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Monday, June 28, 2021

Space policy

From Wikipedia, the free encyclopedia

Space policy is the political decision-making process for, and application of, public policy of a state (or association of states) regarding spaceflight and uses of outer space, both for civilian (scientific and commercial) and military purposes. International treaties, such as the 1967 Outer Space Treaty, attempt to maximize the peaceful uses of space and restrict the militarization of space.

Space policy intersects with science policy, since national space programs often perform or fund research in space science, and also with defense policy, for applications such as spy satellites and anti-satellite weapons. It also encompasses government regulation of third-party activities such as commercial communications satellites and private spaceflight.

Space policy also encompasses the creation and application of space law, and space advocacy organizations exist to support the cause of space exploration.

Space law

Space law is an area of the law that encompasses national and international law governing activities in outer space. There are currently five treaties that make up the body of international space law.

The inception of the field of space law began with the launch of the world's first artificial satellite by the Soviet Union in October 1957. Named Sputnik 1, the satellite was launched as part of the International Geophysical Year. Since that time, space law has evolved and assumed more importance as mankind has increasingly come to use and rely on space-based resources.

Policy by country

Soviet Union

The Soviet Union became the world's first spacefaring state by launching its first satellite, Sputnik 1, on 4 October 1957.

United States

United States space policy is drafted by the Executive branch at the direction of the President of the United States, and submitted for approval and establishment of funding to the legislative process of the United States Congress. The President may also negotiate with other nations and sign space treaties on behalf of the US, according to his or her constitutional authority. Congress' final space policy product is, in the case of domestic policy a bill explicitly stating the policy objectives and the budget appropriation for their implementation to be submitted to the President for signature into law, or else a ratified treaty with other nations.

Space advocacy organizations (such as the Space Science Institute, National Space Society, and the Space Generation Advisory Council, learned societies such as the American Astronomical Society and the American Astronautical Society; and policy organizations such as the National Academies) may provide advice to the government and lobby for space goals.

Civilian and scientific space policy is carried out by the National Aeronautics and Space Administration (NASA, subsequent to 29 July 1958), and military space activities (communications, reconnaissance, intelligence, mapping, and missile defense) are carried out by various agencies of the Department of Defense. The President is legally responsible for deciding which space activities fall under the civilian and military areas. In addition, the Department of Commerce's National Oceanic and Atmospheric Administration operates various services with space components, such as the Landsat program.

The President consults with NASA and Department of Defense on their space activity plans, as potential input for the policy draft submitted to Congress. He or she also consults with the National Security Council, the Office of Science and Technology Policy, and the Office of Management and Budget to take into account Congress's expected willingness to provide necessary funding levels for proposed programs.

Once the President's policy draft or treaty is submitted to the Congress, civilian policies are reviewed by the House Subcommittee on Space and Aeronautics and the Senate Subcommittee on Science and Space. These committees also exercise oversight over NASA's operations and investigation of accidents such as the 1967 Apollo 1 fire. Military policies are reviewed and overseen by the House Subcommittee on Strategic Forces and the Senate Subcommittee on Strategic Forces, as well as the House Permanent Select Committee on Intelligence and the Senate Select Committee on Intelligence. The Senate Foreign Relations Committee conducts hearings on proposed space treaties, and the various appropriations committees have power over the budgets for space-related agencies. Space policy efforts are supported by Congressional agencies such as the Congressional Research Service, the Congressional Budget Office, and Government Accountability Office.

History

President Kennedy committed the United States to landing a man on the Moon by the end of the 1960s decade, in response to contemporary Soviet space successes. This speech at Rice University on 12 September 1962 is famous for the quote "We choose to go to the Moon in this decade and do the other things, not because they are easy, but because they are hard."

The early history of United States space policy is linked to the US–Soviet Space Race of the 1960s. The National Aeronautics and Space Act creating NASA was passed in 1958, after the launch of the Soviet Sputnik 1 satellite. Thereafter, in response to the flight of Yuri Gagarin as the first man in space, Kennedy in 1961 committed the United States to landing a man on the Moon by the end of the decade. Although the costs of the Vietnam War and the programs of the Great Society forced cuts to NASA's budget as early as 1965, the first Moon landing occurred in 1969, early in Richard Nixon's presidency. Under the Nixon administration NASA's budget continued to decline and three of the planned Apollo Moon landings were cancelled. The Nixon administration approved the beginning of the Space Shuttle program in 1972, but did not support funding of other projects such as a Mars landing, colonization of the Moon, or a permanent space station.

The Space Shuttle first launched in 1981, during Ronald Reagan's administration. Reagan in 1982 announced a renewed active space effort, which included initiatives such the construction of Space Station Freedom, and the military Strategic Defense Initiative, and, later in his term, a 30 percent increase in NASA's budget. The Space Shuttle Challenger disaster in January 1986 led to a reevaluation of the future of the national space program in the National Commission on Space report and the Ride Report.

The United States has participated in the International Space Station beginning in the 1990s, the Space Shuttle program has continued, although the Space Shuttle Columbia disaster has led to the planned retirement of the Space Shuttle in mid-2011. There is a current debate on the post-Space Shuttle future of the civilian space program: the Constellation program of the George W. Bush administration directed NASA to create a set of new spacecraft with the goal of sending astronauts to the Moon and Mars, but the Obama administration cancelled the Constellation program, opting instead to emphasize development of commercial rocket systems.

The Vision for Space Exploration established under the George W. Bush administration in 2004 was replaced with a new policy released by Barack Obama on 28 June 2010.

In recent years, U.S. space operators and decisionmakers have become increasingly concerned about threats to U.S. space leadership. In the civil sector, this has been driven largely by U.S. dependence on Russia for crew access to the International Space Station (ISS) since the termination of the space shuttle program in 2011. In national security, foreign development of counterspace systems has become a regular feature of public statements by U.S. defense and intelligence officials. This is reminiscent of similar concerns about the Soviet Union’s space program between the launch of Sputnik 1 in 1957 and the success of the Apollo lunar missions. The threat of Soviet dominance in space turned out to be less formidable than expected, but it continued to drive policy and programmatic decisions for decades, until the Soviet Union ceased to exist.

Europe

The ESA is an international organization whose membership overlaps with, but is not the same as, that of the EU.
  ESA and EU member countries
  ESA-only members
  EU-only members

The European Space Agency (ESA) is the common space agency for many European nations. It is independent of the European Union, though the 2007 European Space Policy provides a framework for coordination between the two organizations and member states, including issues such as security and defence, access to space, space science, and space exploration.

