9
Feb 4, 2005 Astronomy 210 Spring 2005 Astronomy 210 Section 1– MWF 1500-1550 134 Astronomy Building This Class (Lecture 8): Theory of Planetary Motion Next Class: The Two-Body Problem Music: Space Dog – Tori Amos Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm -> 1/6 th HW grade (due Feb 11 th ) Feb 4, 2005 Astronomy 210 Spring 2005 Outline How things move in a gravity field, part 2. Begin the two body problem. Feb 4, 2005 Astronomy 210 Spring 2005 Result Now we know that the orbiting planets are just perpetually falling bodies. This includes the shuttle, satellites, etc. “Weightlessness” is just like falling. There is gravity on the shuttle, but as one is in freefall it is not noticeable. Kepler had thought briefly about this, but he decided he needed forces along the direction of the velocity, not perpendicular to it. So Newton realized that like an apple falling from a tree or a really big tree, the moon must have a force toward the Earth. Newton did not discover gravity, but he realized that it was universal. Feb 4, 2005 Astronomy 210 Spring 2005 Applications We now have two tools in our box: – Newton's laws of motion: how things move with, without forces applied – Newton's gravity: the net force on solar system bodies Now, we need to out the two together: how do bodies move under the inverse square force of gravity.

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Page 1: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

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 8

):

The

ory

of P

lane

tary

Mot

ion

Nex

t Cla

ss:

The

Tw

o-B

ody

Prob

lem

Mus

ic: S

pace

Dog

–T

oriA

mos

Pla

neta

rium

Obs

ervi

ng

Star

dial

Obs

ervi

ng

Kal

erle

ctur

e at

Pla

neta

rium

, F

ri @

7pm

->

1/6

thH

W g

rade

(d

ue F

eb 1

1th)

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Out

line

•H

ow th

ings

mov

e in

a g

ravi

ty f

ield

, pa

rt 2

.

•B

egin

the

two

body

pro

blem

.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Res

ult

•N

ow w

e kn

ow th

at th

e or

bitin

g pl

anet

s ar

e ju

st p

erpe

tual

ly

falli

ng b

odie

s. T

his

incl

udes

the

shut

tle, s

atel

lites

, etc

. •

“Wei

ghtle

ssne

ss”

is ju

st li

ke f

allin

g. T

here

is g

ravi

ty o

n th

e sh

uttle

, but

as

one

is in

fre

efal

l it i

s no

t not

icea

ble.

•K

eple

rha

d th

ough

t bri

efly

abo

ut th

is, b

ut h

e de

cide

d he

ne

eded

for

ces

alon

g th

e di

rect

ion

of th

e ve

loci

ty, n

ot

perp

endi

cula

r to

it.

•So

New

ton

real

ized

that

like

an

appl

e fa

lling

fro

m a

tree

or

a re

ally

big

tree

, the

moo

n m

ust h

ave

a fo

rce

tow

ard

the

Ear

th.

•N

ewto

n di

d no

t dis

cove

r gr

avity

, but

he

real

ized

that

it w

as

univ

ersa

l.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

App

licat

ions

•W

e no

w h

ave

two

tool

s in

our

box

:–

New

ton'

s la

ws

of m

otio

n: h

ow th

ings

mov

e w

ith, w

ithou

t for

ces

appl

ied

–N

ewto

n's

grav

ity: t

he n

et f

orce

on

sola

r sy

stem

bo

dies

•N

ow, w

e ne

ed to

out

the

two

toge

ther

: how

do

bod

ies

mov

e un

der

the

inve

rse

squa

re

forc

e of

gra

vity

.

Page 2: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Kin

etic

Ene

rgy

22

21

21r

mm

vK

E&r

==

http

://w

ww

.nap

.edu

/htm

l/one

univ

erse

/im

ages

/ene

rgy_

12_s

mal

l.jpg

http

://w

ww

.arm

y-te

chno

logy

.com

/pro

ject

s/th

aad/

thaa

d3.h

tml

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Pot

entia

l Ene

rgy

of G

ravi

ty

∫⋅

−=

∆f ir r

rdF

Ur

r

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Pot

entia

l Ene

rgy

of G

ravi

ty drrM

mG

Uf ir r∫

=∆

2

Def

ine

pote

ntia

l ene

rgy

at

r f=

∞to

be

0

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Pot

entia

l Ene

rgy

of G

ravi

ty

rMm

GU

−=

Page 3: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Pot

entia

l Ene

rgy

of G

ravi

ty

rMm

GU

−=

Neg

ativ

e po

tent

ial e

nerg

y?

Wha

t’s

up w

ith th

at?

It r

eally

impl

ies

that

the

obje

ct is

bou

nd b

y th

e gr

avita

tiona

l fie

ld.

In o

rder

to e

scap

e th

e pu

ll of

gra

vity

, it h

as to

be

give

n th

at m

uch

ener

gy.

