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We know, if set anywhere above the earth at rest, thisspace capsule would simply fall.
If propelled in earth’s direction, itwould just build speed and crash.
If propelled directlyopposite the earth, itmight escape (depending on its speed),
or it may decelerate,slowing to a stop,and falling to earthanyway.
If given an initial velocityexactly perpendicular tothe direction of the earth,
it might just orbit!
What conditions must be met
to orbit (and not fall)?
F = 2
Centripetal force:
F
an object needs a continuously applied FORCE exactly perpendicular to its motion.
To be steered from the straight-line paththat inertia would automatically carry it,
And of course, there isa continuously appliedforce acting on thisspace capsule!
The gravitational force we’ve been worrying about bringing it in for a fatal landing!
To stay aloft what v does it need?
v
Fgravity
How fast would an object have to move horizontallyto orbit just above the earth’s atmosphere?
R
mvF
2
=W = mg
gRv =2
gRv =
)104.6)(/8.9( 62 msecmv ×=
= 7,920 m/sec
That’s fast enough to complete anorbit of 2R = 2(6.41024 m) in
vdt vtd /=⇒=)/7920/()104.6(2 6 smmt ×=
= 5077 sec
= 84.6 minutes
17,716 mph!!
Some Planetary Data
RADIUSOF ORBIT
PERIOD OFREVOLUTION
MercuryVenusEarthMarsJupiterSaturnUranusNeptune
5.79 1010 meters 7.60 106 seconds
1.08 1011 meters 1.94 107 seconds
1.49 1011 3.16 107
2.28 1011 5.94 107
7.78 1011 3.74 108
1.43 1012 9.30 108
2.87 1012 2.66 109
4.50 1012 5.20 109
about double
~3
Some Planetary Data
RADIUSOF ORBIT
PERIOD OFREVOLUTION
MercuryVenusEarthMarsJupiterSaturnUranusNeptune
5.79 1010 meters 7.60 106 seconds
1.08 1011 meters 1.94 107 seconds
1.49 1011 3.16 107
2.28 1011 5.94 107
7.78 1011 3.74 108
1.43 1012 9.30 108
2.87 1012 2.66 109
4.50 1012 5.20 109
about triple
~6
Some Planetary Data
RADIUSOF ORBIT
PERIOD OFREVOLUTION
MercuryVenusEarthMarsJupiterSaturnUranusNeptune
5.79 1010 meters 7.60 106 seconds
1.08 1011 meters 1.94 107 seconds
1.49 1011 3.16 107
2.28 1011 5.94 107
7.78 1011 3.74 108
1.43 1012 9.30 108
2.87 1012 2.66 109
4.50 1012 5.20 109
about ten times
~30
Some Planetary Data
RADIUSOF ORBIT
PERIOD OFREVOLUTION
MercuryVenusEarthMarsJupiterSaturnUranusNeptune
5.79 1010 meters 7.60 106 seconds
1.08 1011 meters 1.94 107 seconds
1.49 1011 3.16 107
2.28 1011 5.94 107
7.78 1011 3.74 108
1.43 1012 9.30 108
2.87 1012 2.66 109
4.50 1012 5.20 109
about 30 times
164
T2 R3
The square of the periods of all the planets are proportional to
Johannes Kepler (1571-1630)
the cube of their distance from the sun!
Mercury 0.241 0.387Venus 0.615 0.723Earth 1.000 1.000Mars 1.881 1.523Jupiter 11.862 5.200Saturn 29.458 9.540
PERIOD T(YEARS)
DISTANCE Ravg(AU) T2/Ravg
3
1.0001.0001.0001.0001.0001.000
Distances measured in AUs (Astronomical Unit) simply use the earth’s orbital radius
as the standard unit of measure.
1.000
1.000
€
(0.241)2
(0.387)3
€
0.0580
€
0.0580=
The Galilean Moons of Jupiter
Io
Europa
Ganymede
Callisto
421,700 km
671,034 km
1,070,412 km
1,882,709 km
1.77 days
3.55 days
7.15 days
16.69 days
4.17 10-17
T2/R3
4.17 10-17
4.17 10-17
4.17 10-17
R
va
2
=T
Rv
2=
Isaac Newton (1642 – 1727)
Anything traveling in a circle must be experiencing a continuous
centripetal acceleration:where for an
orbit of period T
?
2
24
T
Ra
=
Isaac Newton (1642 – 1727)
2
24
T
Ra
=For any circular orbit:
For planets: 32 R k T = R k 3
2
1
Ra ∝
If the moon were in orbit twice as far from the earth,its acceleration toward the earth would be:
A. 4 what is is now.B. twice what it is now.C. the same as it is now.D. half of what it is now.E. 1/4th what it is now.F. 1/8th what it is now.
A satellite orbiting the earth at half the moon’s distance has an acceleration toward the earth:
A. 4 that of the moon.B. twice that of the moon.C. the same as the moon’s.D. half that of the moon.E. 1/4th that of the moon.F. 1/8th that of the moon.
Jupiter is ~5 times further from the sun than earth.Jupiter’s acceleration toward the sun is about
A. 5 that of earth’s.B. the same as earth’s.C. 1/5th that of earth’s.D. 1/10th that of earth’s.E. 1/25th that of earth’s.
Apples fall toward the earth
at 9.8 m/sec2.
Something pulls the moon(60 further away at6428.8257 kilometers)
into its orbit of 27.321 days.
That requires a centripetal force accelerating it at
2
24
T
Ra
=)/400,86)(321.27(
)1084399.3(4 82
daysecdays
m×=
= 0.002723 m/sec2
9.8 m/sec2
602= 0.002723
The mass of the earth is 80 timesgreater than the mass of the moon.
A. just as hard asB. twice as hard asC. 80 times harder thanD. 160 times harder thanE. (80)2=6400 times harder than
The earth pulls gravitationally on the moon_______ the moon pulls on the earth.
The earth is approximately equal to80 moon-sized chunks of mass.
Each of these moon-sized pieces pullson the moon (about equally)
and the moon pulls on each of thesemoon-sized chunks…just as hard!
F F
The earth pulls on the moon with a total force of 80F.
The moon pulls on the earth with a total force of 80F.
This suggests the force of gravity is also directly proportional to the masses involved:
221
R
mmF
grav∝
221
R
mmGF
grav=
G is a universal constant measured to be6.67 10-11 N·m2/kg2
0.000 000 000 066 7 N·m2/kg2
How irresistible is the gravitational force of attraction between a pair of us when 1 meter (center-to-center) apart?
G(80 kg) (70 kg)
(1 meter)2 = G 5600kg2
m2
= 0. 000 000 32 N
Fgrav
R