The ESA was founded to serve as a counterweight to the dominant United States and Soviet space programs, and further the economic and military independence of Europe. This has included the development of the Ariane rockets, which by 1985 had captured over 40 percent of commercial launch market in the free world. The ESA budget is split between mandatory and voluntary programs, the latter of which allow individual member nations to pursue their own national space goals within the organization.

The ESA Director General's Proposal for the European Space Policy states, "Space systems are strategic assets demonstrating independence and the readiness to assume global responsibilities. Initially developed as defence or scientific projects, they now also provide commercial infrastructures on which important sectors of the economy depend and which are relevant in the daily life of citizens.... Europe needs an effective space policy to enable it to exert global leadership in selected policy areas in accordance with European interests and values."

In the final part of 2010s the ESA has made strong efforts in order to make Europe stronger in the competition for the development of new strategies regarding space policy. Those included a huge increase in ESA's budget promoted by countries such as Italy, France and Germany.

China

Although Chairman Mao Zedong planned after Russia's Sputnik 1 launch to place a Chinese satellite in orbit by 1959 to celebrate the 10th anniversary of the founding of the People's Republic of China (PRC), China did not successfully launch its first satellite until 24 April 1970. Mao and Zhou Enlai decided on 14 July 1967 that the PRC should not be left behind, and started China's own human spaceflight program. The first success came on 15 October 2003 when China sent its first astronaut into space for 21 hours aboard Shenzhou 5.

The Ministry of Aerospace Industry was responsible for the Chinese space program prior to July 1999, when it was split into the China National Space Administration responsible for setting policy, and the state-owned China Aerospace Science and Technology Corporation, responsible for implementation.

The China National Space Administration states its aims as maintaining the country's overall development strategy, making innovations in an independent and self-reliant manner, promoting the country's science and technology sector and encouraging economic and social development, and actively engaging in international cooperation.

Russian Federation and Ukraine

The Russian Federation inherited their space programs in 1991 from its predecessor state, the Soviet Union. Russia's civilian space agency is the Russian Federal Space Agency, and its military counterpart is the Russian Aerospace Defence Forces. Ukraine's agency is the State Space Agency of Ukraine, which handles both civilian and military programs.

In the 1980s the Soviet Union was considered to be technologically behind the United States, but it outspent the United States in its space budget, and its cosmonauts had spent three times as many days in space as American astronauts. The Soviet Union had also been more willing than the United States to embark on long-term programs, such as the Salyut and Mir space station programs, and increased their investment in space programs throughout the 1970s and 1980s.

After the dissolution of the Soviet Union, the 1990s saw serious financial problems because of the decreased cash flow, which encouraged Roskosmos to improvise and seek other ways to keep space programs running. This resulted in Roskosmos' leading role in commercial satellite launches and space tourism. While scientific missions, such as interplanetary probes or astronomy missions during these years played a very small role, although roskosmos has connections with Russian aerospace forces, its budget is not part of the defense budget of the country, Roskosmos managed to operate the space station Mir well past its planned lifespan, contribute to the International Space Station, and continue to fly additional Soyuz and Progress missions.

The Russian economy boomed throughout 2005 from high prices for exports, such as oil and gas, the outlook for subsequent funding became more favorable. The federal space budget for the year 2009 was left unchanged despite the global economic crisis, standing at about 82 billion rubles ($2.4 billion). Current priorities of the Russian space program include the new Angara rocket family and development of new communications, navigation and remote Earth sensing spacecraft. The GLONASS global navigation satellite system has for many years been one of the top priorities and has been given its own budget line in the federal space budget.

India

The purpose of India's space program was outlined by Vikram Sarabhai (regarded as the father of the Indian space program):

There are some who question the relevance of space activities in a developing nation. To us, there is no ambiguity of purpose....we are convinced that if we are to play a meaningful role nationally, and in the community of nations, we must be second to none in the application of advanced technologies to the real problems of man and society.

The Department of Space (DoS) is the Indian government department responsible for administration of the Indian space program. It manages several agencies and institutes related to space exploration and space technologies. The Indian space program under the DoS aims to promote the development and application of space science and technology for the socio-economic benefit of the country. It includes two major satellite systems, INSAT for communication, television broadcasting and meteorological services, and Indian Remote Sensing Satellites (IRS) system for resources monitoring and management. It has also developed two satellite launch vehicles, Polar Satellite Launch Vehicle (PSLV) and Geosynchronous Satellite Launch Vehicle (GSLV), to place IRS and INSAT class satellites in orbit.

Mars Society

From Wikipedia, the free encyclopedia
 
Mars Society
Mars Society logo.png
FoundedAugust 13, 1998
FounderDr. Robert Zubrin
TypeNonprofit corporation with §501(c)(3) federal income tax exemption.
Legal statusThe Mars Society is a "public charity" and is eligible to receive tax-deductible charitable contributions.
FocusSpace advocacy and Human mission to Mars
Location
Area served
U.S.A.-based internationally active
Key people
Board of Directors:

Officers & Staff:

  • Lucinda Offer, Executive Director
  • Michael Stoltz, Dir. Media & Public Relations
  • Shannon Rupert, Dir. Program Manager, MDRS
  • Kevin Sloan, Dir., University Rover Challenge (URC)
  • James Burk, Dir., IT / Chair, Marspedia / MarsVR
  • Carie Fay, Dir., Administration
  • Frank Crossman, Chief Archivist
  • Nora Hovee, Chapters Coordinator
  • Tam R Czarnik MD, Medical Director (retired)
Websitewww.marssociety.org

The Mars Society is an American worldwide volunteer-driven space-advocacy non-profit organization dedicated to promoting the human exploration and settlement of the planet Mars. Inspired by "The Case for Mars" conferences which were hosted by The Mars Underground at the University of Colorado Boulder, the Mars Society was established by Dr. Robert Zubrin and others in 1998 with the goal of educating the public, the media and government on the benefits of exploring Mars, the importance of planning for a humans-to-Mars mission in the coming decades and the need to create a permanent human presence on the Red Planet.

History

Mars Society, Inc. was formally established in September 1997 under the Colorado Non-Profit Corporation Act. In August 1998 more than 700 delegates – astronomers, scientists, engineers, astronauts, entrepreneurs, educators, students and space enthusiasts – attended a week-end of talks and presentations from leading Mars exploration advocates. Since then, the Mars Society, guided by its steering committee, has grown to over 5,000 members and some 6,000 associate supporters across more than 50 countries around the world. Members of the Mars Society are from all walks of life and actively work to promote the ideals of space exploration and the opportunities for exploring the Red Planet. In 2017 the Marspedia encyclopedia became an official project of the Mars Society.

