Where in our solar system are asteroids that contain ammonia

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Discussion Overview

The discussion revolves around the potential sources of asteroids containing ammonia for the purpose of terraforming Mars. Participants explore the feasibility of redirecting these asteroids to raise the temperature and pressure on Mars, while also considering the implications of such actions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • One participant suggests that asteroids containing ammonia could be found in the asteroid belt or possibly in the rings of Saturn, but seeks clarification on their actual locations.
  • Another participant argues that asteroids or comets beyond Jupiter would likely retain more ammonia ice due to lower temperatures and less solar exposure.
  • Discussion includes the potential of using objects from the Kuiper belt, specifically mentioning Sedna as a source of nitrogen ice, though concerns are raised about its size for collision with Mars.
  • Participants discuss the energy requirements for melting the Martian poles and the size of asteroids needed to achieve this, with calculations suggesting that multiple smaller asteroids may be necessary.
  • There is a suggestion that terraforming Mars could be approached differently, such as using domes filled with existing Martian atmosphere rather than relying solely on asteroid collisions.
  • Concerns are raised about the consequences of colliding asteroids with Mars, indicating a need for further exploration of the potential impacts on the planet.
  • One participant mentions the concept of "detached objects" in the solar system, suggesting that there are many small asteroids that could be viable candidates for this project.

Areas of Agreement / Disagreement

Participants express various viewpoints regarding the sources of ammonia-containing asteroids and the methods for utilizing them for terraforming Mars. There is no consensus on the best approach or the implications of such actions, indicating ongoing debate and uncertainty.

Contextual Notes

Participants note that no asteroid has a fixed location in the solar system due to its movement, and the discussion includes assumptions about the availability and characteristics of asteroids in different regions.

Who May Find This Useful

This discussion may be of interest to researchers and enthusiasts in planetary science, astrobiology, and space exploration, particularly those focused on terraforming and the utilization of extraterrestrial resources.

Tristan27
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Hi! I'm doing a research project titled "Is it possible to colonise Mars?" I'm currently researching how to raise the temperature and pressure - and I've discovered to do this that re-directing asteroids towards Mars containing Ammonia would be vital.

However, where do these asteroids that contain Ammonia come from? Are they in the asteroid belt between Mars? Or are they in the rings of Saturn or somewhere else? Any help would be greatly appreciated.
 
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Tristan27 said:
Hi! I'm doing a research project titled "Is it possible to colonise Mars?" I'm currently researching how to raise the temperature and pressure - and I've discovered to do this that re-directing asteroids towards Mars containing Ammonia would be vital.

However, where do these asteroids that contain Ammonia come from? Are they in the asteroid belt between Mars? Or are they in the rings of Saturn or somewhere else? Any help would be greatly appreciated.
Welcome to the PF.

I'm not able to answer your main question (others will be able to), but I did a search for recent PF threads with Mars in the title, because there have been a few good ones about terraforming Mars and using other techniques. Check out the first few hits on the Search results to see if they help to give you other ideas for your project.

https://www.physicsforums.com/search/33842350/?q=mars&o=relevance&c[title_only]=1

:smile:
 
Sunlight evaporates ice. The tendency to do that diminishes with distance.
Ammonia has a melting point at -77C. Space is a vacuum so molecules sublime below the melting point. An asteroid or comet loses material when it is facing the sun. Average temperatures might be lower but the asteroid still gasses off. You would get a lot more ammonia ice if you look past Jupiter.

Here is nice temperature chart made by NASA with planets on a thermometer.

Pluto's moon Charon has a lot of Nitrogen ice. They are a natural place to put a space elevator and rail launch. Saturn's moon Titan a thick nitrogen atmosphere.

I would skip those and go for the Kuiper belt. Sedna has nitrogen. It has an orbital speed around 2km/s You won't need too much delta v to get a chunk dropping into the lower solar system. It would take a long time to arrive but for teraforming the wait would be trivial.
 
stefan r said:
Sunlight evaporates ice. The tendency to do that diminishes with distance.
Ammonia has a melting point at -77C. Space is a vacuum so molecules sublime below the melting point. An asteroid or comet loses material when it is facing the sun. Average temperatures might be lower but the asteroid still gasses off. You would get a lot more ammonia ice if you look past Jupiter.

Here is nice temperature chart made by NASA with planets on a thermometer.

Pluto's moon Charon has a lot of Nitrogen ice. They are a natural place to put a space elevator and rail launch. Saturn's moon Titan a thick nitrogen atmosphere.

I would skip those and go for the Kuiper belt. Sedna has nitrogen. It has an orbital speed around 2km/s You won't need too much delta v to get a chunk dropping into the lower solar system. It would take a long time to arrive but for teraforming the wait would be trivial.
Thankyou! In this case I'm specifically trying to collide the asteroid with
stefan r said:
Sunlight evaporates ice. The tendency to do that diminishes with distance.
Ammonia has a melting point at -77C. Space is a vacuum so molecules sublime below the melting point. An asteroid or comet loses material when it is facing the sun. Average temperatures might be lower but the asteroid still gasses off. You would get a lot more ammonia ice if you look past Jupiter.

