A consequence of Kepler's Second Law (law of equal areas) is that a planet moves faster in its orbit when it is closer to the Sun and slower when it is farther away. This results in an uneven distribution of orbital velocities throughout the planet's orbit.
Kepler's second law, also known as the law of equal areas, is a consequence of the conservation of angular momentum.
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The second law of thermodynamics states that not all heat energy can be converted into work. Some heat will always be lost in the form of waste heat during energy conversion processes. This law is a fundamental principle that governs the efficiency of energy conversion systems.
Newton's version of Kepler's Third Law states that the square of the period of revolution of a planet around the Sun is directly proportional to the cube of its average distance from the Sun. It can be expressed mathematically as T^2 ∝ r^3, where T is the period and r is the average distance.
Newton's Second Law of Motion states that force is equal to mass times acceleration. This law describes the relationship between the force applied to an object, its mass, and the resulting acceleration.
Kepler's second law, also known as the law of equal areas, is a consequence of the conservation of angular momentum.
... when it is closest to the Sun. (Kepler's Second Law)... when it is closest to the Sun. (Kepler's Second Law)... when it is closest to the Sun. (Kepler's Second Law)... when it is closest to the Sun. (Kepler's Second Law)
Kepler's second law, also known as the law of equal areas, states that a planet sweeps out equal areas in equal times as it moves around the Sun. This means that a planet travels faster when it is closer to the Sun in its orbit and slower when it is farther away.
It implies that the planet must move faster in its orbit when it's closer to the sun, and slower when it's farther from the sun, since, according to the second law, the radius vector joining the planet to the sun must sweep out equal areas in equal increments of time.
When any planet orbits any sun then the line from the planet to the sun sweeps out a certain area every second (or hour etc). For a circular orbit it is obvious that the area swept out is the same for the same time interval, no matter where you start your measurement. It turns out that even for normal, or even highly, elliptical orbits (real planets, or even comets), it remains true that the area swept out per second, or hour etc is constant. Newton showed this to be a direct consequence of an inverse square law of gravitation, and explained this observation of Kepler, deduced from many painstaking observations and measurements.
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Kepler's Third Law, also known as the Harmonic Law, states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
Kepler's first law says Neptune has an elliptical orbit with the Sun at one focus. The same goes for the other planets.
Kepler's law that describes how fast planets travel at different points in their orbits is called the Law of Equal Areas. This law states that a planet will travel faster when it is closer to the Sun and slower when it is farther away, so that the area it sweeps out in a given time is the same regardless of its distance from the Sun.
There are many ways in which you could use the word consequence in a sentence. You could say that the consequence for not paying an electric bill is the shut off of your electricity for example.
Actually Murphy's law has been suggested (humorously) as "the fourth law of thermodynamics". It is only peripherally related the the second law. One of the implications of the second law is that an increase in disorder in the universe is a consequence of natural processes. Some have suggested that Murphy's law (If any thing can go wrong, it will.) is an example of this. Strictly speaking - this is quite different from the 2nd law but when someone screws up, it sure does tend to cause a lot of disorder!
The consequence is license restriction for life and a 12 to 15 thousand dollar fine.