Kepler’s 1st Law
If you have not already done so, launch the NAAP Planetary Orbit Simulator.
• Open the Kepler’s 1st Law tab if it is not already (it’s open by default).
• Enable all 5 check boxes.
• The white dot is the “simulated planet.” One can click on it and drag it around.
• Change the size of the orbit with the semi-major axis slider. Note how the background grid indicates change in scale while the displayed orbit size remains the same.
• Change the eccentricity and note how it affects the shape of the orbit.
Tip: You can change the value of a slider by clicking on the slider bar or by entering a number in the value box.
Be aware that the ranges of several parameters are limited by practical issues that occur when creating a simulator rather than any true physical limitations. We have limited the semi-major axis to 50 AU since that covers most of the objects in which we are interested in our solar system and have limited eccentricity to 0.7 since the ellipses would be hard to fit on the screen for larger values. Note that the semi-major axis is aligned horizontally for all elliptical orbits created in this simulator, where they are randomly aligned in our solar system.
• Animate the simulated planet. You may need to increase the animation rate for very large orbits or decrease it for small ones.
• The planetary orbital options let you set the simulated planet’s parameters to those like our solar system’s planets. Explore these options.
Question It is easy to create an ellipse using a loop of string and two thumbtacks. The string is first stretched over the thumbtacks which act as foci. The string is then pulled tight using the pencil which can then trace out the ellipse. Assume that you wish to draw an ellipse with a semi-major axis of a = 20 cm and e = 0.5. Using what you have learned earlier in this lab, what would be the appropriate distances for a) the separation of the thumbtacks and b) the length of the string? Please fully explain how you determine these values.
Kepler’s 1st Law If you have not already done so, launch the NAAP Planetary Orbit Simulator....
Kepler’s Third Law indicates that the Period (P) of an orbit is related to the semi-major axis (a) of the orbit with: P 2 = ka3 . Kepler noticed that the value of the constant k changes when we observe systems with different central objects. This means that the orbits of all of the planets in the Solar System have the same value for k, but that value is different for the Moon because all of the planets orbit the...
• Use the “clear optional features” button to remove the 1st Law features. • Open the Kepler's 2nd Law tab. • Press the “start sweeping” button. Adjust the semimajor axis and animation rate so that the planet moves at a reasonable speed. • Adjust the size of the sweep using the “adjust size” slider. • Click and drag the sweep segment around. Note how the shape of the sweep segment changes, but the area does not. • Add more sweeps....
• Use the “clear optional features” button to remove the 1st Law features. • Open the Kepler's 2nd Law tab. • Press the “start sweeping” button. Adjust the semimajor axis and animation rate so that the planet moves at a reasonable speed. • Adjust the size of the sweep using the “adjust size” slider. • Click and drag the sweep segment around. Note how the shape of the sweep segment changes, but the area does not. • Add more sweeps....
In Lecture 4, we discussed Kepler’s third law relatingthe orbital period of a planet (p) to the semi-major axis (orbital distance, a) of its orbit(p2= a3). We can apply this law as long the object orbits the Sun or another object of the same mass, and the units of orbital period are in (Earth) years and the orbital distance is in Astronomical Units(AU). [1AU is equal to the distance between the Earth and the Sun]. [Note: Newton extended this law...
could you please solve a and b?
Chapier 2i. Note: you needn't derive Kepler's laws-but do mention when you are using them, an describe the physical concepts involved and the meanings behind the variables. u) Consider two stars Mi and M; bound together by their mutual gravitational force (and isolated from other forces) moving in elliptical orbits (of eccentricity e and semi-major axes ai and az) at distances 11 in n and r from their center of mass located at...
Please help with my car traffic simulator!
Code that I already have below, I do not know how to start it
off!
public class IntersectionSimulation
{
private final static int EAST_WEST_GREEN_TIME = 30 ;
private final static int[] NORTH_SOUTH_GREEN_TIMES = { 20, 24, 30, 42 } ;
private final static int[] CAR_INTERSECTION_RATES = { 3, 5, 10 } ;
private final static int[] CAR_QUEUEING_RATES = { 5, 10, 30 } ;
private final static int[] EXPERIMENT_DURATIONS = { 3*60, 5*60,...