orb

its•

Mod

ern

obse

rvat

ions

and

cal

cula

tions

sho

w n

o “P

lane

t X”

need

ed to

pre

dict

thei

r or

bits

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Rad

ius

0.19

Ear

thSu

rfac

e gr

avity

0.04

Ear

thM

ass

0.00

2 Ea

rth

Aver

age

Dis

tanc

e fr

om S

un39

.5 A

UTi

lt of

Rot

atio

n Ax

is12

2 de

gree

sO

rbit

ecce

ntric

ity0.

249

Year

248.

6 Ea

rth

year

sSo

lar

day

6.39

Ear

th d

ays

(bac

kwar

ds)

Ear

th -

Plu

to C

ompa

riso

n

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

How

Doe

s P

luto

Mea

sure

Up?

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to’s

Orb

it

•H

ighl

y ec

cent

ric

•H

ighl

y in

clin

ed

with

re

spec

t to

the

othe

r pl

anet

s•

From

197

9-19

99,

Plut

o w

as c

lose

r to

the

Sun

than

Nep

tune

!•

Nev

er w

ill c

ollid

e be

caus

e of

3:2

res

onan

ce w

ith N

eptu

ne

Page 3: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to’s

Sur

face

•N

o sp

acec

raft

has

ev

er v

isite

d Pl

uto

•O

ur b

est v

iew

of

Plut

o co

mes

fro

m

Hub

ble

•C

over

ed in

nitr

ogen

, m

etha

ne, a

nd c

arbo

n m

onox

ide

ice

•C

urre

nt s

urfa

ce te

mpe

ratu

re -

abou

t 40

K (

-230

C,

-390

F)!

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to’s

Atm

osph

ere

•O

bser

ved

whe

n Pl

uto

occu

lts

back

grou

nd s

tars

•C

onsi

sts

mos

tly o

f ni

trog

en

(90%

) an

d ca

rbon

mon

oxid

e–

Sim

ilar

to T

rito

n

•A

s Pl

uto

gets

far

ther

fro

m

the

Sun,

atm

osph

ere

may

“f

reez

e ou

t” a

roun

d 20

20

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to’s

Moo

n, C

haro

n•

In 1

977,

Plu

to w

as

foun

d to

hav

e a

moo

n•

Lar

gest

moo

n re

lativ

e to

hos

t pla

net

–A

bout

120

0 km

acr

oss

–A

bout

12%

Plu

to’s

mas

s

•Su

rfac

e co

vere

d in

w

ater

ice

•B

oth

rota

te s

ynch

rono

usly

–Pl

uto

and

Cha

ron

each

kee

p th

e sa

me

face

poi

nted

tow

ards

the

othe

r

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to’s

Moo

n, C

haro

n

•In

197

7, P

luto

was

fo

und

to h

ave

a m

oon

•L

arge

st m

oon

rela

tive

to h

ost p

lane

t•

Abo

ut 1

200

km a

cros

s–

Abo

ut 1

2% P

luto

’s m

ass

•Su

rfac

e co

vere

d in

w

ater

ice

•B

oth

rota

te s

ynch

rono

usly

–Pl

uto

and

Cha

ron

each

kee

p th

e sa

me

face

poi

nted

tow

ards

the

othe

r

Page 4: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Inte

rior

s &

Com

posi

tion

•Pl

uto

is s

imila

r in

den

sity

and

si

ze to

Nep

tune

’s

moo

n T

rito

n•

Lik

ely

a si

mila

r co

mpo

sitio

n, a

ro

ck/ic

e m

ix

(60/

40)

•R

ocky

cor

e, s

urro

unde

d by

wat

er-i

ce m

antle

•Si

nce

it is

sm

alle

r, C

haro

nis

pro

babl

y no

t dif

fere

ntia

ted

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Cu

rren

tly

pla

nn

ed f

or

lau

nch

in 2

006

htt

p:/

/plu

to.jh

uap

l.ed

u

New

Hor

izon

s

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e in

our

Sol

ar S

yste

m

Con

clus

ions

•N

o co

nclu

sive

evi

denc

e ex

ists

for

life

in o

ur s

olar

sy

stem

bes

ides

on

Ear

th

•B

ut, p

ossi

bilit

ies

exis

t for

life

–V

enus

may

hav

e lif

e in

the

clou

ds th

at m

igra

ted

whe

n po

ssib

le o

cean

s bo

iled

away

.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e on

Ven

us?

