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PHYS16 – Lecture 28 Kepler’s Laws and Fluids November 12, 2010

PHYS16 – Lecture 28

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PHYS16 – Lecture 28. Kepler’s Laws and Fluids November 12, 2010. Kepler’s Laws. Orbits are elliptical. Eccentricity = 0, then circular Eccentricity = 1 then linear Most planets have an eccentricity close to 0. Equal areas in equal times. - PowerPoint PPT Presentation

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Page 1: PHYS16 – Lecture 28

PHYS16 – Lecture 28

Kepler’s Laws and Fluids November 12, 2010

Page 2: PHYS16 – Lecture 28

Kepler’s Laws

Page 3: PHYS16 – Lecture 28

Orbits are elliptical

• Eccentricity = 0, then circular

• Eccentricity = 1 then linear

• Most planets have an eccentricity close to 0

Page 4: PHYS16 – Lecture 28

Equal areas in equal times

• The area of the triangle swept out by the object is equal for equal amounts of time

• The further the object is from the sun the lower the speed.

constantdtdA

Page 5: PHYS16 – Lecture 28

Example Question: Earth Speed

• Where is the speed of the earth the greatest?

D

A C

B

Page 6: PHYS16 – Lecture 28

Period-squared is proportional to a3

constant

4

v

3

2

32

2

22

2

aT

rGM

T

rGMr

rGM

Page 7: PHYS16 – Lecture 28

Example Question: Venus’ Period

• Venus has a semi-major axis that is 0.723 times the Earth’s semi major axis. How long does it take Venus to orbit the Sun?

A) 204 daysB) 224 daysC) 264 daysD) 294 days

Page 8: PHYS16 – Lecture 28

Example Question: Seasons

• If the earth spends two less days in the winter half of the orbit than the summer half of the orbit (for N. hemisphere), what is its speed in winter vs. summer?A) FasterB) SameC) SlowerD) Not enough information

Supposed to be sweeping out equal areas in equal times.But if times aren’t equal, then either the areas aren’t equal orthe Earth’s speed is faster in winter…

Page 9: PHYS16 – Lecture 28

Main Points

• Gravitational Force and Potential• Satellites– Orbital energy– Escape velocity– Geostationary orbits

• Kepler’s Laws– Orbits are elliptical– Orbits sweep out equal area in equal time– Orbital period-squared is proportional at a3

Page 10: PHYS16 – Lecture 28

Fluids

Page 11: PHYS16 – Lecture 28

This Week

• Pressure and Pascal’s Principle• Buoyant Force and Archimedes’ Principle• Equation of Continuity• Bernoulli’s Equation

Page 12: PHYS16 – Lecture 28

Fluids

• Fluid = a liquid or a gas, a substance that flows• What happens when you apply a force to a

fluid?– Gas compresses(change density)

– Liquids are incompressible

http://www.swe.org/iac/images/liquid-gas2.jpg

Page 13: PHYS16 – Lecture 28

Pressure

• Pressure (p) – Force per unit area– Direction of pressure is normal to a surface– Unit is Pa=N/m2

• Air Pressure = 1E5 Pa = 1 atm = 760 mmHg

AFP

http://www.school-for-champions.com/science/pressure.htm

Page 14: PHYS16 – Lecture 28

Example: Force due to Air Pressure

• What is the force on the lid of a pop can due to air pressure ? (radius = r = 0.020 m)

N 130m) )(0.02Pa)( 5E1()( 22

FrPPAF

So why doesn’t the pop can get crushed?

Page 15: PHYS16 – Lecture 28

Pascal’s Principle

• Pressure change in a confined fluid is the same at all points in the fluid

• Mechanical advantage in hydraulic lift = Abig/Asmall

http://www.vectorsite.net/tpecp_08.html

m = 1 kg

Page 16: PHYS16 – Lecture 28

Example: Cracking an Egg

• If I apply equal force to all sides of an egg, will it crack?

No!

http://randywakeman.com/TragicEgg.jpg

Page 17: PHYS16 – Lecture 28

Main Points

• Pressure = Force/Area• Pressure change in a confined fluid is the same

at all points