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  2. Human mission to Mars - Wikipedia

    en.wikipedia.org/wiki/Human_mission_to_Mars

    The lowest energy transfer to Mars is a Hohmann transfer orbit, a conjunction class mission which would involve a roughly 9-month travel time from Earth to Mars, about 500 days (16 mo) [citation needed] at Mars to wait for the transfer window to Earth, and a travel time of about 9 months to return to Earth. [9] [10] This would be a 34-month trip.

  3. Exploration of Mars - Wikipedia

    en.wikipedia.org/wiki/Exploration_of_Mars

    Journey to Mars – Science, Exploration, Technology. On October 8, 2015, NASA published its official plan for human exploration and colonization of Mars. They called it "Journey to Mars". The plan operates through three distinct phases leading to fully sustained colonization. [150] The first stage, already underway, is the "Earth Reliant" phase.

  4. Carbon footprint - Wikipedia

    en.wikipedia.org/wiki/Carbon_footprint

    The carbon footprint explained Comparison of the carbon footprint of protein-rich foods [1]. A formal definition of carbon footprint is as follows: "A measure of the total amount of carbon dioxide (CO 2) and methane (CH 4) emissions of a defined population, system or activity, considering all relevant sources, sinks and storage within the spatial and temporal boundary of the population, system ...

  5. Characteristic energy - Wikipedia

    en.wikipedia.org/wiki/Characteristic_energy

    The InSight mission to Mars launched with a C 3 of 8.19 km 2 /s 2. [5] The Parker Solar Probe (via Venus) plans a maximum C 3 of 154 km 2 /s 2. [6] Typical ballistic C 3 (km 2 /s 2) to get from Earth to various planets: Mars 8-16, [7] Jupiter 80, Saturn or Uranus 147. [8] To Pluto (with its orbital inclination) needs about 160–164 km 2 /s 2. [9]

  6. Mars general circulation model - Wikipedia

    en.wikipedia.org/wiki/Mars_General_Circulation_Model

    A first attempt at a Mars general circulation model was created by Leovy and Mintz who used an Earth model and adapted it to Martian conditions. This preliminary model had the capability to predict atmospheric condensation of carbon dioxide and the presence of transient baroclinic waves in the winter mod-latitudes. [ 4 ]

  7. Climate change: Mars and PepsiCo offer lessons in ... - AOL

    www.aol.com/finance/climate-change-mars-pepsico...

    Earlier this year, Mars launched a new coalition with PepsiCo and McCormick , working with Guidehouse to educate suppliers about their carbon footprint and develop tools to reduce their impact on ...

  8. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    In terms of relative abundance of carbon, the C / 84 Kr ratio on Mars is only 10% of that on Earth and Venus. Assuming the three rocky planets have the same initial volatile inventory, then this low C / 84 Kr ratio implies the mass of CO 2 in the early Martian atmosphere should have been ten times higher than the present value. [ 43 ]

  9. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    [36] [37] Although the organic carbon was probably from Mars, it can all be explained by dust and meteorites that have landed on the planet. [38] [39] [40] Because much of the carbon was released at a relatively low temperature in Curiosity's Sample Analysis at Mars (SAM) instrument package, it probably did not come from carbonates in the ...