•Su

rfac

e is

far

too

hot

–If

lead

is li

quid

, thi

nk o

f w

hat h

eat w

ould

do

to

com

plex

org

anic

pol

ymer

s

–N

o co

oler

pol

ar r

egio

ns e

xist

•H

eat i

s un

ifor

m!

•B

ut, h

igh

in th

e cl

ouds

it s

houl

d be

co

oler

?!

–M

aybe

life

can

stil

l exi

st in

the

clou

ds?

Page 5: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Ven

us C

hem

ical

Dis

equi

libri

um

•A

t 50

km u

p, th

e te

mpe

ratu

re is

not

too

hot a

nd

the

pres

sure

is 1

atm

osph

ere.

•H

igh

clou

ds in

the

atm

osph

ere

cont

ain

chem

ical

s th

at h

int a

t the

pre

senc

e of

som

e ki

nd o

f bi

olog

ical

act

ivity

.

•H

ydro

gen

sulf

ide

and

sulf

ur d

ioxi

de -

two

gase

s th

at r

eact

with

eac

h ot

her–

exis

ts in

the

clou

ds.

•So

met

hing

is p

roba

bly

prod

ucin

g th

em.

•H

ardl

y an

y ca

rbon

mon

oxid

e. S

o so

met

hing

is

perh

aps

rem

ovin

g th

e ga

s.

http

://w

ww

.man

son-

valle

y.de

/fot

ogal

erie

/man

son/

imag

es/a

css

/acs

s_32

.jpg

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e on

Ven

us?

•O

ne p

ossi

bilit

y is

that

mic

robe

s liv

ing

in th

e cl

ouds

cou

ld

be c

ombi

ning

sul

fur

diox

ide

with

car

bon

mon

oxid

e an

d po

ssib

ly h

ydro

gen

sulp

hide

or

carb

onyl

sul

phid

e in

a

met

abol

ism

sim

ilar

to th

at o

f so

me

earl

y te

rres

tria

l m

icro

orga

nism

s.

•G

iven

that

the

tem

pera

ture

on

Ven

us w

as o

nce

muc

h co

oler

, the

re m

ay o

nce

have

bee

n oc

eans

on

the

plan

et. L

ife

coul

d ha

ve s

tart

ed th

ere

and

retr

eate

d to

sta

ble

nich

es o

nce

the

runa

way

gre

enho

use

effe

ct b

egan

.

•M

aybe

a m

issi

on to

sco

op u

p so

me

atm

osph

ere?

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e in

our

Sol

ar S

yste

m

Con

clus

ions

•N

o co

nclu

sive

evi

denc

e ex

ists

for

life

in o

ur s

olar

sy

stem

bes

ides

on

Ear

th

•B

ut, p

ossi

bilit

ies

exis

t for

life

–V

enus

may

hav

e lif

e in

the

clou

ds th

at m

igra

ted

whe

n po

ssib

le o

cean

s bo

iled

away

.

–M

ars

may

hav

e so

me

mic

robi

al h

isto

ry li

nked

to w

ater

, an

d pe

rhap

s so

me

subs

urfa

ce li

fe.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Mar

tian

Mic

robe

s?

•M

icro

scop

ic s

hape

s th

at

rese

mbl

e li

ving

and

fos

sil

bact

eria

on

Ear

th–

nano

bact

eria

. Pe

rhap

s w

e ha

ve m

eet o

ur f

irst

ET

?•

With

new

evi

denc

e of

onc

e liq

uid

wat

er, w

e ca

n fu

rthe

r sp

ecul

ate

wha

t hap

pene

d w

hen

the

plan

et’s

atm

osph

ere

disa

ppea

red,

per

haps

life

m

oved

to th

e su

bsur

face

. G

oing

und

ergr

ound

.

Page 6: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e in

our

Sol

ar S

yste

m

Con

clus

ions

•N

o co

nclu

sive

evi

denc

e ex

ists

for

life

in o

ur s

olar

sy

stem

bes

ides

on

Ear

th

•B

ut, p

ossi

bilit

ies

exis

t for

life

–V

enus

may

hav

e lif

e in

the

clou

ds th

at m

igra

ted

whe

n po

ssib

le o

cean

s bo

iled

away

.