The

onl

y ph

ysic

ally

mea

ning

ful q

uant

ity is

rel

ativ

e ch

ange

s in

po

tent

ial e

nerg

y.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Tot

al E

nerg

y in

Gra

vity

•T

E =

KE

+ P

E

rMm

Gm

vE

−=

2

21

Con

serv

ed!!

!!C

onse

rved

!!!!

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Orb

its

Can

cla

ssif

y or

bits

with

tota

l ene

rgy.

θθ

cos

1

)1(

)(

2

e

ae

r+−

=

Can

wri

te a

cir

cle

or e

llips

e in

pol

ar c

oord

inat

es a

s:

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Orb

its

Con

side

r a

circ

le w

ith e

=0 rM

Gv c

=2

that

R

ecal

l

2

21

som

vK

E=

Page 4: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Orb

its

Con

side

r a

circ

le w

ith e

=0

rMm

GP

E−

=B

ut

The

n, K

E =

-PE

/2

And

TE

= K

E +

PE

= P

E/2

TE

< 0

!!

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Spoo

ky O

rbits

Wha

t?N

egat

ive

tota

l ene

rgy?

Is th

at d

ue to

spo

oky

antim

atte

r?

•N

o it

mea

ns th

at y

ou h

ave

to s

uppl

y en

ergy

to s

yste

m to

bre

ak it

apa

rt.

•W

hen

part

icle

s at

res

t, fa

r aw

ay, K

E =

PE

= 0

. To

get t

o th

is s

ituat

ion,

hav

e to

inpu

t ene

rgy

to a

n or

bitin

g sy

stem

.•

Sinc

e en

ergy

is c

onse

rved

, can

't sp

onta

neou

sly

get t

his

ener

gy, s

o sy

stem

is

⇒⇒bo

und!

boun

d!•

Not

e: K

E =

-1/

2PE

gen

eral

ly tr

ue f

or g

ravi

tatin

g sy

stem

s in

equ

ilibr

ium

: “v

iria

lthe

orem

"

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Gen

eral

Orb

its

Elli

pse:

0 <

e <

1

•It

turn

s ou

t tha

t TE

dep

ends

onl

y on

a, n

ot o

n e

•Fr

om c

onse

rvat

ion

of e

nerg

y ca

n se

e:

a

Mm

Gm

vrMm

GT

E2

212

−=

+−

=<

0!!

⇒B

ound

!F

eb 4

, 200

5A

stro

nom

y 21

0 Sp

ring

200

5

Gen

eral

Orb

its

Elli

pse:

0 <

e <

1

•It

turn

s ou

t tha

t TE

dep

ends

onl

y on

a, n

ot o

n e

•Fr

om c

onse

rvat

ion

of e

nerg

y ca

n se

e:

a

Mm

Gm

vrMm

GT

E2

212

−=

+−

=

Page 5: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Gen

eral

Orb

its

Elli

pse:

0 <

e <

1

•It

turn

s ou

t tha

t TE

dep

ends

onl

y on

a, n

ot o

n e

•Fr

om c

onse

rvat

ion

of e

nerg

y ca

n se

e:

−=

ar

GM

v1

22

Thi

s is

cal

led

the

“Vis

Viv

a” e

quat

ion.

T

he m

ost h

andy

orb

ital e

quat

ion.

http

://gr

oups

.msn

.com

/And

ysU

sing

Scie

nceF

ictio

nFor

Edu

catio

nPag

e/vi

sviv

aequ

atio

n.m

snw

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Gen

eral

Orb

its

Para

bola

: e =

1

•C

an w

rite

as:

•W

here

p is

dis

tanc

e at

clo

sest

app

roac

h.

•Ju

st u

nbou

nd s

yste

m (

can

bare

ly e

scap

e to

r=∞

)

E =

0 o

r K

E =

-PE

θco

s1

+=

pr

rMG

v esca

pe2

=

For

Ear

th. V

esca

pe=

11k

m/s

= 2

5000

mph

.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Gen

eral

Orb

its

Hyp

erbo

la: e

> 1

•C

an w

rite

as:

•C

ompl

etel

y un

boun

d sy

stem

(es

cape

s to

r=∞

)

E >

0

•T

hat i

mpl

ies

that

v >

0 a

t r=∞

θθ

cos

1

)1(

)(

2

e

ae

r+−

=

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Lif

e is

a 2

Bod

y P

robl

em

•So

far

, I h

ave

chea

ted

a lit

tle…

or

sim

plif

ied

•N

ot th

e pl

anet

s, n

or th

e Su

n is

nai

led

dow

n.

•Fr

om N

ewto

n’s

thir

d, th

e Su

n m

ust m

ove!

(b

ut m

ore

mas

s so

acc

eler

atio

n is

sm

alle

r)

How

do

bina

ry s

tars

orb

it?

We

have

to u

nder

stan

d a

2 bo

dy s

yste

m.