Mars Society's purpose, mission and goals

The Mars Society's goals aren't purely theoretical. Its aim is to show that Mars is an achievable goal through a practical series of technical and other projects, including:

  • Further development of the Mars Direct mission plan to send humans to Mars
  • The Mars Analog Research Station Program (MARS) – analogues of possible future Mars habitation units, located in Mars-like environments. Established stations include the Flashline Mars Arctic Research Station (FMARS) and the Mars Desert Research Station (MDRS)
  • The University Rover Challenge – a competition to design a pressurized rover vehicle that could be used on Mars that was won by the Michigan Mars Rover Team.
  • MarsVR: Mars Virtual Reality – a multi-phase effort to build virtual reality tools to support the human exploration of Mars, and train the crewmembers at the Mars Desert Research Station.
  • The Mars Gravity Biosatellite - a program to design, build, and launch a satellite rotated to artificially provide partial gravity of 0.38g, equivalent to that of Mars, and hosting a small population of mice, to study the health effects of partial gravity, as opposed to zero gravity; this originated as a Mars Society initiative and is now supported by the YourNameIntoSpace web portal
  • The Mars balloon mission ARCHIMEDES, due to launch in 2018 (conducted by the German Chapter of Mars Society)
  • Tempo3 The Tethered Experiment for Mars inter-Planetary Operations, a CubeSat based satellite that will demonstrate artificial gravity generation using two tethered masses

In addition, the Society:

  • gives talks and presentations on Mars Direct to schools, colleges, universities, professional bodies and the general public
  • promotes the teaching of science, astronomy and spaceflight-related subjects in schools
  • campaigns for greater investment on the part of individual countries in space research and development
  • hosts the largest annual conferences on Mars exploration in the United States, Europe and Australia
  • actively supports NASA, ESA and other space agencies in their on-going exploration of Mars

The current board of directors of the Mars Society includes Robert Zubrin (chairman) and James Heiser.

Notable members of its steering committee include Buzz Aldrin and Peter H. Smith.

Notable former members of the board of directors or steering committee of the Mars Society include Kim Stanley Robinson, Michael D. Griffin, Christopher McKay, Pascal Lee and Elon Musk.

The Society is an organization member of the Alliance for Space Development.

North American Chapters of the Mars Society

The Mars Society has chapters in the U.S. and around the world. Many of these chapters undertake scientific, engineering and political initiatives to further the Mars Society's goals. Some accomplishments of Mars Society chapters are listed below:

Canada

Mars Society of Canada:

  • hosted the Third International Mars Society Convention in 2000 (Toronto)
  • organized a month-long multi-national research expedition (known as Expedition One) to the Mars Desert Research Station in the Utah desert in 2003
  • organized a second multi-national research expedition (known as Expedition Two) in the Australian outback in 2004
  • organized a series of training expeditions (beginning with Expedition Alpha, Beta etc.)

United States

California

Northern California Chapter of the Mars Society:

  • hosted the Fourth International Mars Society Convention in 2001 (Stanford University)
  • raised over $100,000 for the Mars Society hosting a fundraiser banquet with James Cameron, May 5, 2001
  • provides Mission Support services and analog spacesuit designs and refurbishment for crews at the Mars Desert Research Station starting in 2002

The San Diego Chapter of the Mars Society

  • provides Crewmembers and Mission Support services for the Mars Desert Research Station (MDRS) and the Flashline Mars Arctic Research Station (FMARS) since 2002
  • TMS-SD provides public outreach events to classrooms, libraries, museums and other organizations throughout the Southern California region with seven different multimedia programs: "Invasion from Earth - The Robotic Exploration of Mars"; "Mars Exploration Rovers - Year 4"; "Mars on Earth - The Adventures of Space Pioneers in the Utah Desert"; "Mars on Earth - The Adventures of Space Pioneers in the Canadian Arctic: "Humans to Mars - How We'll Get There"; "A Close Look at Mars"; and "Mars in the Movies"
  • TMS-SD offers a 1/4-scale radio controlled Mars Exploration Rover with wireless video that children (of all ages) can operate
  • holds monthly chapter meetings, as well as special program events throughout the year
  • hosts a monthly Mars Movie Night in conjunction with The Mars Movie Guide

Texas

Dallas Chapter of the Mars Society:

  • hosted the Mars Track of the National Space Society's International Space Development Conference in 2007
  • Planning Publicizing, and Politicking a vision of Mars colonization in the Dallas area and beyond.

Washington

Mars Society Seattle:

  • Hosting Space Expo 2018 with Seattle's Museum of Flight.
  • Hosted MarsFest with Seattle's Museum of Flight in 1999 (Polar Lander), 2007 (Phoenix), and 2012 (Curiosity).
  • Staffed outreach table at local events: NSTA conference, Yuri's Night, Norwescon, Rustycon, AIAA, and others.
  • Speaker series (co-sponsored with NSS Seattle) every first Sunday of the month at 7pm in the Red Barn classroom at the Museum of Flight.
  • Website development for the Mars Society in the early days, helped set up chapters.marssociety.org and initial task force websites.

European Chapters of the Mars Society

Austria

The ASF (Österreichisches Weltraum Forum, OeWF) is a national network for aerospace and space enthusiasts, being the Austrian chapter of the Mars Society. The Forum serves as a communication platform between the space sector and the public; it is embedded in a global network of specialists from the space industry, research and policy. Hence, the OeWF facilitates a strengthening of the national space sector through enhancing the public visibility of space activities, technical workshops, and conferences as well as Forum-related projects.

Their research focus is Mars Analogue Research, e.g. the AustroMars mission with roughly 130 volunteers supporting a mission simulation at the Mars Desert Research Station (MDRS) and the ongoing PolAres, a multi-year research program which encompass the development of a Mars analogue rover system and a novel spacesuit prototype dubbed "Aouda.X", culminating in an arctic expedition in 2011.

The Forum has a small, but a highly active pool of professional members contributing to space endeavors, mostly in cooperation with other nations as well as international space organizations. The spectrum of their activities ranges from simple classroom presentation to 15.000-visitors space exhibitions, from expert reports for the Austrian Federal Ministry for Technology to space technology transfer activities for terrestrial applications.

France

The Mars Society French chapter (Association Planète Mars) was established in 1999 as "Association Planète Mars", a non-profit organization with its headquarters in Paris. Its founder and president is Richard Heidmann, a space propulsion engineer, who participated in the founding convention of the Mars Society in August 1998 and is a member of the Mars Society Steering Committee.

