We humans can literally thank our lucky stars for those heavier elements needed to create DNA, specifically carbon, hydrogen, nitrogen, oxygen, phosphorous and sulphur (CHNOPS), forged inside the nuclear furnaces of dying stars that implode leaving behind supernova remnants (Bailey, 2020). Since the first cosmic whiff and most distant detection of O jettisoned by the galaxy MACS1149-JD1 ∼13.28 billion years ago at a time when the universe was <2% of its current age (Hashimoto et al., 2018), this element has become synonymous with life. With the advent of oxygenic photosynthesis, atmospheric levels of the diatomic oxygen (O 2 ) molecule (two Os glued together with a double covalent bond sharing two pairs of valence electrons) increased rapidly during the Proterozoic aeon of the Precambrian period, with each O 2 'pulse' sparking an explosion in Earth's biota, heralding the emergence of complex multicellular life, aerobic respiration and cephalisation. Indeed, the human brain stands as clear testament to our reliance on this precious gas and inherent vulnerability to failure when supply is cut off, given its voracious appetite in the face of little to no O 2 /glycogen reserves (Bailey, 2019). In short, we are all 'obligate neurobes'! But do not take this gas for granted, because atmospheric O 2 levels have started to wax and wane from the 20.93% (ambient P O 2 of 150 mmHg) that we have come to enjoy over the last ∼100 million years or so (Berner et al., 2007). Indeed, conservative estimates based on parabolic modelling (Livina et al., 2015) predict that within ∼3,600 years, living at sea level will feel as uncomfortably hypoxic as if we were atop a ∼5,340 m mountain, equivalent to the highest habitable elevation that humans can 'endure' here on Earth (Bailey, 2019). Complete depletion has been predicted to occur within ∼4.4 millennia, a sobering prospect that seems to have escaped public attention given current preoccupation with rising levels of that other gas, carbon dioxide (CO 2 ), the flipside of the climate coin. Hence the need to consider alternative sources of O 2 is important if we are to continue to sustain life here on Earth, or indeed beyond. This challenge has taken on new significance as humans plan extended missions to the lunar surface and beyond, with a crewed mission to Mars anticipated as early as the 2030s; the next frontier in our quest to becoming a spacefaring, multiplanetary species. Of all the planets in the solar system, Mars most closely resembles Earth, yet the journey to and habitation on the Red Planet pose unique physiological challenges. Astronauts will have to cope with the combined stresses of space radiation, altered gravity, isolation/confinement and closed environments (Patel et al., 2020) for 1,000 days on a planet located anywhere from ∼55 to 400 million km from Earth (dependent on the