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      Synergies Between Venus & Exoplanetary Observations : Venus and Its Extrasolar Siblings

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          Abstract

          Here we examine how our knowledge of present day Venus can inform terrestrial exoplanetary science and how exoplanetary science can inform our study of Venus. In a superficial way the contrasts in knowledge appear stark. We have been looking at Venus for millennia and studying it via telescopic observations for centuries. Spacecraft observations began with Mariner 2 in 1962 when we confirmed that Venus was a hothouse planet, rather than the tropical paradise science fiction pictured. As long as our level of exploration and understanding of Venus remains far below that of Mars, major questions will endure. On the other hand, exoplanetary science has grown leaps and bounds since the discovery of Pegasus 51b in 1995, not too long after the golden years of Venus spacecraft missions came to an end with the Magellan Mission in 1994. Multi-million to billion dollar/euro exoplanet focused spacecraft missions such as JWST, and its successors will be flown in the coming decades. At the same time, excitement about Venus exploration is blooming again with a number of confirmed and proposed missions in the coming decades from India, Russia, Japan, the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA). Here we review what is known and what we may discover tomorrow in complementary studies of Venus and its exoplanetary cousins.

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              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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                Author and article information

                Contributors
                Michael.J.Way@nasa.gov
                Ana.Plesa@dlr.de
                Journal
                Space Sci Rev
                Space Sci Rev
                Space Science Reviews
                Springer Netherlands (Dordrecht )
                0038-6308
                1572-9672
                9 February 2023
                9 February 2023
                2023
                : 219
                : 1
                : 13
                Affiliations
                [1 ]GRID grid.419078.3, ISNI 0000 0001 2284 9855, NASA Goddard Institute for Space Studies, ; 2880 Broadway, New York, NY 10025 USA
                [2 ]GRID grid.8993.b, ISNI 0000 0004 1936 9457, Theoretical Astrophysics, Department of Physics and Astronomy, , Uppsala University, ; Uppsala, Sweden
                [3 ]GRID grid.266097.c, ISNI 0000 0001 2222 1582, Department of Earth and Planetary Sciences, , University of California, ; Riverside, CA 92521 USA
                [4 ]GRID grid.29857.31, ISNI 0000 0001 2097 4281, Department of Geosciences, , Pennsylvania State University, ; University Park, PA USA
                [5 ]GRID grid.21940.3e, ISNI 0000 0004 1936 8278, Department of Earth, Environmental and Planetary Sciences, , Rice University, ; Houston, TX 77005 USA
                [6 ]GRID grid.4556.2, ISNI 0000 0004 0493 9031, Potsdam Institute for Climate Impact Research, ; Potsdam, Germany
                [7 ]GRID grid.12380.38, ISNI 0000 0004 1754 9227, Department of Earth Sciences, , Vrije Universiteit Amsterdam, ; Amsterdam, The Netherlands
                [8 ]GRID grid.4299.6, ISNI 0000 0001 2169 3852, Space Research Institute, , Austrian Academy of Sciences, ; Schmiedlstr. 6, 8042 Graz, Austria
                [9 ]GRID grid.215654.1, ISNI 0000 0001 2151 2636, School of Earth and Space Exploration, , Arizona State University, ; Tempe, AZ USA
                [10 ]GRID grid.13349.3c, ISNI 0000 0001 2201 6490, Institut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Université Paul Sabatier – Toulouse III, , Centre National d’Etudes Spatiales, ; Toulouse, France
                [11 ]GRID grid.7551.6, ISNI 0000 0000 8983 7915, Institute of Planetary Research, DLR, ; Berlin, Germany
                [12 ]GRID grid.261120.6, ISNI 0000 0004 1936 8040, Department of Astronomy and Planetary Science, , Northern Arizona University, ; Box 6010, Flagstaff, AZ 86011 USA
                [13 ]GRID grid.134563.6, ISNI 0000 0001 2168 186X, Habitability, Atmospheres, and Biosignatures Laboratory, , University of Arizona, ; Tucson, AZ USA
                [14 ]GRID grid.134563.6, ISNI 0000 0001 2168 186X, Lunar and Planetary Laboratory, , University of Arizona, ; Tucson, AZ USA
                [15 ]GRID grid.5110.5, ISNI 0000000121539003, Institute of Physics, , University of Graz, ; Graz, Austria
                [16 ]GRID grid.410413.3, ISNI 0000 0001 2294 748X, Institute for Geodesy, , Technical University, ; Graz, Austria
                [17 ]GRID grid.491513.b, ISNI 0000 0001 0944 145X, Lunar and Planetary Institute, ; 3600 Bay Area Blvd., Houston, TX 77058 USA
                Author information
                http://orcid.org/0000-0003-3728-0475
                Article
                953
                10.1007/s11214-023-00953-3
                9911515
                75b99737-abea-4dbc-bea0-5bdc42ab57ec
                © The Author(s) 2023

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 13 April 2022
                : 11 January 2023
                Funding
                Funded by: FundRef http://dx.doi.org/10.13039/100000104, National Aeronautics and Space Administration;
                Funded by: Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (4202)
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                © Springer Nature B.V. 2023

                exoplanets,venus
                exoplanets, venus

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