Category Archives: Transhuman News

We are an international symposium, spanning students and professionals, scientists and laymen alike, all with a desire to colonize and terraform Mars. Our visitors have the opportunity to submit ideas in these evolving fields, knowing they are literally writing the books on Mars. Their articles are discussed by the scientific community until the most comprehensive, efficient and realistic Plan is developed and enacted. Read the

Mr. Gellert also stated that data has been collected during the day and the night, and both have good data. The importance of this statement, beyond having a working spectrometer, is that the APXS sensor is sensitive enough to pick up thermal noise in the sensor between the day and night. The MER detectors

Ken Edgett, the MAHLI Primary Investigator, was next to speak and showed

During the Q&A session, Joy Crisp, MSL Deputy Project Scientist, fielded a question about the

The

- posted by Jim@ 23:51 EST

The conference was kicked off with Jennifer Trosper, MSL Mission Mananger, re-assuring us that we are in the final Sol of characterization. Today, Sol 37 puts the team one day behind schedule, but, according to Trosper, in her experience on Pathfinder, which she noted lost 1 in 3 sols to unexpected events, and MER, which lost 1 in 10, that the MSL team is doing well. Thus far, Curiosity has shown that her arm can reach all of the calibration targets and "teach points," which are points that would be needed to be reached to fulfill the science mission, such as moving over the

Ms. Trosper also noted that over the next couple of days the MastCam will be pointed to the sun to watch the transits of Phobos and Deimos, and event that only happens twice a Martian Year. MastCam will take video of the transit, but will only transmit back a few frames to Earth. The rest will be stored until a later date because of constraints on bandwidth and the importance of engineering data at the moment.

Additionally, it was added that the RTGs are producing 115W of energy and the rover is kept between 7C and 37C, right where they should be. Also, the rover has driven 109m according to the odometer, but only 82m the way the crow flies. Glenelg is approximately 400m away and Curiosity can move 30m/sol to 40m/sol depending on the terrain and science-team needs.

Over the next two months, the team will attempt to move back to Earth-time. Currently the team is using Mars-time in order to maximize the time they have before needing to send commands to the rover from the time they get the downlink. Currently it takes approximately 8 hours to figure out what the team wants to do and another 8 hours to turn that into a sequence of commands. By Sol 90, it is hoped that the team will be fast enough to allow them to function on Earth-time.

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Red Colony - Colonizing and Terraforming Mars

"Red Mars" redirects here. For the planet, see Mars.

The Mars trilogy is a series of award-winning science fiction novels by Kim Stanley Robinson that chronicles the settlement and terraforming of the planet Mars through the intensely personal and detailed viewpoints of a wide variety of characters spanning almost two centuries. Ultimately more utopian than dystopian, the story focuses on egalitarian, sociological, and scientific advances made on Mars, while Earth suffers from overpopulation and ecological disaster.

The three novels are Red Mars (1993), Green Mars (1994), and Blue Mars (1996). The Martians (1999) is a collection of short stories set in the same fictional universe. The main trilogy won a number of prestigious awards. Icehenge (1984), Robinson's first novel about Mars, is not set in this universe but deals with similar themes and plot elements. The trilogy shares some similarites with Robinson's more recent novel 2312 (2012), for instance, the terraforming of Mars and the extreme longevity of the characters in both novels.

Red Mars starts in 2026 with the first colonial voyage to Mars aboard the Ares, the largest interplanetary spacecraft ever built (interestingly, from clustered space shuttle external fuel tanks which, instead of incinerating in the atmosphere, have been boosted into orbit until enough had been amassed to build a ship and also used as landing craft) and home to a crew who are to be the first hundred Martian colonists. The mission is a joint Russian-American undertaking, and seventy of the First Hundred are drawn from these countries (except, for example, Michel Duval, a French psychologist assigned to observe their behavior). The book details the trip out, construction of the first settlement on Mars (eventually called Underhill) by Nadia Chernyshevski, as well as establishing colonies on Mars' hollowed out asteroid-moon Phobos, the ever-changing relationships between the colonists, debates among the colonists regarding both the terraforming of the planet and its future relationship to Earth. The two extreme views on terraforming are personified by Saxifrage "Sax" Russell, who believes their very presence on the planet means some level of terraforming has already begun and that it is humanity's obligation to spread life as it is the most scarce thing in the known universe, and Ann Clayborne, who stakes out the position that humankind does not have the right to change entire planets at their will.