While fully supporting the ideas and actions of the Mars Society, it considers that those must be adapted to the specific cultural and political context of France and Europe. The main activities of Association Planète Mars are devoted to public communication, through conferences, exhibits, events, media appearances (TV, radio, magazines...). It also acts occasionally as an adviser for journalists or film makers.

Whenever possible, it cooperates with other associations or science outreach organisms, which permits to reinforce its action and reach a wider public.

Association Planète Mars seeks to interest younger people: 25% of its paid members are under the age of 25. It aims to encourage Mars-related projects to be undertaken by engineering students. The association also encourages the formation of working groups on miscellaneous topics. Today, three groups are active, respectively on mission safety, Martian architecture and medical aspects. It has participated in several MDRS and FMARS missions, including a prototype of a "Cliff Exploration Vehicle".

Another major field of action is lobbying, aiming at both political and institutional groups, in France and at the European level (European Council, ESA). In doing so, it relies on the networks established by some of its managers. On the occasion of most critical events, the association publishes political documents to support its views, which are distributed both to opinion formers and to the press. This has been the case in June 2004, in the wake of the US Space Exploration Initiative, and in September 2008 in preparation of the ESA ministerial council.

Germany

The German Chapter of the Mars Society (Mars Society Deutschland e.V. | eingetragener Verein | - MSD) was founded in 2001 based on the Founding Declaration of the Mars Society of the US from 1998 and has about 230 members. The MSD is registered in Germany as a non-profit association (gemeinnütziger Verein). Registered members pay a yearly membership fee of 60 Euro. However, students and firms pay a different fee. The activities of the MSD are focused on technical-scientific projects such as the Mars Balloon Probe ARCHIMEDES as well as on all Mars exploration and general manned space matters. The main means of communication with members and the general public is the MSD Website with information on the ARCHIMEDES project, publications on Mars and other space subjects, the regular news, which can be commented by visitors of the website, the Space Forum and informative meetings.

The MSD Board comprises five members. Since June 2009 its president is the Space Physicist Dr. Michael Danielides. The development of ARCHIMEDES is led by Dipl. Ing. Hannes Griebel, who is also a member of the MSD Board and prepares his doctorate thesis on ARCHIMEDES.

ARCHIMEDES is presently under development and the major project of the MSD since 2001. Starting in 2006, flight tests have been undertaken for testing the innovative balloon system in the low-gravity environment. Test carriers were so far the Airbus A300 for short duration parabolic flights and the sounding rocket test campaigns REXUS3-REGINA and REXUS4-MIRIAM for longer duration flight tests under free space conditions. Further flights tests are planned for the coming years (e.g. MIRIAM II) with the objective of qualifying ARCHIMEDES for its Mars mission by 2018. ARCHIMEDES will be carried to Mars on board an AMSAT Mars Probe or a similar satellite. ARCHIMEDES is developed by the MSD with the support of the Bundeswehr University Munich, of the IABG in Ottobrunn, the DLR-MORABA for rocket flight opportunities, other universities, and several industrial companies supporting specific technical areas.

Netherlands

The Mars Society Netherlands chapter was wound up in 2011. The board and members moved over to a new Mars-oriented organization. The Dutch Mars Society is being relaunched in 2019.

Poland

The Polish Mars society (Mars Society Polska (MSP)) is actively participating in the creation of the Polish space industry. Since this sector is still developing, the organization is taking the opportunity to provide a strong Mars-related element for the years to come. Poland was the last member state of the EU to sign the cooperation agreement with ESA. Most projects in Poland currently focus on satellite technology, so MSP is the only leading organization promoting exploration and manned spaceflight. Besides private sponsors, it relies on resources obtained from the Ministry of Science and Higher Education and local authorities, proposing projects to be undertaken with local communities and thus engaging with the general public.

MSP's first project was the Polish MPV (pressurized rover) design, for which some hardware was produced. This enabled development of the Polish Mars Society itself, together with a number of educational activities for Polish schools. This was followed by the joint organization of the Polish edition of the Red Rover Goes to Mars contest and organization of a Mars colonization negotiation game (Columbia Memorial Negotiations). In 2007 MSP organized the first Mars Festival, a two-day event which drew 600 visitors, with Discovery Channel as the main sponsor. Mars Festival 2008 was smaller due to the efforts being made in other projects, particularly the Polish URC rover, named Skarabeusz.

The flagship MSP project is the Polish Martian habitat, based on a design by Janek Kozicki. It has three inflatable modules attached and a usable surface of 900 m². The habitat is to be located close to a large town, meaning that beyond its role as a test site, largely for materials and design, it will be accessible to the wider public and media.

MSP has established a constant presence in the mainstream Polish media and is working on a documentary about itself. It is also developing software projects, IT systems for the future martian habitat, with a Virtual Mars Base and remote access. Jan Kotlarz of MSP has created RODM software for the modeling of the Martian surface based on high-resolution photographs from Mars Reconnaissance Orbiter. RODM is currently being tested by NASA and ESA.

Switzerland

The Mars Society Switzerland ("MSS") was founded in February 2010. It covers the French and German speaking parts of Switzerland. It keeps close links with the French branch ("association planète Mars", see above). Its aim is to convince the Swiss public of the interest and feasibility of the Martian exploration with inhabited flights through the Mars direct concept such as described by Robert Zubrin. It wants to gather around the scientists working on Mars in Switzerland, all people who share their interest on the matter.

In November 2010, MSS participated to the 8th Swiss Geoscience Meeting which was the opportunity to discuss the main topics related to Mars geology, the making of the planet, the role of water and the atmosphere.

In 2011 (September 30 until October 2), MSS held the 11th European Mars Convention ("EMC11") in the frame of the University of Neuchâtel. Through 24 presentations and two debates with major Swiss media, this convention covered all subjects related to Mars exploration; from astronautics to architecture, including the study of geology which remains its key objective.

On September 10, 2012, in the Natural History Museum Bern ("NHMB"), it held a conference on the theme "Searching for Life on Mars". The conference was centered upon a presentation by Professor André Maeder (a well-known astrophysicist at the University of Geneva) following the publishing of his book "L'unique Terre habitée?" (Favre editions). Another presentation was made by Dr. Beda Hofmann, Head of the Earth Science Dept. of the NHMB. He showed and commented photos of primitive forms of life which he gathered to serve as references for the observations to be made by the ESA ExoMars mission (to be launched in 2018). Pierre Brisson, president of the Mars Society Switzerland introduced the conference, speaking about the instruments aboard Curiosity and the targets of exploration of the rover.