Here is nice temperature chart made by NASA with planets on a thermometer.

Pluto's moon Charon has a lot of Nitrogen ice. They are a natural place to put a space elevator and rail launch. Saturn's moon Titan a thick nitrogen atmosphere.

I would skip those and go for the Kuiper belt. Sedna has nitrogen. It has an orbital speed around 2km/s You won't need too much delta v to get a chunk dropping into the lower solar system. It would take a long time to arrive but for teraforming the wait would be trivial.
Thankyou! However in this scenario, I'm trying to collide the asteroid with Mars rather than mine the resources from it. This way it can be used to collide with the poles of the planet and raise the temperature, simultaneously releasing the nitrogen from it.

Therefore, Sedna is far too big to collide with Mars. Are there any other asteroids elsewhere in the solar system which contain nitrogen ice and have a radious closer to around 10km-20km which could be used? With my calculations I've worked out around 125,000,000Mt of energy would be required just to melt the North Pole, 4 asteroids colliding that are 20km in diameter would just about give energy to melt the pole. Similarly, do you know if there would be any consequences of doing this for the planet? Thanks again!
 
Tristan27 said:
Hi! I'm doing a research project titled "Is it possible to colonise Mars?" I'm currently researching how to raise the temperature and pressure
Tristan27 said:
T This way it can be used to collide with the poles of the planet and raise the temperature, simultaneously releasing the nitrogen from it.

... Similarly, do you know if there would be any consequences of doing this for the planet? Thanks again!

You should change the title and use the word "terraform" instead of "colonize". A colony does not need to have a planet wide atmosphere. It is actually much easier to build a dome (or tunnel etc). You can fill a lot of domes with the nitrogen and oxygen already in Mar's atmosphere.

The goal is to mess up Mars. It there were no consequences for Mars then the terraforming project obviously failed.

Tristan27 said:
... Sedna is far too big to collide with Mars. Are there any other asteroids elsewhere in the solar system which contain nitrogen ice and have a radious closer to around 10km-20km which could be used?

You do not need or want to bring back all of it. The stuff that you do not use can be used for reaction mass. The Delta-v needed to escape Sedna is 440 m/s which is well below what can be done with tethers. Sedna's rotational period is 10 hours so the equator is already at 170 m/s. A space elevator could fling a package toward one of the gas giants once every 10 hours. Fixing the 12° inclination is a bigger issue than escaping from the gravity.

For every object with 1000 to 2000km diameter in the Kuiper belt (or oort cloud) there should be a million objects with 10 to 20 km. A 15km object in Sedna's orbit is not visible to our current telescopes. Sedna has a name. Wikipedia has an estimated chemical composition of the surface. Sedna has published orbital characteristics. Sedna is on a highly elliptical orbit (eccentricity 0.85) and under 12° degrees inclination. The ideal comet would be closer to 0° inclination and higher eccentricity.

No asteroid has a fixed location in the solar system. The solar system is moving. You can group objects and say something like "it is in the asteroid belt". So take your nitrogen from a "detached object". Since you might have millions or hundreds of millions of detached objects to choose from take one that is fairly close to the ecliptic plain. The "sednoids" are a subset of the "detached objects". Sedna is the big example we have have a sednoid. "Sednoid" is a location in the solar system.
 
stefan r said:
You do not need or want to bring back all of it. The stuff that you do not use can be used for reaction mass. A space elevator could fling a package toward one of the gas giants once every 10 hours.
Alright, thank you for the explanation on why Sedna would be more ideal than a random asteroid. Is it possible for you to explain how you could only bring back a part of it and what you mean by reaction mass in this situation?

Also when you say a "package" do you mean, for example, a piece of Sedna around 15km wide? The importance of this step is not just the nitrogen but using something to provide energy too heat up the poles which is why I believe using asteroids would be beneficial, so does this method still ultimately allow that to happen?

Sorry for all the questions aha, big thanks.
 
The problem with any idea of terraforming Mars is that Mars doesn't have a magnetic field. Any attempt to build up a strong atmosphere would be lost as it's swept away by solar winds.
 
Bigjoemonger said:
The problem with any idea of terraforming Mars is that Mars doesn't have a magnetic field. Any attempt to build up a strong atmosphere would be lost as it's swept away by solar winds.

Over what time scale? Over the course of a few million years you could drop in a lot of comets. Mars lost its atmosphere over several hundred million years.

We could compare the mass of an orbital magnet large enough to redirect solar wind and the mass of an Earth like atmosphere. The magnet is very lite in comparison. If the goal is to have an earth-like ecosystem you probably need some mirrors in space too.
 

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