–M

ars

may

hav

e so

me

mic

robi

al h

isto

ry li

nked

to w

ater

, an

d pe

rhap

s so

me

subs

urfa

ce li

fe.

–Ju

pite

r’s

atm

osph

ere

is r

ich

in p

re-b

ioti

c m

olec

ules

.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Flo

atin

g L

ife

•M

aybe

sim

ilar

to w

hale

s–m

ixtu

re b

etw

een

jelly

fish

an

d bi

rds?

•B

ig b

ags

of h

yrdr

ogen

gas

feed

ing

on s

mal

ler

mic

robe

s.

•O

f co

urse

, thi

s is

all

spec

ulat

ive,

and

ther

e is

no

way

to d

etec

t suc

h lif

e.

http

://w

ww

.epi

logu

e.ne

t/cg

i/da

taba

se/a

rt/l

ist.p

l?ga

ller

y=31

26

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e in

our

Sol

ar S

yste

m

Con

clus

ions

•N

o co

nclu

sive

evi

denc

e ex

ists

for

life

in o

ur s

olar

sy

stem

bes

ides

on

Ear

th

•B

ut, p

ossi

bilit

ies

exis

t for

life

–V

enus

may

hav

e lif

e in

the

clou

ds th

at m

igra

ted

whe

n po

ssib

le o

cean

s bo

iled

away

.

–M

ars

may

hav

e so

me

mic

robi

al h

isto

ry li

nked

to w

ater

, an

d pe

rhap

s so

me

subs

urfa

ce li

fe.

–Ju

pite

r’s

atm

osph

ere

is r

ich

in p

re-b

ioti

c m

olec

ules

.

–E

urop

a’s

sub-

crus

talo

cean

s m

ay h

arbo

r lif

e, e

ven

fish

-lik

e lif

e.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Io•

Inne

rmos

t Gal

ilean

moo

n –

the

“piz

za m

oon”

•T

he m

ost v

olca

nica

lly a

ctiv

e bo

dy in

the

sola

r sy

stem

.•

Voy

ager

1 d

isco

vere

d pr

esen

ce o

f vo

lcan

oes

•In

tern

al h

eatin

g by

Jup

iter’

s tid

es•

Atm

osph

eric

gas

es r

ippe

d of

f by

Jup

iter’

s m

agne

tic f

ield

–io

n to

rus

Pill

anP

ater

aer

uptio

nB

efor

e &

afte

r

Page 7: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Eur

opa

•Pe

rhap

s lik

e Io

, Eur

opa

is a

lso

heat

ed f

rom

w

ithi

n?•

Lik

ely

that

ther

e is

liqu

id w

ater

bel

ow th

e ic

e su

rfac

e.•

Lif

e co

uld

exis

t bel

ow th

e su

rfac

e ic

e be

low

th

e su

rfac

e, a

roun

d hy

drot

herm

al v

ents

.•

Ear

ly li

fe o

n E

arth

, may

hav

e fo

rmed

ar

ound

suc

h ve

nts.

•W

e do

n’t h

ow th

ick

the

ice

is y

et.

•Fu

ture

mis

sion

s, w

ill h

ave

to

em

ploy

sm

ash

and

dive

spa

cecr

aft.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e in

our

Sol

ar S

yste

m

Con

clus

ions

•N

o co

nclu

sive

evi

denc

e ex

ists

for

life

in o

ur s

olar

sy

stem

bes

ides

on

Ear

th

•B

ut, p

ossi

bilit

ies

exis

t for

life

–V

enus

may

hav

e lif

e in

the

clou

ds th

at m

igra

ted

whe

n po

ssib

le o

cean

s bo

iled

away

.

–M

ars

may

hav

e so

me

mic

robi

al h

isto

ry li

nked

to w

ater

, an

d pe

rhap

s so

me

subs

urfa

ce li

fe.

–Ju

pite

r’s

atm

osph

ere

is r

ich

in p

re-b

ioti

c m

olec

ules

.

–E

urop

a’s

sub-

crus

talo

cean

s m

ay h

arbo

r lif

e, e

ven

fish

-lik

e lif

e.