Page 6: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Con

side

r a

Box

•A

box

in s

pace

with

mas

s aw

ay f

rom

any

gra

vity

fi

eld.

•W

hat i

f th

e bo

x ha

d m

any

piec

es in

side

of

it, h

ow

wou

ld it

mov

e?

•H

ow w

ould

it m

ove?

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Con

side

r a

Box

•L

et o

ur b

ox h

ave

2 ob

ject

s w

ith m

asse

s m

1an

d m

2

•H

ow w

ould

it m

ove?

No

mat

ter

wha

t th

e pi

eces

do,

th

e bo

x st

ill a

cts

as a

fre

e bo

dy.

⇒C

onst

ant

velo

city

.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Con

side

r a

Box

•If

you

are

mov

ing

with

the

box,

at t

he s

ame

velo

city

:

?

Can

we

say

anyt

hing

abo

ut w

here

the

seco

nd m

ass

has

to b

e?

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uce

Pro

blem

m1

m2

M =

m1

+ m

2

If w

e tr

eat a

s a

sing

le o

bjec

t of

mas

s M

with

no

exte

rnal

for

ces

(onl

y gr

avity

bet

wee

n th

em),

then

how

doe

s th

e bo

x m

ove?

Page 7: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Cen

ter

of M

ass

(CO

M)

21

22

11

mm

rm

rm

R++

=r

rr

1rr

2rr

m1

m2

Rrrr

M

12

rr

rr

rr

−=

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Cen

ter

of M

ass

(CO

M)

m1

m2

Rr

M

0R

cons

tant

0=

=⇒

=&r

&r&&r

RR

With

no

exte

rnal

for

ces,

can

sho

w th

at

Can

pic

k in

ertia

fra

me

whe

re

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Cen

ter

of M

ass

(CO

M)

1rrm

1m

2

M

0R

cons

tant

0=

=⇒

=r

&r&&r

RR

With

no

exte

rnal

for

ces,

can

sho

w th

at

Can

pic

k re

fere

nce

fram

e w

here

2rr

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Cen

ter

of M

ass

(CO

M)

m1

m2

Rr

M

Wha

t we

are

real

ly d

oing

is t

radi

ng o

ne p

air

of v

ecto

rs (

posi

tions

of

each

mas

s) f

or a

dif

fere

nt p

air

(CO

M a

nd r

elat

ive

sepa

ratio

n) w

hich

ar

e m

ore

conv

enie

nt a

nd n

atur

al...

Page 8: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

CO

M•

So c

an th

ink

of tw

o ob

ject

s or

bitin

g th

e ce

nter

of

mas

s M

= m

1+

m2

•E

ach

star

has

its

own

orbi

t with

the

sam

e ec

cent

rici

ty a

nd a

dif

fere

nt,

but r

elat

ed s

emim

ajor

axis

.

•T

he s

tars

are

alw

ays

oppo

site

eac

h ot

her

abou

t the

cen

ter-

of-m

ass.

B

oth

star

s w

ill r

each

per

istr

on(c

lose

st a

ppro

ach)

at s

ame

time.

•If

m1>

> m

2, th

en w

e’re

bac

k to

12

1

12

1

22

11

mm

mM

rm

m

rm

rm

R

≈+

=

≈++

=r

rr

r

m1

m2

RrM

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

For

ce in

the

Box

rrm

mG

32

121

−=

rr

rmm

Gr

32

1=

m1

m2

2112

FF

rr

−=

rr

rrm

mG

22

112

=r

New

ton’

s 3rd

Law

!

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uced

Mas

s

1rr

2rr

m1

m2

212

2

121

1

Fr

m

Fr

mr

&&r

r&&r

==

rr

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uced

Mas

s

1rr

2rr

m1

m2

rr

+=

21

21

21m

m

mm

Fr

Page 9: Outline Applicationslwl/classes/astro210/... · 2010. 2. 11. · Space Dog Planetarium Observing Stardial Observing Kaler lecture at Planetarium, Fri @ 7pm – Tori Amos-> 1/6 th

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uced

Mas

s

ssre

duce

d m

am

m

mm

defi

ne

2

1

21 +

=µ 1rr

2rr

m1

m2

rr

21

Fr

then

r&&r=

µ

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uced

Mas

s

rm

mmm

mth

enm

mif

note

&&r&&r

221

21

21

12

For

:

==

≈<<

µ

1rr

2rr

m1

m2

rr

21Fr

r&&r=

µId

entic

al to

sim

plif

ied

case

, but

now

mas

s is

mod

ifie

d.

Feb

4, 2

005

Ast

rono

my

210

Spri

ng 2

005

Red

uced

Mas

s Mµ

rr

21Fr

r&&r=

µ•

Syst

em c

an b

e th

ough

t of

a te

st p

arti

cle

of r

educ

ed

mas

s th

at is

orb

iting

a m

ass

M =

m1

+ m

2

•D

iffe

rent

ref

eren

ce f

ram

es.