
Gravitation
Newton and Gravity
- Newton observed falling apple and orbiting moon, saw both were accelerating, so both
had net force.
- Newton wondered if force on apple was same as force on moon
- First to realize force of gravitation is universal, exists between all objects with
mass
Law of Universal Gravitation
- Force between any two objects is directly prop to product of their masses, inversely
prop to square of distance between their centers of mass.
- To calculate force, proportionality constant is needed-first measured by Cavendish in
his optical lever experiment
- F = (Gm1m2)/d2 ; where
F is the force exerted on each body by the other (3rd law), m1 and
m2 are the masses of the two bodies, d is the distance between the centers of mass
of the two bodies and G = 6.67 x 10-11 Nm2/kg2, the universal gravitation constant.
An Inverse-Square Law
- Force of gravity varies inversely with square of distance between objects
- If distance is doubled, force is one-fourth as much; if tripled, force is one-ninth
(1/3)2
- If distance is halved, force is 4 times as much; if distance is 1/3 as much, force
is 9 times as great.
- Due to spreading of force into surrounding space
The Mass of the Earth
- When G was finally measured, it allowed us to find the mass of the earth by using an object
of known mass and weight at one earth radius distance (also known)
- Also allowed us to calculate g at any location near any celestial body:
g = GM/d2
- Gravity depends on distance from center of earth or other planet and its mass
Weight
- Weight is force due to gravitational attraction, depends on location.
- Sensation of weight requires supporting force; feel weightless without it: amusement park
rides, astronauts
Gravitational Field
- Force is felt in area surrounding large body
- Called gravitational field, can be mapped by measuring force at many locations
- Vector field whose direction points to center of planet, magnitude depends on distance
Gravitational Field Inside Earth
- If hole were drilled through earth and you fell in, mass below you pulls down, mass
above you pulls up.
- No force at center of earth, pull equal in all directions
- You would accelerate with decreasing acceleration until you reached the center, then decelerate
as you approach opposite surface.
Mechanism of Gravity
- How force acts at a distance is not well understood
- Explained by Einstein's general relativity theory: large mass distorts fabric of space-time
causing nearby objects to be pulled in
- Particle theorists suggest exchange of particles called gravitons carried by gravity waves
between objects
Kepler's Laws
- Johannes Kepler examined orbits of planets and formulated 3 laws for all satellites
- Law of Orbits: all planets move in elliptical orbits with the sun at one focus
- Law of Areas: a line that connects a planet to the sun sweeps out equal areas in equal
times
- Law of Periods: The square of the period of any planet is proportional to the cube
of the semimajor axis of its orbit
- Period is time for one revolution
- Semimajor axis is longest radius dimension of ellipse
Earth Satellites
- Satellites are projectiles
- Must have enough horizontal velocity so vertical fall matches earth's curvature
- Earth's surface drops 4.9 m in 8000 m horizontal distance
- Since projectiles fall 4.9 m in 1 second, must travel 8 km/s to be in orbit (29000
km/hr or 18000 mi/hr)
Circular Orbits
- In circular orbit, gravity always pulls perpendicular to velocity
- Speed doesn't change, only direction.
- Time (period) for close orbit about 90 min., greater for higher orbits
- If period is 24 hours, satellite remains over same point on earth--communication
satellites do this (geosynchronous orbit)
Elliptical Orbits
- If speed is faster than needed for circular orbit, elliptical orbit can result
- Ellipse is oval with two focal points (foci)
- Earth (or other planet or sun) is at one focus of ellipse
- Speed varies in elliptical orbit
- Faster speed close to earth, slower when farther away
Escape Speed
- Vertical launch speed needed for escape from earth is 11.2 km/s
- Different from the 8 km/s horizontal speed needed for orbit
- Any speed sustained indefinitely will escape earth
Gravitation and the Universe
- "Big Bang" theory says universe hurled outward from big explosion
- Universe is expanding, only pull of gravitation can stop it.
- Unknown whether enough matter exists to stop expansion and begin contraction leading
to "Big Crunch" and another big bang-expansion-contraction cycle.
Tides
- Change in sea level due to difference in gravitational pull between earth and moon
on opposite sides of earth.
- Causes elongation of earth and moon along line of force, bulging on near and far
side.
- Earth turns underneath high water levels causing 2 high tides and two low tides
per day.
- Sun also creates tides but effect is less than moon because distance difference is
not as large a part of total distance.
- Extra large spring tides caused by sun-moon alignment on same
side of earth
- Smaller neap tides occur when sun and moon are on opposite sides of earth
Eclipses
- When sun-moon-earth alignment is perfect, eclipses occur
- When earth is between sun and moon, moon is in shadow and lunar eclipse occurs.
- When moon is between sun and earth, parts of earth in moon's shadow see solar eclipse
Black Holes
- In stars, expansion forces due to nuclear fusion are balanced by contraction force
of gravity.
- When solar fuel runs out, stars collapse
- Small stars will become dense, cool, black dwarfs.
- Large stars will continue collapse to enormous density with gravitational forces too strong
for anything to escape
- Even light, radio communications are trapped--nothing can escape black hole.
- Fabric of space-time is warped by tremendous gravity inside black hole
- Mass of black hole is same as star that created it so gravity outside black hole is same
as if original star were still there.