–T

itan

is v

ery

inte

rest

ing

•T

hick

atm

osph

ere

•R

educ

ing

chem

istr

y

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Tita

n

Tita

n’s

atm

osph

ere

•L

iqui

d/ic

e hy

droc

arbo

ns?

•O

rgan

ic c

ompo

unds

–li

fe?

•Pr

obab

ly n

ot –

too

cold

: 95

K•

May

be

a “d

eep

free

ze”

of th

e ch

emic

al

com

posi

tion

of a

ncie

nt E

arth

•C

ould

ther

e be

a “

fish

” sw

imm

ing

in li

quid

m

etha

ne?

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

No

Inte

llige

nt L

ife

•W

e m

ight

fin

d ev

iden

ce o

f so

me

sort

of

life

in o

ur

Sola

r Sy

stem

in th

e ne

xt d

ecad

e, b

ut v

ery

unlik

ely

to f

ind

com

plex

ity n

eede

d fo

r in

telli

gent

and

co

mm

unic

ativ

e lif

e.

•A

ppar

ently

in o

ur s

yste

m, E

arth

’s c

ondi

tions

are

ne

cess

ary.

•O

ther

pla

nets

may

hav

e m

icro

bial

for

ms

of li

fe,

and

may

beco

mpl

ex f

ish-

like

orga

nism

s, b

ut w

e do

n’t e

xpec

t com

mun

icat

ive

bein

gs.

Page 8: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

How

to s

earc

h fo

r lif

e?

•H

ow d

o w

e se

arch

for

life

in o

ur S

olar

Sys

tem

and

be

yond

?•

Wha

t tes

t will

indi

cate

life

exc

lusi

vely

?•

Is is

cle

ar th

at f

utur

e m

issi

ons

need

to la

nd a

s ne

ar a

s po

ssib

le to

site

s of

sub

surf

ace

wat

er o

r ot

her

solv

ents

.•

Wha

t if

the

life

is s

till i

n th

e pr

otol

ife

stag

e? C

an w

e de

tect

that

?•

The

bou

ndar

y be

twee

n ch

emic

al a

nd b

iolo

gica

l pro

cess

es

is d

iffi

cult

to d

istin

guis

h.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Dec

isio

n T

rees

–Se

arch

for

Lif

e

•W

ait f

or it

to c

ome

to u

s vi

a m

eteo

rite

s or

com

ets.

•R

obot

ic o

ne-w

ay in

vest

igat

ions

–M

ars

rove

rs.

•Fe

tch

and

retu

rn w

ith s

ampl

es.

http

://w

ww

.ibib

lio.

org/

wm

/pai

nt/a

uth/

frie

dric

h/tr

ee.jp

g

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Pro

blem

s

•In

the

last

2 c

ases

, we

have

the

prob

lem

of

cont

amin

atio

n by

E

arth

life

.

•O

rgan

ism

s ca

n liv

e in

Mar

s-lik

e co

nditi

ons

on E

arth

.

•If

som

e E

arth

life

sur

vive

s th

e sp

ace

jour

ney,

it c

ould

col

oniz

e M

ars,

pos

sibl

y de

stro

y an

y M

artia

n lif

e. T

hink

of

Kud

zu.

•C

urre

nt m

issi

ons

mus

t be

ster

ilize

d.ht

tp://

ww

w.h

ope.

edu/

acad

emic

/bio

logy

/fac

ulty

/eva

ns/i

mag

es/A

ngio

sper

ms/

Cor

eEud

icot

s/E

uros

idsI

/Fab

acea

e/K

udzu

.JP

G

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Bio

mar

kers

: H

ow to

look

for

ext

raso

lar

life.

•W

e ne

ed to

dec

ide

how

to s

earc

h fo

r bi

omar

kers

or

chem

ical

si

gnat

ures

of

life.

•O

n E

arth

, met

hane

and

oxy

gen

are

indi

cato

rs.

The

y no

rmal

ly

reac

t. S

omet

hing

is k

eepi

ng it

ou

t of

equi

libri

um.

Sort

of

like

Ven

us d

iseq

uilib

rium

.

•T

he G

alile

o sp

acec

raft

on

its w

ay

out t

o Ju

pite

r, tu

rned

and

look

ed

at th

e E

arth

.

