2.3 
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Videos:
Interactive Simulations   Position and displacement in one dimension    Displacement and position in two dimensions    Solve v=dx/dt for dt    Velocity, position, and time (basic version)    Velocity, position, and time (more advanced version)    Acceleration (basic version)    Acceleration (more advanced version)    Static equilibrium    Static equilibrium and the lever    Newton's second law (basic version)    Newton's second law (more advanced version)    Circular motion interactive simulation    Orbits of the planets and dwarf planets    Orbits simulation Interactive Calculators   Speed calculator    Velocity calculator    Acceleration calculator    Velocity in accelerated motion    Average velocity calculator    Hooke's law calculator    Torque calculator    Rotational equilibrium and torque    Newton's second law calculator    Momentum calculator    Angular velocity    Linear velocity and angular velocity    Centripetal acceleration    Centripetal force    Law of universal gravitation calculator
1 - Science of Physics
2 - Forces and Motion      Chapter 2 at a glance      2.1 - Motion      2.2 - Force, momentum, and Newton's laws      2.3 - Circular motion      2.4 - Solving harder physics problems      2.5 - Chapter review3 - Energy Transformations4 - Waves and Sound
5 - Electricity and Magnetism
6 - Light and Optics
7 - The Atom
8 - Linear Motion
9 - Vectors and Forces
10 - Forces
11 - Newton's Laws and Gravitation
12 - Circular Motion and Gravitation
13 - Torque and Static Equilibrium
14 - Momentum and Collisions
15 - Angular momentum
16 - Power and Machines
17 - Harmonic Motion
18 - Waves
19 - Sound
20 - Electricity
21 - Electric and Magnetic Fields
22 - Electromagnetism and Induction
23 - Light and Color
24 - Geometrical Optics
25 - Electromagnetic Radiation
26 - The Properties of Matter
27 - Thermodynamics and Heat Transfer
28 - The Atom
29 - The Quantum Theory
30 - TBD
31 - TBD
32 - TBD
33 - TBD
34 - TBD
35 - TBD
36 - TBD
37 - The atomic nucleus and radioactivity
38 - Nuclear reactions
39 - Relativity
40 - Particle physics and the standard model
41 - Electronics (semiconductors)
42 - Nuclear technology
43 - Lasers and photonics
44 - Metals, alloys and materials science
45 - Communications technology
46 - Buildings and structures
47 - Energy technology
48 - Biophysics
49 - Matter and Energy, Space and Time
50 - Energy Transformations
51 - Nanotechnology
52 - Website Videos
53 - ExtraStuff
55 - Modeling Motion, Friction, and Center of Mass
56 - Work and the Conservation of Energy
2G: Orbits
How does velocity relate to a planet's orbital radius?
How do you send a satellite from Earth to another planet's orbit?
The planets in the Solar System orbit the Sun in ellipses—elongated circles—although many of the planets have nearly-circular orbits. As a planet is placed further from the Sun, it experiences a smaller acceleration due to the Sun's gravity and hence travels with a different orbital velocity. In this investigation you will determine the velocities of different planetary bodies in the Solar System and correlate that with their distance from the Sun.
Part 1: Orbital velocities of the planets

How to use the orbits simulation
  1. In the interactive simulation, select the planet Earth.
  2. Vary the orbital velocity v to find your best match for the Earth's true orbit. Also record the average distance from the Sun (the semi-major axis).
  3. Repeat for the other seven planets.
  1. Does Jupiter move faster or slower than the Earth?
  2. How does orbital velocity vary with distance from the Sun?
  3. Graph orbital velocity v against distance from the Sun r. Is it a straight line?
  4. Devise a new graph of v against a different quantity derived from r that will be a straight line. Measure its slope (including its units). Show Shapes of different orbits
Orbits of the planets and dwarf planets In this interactive simulation, you will create orbits for the planets, dwarf planets, and other Trans-Neptunian objects (TNOs). When you select a particular planet, its true orbit will be plotted in the simulation. You will adjust the initial orbital velocity—in particular, you are varying the velocity at its closest approach, known as the perihelion velocity vperi—in order to get the best match to its true orbit. Show Astronomical units
Part 2: Transfer orbits

Transfer orbit from Earth to Mars In order to send a satellite from one planet to another, it is necessary to change the satellite's velocity. These trajectories are called transfer orbits.
  1. Select Earth. Determine the initial velocity necessary to propel a satellite initially from Earth's orbit to just barely reach Mars's orbit.
  1. Compare the average velocity for Earth's orbit (from part 1) with the velocity necessary to reach Mars's orbit. How much does it need to change?
  2. What provides this change in velocity of the satellite?
  3. How much “elapsed time” does it take for this satellite to reach Mars? Compare this length of time to typical missions of the Space Shuttle and International Space Station.

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