Russell's view is initially purely scientific but in time comes to blend with the views of Hiroko Ai, the chief of the Agricultural Team who assembles a new belief system (the "Areophany") devoted to the appreciation and furthering of life ("viriditas"); these views are collectively known as the "Green" position, while Clayborne's naturalist stance comes to be known as "Red." The actual decision is left to the United Nations Organization Mars Authority (UNOMA), which greenlights terraforming, and a series of actions get underway, including the drilling of "moholes" to release subsurface heat; thickening of the atmosphere according to a complicated bio-chemical formula that comes to be known as the "Russell cocktail" after Sax Russell; and the detonation of nuclear explosions deep in the sub-surface permafrost to release water. Additional steps are taken to connect Mars more closely with Earth, including the insertion of a geosynchronous asteroid "Clarke" to which a space elevator cable is tethered.

Against the backdrop of this development is another debate, one whose principal instigator is Arkady Bogdanov of the Russian contingent (possibly named in homage to the Russian polymath and science fiction writer Alexander Bogdanov). Bogdanov argues that Mars need not and should not be subject to Earth traditions, limitations, or authority. He is to some extent joined in this position by John Boone, famous as the "First Man on Mars" from a preceding expedition and rival to Frank Chalmers, the technical leader of the American contingent. Their rivalry is further exacerbated by competing romantic interest in Maya Katarina Toitovna, the leader of the Russian contingent. (In the opening of the book, Chalmers instigates a sequence of events that leads to Boone being assassinated; much of what follows is a retrospective examination of what got things to that point.)

Earth meanwhile increasingly falls under the control of transnational corporations (transnats) that come to dominate its governments, particularly smaller nations adopted as "flags of convenience" for extending their influence into Martian affairs. As UNOMA's power erodes, the Mars treaty is renegotiated in a move led by Frank Chalmers; the outcome is impressive but proves short-lived as the transnats find ways around it through loop-holes. Things get worse as the nations of Earth start to clash over limited resources, expanding debt, and population growth as well as restrictions on access to a new longevity treatment developed by Martian scienceone that holds the promise of lifespans into the hundreds of years. In 2061, with Boone dead and exploding immigration threatening the fabric of Martian society, Bogdanov launches a revolution against what many now view as occupying transnat troops operating only loosely under an UNOMA rubber-stamp approval. Initially successful, the revolution proves infeasible on the basis of both a greater-than-expected willingness of the Earth troops to use violence and the extreme vulnerability of life on a planet without a habitable atmosphere. A series of exchanges sees the cutting of the space elevator, bombardment of several Martian cities (including the city where Bogdanov is himself organizing the rebellion; he is killed), the destruction of Phobos and its military complex, and the unleashing of a great flood of torrential groundwater freed by nuclear detonations.

By the end, most of the First Hundred are dead, and virtually all who remain have fled to a hidden refuge established years earlier by Ai and her followers. (One exception is Phyllis Boyle, who has allied herself with the transnats; she is on Clarke when the space elevator cable is cut and sent flying out of orbit to a fate unknown by the conclusion of the book.) The revolution dies and life on Mars returns to a sense of stability under heavy transnat control. The clash over resources on Earth breaks out into a full-blown world war leaving hundreds of millions dead, but cease-fire arrangements are reached when the transnats flee to the safety of the developed nations, which use their huge militaries to restore order, forming police-states. But a new generation of humans born on Mars holds the promise of change. In the meantime, the remaining First Hundredincluding Russell, Clayborne and Chernyshevskisettle into life in Ai's refuge called Zygote, hidden under the Martian south pole.

