Add to ORKGThis report examines the feasibility of transporting coal from the Earth to Mars to increase the Martian atmospheric density. This is done by releasing CO2 through combustion, which would terraform the planet. It was found that this was unfeasible due to the large values required: 3.15 x 1019 Kg of coal and 1.97x1027 J of energy to transport it outside of the Earth’s gravitational potential
There is a good possibility that long-term production of deep biosphere methane (CH4) has occurred o...
Volatile transport of carbon dioxide is most relevant on two planetary bodies in our solar system: M...
With a Monte Carlo model we investigate the escape of hot oxygen and carbon from the Martian atmosph...
In this work consideration is given for a technological method of attaining high pressurized vessels...
The compression of CO2 from the Martian atmosphere for production of O2 via an electrochemical cell ...
Mars is a potentially habitable planet given the appropriate planetary engineering efforts. In order...
International audienceIt has been recently shown that several valley networks, like Naktong Vallis [...
The manned mission is seen as a first step towards a Mars surface exploration base-station and, late...
Results are presented of one-dimensional radiation convection modeling of the early Mars atmosphere....
Terraforming Mars is a tantalizing topic for the future of humanity. It has been estimated that an i...
We have completed preliminary calculations of the minimum sizes of bolides that would penetrate vari...
It is pointed out that in addition to the 1 to 5 bar CO2 total inventory, a high level of global vol...
Global energy balance models of the Martian atmosphere predict that, for a range of total CO_2 inven...
We have measured the abundance and stable isotopic composition of magmatic carbon extracted from a s...
NASA now looks to Mars as the next step in human space exploration. A couple of challenges of such a...
There is a good possibility that long-term production of deep biosphere methane (CH4) has occurred o...
Volatile transport of carbon dioxide is most relevant on two planetary bodies in our solar system: M...
With a Monte Carlo model we investigate the escape of hot oxygen and carbon from the Martian atmosph...
In this work consideration is given for a technological method of attaining high pressurized vessels...
The compression of CO2 from the Martian atmosphere for production of O2 via an electrochemical cell ...
Mars is a potentially habitable planet given the appropriate planetary engineering efforts. In order...
International audienceIt has been recently shown that several valley networks, like Naktong Vallis [...
The manned mission is seen as a first step towards a Mars surface exploration base-station and, late...
Results are presented of one-dimensional radiation convection modeling of the early Mars atmosphere....
Terraforming Mars is a tantalizing topic for the future of humanity. It has been estimated that an i...
We have completed preliminary calculations of the minimum sizes of bolides that would penetrate vari...
It is pointed out that in addition to the 1 to 5 bar CO2 total inventory, a high level of global vol...
Global energy balance models of the Martian atmosphere predict that, for a range of total CO_2 inven...
We have measured the abundance and stable isotopic composition of magmatic carbon extracted from a s...
NASA now looks to Mars as the next step in human space exploration. A couple of challenges of such a...
There is a good possibility that long-term production of deep biosphere methane (CH4) has occurred o...
Volatile transport of carbon dioxide is most relevant on two planetary bodies in our solar system: M...
With a Monte Carlo model we investigate the escape of hot oxygen and carbon from the Martian atmosph...