In October (12th till 14th) The Mars Society Switzerland participated to the 12th EMC ("EMC12") in Neubiberg, Germany (University of the German Armed Forces, near Münich). In this frame, Pierre Brisson discussed the past possibility of an Ocean in the Northern Lowlands of the planet.

A key event of the year 2013 (March 26), was a conference organized with "Club 44" in La Chaux de Fonds, during which Professor Michel Cabane, LATMOS and co-PI of the SAM Instruments aboard Curiosity, presented the findings of his instruments dedicated to the study of the molecular and atomic compositions of the rocks and atmosphere of the planet Mars.

United Kingdom

The Mars Society UK is the oldest Mars Society outside the United States. It held its first public meeting on July 4, 1998, in London. Professor Colin Pillinger, head of the Beagle 2 project, was the Guest Speaker, and the event marked the first time Beagle 2 had been presented to the general public in the UK. From 1998 through to 2003, the Mars society UK (MSUK) continued to support Beagle 2, providing numerous public events at which members of the Beagle 2 project team could speak, and the Beagle 2 model be displayed.

Highlights of the MSUK's history include:

  • It hosted the first Mars Society European Leaders Meeting, with representatives from France, Germany, Poland, Spain and the Netherlands.
  • The first UK Mars Day, attended by some 200 members of the public took place in 2002. It was covered by all the UK's leading television media (BBC, ITN, Sky News).
  • In 2003, it had white papers accepted and published by the UK government as a part of a review of UK Space Policy. It also actively lobbied for UK involvement in human spaceflight endeavours.
  • Since 2006 it helped establish the Sir Arthur Clarke Award, the most prodigious award given in the United Kingdom for contribution in all field of space research and exploration. it also continued to provide consultation and white papers on the UK's changing space policy and helped determine the UK government's decision to actively engage in human spaceflight activities from 2010.
  • * MSUK had been allied with attempts to initiate a formally recognized and fully founded UK Space Conference (UKSC) with the first such event being held in April 2009.
  • The first UK University Rover Challenge was conducted in 2015. Established by the UK Mars Society Manchester Chapter, its primary goal is to encourage the UK's students to develop skills in robotics.
  • In 2018, the London Chapter of the Mars Society was formed and is working with other space outreach activists in the UK.
  • The UK wide Mars Society was relaunched in 2019 during an inaugural event in Oxford.

Asia

Mars Society South Asia (MSSA)

Mars Society South Asia (MSSA) was established by Sagar Dhaka and Harshit Sharma, and their associates from various Mars rover teams of South Asia on September 2, 2019. The ignition point behind this was the success of Indian Rover Challenge 2019 for which Sagar was the Event Manager. During their college at Manipal Institute of Technology, both Sagar and Harshit were active members of student rover team 'Mars Rover Manipal'. The main objectives of MSSA are:-

Broad public outreach to instill the vision of pioneering Mars.

Provide an effective platform to all the Mars Rover teams of South Asia to test and hone their rover designing and development skills.

Encourage students of South Asia to utilize their technical expertise in the applications of robotics in interplanetary missions and exploration of the extra-terrestrial environment.

Encourage South Asian participation in space science, engineering and research at education, industry and government level.

MSSA acts as a regulatory authority and co-organizer for Indian Rover Challenge (IRC). The IRC is an annual robotics competition which features an engineering challenge to engage students worldwide in the next phase of space exploration. IRC is the only robotics and space exploration competition of its kind in Asia-Pacific which aims to ignite and encourage the spirit of innovation amongst budding engineers as they set on a quest to build a space exploration rovers, using their skills and ideas. The competition challenges college students to design and develop next-generation Mars Rovers and compete in Mars Simulated conditions. Indian Rover Challenge is a part of the Rover Challenge Series (RCS) of The Mars Society.  The first event of MSSA was Indian Rover Challenge 2020, the finals of which took place in Vellore Institute of Technology, Chennai during 17-20 January 2020. 35 teams registered for the event and 20 were shortlisted for the finals.

In May 2020 MSSA started a new competition known as 'Indian Rover Design Challenge (IRDC)'. IRDC is a competition for university students which challenges them to design Mars rovers which shall be fully equipped and mission ready for Operation on Mars. The first edition took place during June-July 2020 and was attended by 28 teams from 7 countries.  IRDC was an entirely online competition where teams were judged on the basis of their 'Engineering Design Review'. Teams are supposed to carefully plan each subsystem of the rover considering various extra-terrestrial parameters in the design. This competition is designed for students to explore their mind and spark the innovative design thinking of Individuals without putting any constraints on available physical resources. Students are encouraged to be as imaginative, creative and insightful as possible within practical implementable limits for the human race.

India

The Mars Society India chapter (MSI) was founded in January 2012 by Dhruv Joshi, an alumnus of the Indian Institute of Technology Bombay. Dhruv Joshi was inspired to set up the chapter in India after he attended a presentation by Mars society Switzerland chapter; during his visit to Switzerland. MSI was launched on March 2, 2012 at Mumbai, with collaboration from Nehru center (Planetarium) and students of Indian Institute of Technology - Bombay (IIT-B). MSI endeavors to set a platform for bringing immense talent pool of Indian students to the forefront and achieve country's ambitious space missions.

Mars Society South Asia (MSSA) is a volunteer-driven non-profit space advocacy organization dedicated to advancing the scientific study, exploration, and public understanding of cosmos, in particular, the human exploration and settlement of planet Mars. MSSA is the official regional chapter of The Mars Society, USA for South Asia. It is the main regulatory authority for annual Mars rover competition Indian Rover Challenge (IRC) and Indian Rover Design Challenge (IRDC).

Bangladesh

Mars Society Bangladesh chapter was found in 2016. A group of 40 students and three teams from Bangladesh participated in 2016 University Rover Challenge (URC 2016) powered by Mars Society, held in June 2016 at Utah, USA.