Green Mars takes its title from the stage of terraforming that has allowed plants to grow. It picks up the story 50 years after the events of Red Mars in the dawn of the 22nd century, following the lives of the remaining First Hundred and their children and grandchildren. Hiroko Ai's base under the south pole is attacked by UN Transitional Authority (UNTA) forces, and the survivors are forced to escape into a (less literal) underground organization known as the Demimonde. Among the expanded group are the First Hundred's children, the Nisei, a number of whom live in Hiroko's second secret base, Zygote.

As unrest in the multinational control over Mars' affairs grow, various groups start to form with different aims and methods. Watching these groups evolve from Earth, the CEO of the Praxis Corporation sends a representative, Arthur Randolph, to organize the resistance movements. This culminates into the Dorsa Brevia agreement, in which nearly all the underground factions take part. Preparations are made for a second revolution beginning in the 2120s, from converting moholes to missiles silos or hidden bases, sabotaging orbital mirrors, to propelling Deimos out of Mars' gravity well and out into deep space so it could never be used as a weapons platform as Phobos was.

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Mars trilogy - Wikipedia, the free encyclopedia

From Ad Astra July/August 1996

Among extraterrestrial bodies in our solar system, Mars is singular in that it possesses all the raw materials required to support not only life, but a new branch of human civilization. This uniqueness is illustrated most clearly if we contrast Mars with the Earth's Moon, the most frequently cited alternative location for extraterrestrial human colonization.

In contrast to the Moon, Mars is rich in carbon, nitrogen, hydrogen and oxygen, all in biologically readily accessible forms such as carbon dioxide gas, nitrogen gas, and water ice and permafrost. Carbon, nitrogen, and hydrogen are only present on the Moon in parts per million quantities, much like gold in seawater. Oxygen is abundant on the Moon, but only in tightly bound oxides such as silicon dioxide (SiO2), ferrous oxide (Fe2O3), magnesium oxide (MgO), and aluminum oxide (Al2O3), which require very high energy processes to reduce. Current knowledge indicates that if Mars were smooth and all its ice and permafrost melted into liquid water, the entire planet would be covered with an ocean over 100 meters deep. This contrasts strongly with the Moon, which is so dry that if concrete were found there, Lunar colonists would mine it to get the water out. Thus, if plants could be grown in greenhouses on the Moon (an unlikely proposition, as we've seen) most of their biomass material would have to be imported.

The Moon is also deficient in about half the metals of interest to industrial society (copper, for example), as well as many other elements of interest such as sulfur and phosphorus. Mars has every required element in abundance. Moreover, on Mars, as on Earth, hydrologic and volcanic processes have occurred that are likely to have consolidated various elements into local concentrations of high-grade mineral ore. Indeed, the geologic history of Mars has been compared to that of Africa, with very optimistic inferences as to its mineral wealth implied as a corollary. In contrast, the Moon has had virtually no history of water or volcanic action, with the result that it is basically composed of trash rocks with very little differentiation into ores that represent useful concentrations of anything interesting.

You can generate power on either the Moon or Mars with solar panels, and here the advantages of the Moon's clearer skies and closer proximity to the Sun than Mars roughly balances the disadvantage of large energy storage requirements created by the Moon's 28-day light-dark cycle. But if you wish to manufacture solar panels, so as to create a self-expanding power base, Mars holds an enormous advantage, as only Mars possesses the large supplies of carbon and hydrogen needed to produce the pure silicon required for producing photovoltaic panels and other electronics. In addition, Mars has the potential for wind-generated power while the Moon clearly does not. But both solar and wind offer relatively modest power potential tens or at most hundreds of kilowatts here or there. To create a vibrant civilization you need a richer power base, and this Mars has both in the short and medium term in the form of its geothermal power resources, which offer potential for large numbers of locally created electricity generating stations in the 10 MW (10,000 kilowatt) class. In the long-term, Mars will enjoy a power-rich economy based upon exploitation of its large domestic resources of deuterium fuel for fusion reactors. Deuterium is five times more common on Mars than it is on Earth, and tens of thousands of times more common on Mars than on the Moon.

