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Venus, the Planet : Introduction to the Evolution of Earth's Sister Planet

O'Rourke, Joseph G. (författare)
Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85281 USA.
Wilson, Colin F. (författare)
Univ Oxford, Dept Phys, Oxford, England.;ESA, ESTEC, Noordwijk, Netherlands.
Borrelli, Madison E. (författare)
Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85281 USA.
visa fler...
Byrne, Paul K. (författare)
Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA.
Dumoulin, Caroline (författare)
Univ Angers, Nantes Univ, Lab Planetol & Geosci UMR6112, CNRS, Nantes, France.
Ghail, Richard (författare)
Royal Holloway Univ London, Earth Sci, Egham, Surrey, England.
Gülcher, Anna J. P. (författare)
Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85281 USA.;Swiss Fed Inst Technol, Inst Geophys, Dept Earth Sci, Zurich, Switzerland.
Jacobson, Seth A. (författare)
Michigan State Univ, Dept Earth & Environm Sci, E Lansing, MI 48824 USA.
Korablev, Oleg (författare)
Space Res Inst RAS IKI, Profsoyuznaya 84-32, Moscow 117997, Russia.
Spohn, Tilman (författare)
Int Space Sci Inst, Bern, Switzerland.;DLR Inst Planetary Res, Berlin, Germany.
Way, Michael J. (författare)
Uppsala universitet,Teoretisk astrofysik,NASA, Goddard Inst Space Studies, 2880 Broadway, New York, NY 10025 USA
Weller, Matt (författare)
Brown Univ, Dept Earth Environm & Planetary Sci, Providence, RI 02912 USA.;USRA, Lunar & Planetary Inst, Houston, TX USA.
Westall, Frances (författare)
CNRS, Ctr Biophys Mol, Orleans, France.
visa färre...
Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85281 USA Univ Oxford, Dept Phys, Oxford, England.;ESA, ESTEC, Noordwijk, Netherlands. (creator_code:org_t)
2023-02-06
2023
Engelska.
Ingår i: Space Science Reviews. - : Springer. - 0038-6308 .- 1572-9672. ; 219:1
  • Forskningsöversikt (refereegranskat)
Abstract Ämnesord
Stäng  
  • Venus is the planet in the Solar System most similar to Earth in terms of size and (probably) bulk composition. Until the mid-20th century, scientists thought that Venus was a verdant world-inspiring science-fictional stories of heroes battling megafauna in sprawling jungles. At the start of the Space Age, people learned that Venus actually has a hellish surface, baked by the greenhouse effect under a thick, CO2-rich atmosphere. In popular culture, Venus was demoted from a jungly playground to (at best) a metaphor for the redemptive potential of extreme adversity. However, whether Venus was much different in the past than it is today remains unknown. In this review, we show how now-popular models for the evolution of Venus mirror how the scientific understanding of modern Venus has changed over time. Billions of years ago, Venus could have had a clement surface with water oceans. Venus perhaps then underwent at least one dramatic transition in atmospheric, surface, and interior conditions before present day. This review kicks off a topical collection about all aspects of Venus's evolution and how understanding Venus can teach us about other planets, including exoplanets. Here we provide the general background and motivation required to delve into the other manuscripts in this collection. Finally, we discuss how our ignorance about the evolution of Venus motivated the prioritization of new spacecraft missions that will rediscover Earth's nearest planetary neighbor-beginning a new age of Venus exploration.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

Venus
Planetary probes
Planetary climates
Planetary structure
Planetary dynamics
Planetary system formation

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