Oceania Chapters of the Mars Society

Australia

There is a chapter in Australia, with branches in Australian Capital Territory (ACT), New South Wales (NSW), Northern Territory, Queensland, South Australia, Tasmania, Victoria, and Western Australia.[30] The main goals for Mars Society Australia are to support government funded programs geared towards exploring Mars and reach out to the public about both exploring Mars and the importance of studying planetary sciences and engineering.[31]

New Zealand

The NZ Mars Society has the same list of goals as Australia.[32] In an effort to help put people on Mars, they plan to have their members test surface exploration strategies and technologies in locations dedicated to Mars analogue.[33] One of these Mars analogue locations is Mars Desert Research Station in Utah.[34]

 

The Case for Mars

From Wikipedia, the free encyclopedia
 
The Case for Mars: The Plan to Settle the Red Planet and Why We Must
Caseformars.jpg
AuthorRobert Zubrin
Richard Wagner
Arthur C. Clarke
LanguageEnglish
SubjectNon-fiction
Science
PublisherTouchstone
Publication date
1996
Pages368
ISBN978-0684835501
OCLC34906203
919.9/2304-dc20
LC ClassQB641.Z83 1996

The Case for Mars: The Plan to Settle the Red Planet and Why We Must is a nonfiction science book by Robert Zubrin, first published in 1996, and revised and updated in 2011.

The book details Zubrin's Mars Direct plan to make the first human landing on Mars. The plan focuses on keeping costs down by making use of automated systems and available materials on Mars to manufacture the return journey's fuel in situ. The book also reveals possible Mars colony designs and weighs the prospects for a colony's material self-sufficiency and for the terraforming of Mars.

Mars Direct

The Mars Direct plan was originally detailed by Zubrin and David Baker in 1990. The Case for Mars is, according to Zubrin, a comprehensive condensation for laymen of many years' work and research. Chapters one and four deal with Mars Direct most completely.

Colonization

For Robert Zubrin, the attractiveness of Mars Direct does not rest on a single cost-effective mission. He envisions a series of regular Martian missions with the ultimate goal of colonization, which he details in the seventh through ninth chapters. As initial explorers leave hab-structures on the planet, subsequent missions become easier to undertake.

Large mall like structures buried in regolith, pressurized habitats would be the first step toward human settlement; the book suggests they can be built as Roman-style atria on the surface and then be buried with regolith, with easily produced Martian brick. During and after this initial phase of habitat construction, hard-plastic radiation- and abrasion-resistant geodesic domes could be deployed on the surface for eventual habitation and crop growth. Nascent industry would begin using indigenous resources: the manufacture of plastics, ceramics and glass.

The larger work of terraforming requires an initial phase of global warming to release atmosphere from the regolith and to create a water cycle. Three methods of global warming are described in the work and, Zubrin suggests, are probably best deployed in tandem: orbital mirrors to heat the surface; factories on the surface to pump halocarbons such as perfluromethane into the atmosphere; and the seeding of bacteria which can metabolize water, nitrogen and carbon to produce ammonia and methane (these would aid in global warming). While the work of warming Mars is on-going, true colonization can begin.

The Case for Mars acknowledges that any Martian colony will be partially Earth-dependent for centuries. However, it suggests that Mars may be a profitable place for two reasons. First, it may contain concentrated supplies of metals of equal or greater value to silver which have not been subjected to millennia of human scavenging and may be sold on Earth for profit. Secondly, the concentration of deuterium – a possible fuel for commercial nuclear fusion – is five times greater on Mars. Humans emigrating to Mars thus have an assured industry and the planet will be a magnet for settlers as wage costs will be high. The book asserts that “the labor shortage that will prevail on Mars will drive Martian civilization toward both technological and social advances.”

Wider considerations

While detailing the exploration and colonization, The Case for Mars also addresses a number of attendant scientific and political factors.

Risks confronted

The fifth chapter analyzes various risks that putatively rule out a long-term human presence on Mars. Zubrin dismisses the idea that radiation and zero-gravity are unduly hazardous. He claims that cancer rates do increase for astronauts who have spent extensive time in space, but only marginally. Similarly, while zero-gravity presents challenges, “near total recovery of musculature and immune system occurs after reentry and reconditioning to a one-gravity environment.” Furthermore, since his plan has the spacecraft spinning at the end of a long tether to create artificial gravity, worries about zero gravity do not apply to this mission in any case. Back-contamination – humans acquiring and spreading Martian viruses – is described as "just plain nuts", because there are no host organisms on Mars for disease organisms to have evolved.

In the same chapter, Zubrin decisively denounces and rejects suggestions that the Moon should be used as waypoint to Mars or as a training area. It is ultimately much easier to journey to Mars from low Earth orbit than from the Moon and using the latter as a staging point is a pointless diversion of resources. While the Moon may superficially appear a good place to perfect Mars exploration and habitation techniques, the two bodies are radically different. The Moon has no atmosphere, no analogous geology and a much greater temperature range and rotational period. Antarctica or desert areas of Earth provide much better training grounds at lesser cost.

Viability

In the third and tenth chapters, The Case for Mars addresses the politics and costs of the ideas described. The authors argue that the colonization of Mars is a logical extension of the settlement of North America. They envision a frontier society, providing opportunities for innovation and social experimentation.

Zubrin suggests three models to provide the will and capital to drive Mars exploration forward: the J.F.K. model, in which a far-sighted U.S. leader provides the funding and mobilizes national public opinion around the idea; the Sagan model, in which international co-operation is the driving force; and the Gingrich approach, which emphasizes incentives and even prizes for private sector actors who take on research and development tasks. In keeping with the third idea, Zubrin describes twelve challenges that address various aspects of the exploration program. A monetary prize – from five hundred million to twenty billion dollars – is offered to companies who successfully complete the challenges.

The prize-based approach to hardware development has emerged within the private aeronautics community, though not yet on the scale envisioned by Zubrin. Ventures such as the Ansari X-Prize and Robert Bigelow's America's Space Prize seek low-cost spaceflight development through private enterprise, and crucially, for the attainment of very specific predetermined goals in order to win the prizes.

The underlying political and economic problems of raising sufficient capital for terraforming using halocarbon emissions is critiqued by John Hickman.

Translations

In 2017, a Russian translation of the book was published under the title of Курс на Марс (On Course for Mars) (ISBN 978-5-699-75295-9).

 

Colonization of Venus

From Wikipedia, the free encyclopedia

Artist's rendering of a crewed floating outpost on Venus of NASA's High Altitude Venus Operational Concept (HAVOC).

The colonization of Venus has been a subject of many works of science fiction since before the dawn of spaceflight, and is still discussed from both a fictional and a scientific standpoint. However, with the discovery of Venus's extremely hostile surface environment, attention has largely shifted towards the colonization of the Moon and Mars instead, with proposals for Venus focused on colonies floating in the upper-middle atmosphere and on terraforming.

With discoveries as of 2020 of traces of possibly indigenous life in the atmosphere of Venus, attempts of any humanization of Venus have become an increased issue of planetary protection, since uncontrolled effects of human presence might endanger such life.

Reasons for colonization

Space colonization is a step beyond space exploration, and implies the permanent or long-term presence of humans in an environment outside Earth. Colonization of space was claimed by Stephen Hawking to be the best way to ensure the survival of humans as a species. Other reasons for colonizing space include economic interests, long-term scientific research best carried out by humans as opposed to robotic probes, and sheer curiosity. Venus is the second largest terrestrial planet and Earth's closest neighbor, which makes it a potential target.

Advantages

Scale representations of Venus and the Earth shown next to each other. Venus is only slightly smaller.

Venus has certain similarities to Earth which, if not for the hostile conditions, might make colonization easier in many respects in comparison with other possible destinations. These similarities, and its proximity, have led Venus to be called Earth's "sister planet".

At present it has not been established whether the gravity of Mars, 0.38 times that of the Earth, would be sufficient to avoid bone decalcification and loss of muscle tone experienced by astronauts living in a micro-g environment. In contrast, Venus is close in size and mass to the Earth, resulting in a similar surface gravity (0.904 g) that would likely be sufficient to prevent the health problems associated with weightlessness. Most other space exploration and colonization plans face concerns about the damaging effect of long-term exposure to fractional g or zero gravity on the human musculoskeletal system.

Venus's relative proximity makes transportation and communications easier than for most other locations in the Solar System. With current propulsion systems, launch windows to Venus occur every 584 days, compared to the 780 days for Mars. Flight time is also somewhat shorter; the Venus Express probe that arrived at Venus in April 2006 spent slightly over five months en route, compared to nearly six months for Mars Express. This is because at closest approach, Venus is 40 million km (25 million mi) from Earth (approximated by perihelion of Earth minus aphelion of Venus) compared to 55 million km (34 million mi) for Mars (approximated by perihelion of Mars minus aphelion of Earth) making Venus the closest planet to Earth.

Venus's atmosphere is made mostly out of carbon dioxide. Because nitrogen and oxygen are lighter than carbon-dioxide, breathable-air-filled balloons will float at a height of about 50 km (31 mi). At this height, the temperature is a manageable 75 °C (348 K; 167 °F). At 5 km (3.1 mi) higher, it is a temperate 27 °C (300 K; 81 °F).

The atmosphere also provides the various elements required for human life and agriculture: carbon, hydrogen, oxygen, nitrogen, and sulfur.

Additionally, the upper atmosphere could provide protection from harmful solar radiation comparable to the protection provided by Earth's atmosphere. The atmosphere of Mars, as well as the Moon provide little such protection.

Difficulties

Air pressure on Venus, beginning at a pressure on the surface 90 times that of Earth and reaching a single bar by 50 kilometers

Venus also presents several significant challenges to human colonization. Surface conditions on Venus are difficult to deal with: the temperature at the equator averages around 450 °C (723 K; 842 °F), higher than the melting point of lead, which is 327 °C. The atmospheric pressure on the surface is also at least ninety times greater than on Earth, which is equivalent to the pressure experienced under a kilometer of water. These conditions have caused missions to the surface to be extremely brief: the Soviet Venera 5 and Venera 6 probes were crushed by high pressure while still 18 km above the surface. Following landers such as Venera 7 and Venera 8 succeeded in transmitting data after reaching the surface, but these missions were brief as well, surviving no more than a single hour on the surface.

The surface of venus is completely covered by clouds which prevents any heat from escaping.

Furthermore, water, in any form, is almost entirely absent from Venus. The atmosphere is devoid of molecular oxygen and is primarily carbon dioxide. In addition, the visible clouds are composed of corrosive sulfuric acid and sulfur dioxide vapor.

Exploration and research

Over 20 successful space missions have visited Venus since 1962. The last European probe was ESA's Venus Express, which was in polar orbit around the planet from 2006 to 2014. A Japanese probe, Akatsuki, failed in its first attempt to orbit Venus, but successfully reinserted itself into orbit on 7 December 2015. Other low-cost missions have been proposed to further explore the planet's atmosphere, as the area 50 km (31 mi) above the surface where gas pressure is at the same level as Earth has not yet been thoroughly explored.

Aerostat habitats and floating cities

Hypothetical floating outpost studying habitation of Venus around 50 km above the surface supported by a torus full of hydrogen

At least as early as 1971 Soviet scientists have suggested that rather than attempting to settle Venus' hostile surface, humans might attempt to settle the Venerian atmosphere. Geoffrey A. Landis of NASA's Glenn Research Center has summarized the perceived difficulties in colonizing Venus as being merely from the assumption that a colony would need to be based on the surface of a planet:

However, viewed in a different way, the problem with Venus is merely that the ground level is too far below the one atmosphere level. At cloud-top level, Venus is the paradise planet.

Landis has proposed aerostat habitats followed by floating cities, based on the concept that breathable air (21:79 oxygen/nitrogen mixture) is a lifting gas in the dense carbon dioxide atmosphere, with over 60% of the lifting power that helium has on Earth. In effect, a balloon full of human-breathable air would sustain itself and extra weight (such as a colony) in midair. At an altitude of 50 kilometres (31 mi) above the Venerian surface, the environment is the most Earth-like in the Solar System – a pressure of approximately 1 atm or 1000 hPa and temperatures in the 0 to 50 °C (273 to 323 K; 32 to 122 °F) range. Protection against cosmic radiation would be provided by the atmosphere above, with shielding mass equivalent to Earth's.

At the top of the clouds the wind speed on Venus reaches up to 95 m/s (340 km/h; 210 mph), circling the planet approximately every four Earth days, in a phenomenon known as "super-rotation". Compared to the Venusian solar day of 118 Earth days, colonies freely floating in this region could therefore have a much shorter day-night cycle. Allowing a colony to move freely would also reduce structural stress from the wind that they would experience if tethered to the ground.

Advantages

Because there is not a significant pressure difference between the inside and the outside of the breathable-air balloon, any rips or tears would cause gases to diffuse at normal atmospheric mixing rates rather than an explosive decompression, giving time to repair any such damages. In addition, humans would not require pressurized suits when outside, merely air to breathe, protection from the acidic rain and on some occasions low level protection against heat. Alternatively, two-part domes could contain a lifting gas like hydrogen or helium (extractable from the atmosphere) to allow a higher mass density. Therefore, putting on or taking off suits for working outside would be easier. Working outside the vehicle in non-pressurized suits would also be easier.