•D

id it

det

ect l

ife?

Page 9: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Bio

mar

kers

: L

ooki

ng a

t Ear

th.

•St

rong

“re

d ed

ge”

from

ref

lect

ed li

ght.

Abs

orpt

ion

from

ph

otos

ynth

esis

.•

Stro

ng O

2. K

eepi

ng o

xyge

n ri

ch a

tmos

pher

e re

quir

es s

ome

proc

ess.

It s

houl

d sl

owly

com

bine

with

roc

ks.

•St

rong

met

hane

. Sho

uld

oxid

ize.

Rep

leni

shed

by

life.

•St

rang

e ra

dio

emis

sion

s th

at c

ould

be

inte

llige

nt li

fe.

•R

ecen

tly, r

esea

rche

rs h

ave

look

ed a

t the

Ear

thsh

ine

from

the

moo

n.•

The

y ag

ree

with

Gal

ileo

resu

lt.

The

re is

life

on

Ear

th.

–W

ater

–O

xyge

n–

Ten

tativ

e de

tect

ion

of “

red

edge

http

://e

pod.

usra

.edu

/arc

hive

/epo

dvie

wer

.php

3?oi

d=56

256

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Bey

ond

Plu

to –

The

Kui

per

Bel

t

•A

“re

serv

oir”

of

icy

bodi

es b

eyon

d Pl

uto

•Pr

opos

ed to

exp

lain

sh

ort-

peri

od c

omet

s

•T

he f

irst

Kui

per

Bel

t O

bjec

t (K

BO

) w

as

dete

cted

in 1

992

•T

ypic

al s

izes

10

-50

km, v

ery

fain

t–

Smal

l one

s ar

e po

tent

ial c

omet

s

–A

few

are

larg

e, h

undr

eds

of k

m a

cros

s

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Qua

oar

& S

edna

•C

urre

ntly

the

larg

est k

now

n K

BO

s•

Prob

ably

si

mil

ar in

co

mpo

sitio

n to

Cha

ron

•Su

rfac

e te

mpe

ratu

res

arou

nd 3

0 K

(-2

40 C

)!

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Dis

cove

ry im

ages

Qua

oar

•O

rbita

l dis

tanc

e ~

42 A

U

•A

bout

50%

the

diam

eter

of

Plu

to

Page 10: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Sedn

a

•A

bout

75%

the

diam

eter

of

Plut

o

•C

urre

ntly

at 6

7 A

U f

rom

the

Sun

•O

rbit

take

s it

over

90

0 A

U a

way

•10

,500

yr

orbi

t

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Plu

to, P

lane

t or

KB

O?

•Pl

anet

?–

Odd

pla

net:

all

othe

r ou

ter

plan

ets

are

gian

ts–

Ver

yec

cent

ric

orbi

t–

Orb

it hi

ghly

tilte

d w

ith r

espe

ct to

the

othe

r pl

anet

s

•K

uipe

r B

elt O

bjec

t?–

Lar

ger

than

oth

er K

BO

s(b

ut c

lose

in s

ize

to Q

uaoa

r&

Sed

na)

–H

as a

n at

mos

pher

e (l

ike

Tri

ton)

•B

ecau

se o

f si

ze &

clo

sene

ss to

the

Sun

–T

ypic

al K

BO

com

posi

tion

(icy

-roc

k m

ix)

–O

rbit

typi

cal f

or a

KB

O

•M

any

KB

Os

are

also

in r

eson

ance

with

Nep

tune

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Pla

net?

Und

efin

ed!

•W

e ha

ve n

ode

fini

tion

of

a pl

anet

!–

Its

like

art:

We

know

on

e w

hen

we

see

it

•If

Plu

to is

a

plan

et, w

hy n

otSe

dna

or Q

uaoa

r?

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Way

s of

Def

inin

g a

Pla

net

1.H

isto

rica

l–

Just

the

orig

inal

nin

e!

2.H

isto

rica

l Plu

s–

Any

thin

g bi

gger

than

Plu

to

–…

and

not s

omet

hing

’s m

oon!