But the biggest problem with the Moon, as with all other airless planetary bodies and proposed artificial free-space colonies, is that sunlight is not available in a form useful for growing crops. A single acre of plants on Earth requires four megawatts of sunlight power, a square kilometer needs 1,000 MW. The entire world put together does not produce enough electrical power to illuminate the farms of the state of Rhode Island, that agricultural giant. Growing crops with electrically generated light is just economically hopeless. But you can't use natural sunlight on the Moon or any other airless body in space unless you put walls on the greenhouse thick enough to shield out solar flares, a requirement that enormously increases the expense of creating cropland. Even if you did that, it wouldn't do you any good on the Moon, because plants won't grow in a light/dark cycle lasting 28 days.

But on Mars there is an atmosphere thick enough to protect crops grown on the surface from solar flare. Therefore, thin-walled inflatable plastic greenhouses protected by unpressurized UV-resistant hard-plastic shield domes can be used to rapidly create cropland on the surface. Even without the problems of solar flares and month-long diurnal cycle, such simple greenhouses would be impractical on the Moon as they would create unbearably high temperatures. On Mars, in contrast, the strong greenhouse effect created by such domes would be precisely what is necessary to produce a temperate climate inside. Such domes up to 50 meters in diameter are light enough to be transported from Earth initially, and later on they can be manufactured on Mars out of indigenous materials. Because all the resources to make plastics exist on Mars, networks of such 50- to 100-meter domes couldbe rapidly manufactured and deployed, opening up large areas of the surface to both shirtsleeve human habitation and agriculture. That's just the beginning, because it will eventually be possible for humans to substantially thicken Mars' atmosphere by forcing the regolith to outgas its contents through a deliberate program of artificially induced global warming. Once that has been accomplished, the habitation domes could be virtually any size, as they would not have to sustain a pressure differential between their interior and exterior. In fact, once that has been done, it will be possible to raise specially bred crops outside the domes.

The point to be made is that unlike colonists on any known extraterrestrial body, Martian colonists will be able to live on the surface, not in tunnels, and move about freely and grow crops in the light of day. Mars is a place where humans can live and multiply to large numbers, supporting themselves with products of every description made out of indigenous materials. Mars is thus a place where an actual civilization, not just a mining or scientific outpost, can be developed. And significantly for interplanetary commerce, Mars and Earth are the only two locations in the solar system where humans will be able to grow crops for export.

Mars is the best target for colonization in the solar system because it has by far the greatest potential for self-sufficiency. Nevertheless, even with optimistic extrapolation of robotic manufacturing techniques, Mars will not have the division of labor required to make it fully self-sufficient until its population numbers in the millions. Thus, for decades and perhaps longer, it will be necessary, and forever desirable, for Mars to be able to import specialized manufactured goods from Earth. These goods can be fairly limited in mass, as only small portions (by weight) of even very high-tech goods are actually complex. Nevertheless, these smaller sophisticated items will have to be paid for, and the high costs of Earth-launch and interplanetary transport will greatly increase their price. What can Mars possibly export back to Earth in return?

It is this question that has caused many to incorrectly deem Mars colonization intractable, or at least inferior in prospect to the Moon. For example, much has been made of the fact that the Moon has indigenous supplies of helium-3, an isotope not found on Earth and which could be of considerable value as a fuel for second generation thermonuclear fusion reactors. Mars has no known helium-3 resources. On the other hand, because of its complex geologic history, Mars may have concentrated mineral ores, with much greater concentrations of precious metal ores readily available than is currently the case on Earth because the terrestrial ores have been heavily scavenged by humans for the past 5,000 years. If concentrated supplies of metals of equal or greater value than silver (such as germanium, hafnium, lanthanum, cerium, rhenium, samarium, gallium, gadolinium, gold, palladium, iridium, rubidium, platinum, rhodium, europium, and a host of others) were available on Mars, they could potentially be transported back to Earth for a substantial profit. Reusable Mars-surface based single-stage-to-orbit vehicles would haul cargoes to Mars orbit for transportation to Earth via either cheap expendable chemical stages manufactured on Mars or reusable cycling solar or magnetic sail-powered interplanetary spacecraft. The existence of such Martian precious metal ores, however, is still hypothetical.

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The Case for Colonizing Mars, by Robert Zubrin