Bode's Law, also known as Titius-Bode law, provides a numerical pattern that predicts the position of most planets in our Solar System, including Jupiter. It, however, fails to accurately predict the location of Uranus and Neptune. The fundamental principles of planetary motion were established by Kepler's laws and later consolidated by Newton in his Universal Law of Gravitation.
This question pertains to Bode's Law, a rule of planetary distances at times referred to as the Titius-Bode Law. The rule indicates a pattern of increasing distances of the planets from the sun, which interestingly correlates to the position of most planets in our Solar System, including Jupiter. However, exceptions, particularly Uranus and Neptune, don't fit precisely into this pattern.
The origins of planetary motions can be traced back to the work of scientists like Herr Tycho Brahe, Johannes Kepler, and Sir Isaac Newton. Kepler's work in particular developed three fundamental laws of planetary motion using Brahe's meticulously collected data. These laws describe the behavior of planets in their orbits and together provide the foundation of the Universal Law of Gravitation as later synthesized by Newton.
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When you eat the right amount of food for your diet and could not attain the desired figure you want, you should change the routine of your exercise. It might be because your exercise is not efficient for your body type.
Answer:
Stick to the schedule anyway. Learning what does not work can be just as valuable as learning what does work. You can reevaluate the schedule at the end of the week and change it as necessary.
Answer:
Schwarzschild radius
Explanation:
A black hole is defined as that object from which light cannot escape form the surface of the object because object is very small an very dense. There are numerous black hole sin the universe.
Black hole is well understood by the concept of "escape velocity". Escape velocity is the speed of any object to break the gravitational pull from another object.
Escape velocity depends on mass of the object and the distance from the center of the object ( how big or small the object is ). If the object is smaller or more denser, than the escape velocity is more. If we squeeze our earth to a radius of about 9 mm sphere, then the escape velocity of any object becomes equal to the velocity of light.
And the radius of any object which have an escape velocity which is same as the velocity of light is known as the 'Schwarzschild radius'.
Any object which is smaller than the "Schwarzschild radius' has an escape velocity more than the speed of light and is termed as a black hole.
Thus, any object which is squeezed beyond the Schwarzschild radius be becomes a black hole.
a. True
b. False
Answer:The amplitude is approximately 4.52 h x 2.3 f(t)
Explanation: