What Are the Challenges and Proposed Solutions for Terraforming Mars?

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Mars presents significant challenges for terraforming, including low atmospheric pressure, extreme temperatures, a toxic atmosphere, and a lack of liquid water. Proposed solutions involve melting the ice caps to release CO2 and H2O, potentially using nuclear explosions or microwave lasers to achieve this. There is discussion about introducing engineered extremophile bacteria to convert CO2 into oxygen and the need for nitrogen sources, possibly through ammonia impacts. The conversation also highlights the risks of large-scale interventions and the importance of controlled, incremental approaches to colonization. Overall, the goal remains to make Mars more Earth-like while carefully considering the ecological and logistical implications of such efforts.
  • #61
maze said:
I think you are confusing pseudoscience with impractical science.

Due to the fact that nukes in space are outlawed by the order of international space law, it's currently impractical and will remain that way intil those laws are changed.
 
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  • #62
Overly Speculative Posts:
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  • #63
Those rules apply to crackpot theories of the laws of physics, not strangely novel applications of correct laws of physics.

I find it hard to believe the level of hatred this thread is generating.
 
  • #64
It is not hatred, it is frustration. The thread started on a bad footing and just got worse.

Thread reported.
 
  • #65
maze said:
Those rules apply to crackpot theories of the laws of physics, not strangely novel applications of correct laws of physics.

I find it hard to believe the level of hatred this thread is generating.

It's not hatred as I share the same dreams as you do and have had the exact same thoughts as you're having. It's just that you have to know where to draw the line with practicality.
 
  • #66
The proposals for terraforming, particularly with thermonuclear bombs, were presumptive and didn't address some fundamental issues with respect to feasibility, particularly with respect to atmospheric retention. One must consider what is available to terraform Mars and the goal of such a program.


Mars information from http://en.wikipedia.org/wiki/Mars
The solar day (or sol) on Mars is only slightly longer than an Earth day: 24 hours, 39 minutes, and 35.244 seconds.

Martian year is equal to 1.8809 Earth years, or 1 year, 320 days, and 18.2 hours. Mars's axial tilt is 25.19°, which is similar to the axial tilt of the Earth. So a Martian winter would be nearly twice as long as one on earth, and perhaps much colder.

Surface temp.
min . mean . max
186 K 227 K 268 K
-87°C -46°C -5°C

So for humans to live in an environment similar to that of Earth, the max temperature of Mars would have to be increased by about 30-35°C, and ideally the minimum would increase by about 50°C, otherwise significant thermal differentials would drive extreme weather (i.e. high wind velocities). Given that Mars is 1.52 AU from the sun, it receives less than half the solar energy flux as the Earth (~43%).


But one has to ask, why Mars doesn't have an atmosphere. Well, it simply doesn't have enough gravity to retain the light gases like N2, O2, and water vapor H2O. So, even if the CO2 on Mars was released and converted to O2, and the water was released as vapor, the O2 and H2O would simply escape to space, especially if the temperature were to be increased to levels experienced by Earth's atmosphere.

http://zebu.uoregon.edu/~soper/Mars/atmosphere.html

So the gravity would have to be increased on Mars by adding mass,
but then from where would the extra mass come. Phobos? Deimos? Asteroids?

Consider the following:

Mars - mass = 6.4185×1023 kg / 0.107 Earths
Equatorial surface gravity 3.69 m/s² (0.376 g)

Phobos - mass = 1.07×1016 kg (1.8 nEarths)
Deimos - mass = 1.48×1015 kg

The masses of Phobos and Deimos are inconsequential, being less than one ten-millionth of the mass of Mars.


Well - what about the asteroids?


More than half the mass within the main belt is contained in the four largest objects: Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea. All of these have mean diameters of more than 400 km, while Ceres has a diameter of about 950 km.

From - http://en.wikipedia.org/wiki/Ceres_(dwarf_planet)#Physical_characteristics
The combined mass of the current asteroid belt is only a small fraction of the mass of the Earth's Moon - mass 7.3477×1022 kg (0.0123 Earths)

The mass of Ceres has been determined by analysis of the influence it exerts on small asteroids. The mass of Ceres comprises about a third of the estimated total 3.0 ± 0.2 ×1021 kg mass of the asteroids in the solar system, together totalling about 4% of the mass of the Moon.

Ceres - mass 9.43 ± 0.07×1020 kg, orbit semi-major axis 414,703,838 km
Kovacevic, A.; Kuzmanoski, M. (2007), "A New Determination of the Mass of (1) Ceres". Earth, Moon, and Planets 100: 117–123.
http://adsabs.harvard.edu/abs/2007EM&P..100..117K

Pitjeva, E.V. (2005), "High-Precision Ephemerides of Planets — EPM and Determination of Some Astronomical Constants," Solar System Research 39 (3): 176.
http://iau-comm4.jpl.nasa.gov/EPM2004.pdf

4 Vesta - mass 2.7×1020 kg, orbit semi-major axis 353,268,000 km

2 Pallas - mass 2.2×1020 kg, orbit semi-major axis 414,784,000 km

10 Hygeia - mass 8.6 ± 0.7 ×1019 kg, orbit semi-major axis 469,345,000 km

http://en.wikipedia.org/wiki/Image:Moon_and_Asteroids_1_to_10.svg


Collecting all the asteroid mass in solar system, would yield about 4% (0.04) of the lunar mass, which is 11.4% (0.114) mass of Mars. So adding all the asteroid mass to Mars would increase its mass 0.04 * 0.114 = 0.00456, and that would still be insufficient to retain an atmosphere with density and temperature similar to earth. Even adding the moon with the asteroids would only increase the mass of Mars by approximately 12%, and it would still be insufficient.


What about the moons of Jupiter and Saturn? Well, they are a long way off, and one would have to lift the moons out of the gravity wells of Jupiter and Saturn.


Jupiter - orbit semi-major axis 778,547,200 km

Saturn - orbit semi-major axis 1,433,449,370 km
 
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