3.G

ravi

tatio

nally

Rou

nd–

Big

eno

ugh

that

its

grav

ity m

akes

it r

ound

4.Po

pula

tion

Cla

ssif

icat

ion

–Is

olat

ed b

odie

s vs

. mem

bers

of

larg

e po

pula

tions

Page 11: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Cla

ss Q

uest

ion

Plut

o. I

s it

a pl

anet

, or

is it

a K

uipe

r B

elt O

bjec

t?

How

do

you

thin

k Pl

uto

shou

ld b

e cl

assi

fied

?

Dis

cuss

this

with

you

r cl

assm

ates

and

wri

te d

own

your

gro

up’s

con

clus

ion.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Com

ets

•A

ppar

ition

s th

at a

ppea

r lik

e gh

ostly

fir

ebal

ls f

roze

n in

the

sky

•In

anc

ient

tim

es, t

he a

ppea

ranc

e of

a c

omet

was

oft

en c

onsi

dere

d a

harb

inge

r of

doo

m•

Iron

ical

ly, l

ife

on E

arth

may

ha

ve b

een

impo

ssib

le w

ithou

t th

em•

Als

o co

met

s an

d m

eteo

roid

s ar

e th

e ol

dest

ori

gina

l sol

ar s

yste

m

mat

eria

l! L

eft o

ver

build

ing

mat

eria

ls.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Wha

t is

a C

omet

?

•D

irty

iceb

ergs

in

spa

ce–

10-5

0 km

ac

ross

•C

ompo

sed

mos

tly o

f w

ater

ic

e (b

ut a

lso

CO

2

and

CH

4), w

ith

som

e so

lid d

ust,

rock

&

met

al–

Dar

k su

rfac

es!

•V

ery

ellip

tical

orb

its ⇒

vary

ing

r im

plie

s va

ryin

g T

•W

hen

one

appr

oach

es th

e Su

n, s

unlig

ht s

ublim

ates

M

ar 1

8, 2

005

Ast

rono

my

210

Spri

ng 2

005

Com

ets

Cha

ngin

g r

impl

ies

a ch

ange

in T

Page 12: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Com

ets

•C

oma

–Su

nlig

ht e

vapo

rate

s co

met

su

rfac

e–

Form

s a

clou

d of

gas

& d

ust

arou

nd th

e nu

cleu

s

•T

ails

–G

as is

ioni

zed

by th

e su

n’s

UV

lig

ht

–G

as &

dus

t pus

hed

away

by

the

sola

r w

ind

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Whe

re D

o C

omet

s L

urk?

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Whe

re D

o C

omet

s L

urk?

•T

he v

ast m

ajor

ity li

ve f

ar o

ut in

the

Sola

r Sy

stem

, bey

ond

the

plan

ets

•Sh

ort p

erio

d co

met

s: K

uipe

r B

elt (

aka

tran

s-N

eptu

nian

)–

Orb

ital p

erio

ds o

f hu

ndre

ds o

f ye

ars

–A

roun

d an

d be

yond

the

orbi

t of

Plut

o (3

0-50

0 A

U),

pr

obab

ly f

orm

ed th

ere.

–N

ow a

bout

240

ish

the

size

of

10%

Plu

to

•L

ong-

peri

od c

omet

s: O

ort C

loud

–E

dge

of S

un's

gra

vita

tiona

l inf

luen

ce

–O

ut to

50,

000

AU

–Pe

riod

s >

105

yrs

–Pr

obab

ly d

id n

ot f

orm

ther

e. E

ject

ed b

odie

s by

Jov

ians

.

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Fal

ling

Into

the

Sola

r Sy

stem

•O

ccas

iona

lly, c

omet

orb

its

get “

pert

urbe

d” b

y pa

ssin

g st

ars

•T

hey

fall

into

the

inne

r So

lar

Syst

em o

n hi

ghly

elli

ptic

al

orbi

ts

•In

tera

ctio

ns w

ith p

lane

ts c

an

shor

ten

thei

r or

bits

Page 13: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e &

Dea

th o

f a

Com

et•

Eve

n co

met

s on

sho

rten

ed o

rbits

liv

e m

ostly

in th

e ou

ter

sola

r sy

stem

•E

very

orb

it, th

ey lo

se

1% o

f th

eir

mas

ses

to s

olar

ev

apor

atio

n–

Hal

ley’

