Orbital mechanics is a very difficult and complex science, because we do not have a generalized way to compute the gravitational attractions between a large number of objects. But in any system with two large masses, such as the Earth and the Moon, or between the Sun and the Earth, there are five relatively stable points. These are called Lagrange Points.
Lagrange points maintain their positions in respect to two large masses throughout the entire orbital period.
The L1 point is between the Earth and the Sun where the pull of gravity from each body is cancelled out. Because of the higher gravity from the Sun, the L1 point is closer to the Earth than the Sun.
The first Lagrange Point, L1, is directly between the two masses, but closer to the smaller mass, where the pull of gravity from each body is more-or-less cancelled out. In the Earth-Moon system, the L1 point is about 38,000 miles from the Moon. The L2 point is along the line from the Earth to the Moon, about 38000 miles past the Moon.
The L3 point is in the Moon's orbit, directly opposite the Earth from the Moon.
The L4 and L5 points lie in the Moon's orbit, 60 degrees ahead of and 60 degrees behind the Moon in its orbit. Many science fiction stories depict space stations in the L5 point, because this would be a stable location in the system; things would tend to "fall into" the L4 or L5 points and tend to remain there.
Example:
earth rotating around the sun
place (nominal mass) object in between at nominal point close to the sun
measure the net gravitational pull (assume its toward the sun)
calculate the orbital velocity required to balance this with centripetal force
orbit time should be less than the earths
move object closer to the earth until the required orbit time matches the earth
this is one of the legrange points of this system
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Additional notes:
1. This is a L1 lagrange point (there are 5 such points on this type of arrangement).
2. The centre of gravity of the earth / sun system should be taken into account
when calculating the orbital velocity from : v = sq root ( r * net gravity)
Net gravity calcs are from sun / earth centres, but the orbital radius (r) of the object is measured from the centre of gravity of the sun / earth system.
*** original answer *** i dont have a clue what you are talking about but the earth is far bigger than the moon ******************* *** correct answer *** There are actually 5 Lagrange points in any two body system. I assume you're referring to the L1 point. This is the point along the line between the Earth and Moon where the gravitational forces from each body equal each other. That point is roughly 345,000 km from the center of the Earth (the Earth's radius is ~6378 km). The total distance from the Earth to the Moon is about 384,000 km. *******************
The asteroid will always take the path minimizing its Lagrangian, known as the least action principle in Lagrangian mechanics. With conservative forces, there are four basic shapes for two different cases. Either the asteroid is trapped in the gravitational pull of an object, or it is not trapped. If the asteroid's energy is low enough to be trapped, then it can have either a circular or elliptical orbit. If it is not trapped, then this 'free asteroid' (much like a free electron) can have either an parabolic or hyperbolic path. Much of this information came from "Classical Mechanics" by kibble and Berkshire (although there are much better books). Depends on the asteroid. Most of them in our solar system rotate around the sun like we do. The path, as with all the planets is an ellipse.
A point of view is the point of view from each individual person. You have a point of view from your perspective. Your mother, your father, your brother, your sister, your teacher, they all have their own point of view. Everyone has their own point of view. Their own particular way of looking at the world from their experience, and thoughts, beliefs, and way of thinking. Everyones' point of view is different.
The point at which a line between the satellite and the centre of the Earth intersects the Earth's surface is called the subsatellite point.
The point is called a perigee.
SOHO (Solar and Heliospheric Observatory) was launched into the Earth/Sun L1 Lagrangian point in 1995. This point balances the gravity from the Sun and Earth and allows for very little energy to remain in a stable orbit. There are 5 Lagrangian points for SOHO but L1 is the best positioned for Earth communications.
In lagrangian we use scalar quantity which is much easier to solve then vector quantites used in newtonian.also lagrangian is invariant under gauge transformation and the same not hold good for newtonian.
It starts at the base of the head (C1) and ends at the lumbar vertebrae (L1).
