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      The potential of Deception Island, Antarctica, as a multifunctional Martian analogue of astrobiological interest

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          Abstract

          The establishment of the possible presence of life on Mars (past or present) is based on the study of planetary analogues, which allow in situ analysis of the environments in which living organisms adapt to often extreme conditions. Although Mars has been a candidate for hosting life, based on observations made decades ago, it is thanks to the characteristics identified in environments, mainly volcanic, that it has been possible to calibrate instruments and detail the features of the red planet. In this paper, we present a review of the main characteristics of different planetary analogues, particularly deepening the study of Antarctica, to later expose the factors studied in Deception Island that have contributed to considering it as an analogue of Mars from different perspectives. Although geological and geomorphological studies on the analogies of the island already exist, detailed analyses that present the approach of astrobiological analogues are required, thus allowing further research.

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          Earth's early atmosphere.

          J. Kasting (1993)
          Ideas about atmospheric composition and climate on the early Earth have evolved considerably over the last 30 years, but many uncertainties still remain. It is generally agreed that the atmosphere contained little or no free oxygen initially and that oxygen concentrations increased markedly near 2.0 billion years ago, but the precise timing of and reasons for its rise remain unexplained. Likewise, it is usually conceded that the atmospheric greenhouse effect must have been higher in the past to offset reduced solar luminosity, but the levels of atmospheric carbon dioxide and other greenhouse gases required remain speculative. A better understanding of past atmospheric evolution is important to understanding the evolution of life and to predicting whether Earth-like planets might exist elsewhere in the galaxy.
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            HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: NEW ESTIMATES

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              Habitable Zones around Main Sequence Stars

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                Journal
                International Journal of Astrobiology
                International Journal of Astrobiology
                Cambridge University Press (CUP)
                1473-5504
                1475-3006
                2025
                February 13 2025
                2025
                : 24
                Article
                10.1017/S1473550425000023
                2ba2626b-5e36-4f0f-a45b-be5e20e82589
                © 2025

                Free to read

                http://creativecommons.org/licenses/by/4.0/

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