Abstract
In order to make Mars a better planet, in this paper, photo-dissociation technology, mathematical modeling, and a series of chemical reaction methodology have been proposed to create a vibrant ecosystem and balance the atmosphere on Mars. Since CO2 is a stable compound, breaking it down into C and O2 always is challenging, but exciting thought. Interestingly, my recent research revealed that photo-dissociation by utilizing UVV (laser) could be an exciting technology to split CO2 into C + O2 since the theoretical reaction suggested that the production of C + O2 channel from CO2 photo-exciting technology releases the energetic level threshold of C(3P2) + O2(X3∑ −g ) that can be detected by ultraviolet laser pump-probe spectroscopy. Subsequently, a mathematical model for creating of ocean on Mars by breaking its substantial polar ice has been performed considering algorithms for surface and coordinate between the barotropic momentum and continuity equations, and interestingly the calculation suggested that it is very much possible to flow ocean on Mars surface to meet its water demand. Subsequently, proposed series of chemical reaction technology suggested that implementation of carbonator looping and plasma reaction paths can convert photo-dissociated carbon (C) into N2 and NH3 to enrich Mars’ soil in order to grow vegetation as well as to create a balance ecosystem in Mars eventually. Finally, sustainable green technology has been proposed for the development of Mars to be a complete balanced planet to deliver all basic and modern needs to run daily life smoothly. Thus, implication of chemical reaction technologies along with sustainable development plans can indeed make the Mars a vibrant environment to live there in clean and green.
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References
Arakawa A, Lamb VR (1977) Computational design of the basic dynamical processes of the UCLA general circulation model. Methods Comput Phys 17:174–267
Atsoniosa K et al (2013) Integration of calcium looping technology in existing cement plant for CO2 capture: process modeling and technical considerations. Fuel 53:210–223
Bai M, Zhang Z, Bai M, Ba X (2008) Conversion of methane to liquid products, hydrogen, and ammonia with environmentally friendly condit. J Air Waste Manag 58:1616–1621
Baker VR, Strom RG, Gulick VC, Kargel JS, Komatsu G, Kale VS (1991) Ancient oceans, ice sheets and the hydrological cycle on Mars. Nature 352:589–594. doi:10.1038/352589a0
Bibring JP et al (2004) Perennial water ice identified in the south polar cap of Mars. Nature 428:627
Dohm JM, Baker VR, Boynton WV et al (2009) GRS evidence and the possibility of paleooceans on Mars. Planet Space Sci 57:664–684. doi:10.1016/j.pss.2008.10.008
Gao H, Song Y, Jackson WM, Ng CY (2013) Communication: state-to-state photodissociation study by the two-color VUV-VUV laser pump-probe time-slice velocity-map-imaging-photoion method. J Chem Phys 138:191102
Hartogh P et al (2010) HIFI observations of water in the atmosphere of comet C/2008 Q3 (Garradd). Astron Astrophys 521:150
Hossain M (2016a). Theory of global cooling. Energ Sustain Soc 6:24. doi:10.1186/s13705-016-0091-y
Hossain M (2016b) Solar energy integration into advanced building design for meeting energy demand and environment problem. Int J Energy Res 40:1293
Howard A, Moore JM, Irwin RP (2005) An intense terminal epoch of widespread fluvial activity on early Mars: 1. Valley network incision and associated deposits. J Geophys Res. doi:10.1029/2005JE002459
Hyungwoong A et al (2013) Process configuration studies of the amine capture process for coal-fired power plants. Int J Greenh Gas Control 16:29–40
Liu CJ (1998) Nonoxidative methane conversion to acetylene over zeolite in a low temperature plasma. J Catal 179:326–334
Liu NN, Bai MD, Wang MX, Liu KY (2013) Hydrogen production by methane reforming based on micro-gap discharge. J Phys Conf Ser 418:012146
Lu Z, Chang YC, Yin Q-Z, Ng CY, Jackson WM (2014) Evidence for direct molecular oxygen production in CO2 photodissociation. Science 346:61–64
Mahaffy PR et al (2013) Abundance and Isotopic composition of gases in the martian atmosphere from the curiosity rover. Science 341:263–266
Mann ME, Bradley RS, Hughes MK (1998) Global-scale temperature patterns and climate forcing over the past six centuries. Nature 392:779–787
Martín-Torres FJ, Zorzano MP, Valentín-Serrano P, Harri AM, Genzer M (2015) Transient liquid water and water activity at Gale crater on Mars. Nat Geoci 8(357–361):2015. doi:10.1038/ngeo2412
Meslin PY et al. (2013) Soil diversity and hydration as observed by ChemCam at Gale Crater, Mars. Science 341(6153):1238670
NASA (2016a) Mars ice deposit holds as much water as lake superior. November 22, 2016. Retrieved 23 Nov 2016
NASA (2016b) Scalloped terrain led to finding of buried ice on Mars. Retrieved 23 Nov 2016
Ojha L, Wilhelm MB, Murchie SL, McEwen AS, Wray JJ, Hanley J, Massé M, Chojnacki M (2015) Spectral evidence for hydrated salts in recurring slope lineae on Mars. Nat Geosci 8:829–832. doi:10.1038/ngeo2546
Rummel JD, Beaty DW, et al. (2014) A new analysis of Mars “special regions”: findings of the second MEPAG special regions science analysis group (SRSAG2). Astrobiology 78:32–42
Townsend D et al (2004) The roaming atom: straying from the reaction path in formaldehyde decomposition. Science 306:1158–1161
Villanueva G, Mumma M et al. (2015) Strong water isotopic anomalies in the martian atmosphere: probing current and ancient reservoirs. Science 348:218–221. doi:10.1126/science.aaa3630
Willebrand J, Barnier B, Böning C, Dieterich C, Kill-Worth PD, LeProvost C, Jia Y, Molines J-M, New AL (2001) Circulation characteristics in three eddy-permitting models of the North Atlantic. Prog Oceanogr 48:123–161
Wray JP (2013) Volatile, isotope, and organic analysis of martian fines with the Mars curiosity Rover. Science. doi:10.1126/science.1238937overview
Yue H et al (2017) Process integration of a calcium-looping process with a natural gas combined cycle power plant for CO2 capture and its improvement by exhaust gas recirculation. Appl Energy 187:480–488
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This research was partially supported by Green Globe Technology under Grant RD-2017-01. Any findings, conclusions, and recommendations expressed in this paper are solely those of the author and do not necessarily reflect those of IBTS and/or Green Globe Technology.
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Hossain, M.F. Application of advanced technology to build a vibrant environment on planet mars. Int. J. Environ. Sci. Technol. 14, 2709–2720 (2017). https://doi.org/10.1007/s13762-017-1354-7
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DOI: https://doi.org/10.1007/s13762-017-1354-7