Calculating relativistic effects of motion in solar system

In summary, the conversation discusses the calculation of an impactor hitting a specific spot on Mercury, taking into account the relativistic precession of the planet. Pauline explains that without factoring in this effect, the trajectory would miss by 13.39 kilometers. The accuracy of the numbers is questioned, but the concept is a classic test of General Relativity. The conversation also touches on the difficulty of launching a probe to Mercury without the use of course corrections and the need for precise calculations.
  • #1
KenJackson
63
10
This question and answer are posed in Kim Stanley Robinson's novel "2312".

"Pauline, if someone had calculated the trajectory of an impactor to hit [an exact spot on the planet Mercury], but they forgot to include the relativistic precession of Mercury in their calculation and only used the classical calculus of orbital mechanics, how far would they miss by? Assume the impactor was launched from the asteroid belt a year earlier."

Pauline said, "The precession of Mercury is 5603.24 arc seconds per Julian century, but the portion of that caused by the curvature of space-time as described by general relativity is 42.98 arc seconds per century. Any trajectory a year in duration, plotted without that factored in, would therefore miss by 13.39 kilometers."

My question is, is this all made up? Or might it be accurate?
 
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  • #3
Interesting. The numbers are in the novel the way I typed them.

Even though Pauline answered only the precession part of the question, I was fascinated by the possibility of the whole calculation. In recent years, NASA and other countries' space agencies have sent probes to Mars, asteroids and even a comet. But I think they all had thrusters to do course corrections along the way.

But if you throw a rock at Mercury from the asteroid belt, how would you calculate (even in theory) the direction and speed to make it hit a specific spot after a year's travel--with no mid-course corrections!?
 
  • #4
KenJackson said:
In recent years, NASA and other countries' space agencies have sent probes to Mars, asteroids and even a comet. But I think they all had thrusters to do course corrections along the way.

They did, but the course corrections are very small; a probe can't carry enough fuel to make large course corrections, so it has to be launched very accurately to begin with. The course corrections are not always needed, but NASA allows for the possibility to be safe.

KenJackson said:
if you throw a rock at Mercury from the asteroid belt, how would you calculate (even in theory) the direction and speed to make it hit a specific spot after a year's travel--with no mid-course corrections!?

You would have to know the precise positions of the asteroid, the Sun, and the planets at launch, so you could compute the rock's trajectory to the required accuracy. It's tedious, but straightforward; you start out with the asteroid and Mercury moving in the field of the Sun as your first approximation, then just add in effects of other planets until you've taken into account every effect that's large enough to matter. Nowadays computers would do all the grunt work anyway.
 

1. What is the theory of relativity and how does it apply to motion in the solar system?

The theory of relativity, proposed by Albert Einstein, is a fundamental principle in physics that explains the relationship between space and time. It states that the laws of physics are the same for all observers in uniform motion. This theory applies to the motion of objects in the solar system by taking into account the effects of gravity and the speed of light.

2. How do you calculate the relativistic effects of motion in the solar system?

To calculate the relativistic effects of motion in the solar system, you would need to use Einstein's special theory of relativity. This involves calculating the Lorentz factor, which takes into account the speed of the object and its distance from the gravitational source. This factor is then used to adjust the measurements of time and space, resulting in more accurate calculations.

3. What are some examples of relativistic effects in the solar system?

One example of relativistic effects in the solar system is the bending of light around massive objects like the sun. This is known as gravitational lensing and is a result of the curvature of space and time caused by the sun's gravitational pull. Another example is the time dilation experienced by objects moving at high speeds in the solar system, which causes their clocks to run slower compared to stationary objects.

4. How do relativistic effects affect space travel in the solar system?

Relativistic effects have a significant impact on space travel in the solar system. For example, the closer an object gets to the speed of light, the more energy is required to accelerate it further. This means that objects traveling at high speeds will experience time dilation and will age slower compared to objects that are stationary. Additionally, the effects of gravity on objects in motion must be taken into account when plotting trajectories and planning missions.

5. How does the study of relativistic effects in the solar system contribute to our understanding of the universe?

The study of relativistic effects in the solar system is crucial in helping us understand the fundamental laws of the universe. It has allowed us to make accurate predictions and calculations about the behavior of objects in the solar system and beyond. It also helps us better understand the nature of space and time and how they are interconnected. Additionally, the study of relativistic effects has led to groundbreaking theories and discoveries in physics, such as black holes and the expansion of the universe.

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