s C

omet

will

onl

y la

st a

bout

56

00 m

ore

year

s

•W

hen

they

bec

ome

too

smal

l, th

ey

brea

k ap

art

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lif

e &

Dea

th o

f a

Com

et

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Dee

p Im

pact

http

://r

eals

erve

r1.jp

l.nas

a.go

v:80

80/r

amge

n/V

ideo

-NA

SA

1st-

Pesr

son-

Yeo

man

s-A

VC

2005

-016

.rm

Dee

p Im

pact

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Dis

cove

ry o

f th

e A

ster

oids

•In

180

1, G

iuse

ppe

Piaz

zino

ticed

an

unch

arte

d “s

tar”

th

at s

hift

ed p

ositi

on a

mon

g th

e st

ars

over

sev

eral

nig

hts

•C

ould

it b

e an

othe

r pl

anet

?–

Its

orbi

t was

bet

wee

n M

ars

and

Jupi

ter

–V

ery

dim

, so

it m

ust b

e sm

all

–T

oo s

mal

l to

be a

pla

net

•It

was

an

aste

roid

, a “

min

or p

lane

t”

Page 14: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Ast

eroi

ds

•Sm

all s

izes

–L

arge

st –

Cer

es: 9

40 k

m a

cros

s–

Onl

y 3

mor

e th

an 3

00 k

m–

Abo

ut 2

40 b

igge

r th

an 1

00 k

m–

Mill

ions

und

er

1 km

•C

ompo

sitio

n–

Roc

ks (

silic

ates

) an

d ir

on/n

icke

l

Ida

and

Dac

tyl f

rom

Gal

ileo

55 k

m

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

The

Ast

eroi

d B

elt

•M

ost a

ster

oids

are

fo

und

betw

een

2 to

3.5

AU

–B

etw

een

Mar

s &

Ju

pite

r

–R

egio

n is

cal

led

the

Ast

eroi

d B

elt

–N

earl

y ci

rcul

ar o

rbits

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

The

pos

sibi

lity

of s

ucce

ssfu

lly

navi

gatin

g an

ast

eroi

d fi

eld…

•A

ctua

lly, N

ASA

ha

s se

nt m

any

spac

e pr

obes

in

to a

nd th

roug

h th

e A

ster

oid

Bel

t•

Unl

ike

in S

tar

War

s, th

e A

ster

oid

Bel

t is

not t

hat c

row

ded

•A

vera

ge s

epar

atio

n be

twee

n si

zabl

e as

tero

ids

is 1

0 m

illio

n km

!

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Des

troy

ed…

by

the

Em

pire

•A

re th

e as

tero

ids

a de

stro

yed

plan

et?

No

–C

ombi

ned,

the

aste

roid

s ha

ve a

mas

s ab

out 0

.1%

th

at o

f th

e E

arth

–L

ess

than

10%

that

of

our

Moo

n

•T

he a

ster

oids

mig

ht b

e a

fail

edpl

anet

–Ju

pite

r’s

grav

ity k

ept t

he a

ster

oids

fro

m c

oale

scin

g in

to

a pl

anet

–Ju

pite

r pr

obab

ly e

ject

ed m

any

aste

roid

s fr

om th

e So

lar

Syst

em

Page 15: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Apo

llos

and

Tro

jans

•So

me

aste

roid

s ar

e on

orb

its th

at c

ross

E

arth

’s o

rbit

–C

alle

d A

pollo

ast

eroi

ds–

At l

east

169

0 ar

e kn

own

–In

197

2, o

ne s

kipp

ed

off

the

Ear

th’s

at

mos

pher

e

•O

ther

ast

eroi

ds s

hare

Ju

pite

r’s

orbi

t!–

Cal

led

Tro

jan

aste

roid

s–

Lea

d an

d tr

ail J

upite

r ar

ound

the

Sun

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Lan

ding

on

Ero

s

•In

200

1, N

ASA

land

ed a

sp

acec

raft

on

the

aste

roid

Ero

s

•H

eavi

ly c

rate

red

surf

ace

•B

ould

ers

buri

ed in

the

rego

lith

•A

ncie

nt –

4.6

billi

on y

ears

old

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Ast

eroi

ds -

Ear

ly S

olar

Sys

tem

L

efto

vers

•T

he a

ster

oids

wer

e to

o sm

all t

o ha

ve m

uch

inte

rnal

hea

t –

No

diff

eren

tiatio

n

–N

o ge

olog

ic a

ctiv

ity

–T

he s

ame

as w

hen

they

for

med

4.

