Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

Examining Orbits: Circular, Parabolic & Hyperbolic, Summaries of Physics

This document delves into the intricacies of gravitational forces and their impact on planetary motion. Topics include the relationship between weight, velocity, and location, the effects of changing earth's rotation rate, and kepler's laws of planetary motion. Students will gain a deeper understanding of circular, parabolic, and hyperbolic orbits, as well as the concepts of gravitational potential energy and escape speed.

Typology: Summaries

2021/2022

Uploaded on 01/30/2024

joan-gabrielle
joan-gabrielle 🇨🇦

1 document

1 / 10

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
o
weight Fg onyou at aparticular
locationyou'reat
directed
towardsthe
centeroftheEarth
Apparentweight
for w2
24hours
na
WF
g
ITyourvelocitytangentialtothe
equator
htnormal
farceaway
fromthe
center
Top down view
IEx FIf IwR
wGI N
Rt
WNmat acvp wmy
µWma c
wfHE
g
NWtage
WaNapparentweight
pf3
pf4
pf5
pf8
pf9
pfa

Partial preview of the text

Download Examining Orbits: Circular, Parabolic & Hyperbolic and more Summaries Physics in PDF only on Docsity!

o

weight

Fg

on

you

at

a

particular

location

you're

at

directed

towards

the

center

of

the

Earth

Apparent weight

for

w

2

24 hours

na

W

F

g

I

T

your

velocitytangential

to the

equator

ht normal

farce

away

from

the

center

Top

down view

I

Ex F

If

I

w R

w

GI

N

R

t

W

N

mat

a c

vp

w

my

μ

W

ma

c

w

f

HE

g

N

W

t

age

W

a

N

apparentweight

v w

R

e

2

Re

465

Sowhen

you're

standing

in

the

equator

you're

moving

at

a

tangential

velocity

r

of

465

closer

to

the

pole

N

will

be

lower

AT

VII

O

0339

m

s

g

W

no

ratio

of

ac

to

g

centripetal

free

fall

Agg

0

gl

3g3,

O

Cc

l

μ

l

o

00346

W

W

reading

onthe

weighing

scale

is

3

less

what

if

we increase the

rate

at

which theEarth

is spinning

your

apparent

weight

is

gonna

go

down

because

as

you

start

spinning

faster

you

r

a

e goes

up

and

you

need

more

Fnet

towards

the

oath

so the

fixed

Fg

towards

thecertes

and

gets

smaller

W A

WA

O v

I V

T W

A

w

l

a

c

g

vr

g

riff

ooo

apparent weight O

Orbital

Motion

i

Ti

n

hyperbolic

ii

PIT

unbound

i

ti

i

i

i

i

i

n

fi

i

parabolic

circular

circular

Orbits

Fg

Garmin

MAJ

ing

art

is

v

f

speed

of

circular

orbits

rcraa.aa.name

o

l

Mercury

O

As r

increases or

you

are

movingfurther

out

the

v

goes

smaller

or

you're

going

slower

and

slower

ee

outline

what

you

expect

why

darter

r

v

atf

T

4I

4

r

Iepiefsksraelawg

Planetary

Motion

e

g

geosynchronous

orbit

view

top

down

gg

joTIuhourd

4IImr3geo 7rgeo

42,2ookm 6.6RE

geo

i

i

i 1 1 1

1

io

GRE

Kepler's

Laws

1 FirstLaw

Planets

move on

elliptical

orbits

around

the

sun

perihelion

J

aphehilion

3

Third Law

T

_41T

T4yrs

a3CAu

earth

6M

a semi

major

axisla

annals

rper

107

km

u

o raph

526

109

km

o

a

rpertraph

Toper

o

g

L

6711109km

ap sur

b

b

eccentricity

e

Neptune rper

all

e

mad

Odell

c period

T

T

ftp

z

75.5years6Msun

Newton's Generalizations

teal.pe

ighyoliI

Voasr

a

asr

a

bound

I

orbit C

O.M

i

i

M.gg

w

i

T

4th

Enja

bothmTasses

are

accounted

for

Gravitational

Potential

Energy

m

riff

V

o

AtktEUgenergystmedingnavilatorialfield

Fg

af

Mand m

rf.fr

1Ug

IK

oWg

O

b

b

tr

fig.di

ftp MrY

fr

drr

M

tf

GMrIdr

6111

AUgif

GMIJ.fm

Ug

GMrm

tanst

UgCr

hi

r

A

T

Ic

yay

iii

K required

at

n

I

I

f

f

N

F

i

i

i

ii

increasespeed

by

41

no