Lagrangian (L) summarizes the dynamics of the system.Generally, in classical physics, the Lagrangian is defined as follows:L=T-Vwhere T is kinetic energy of the system and V is its potential energy. If the Lagrangian of a system is has been defined, then the equations of motion of the system may also be obtained.
The next generation telescope will have the two or twin telescopes. One will have to be stationed at the Lagrangian point 4 and the other at the Lagrangian point 5. So together they will act like the pair of your eyes. So you can penetrate in the space out of your universe also. Then you can locate the source of cosmic microwave back ground also, most probably. The cosmic dust coming in the way of one telescope and not in the way of other can be easily deleted by simple computer. By this mechanism you can increase the size of the lens of the telescope to hundreds of thousands of kilo meters. The processing unit can be kept at Lagrangian point one. This telescope should cost less than or about the same as the James Web telescope.
UP, SQUARE, SQUARE, DOWN, LEFT, SQUARE, SQUARE, RIGHT Weapon set 1 UP, CIRCLE, CIRCLE, DOWN, LEFT, CIRCLE, CIRCLE, RIGHT Weapon set 2 UP, X, X, DOWN, LEFT, X, X, RIGHT Weapon set 3 L1, R1, TRIANGLE, L1, R1, CIRCLE, L1, R1 Money Cheat ($250,000) L1, R1, CIRCLE, L1, R1, X, L1, R1 Full Armor (Blue Bar) L1, R1, X, L1, R1, SQUARE, L1, R1 Full Health (Red Bar) L1, R1, SQUARE, L1, R1, TRIANGLE, L1, R1 Raise Wanted Level L1, L1, TRIANGLE, R1, R1, X, SQUARE, CIRCLE Never Wanted CIRCLE, X, DOWN, CIRCLE, X, UP, L1, L1 Cars Drive on Water X, X, R1, CIRCLE, CIRCLE, L1, TRIANGLE, TRIANGLE White Cars CIRCLE, CIRCLE, R1, TRIANGLE, TRIANGLE, L1, SQUARE, SQUARE Black Cars L1, UP, RIGHT, R1, TRIANGLE, SQUARE, DOWN, X Raise Media Attention TRIANGLE, CIRCLE, DOWN, TRIANGLE, CIRCLE, UP, L1, L1 Spawn Trash master L1, L1, LEFT, L1, L1, RIGHT, SQUARE, TRIANGLE Random random Outfit L1, L1, CIRCLE, R1, R1, SQUARE, TRIANGLE, X Sunny Weather UP, DOWN, CIRCLE, UP, DOWN, SQUARE, L1, R1 Clear Weather UP, DOWN, X, UP, DOWN, TRIANGLE, L1, R1 Overcast Weather UP, DOWN, SQUARE, UP, DOWN, CIRCLE, L1, R1 Rainy Weather UP, DOWN, TRIANGLE, UP, DOWN, X, L1, R1 Foggy Weather L1, L1, LEFT, L1, L1, RIGHT, TRIANGLE, CIRCLE Spawn Rhino L1, L1, LEFT, L1, L1, RIGHT, CIRCLE, X Faster Clock L1, L1, LEFT, L1, L1, RIGHT, X, SQUARE Destroy All Cars L1, L1, R1, L1, L1, R1, LEFT, SQUARE Peds Riot L1, L1, R1, L1, L1, R1, UP, TRIANGLE Peds Attack You R1, R1, L1, R1, R1, L1, RIGHT, CIRCLE Peds Have Weapons
the cheat is: L1, L1, LEFT, L1, L1, RIGHT, TRIANGLE, CIRCLE
L1,L1,left,L1,L1,right,triangle,circle
The cheat code is L1, L1, LEFT, L1, L1, RIGHT, TRIANGLE, CIRCLE
The cheat is: O, X ,L1 ,O ,O, L1 ,O, R1, R2 ,L2, L1 ,L1
For GTA: San Andreas (PS2):Spawn a Hunter: O X L1 O O L1 O R1 R2 L2 L1 L1
L1,L1,LEFT,L1,L1,RIGHT,SQUARE,CIRCLE. the tank will fall on the road. or it might fall behind you