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

Exoplanets Venus

Journal

Space science reviews
ISSN: 0038-6308
Titre abrégé: Space Sci Rev
Pays: Netherlands
ID NLM: 100971458

Informations de publication

Date de publication:
2023
Historique:
received: 13 04 2022
accepted: 11 01 2023
entrez: 14 2 2023
pubmed: 15 2 2023
medline: 15 2 2023
Statut: ppublish

Résumé

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.

Identifiants

pubmed: 36785654
doi: 10.1007/s11214-023-00953-3
pii: 953
pmc: PMC9911515
doi:

Types de publication

Journal Article Review

Langues

eng

Pagination

13

Informations de copyright

© The Author(s) 2023.

Déclaration de conflit d'intérêts

Competing InterestsThe authors declare no competing interests.

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Auteurs

M J Way (MJ)

NASA Goddard Institute for Space Studies, 2880 Broadway, New York, NY 10025 USA.
Theoretical Astrophysics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.

Colby Ostberg (C)

Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521 USA.

Bradford J Foley (BJ)

Department of Geosciences, Pennsylvania State University, University Park, PA USA.

Cedric Gillmann (C)

Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, TX 77005 USA.

Dennis Höning (D)

Potsdam Institute for Climate Impact Research, Potsdam, Germany.
Department of Earth Sciences, Vrije Universiteit Amsterdam, Amsterdam, The Netherlands.

Helmut Lammer (H)

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, Austria.

Joseph O'Rourke (J)

School of Earth and Space Exploration, Arizona State University, Tempe, AZ USA.

Moa Persson (M)

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.

Ana-Catalina Plesa (AC)

Institute of Planetary Research, DLR, Berlin, Germany.

Arnaud Salvador (A)

Department of Astronomy and Planetary Science, Northern Arizona University, Box 6010, Flagstaff, AZ 86011 USA.
Habitability, Atmospheres, and Biosignatures Laboratory, University of Arizona, Tucson, AZ USA.
Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA.

Manuel Scherf (M)

Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, Austria.
Institute of Physics, University of Graz, Graz, Austria.
Institute for Geodesy, Technical University, Graz, Austria.

Matthew Weller (M)

Lunar and Planetary Institute, 3600 Bay Area Blvd., Houston, TX 77058 USA.

Classifications MeSH