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MYSTERIES OF EARTHMYSTERIES OF EARTHAND MARSAND MARS
Unit OneUnit OnePhysical SciencePhysical Science
(or, getting there from here)(or, getting there from here)
An Overview By- Jack Forristel -
Unit One ContentUnit One Content
Article 1.1 - Destination Mars
Article 1.2 - Energizing An Orbiter
Article 1.3 - Building A Rover
Article 1.4 - Water - Water
....Nowhere
Activity 1.1 - Build A Rocket
Activity 1.2 - Facts Of Friction
Activity 1.3 - Safe Landing
Activity 1. 4 - Properties Of
Salt/Fresh Water
Science Topics CoveredScience Topics Covered• Orbits
• Gravity
• Newton's Laws Of Motion
• Force
• Mass
• Energy
• Potential Energy
• Kinetic Energy
• Energy Transfer
• Conservation Of Energy
• Friction
• Design (Considerations)
• Engineering Constraints
• Properties Of Water
• Phase Changes
• Atmospheric Pressure
When To “Shoot”When To “Shoot”
• Closest @ 69M Km on 10/27/05?
• Furthest @ 390M Km on 9/27/06?
• Considerations- Daylight at launch/arrival- Wx at launch- Solar activity- Flight time- Length of flight
- On & on & on & on
ORBITAL MECHANICSORBITAL MECHANICS
ORBITAL MECHANICSORBITAL MECHANICS
ORBITAL MECHANICSORBITAL MECHANICS
Trajectory To LandingTrajectory To Landing
27 August, 200327 August, 2003Closest to earth in thousands of yearsClosest to earth in thousands of years
56M Km56M Km
9/23/05 Positions9/23/05 Positions
SIR ISAAC NEWTONSIR ISAAC NEWTON1642 - 1727
• Graduated from Cambridge University WITHOUT DISTINCTION.
• At age 23, began formulating his (1) Law of Universal Gravitation, (2) Calculus, (3) extended Galileo's work, (4) developed his 3 laws of motion and, (5), clarified the nature of light.
ISAAC NEWTONISAAC NEWTON1642 - 1727
When asked how he was able to make so many discoveries, he replied that he found his solutions to problems not by sudden insight but by thinking
very long and hard about them until he worked them out.
(I wish I had thought this way when I was a college student. May have helped.)
NEWTON’S FIRST LAW OF NEWTON’S FIRST LAW OF MOTIONMOTION
A body at rest or in uniform motion will remain at rest or in uniform motion unless some external force is applied to it.
Often referred to as the”law of inertia”.
NEWTON’S SECOND LAW NEWTON’S SECOND LAW OF MOTIONOF MOTION
The net force on an object is equal to the product of its acceleration and its mass.
F = ma
One of the most famous formulas in our world.
NEWTON'S THIRD LAW OF NEWTON'S THIRD LAW OF MOTIONMOTION
To every action force there is an equal and opposite reaction force.
Sometimes called the law of momentum.
M = mv
NEWTON’S LAW OF NEWTON’S LAW OF UNIVERSAL GRAVITATIONUNIVERSAL GRAVITATION
Every mass attracts every other mass with a force that, for any two masses, is directly proportional to the product of the masses and inversely proportional to the square of the distance separating them.
F = m1m2/d2
FORCEFORCE((Any influence that can cause an object to be
accelerated)
Typical Forces
• Gravity
• Friction
• Turning moments
• Pressure
• Balanced
• Unbalanced
Can Make Things• Speed up• Slow down• Change direction• Change shape• Turn• Change Size• Change Temperature
ENERGYENERGY
• POTENTIALPOTENTIAL energy is stored energy. It is there, it is available, it is useable.
• KINETICKINETIC energy is the energy of motion. Falling and moving bodies posses kinetic energy.
MORE ABOUT MORE ABOUT ENERGYENERGY
AEROBRAKINGAEROBRAKING
A technique used by spacecraft in which it uses drag within a planetary atmosphere to reduce its velocity relative to the planet. This removes a large amount of kinetic energy over a short period of time, most of which is converted into heat by shock heating the air ahead of the spacecraft.
AEROBRAKINGAEROBRAKINGGlobal SurveyorGlobal Surveyor
DESIGN CONSIDERATIONSDESIGN CONSIDERATIONS(Going-Landing-Roving)
• Structures (weight/strength)
• Energy (how much, what kind & when)
• Heating (going, entry, roving)
• Pressures (dynamic, atmospheric, gravity)
• Radiation (thermal, EMS)
• Others
NEXT: A FILMNEXT: A FILM
THEN: FLY A ROCKETTHEN: FLY A ROCKET
FOLLOWED BY: DROPPING FOLLOWED BY: DROPPING EGGSEGGS
From Here To There Via From Here To There Via Newton (and others)Newton (and others)
QuickTime™ and aSorenson Video decompressorare needed to see this picture.