6 bi

llion

yea

rs a

go

•Fo

ssils

of

the

earl

y so

lar

syst

em!

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Met

eors

•W

hen

you

see

a “s

hoot

ing

star

”,

that

is a

met

eor

–A

pie

ce o

f so

lar

syst

em d

ebri

s (a

m

eteo

roid

) in

tera

ctin

g w

ith o

ur

atm

osph

ere

•M

ost “

burn

up”

or

disi

nteg

rate

in

the

uppe

r at

mos

pher

e, b

ut s

ome

do

surv

ive

fall

–T

hese

are

met

eori

tes

•C

ompo

sitio

n: r

ock,

som

e m

etal

s

Page 16: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

S. N

umaz

awa

Met

eor

Show

ers

•M

eteo

rs h

it E

arth

all

the

time

•In

the

earl

y m

orni

ng, y

ou c

an

typi

cally

see

abo

ut 3

per

hou

r•

Seve

ral t

imes

a y

ear,

the

rate

in

crea

ses

–M

aybe

mor

e th

an a

met

eor

per

min

ute

–C

alle

d m

eteo

r sh

ower

s

•Se

em to

ori

gina

te f

rom

a

sing

le p

oint

in th

e sk

y

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Met

eor

Show

ers

•W

hen

a co

met

ent

ers

the

inne

r So

lar

Syst

em, i

t lea

ves

a tr

ail o

f du

st•

Whe

n E

arth

pas

ses

thro

ugh

this

dus

t, w

e ge

t a m

eteo

r sh

ower

•M

eteo

r sh

ower

s do

n’t

typi

cally

pro

duce

met

eori

tes

–It

s al

l dus

t, no

t roc

ks

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Pee

kski

ll F

ireb

all

(Oct

ober

9, 1

992)

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Typ

es o

f M

eteo

rite

s

•94

% o

f m

eteo

rite

s ar

e st

ony

–M

ade

of s

ilica

tes,

ha

rd to

dis

tingu

ish

from

Ear

th r

ocks

•5%

are

iron

s–

Iron

-nic

kel c

ryst

als

•1%

sto

ny-i

rons

–Si

licat

es w

ith ir

on in

clus

ions

Page 17: Pluto– Planet or Largest Kuiper Belt Object? • Life in ...eeyore.astro.illinois.edu/~lwl/classes/astro210/spring05/Lectures/lecture25.pdf · Pluto’s Atmosphere Astronomy 210

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Met

eori

tes

are

Anc

ient

•M

eteo

rite

s ar

e th

e ol

dest

ob

ject

s in

the

Sola

r Sy

stem

•R

emna

nts

of th

e So

lar

Syst

em’s

for

mat

ion

•T

he o

ldes

t are

car

bona

ceou

s ch

ondr

ites

(a ty

pe o

f st

one)

–A

bund

ant i

n ca

rbon

and

wat

er–

Con

tain

am

ino

acid

s -

build

ing

bloc

ks o

f lif

e!–

4.56

bill

ion

year

s ol

d

•So

me

have

dia

mon

ds p

rodu

ced

by in

ters

tella

r sh

ock

wav

es!

Car

bona

ceou

s ch

ondr

ite

Mar

18,

200

5A

stro

nom

y 21

0 Sp

ring

200

5

Met

eori

te O

bser

ving

•T

he U

ofI

has

a sm

all m

eteo

rite

col

lect

ion

in th

e N

atur

al H

isto

ry B

uild

ing

•A

ctiv

ities

:–

Cou

nt th

e nu

mbe

rs o

f ea

ch ty

pe o

f m

eteo

rite

, com

pare

to

the

frac

tions

that

exi

st in

spa

ce–

Why

do

we

know

whe

n m

ost o

f th

e st

ony

met

eori

tes

fell,

but

not

the

iron

one

s?–

Vis

it a

web

-site

, lea

rn a

bout

how

to id

entif

y m

eteo

rite

s

•E

xtra

Cre

dit R

epor

t: D

ue A

pril

8th, w

orth

1/3

a

hom

ewor

k.