Exploring Orbital Motion Around Earth

In summary, when an object is launched into space and its forward momentum is stopped, it will not necessarily come back to the same point after a year due to the effects of gravity. The object will be pulled into an elliptical orbit and will continue to cross paths with the Earth until eventually colliding with it. The amount of orbits before this collision will vary depending on the object's initial speed and distance from the sun. The sun is actually the most difficult place to reach in the universe due to the high delta v required. Ultimately, the object and the Earth will collide unless outside forces change their orbit.
  • #1
Guiwee
2
0
orbiting earth!

Hope iposted this question in the right spot!.
If i launched something in space and then stopped its forward momentum
wouldnt the Earth gradually move away from it and pick it up again so to speak..a year later?
 
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  • #2


Motion is always relative to something, so in this case I assume you mean to stop the motion of an object relative to the sun at some point near the Earth and then want to know if the Earth will move around the sun and then come back to this point a year later? If you were to ignore gravity on the object, then the answer would more or less be yes, but if you include gravity then the answer would be no, as the object would fall toward the sun.
 
  • #3


In fact, the object would fall toward the Sun and miss, which is kind of the definition of an orbit. Your object would be pulled into a very ellipticle orbit, with the highest point being equal to the distance from which it originaly fell, which is the distance from the Sun to the Earth (1 AU). Unless it made a close pass by Venus or Mercury, or had some other outside force change its orbit, it would continue going in close to the Sun and back out to where the Earth orbits until it eventually gets to Earth's orbit at the same time Earth is passing through that point in its orbit. Then, of course, it would hit Earth (or Earth would hit it).
 
  • #4


LURCH said:
In fact, the object would fall toward the Sun and miss, which is kind of the definition of an orbit. Your object would be pulled into a very ellipticle orbit, with the highest point being equal to the distance from which it originaly fell, which is the distance from the Sun to the Earth (1 AU). Unless it made a close pass by Venus or Mercury, or had some other outside force change its orbit, it would continue going in close to the Sun and back out to where the Earth orbits until it eventually gets to Earth's orbit at the same time Earth is passing through that point in its orbit. Then, of course, it would hit Earth (or Earth would hit it).

Any object that is even a bit slower than Earth at Earth's distance from the sun would be in an orbit with a different orbital time than earth, so after a year it it will not be where Earth is. If we assume this special object is put into an orbit where perihelios (closest point to sun) is approximately zero, the period of the object would be around 130 days.
 
  • #5


So, how many orbits before it would hit Earth?
 
  • #6


LURCH said:
So, how many orbits before it would hit Earth?

Well, after one year the object would have done 2 orbits and will be around 22 days from completing its third. In other words, everything else being equal it would miss Earth with 22 days on its third orbit.
 
  • #7


By the way, the delta v required to get to the sun is very high, much higher than the delta v required to escape the sun. In that sense, the sun is the most difficult place to reach in the universe. You can get anywhere else with less fuel (ignoring, of course, fancy maneuvers like gravitational slingshot etc).
 
  • #8


Filip Larsen said:
Well, after one year the object would have done 2 orbits and will be around 22 days from completing its third. In other words, everything else being equal it would miss Earth with 22 days on its third orbit.
And, if my rough guesses are close, there is a point about 5 or 6 years out where it misses by lass than a week, and around 10 years down the road I think it gets so close that our gravity would do the rest. These are just estimates by picturing the orbits in my head, of course; I'll try to do the maths (internet has been down for almost a week).

The point is, the two cannot just keep crossing paths forever; they must eventually colide.
 

Related to Exploring Orbital Motion Around Earth

1. What is orbital motion around Earth?

Orbital motion around Earth refers to the path that an object takes as it revolves around the Earth. This motion is caused by the gravitational pull of the Earth on the object.

2. What factors affect orbital motion around Earth?

The main factors that affect orbital motion around Earth are the mass and velocity of the object, as well as the distance between the object and the Earth. Other factors such as atmospheric drag and the gravitational pull of other celestial bodies can also impact orbital motion.

3. How does orbital motion around Earth differ from other types of motion?

Unlike linear or circular motion, orbital motion around Earth is a combination of both. The object is constantly moving in a circular path around the Earth while also moving forward along its orbital path. This results in a curved trajectory known as an orbit.

4. How do we calculate orbital motion around Earth?

To calculate orbital motion around Earth, we use Kepler's laws of planetary motion and Newton's law of universal gravitation. These laws allow us to determine the velocity, period, and shape of the orbit based on the object's mass and distance from the Earth.

5. What are some applications of studying orbital motion around Earth?

Studying orbital motion around Earth is crucial for space exploration and satellite technology. It helps us understand the mechanics of orbits and how to maintain them, as well as predict the movement of celestial bodies. This knowledge also aids in the development of space missions and satellite communication systems.

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