Remaining problems

Structural and industrial materials would be hard to retrieve from the surface and expensive to bring from Earth/asteroids. The sulfuric acid itself poses a further challenge in that the colony would need to be constructed of or coated in materials resistant to corrosion by the acid, such as PTFE (a compound consisting wholly of carbon and fluorine).

Studies

In 2015, NASA developed the High Altitude Venus Operational Concept (HAVOC) for exploring the possibility of setting up an atmospheric crewed mission.

Artificial mountains

As an alternative to floating cities, it has been proposed that a large artificial mountain, dubbed the "Venusian Tower of Babel", could be built on the surface of Venus. It would reach up to 50 kilometres (31 mi) into the atmosphere where the temperature and pressure conditions are similar to Earth's. Such a structure could be built using autonomous robotic bulldozers and excavators that have been hardened against the extreme temperature and pressure of the Venus atmosphere. Robotic machines would be covered in a layer of heat and pressure shielding ceramics, with internal helium-based heat pumps inside of the machines to cool both an internal nuclear power plant and to keep the internal electronics and motor actuators of the machine cooled to within operating temperature. These machines could be designed to operate for years without external intervention for the purpose of building colossal mountains on Venus to serve as islands of colonization in the skies of Venus.

Terraforming

Artist's conception of a terraformed Venus. The cloud formations are depicted assuming the planet's rotation hasn't been sped up.

Venus has been the subject of a number of terraforming proposals. The proposals seek to remove or convert the dense carbon dioxide atmosphere, reduce Venus's 450 °C (723 K; 842 °F) surface temperature, and establish a day/night light cycle closer to that of Earth.

Many proposals involve deployment of a solar shade or a system of orbital mirrors, for the purpose of reducing insolation and providing light to the dark side of Venus. Another common thread in most proposals involves some introduction of large quantities of hydrogen or water. Proposals also involve either freezing most of Venus's atmospheric CO2, or converting it to carbonates, urea, or other forms.

 

Aerospace architecture

From Wikipedia, the free encyclopedia

Aerospace architecture is broadly defined to encompass architectural design of non-habitable and habitable structures and living and working environments in aerospace-related facilities, habitats, and vehicles. These environments include, but are not limited to: science platform aircraft and aircraft-deployable systems; space vehicles, space stations, habitats and lunar and planetary surface construction bases; and Earth-based control, experiment, launch, logistics, payload, simulation and test facilities. Earth analogs to space applications may include Antarctic, desert, high altitude, underground, undersea environments and closed ecological systems.

The American Institute of Aeronautics and Astronautics (AIAA) Design Engineering Technical Committee (DETC) meets several times a year to discuss policy, education, standards, and practice issues pertaining to aerospace architecture.

The role of Appearance in Aerospace architecture

"The role of design creates and develops concepts and specifications that seek to simultaneously and synergistically optimize function, production, value and appearance." In connection with, and with respect to, human presence and interactions, appearance is a component of human factors and includes considerations of human characteristics, needs and interests.

Appearance in this context refers to all visual aspects – the statics and dynamics of form(s), color(s), patterns, and textures in respect to all products, systems, services, and experiences. Appearance/esthetics affects humans both psychologically and physiologically and can effect/improving both human efficiency, attitude, and well-being.

In reference to non-habitable design the influence of appearance is minimal if not non-existent. However, as the industry of aerospace continues to rapidly grow, and missions to put humans on Mars and back to the Moon are being announced. The role that appearance/esthetics to maintain crew well-being and health of multi-month or year missions becomes a monumental factor in mission success.

Habitable Structures within Earth's Atmosphere

Appearance/esthetics

Appearance/esthetics in aerospace design must at least co-exist, if not be synergistic, with the overall/societal fundamentals/metrics of aerospace engineering design. These metrics, for atmospheric flight consist of overall/societal factors directed toward productivity, safety, environmental issues such as noise/emissions and accessibly/ affordability. Furthermore, technological parameters such as space, weight and drag minimization and propulsion efficiency highly dictate and restrain the boundaries of appearance/esthetic design. Major factors that need to be considered in atmospheric flight design include producability, maintainability, reliability, flyability, inspectability, flexibility, repairability, operability, durability, and airport compatibility.

Habitable Structures outside of Low-Earth Orbit (LEO)

What is different concerning space in reference to human-centered design thinking is the nearly complete lack of human presence. Human-centered design influence wholly operates within the context of human interactions; how operations/ missions are run (operability) or how products, systems, services, or experiences (PSSE's) affect end users (usability). Currently the human presence involves the space station and the relatively few international rocket systems.

Human-Centered Design

Due to the large space boom and technological advancements, over the past decade numerous countries and companies have released statements that human expeditions to our solar system are far from done. With long duration confinement in limited interior space in micro-g with little-to-no real variability in environment, attention towards user [crew] subjects well-being, and mental alertness will pose complex human-centered design issues. Mars transit vehicles and surface habitats will constitute highly confined, technical settings characterized by social, emotional and physical deprivation while affording little opportunity to experience privacy and environmental variation. And esthetic/appearance measures for human exploration will emphasize upon “naturalistic countermeasures” to the innate/multitudinous stresses of such expeditions.

Although human wants, needs, and limitations both physically and mentally need to be evaluated and address when designing for space. Design decisions must at least co-exist, if not be synergistic, with the overall metrics of aerospace engineering design. Ex. The International Space Station Toilet. Human factors and habitability design are important topics for all working and living spaces. For space exploration, they are vital. While human factors and certain habitability issues have been integrated into the design process of manned spacecraft, there is a crucial need to move from mere survivability to factors that support thriving. As of today, the risk of an incompatible vehicle or habitat design has already been identified by NASA as recognized key risk to human health and performance in space. Habitability and human factors will become even more important determinants for the design of future long-term and commercial space facilities as larger and more diverse groups occupy off-earth habitats.

Past Examples

A study conducted in 1989 (reference 2) found that when given multiple photographs and paintings as potential decoration of the international space station. Test (crew) subjects all individually preferred those with naturalistic, irrespective themes, and a large depth of field. Other examples of human-centered design is using pastel paints on the International Space Station (ISS) to contrast and provide “up/down” cues in micro-g environments or the concept of dynamically and spatially adjusting lighting color and intensities to conform to daily and even seasonal biorhythms similar to earth to mitigate the societal separation effects experienced in space.

Thermodynamic diagrams

From Wikipedia, the free encyclopedia https://en.wikipedia.org/wiki/Thermodynamic_diagrams Thermodynamic diagrams are diagrams used to repr...