day 4. discussion on yesterday’s probes work on today’s probes
TRANSCRIPT
MSP STEMDay 4
Discussion on Yesterday’s Probes
Work on Today’s Probes
Astronomy Probes
Here’s another approach for having your students present the solar system facts to each other.
Yes, you are going to present to us today
Solar System PBL / Math Pullout
Meteor’s & Meteorites
See separate Power Point
GravityIt’s a heavy topic!
Universal Gravitation
You are attractive to the person next to you!
Falling Bodies Newton knew that bodies continued in a
straight line unless another force acted on it (___ Law). What force kept the moon around the earth?
Moon must have _________ velocity to keep going, not away and not into, but around the Earth
This would have to be tested to be proven true to go from hypothesis to theory (law).
1st
tangential
Falling Bodies (cont.) Decided to use an apple to
compare movement of moon Known for Newton:
Moon 60 times farther than an apple Apple fell 4.9 m in first second Gravity is “diluted” by distance Moon should “fall” about 1.4 mm (and
it did as he proved by Geometry)
Falling Bodies (cont.) Newton put his findings away for
20 years until his “new branch” of mathematics (_______) helped further prove his calculations
This also proved the Copernican theory that the _____ revolves around the sun
Nothing crashes into the sun unless its tangential velocity is ______
Calculus
Earth
zero
Newton’s Law of Universal Gravitation Law states: “Every object attracts
every other object with a force that for any two objects is directly proportional to the mass of each object and inversely proportional to the square of the distance between them”
Or…F ~(m1)(m2)/d2
Newton’s Law of Universal Gravitation (cont.) Newton didn’t discover gravity,
just that it is universal. To put his law into a useable
equation, we have to establish the universal gravitational constant, G.
G = _________________This is very small because the force
is very weak
6.67 x 10-11 N•m2/kg2
Try One! Calculate the force of gravity
between a newborn baby (mass = 4.0 kg) and the planet Mars (mass = 6.4 x 1023 kg) when Mars is at its closest to Earth (distance = 8.0 x 1010 m).
2.67 x 10-8 N
May I have another? Calculate the force of gravity
between the same newborn and the obstetrician (mass = 75 kg), who is 0.30 m from the baby. Which exerted more force on the baby, Mars or the obstetrician?
2.22 x 10-7 N, Obstetrician
The Inverse-Square Law
The Inverse-Square Law (cont.) Similar to Mr. Hewitt’s butter gun,
the inverse square law is also applied to _________ and __________
If the distance between two objects doubles, the force between them is cut in ___________
In other words, the greater the distance from the Earth’s center, the less an object will weigh
gravity light
fourth
The Inverse-Square Law (cont.) See How to use the Rule of 1 on the
board... Two parts:
Replace whatever changed by the change factor
Replace everything else with a “1”. What happens to your weight if the
distance between the earth and you triples?
What happens to the force of gravity if both masses double?
Universal Gravitation Results Natural Proofs:
the Earth is round Planets deviate from their orbits when
they are near each other (perturbation)
Neptune and Pluto were found
Kepler’s Laws of Planetary Motion1. The paths of the planets are
ellipse with the center of the sun as one focus.
2. An imaginary line from the sun to a planet sweeps out equal areas in equal time intervals. Therefore, faster closer to sun, slower away from sun
3. (Ta/Tb)2=(ra/rb)3
Kepler’s Laws of Planetary Motion First two laws
deal with a planet or satellite individually.
Third law relates multiple planets or satellites to each other.
“r” in the third law is the average distance from the sun.
The “Rubber” sheet
Theoretical Gravity Activity
Calculating Your Weight
Books
Info on Fernbank◦ 10:00 AM◦ Meet in garden at front, Left◦ Missing Sign
Discussion on Today’s Probes
Wrapping up