Search Publications

Atmospheric composition, chemistry, and clouds
DOI: 10.1029/176GM06 Bibcode: 2007GMS...176...73M

Esposito, Larry W.; Yung, Yuk L.; Mills, Franklin P.

Venus' atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hydrogen, and oxygen radicals. The chemical regimes in the atmosphere range from ion-neutral reactions in the ionosphere to photochemistry in the middle atmosphere to thermal equilibrium chemistry and surface-atmosphere reactions in the lower atmosphere…

2007 Geophysical Monograph Series
VenusExpress 58
Astrobiology and Venus exploration
DOI: 10.1029/176GM12 Bibcode: 2007GMS...176..191G

Bullock, Mark A.; Grinspoon, David H.

For hundreds of years prior to the space age, Venus was considered among the most likely homes for extraterrestrial life. Since planetary exploration began, Venus has not been considered a promising target for Astrobiological exploration. However, Venus should be central to such an exploration program for several reasons. At present Venus is the o…

2007 Geophysical Monograph Series
VenusExpress 38
Radiation in the atmosphere of Venus
DOI: 10.1029/176GM08 Bibcode: 2007GMS...176..121T

Bullock, Mark A.; Crisp, David; Taylor, Fredric W. +3 more

This chapter reviews the observations of the radiative fluxes inside and outside the Venusian atmosphere, along with the available data about the planetary energy balance and the distribution of sources and sinks of radiative energy. We also briefly address the role of the heat budget on the atmospheric temperature structure, global circulation, t…

2007 Geophysical Monograph Series
VenusExpress 34
Geochemistry of Venus' Surface: Current limitations as future opportunities
DOI: 10.1029/176GM03 Bibcode: 2007GMS...176....7T

Treiman, Allan H.

Geochemical data about Venus' surface materials are quite limited and of poor precision. The Venera and VEGA lander missions (sources of the available data) were engineering and scientific triumphs, but their chemical analyses of the Venus surface do not permit detailed confident interpretation, such as are routine for terrestrial analyses and MER…

2007 Geophysical Monograph Series
VenusExpress 28
Tectonic and thermal evolution of Venus and the role of volatiles: Implications for understanding the terrestrial planets
DOI: 10.1029/176GM05 Bibcode: 2007GMS...176...45S

Sotin, Christophe; Stofan, Ellen R.; Smrekar, Suzanne E. +5 more

Venus is similar to Earth in size and bulk composition. The dramatic differences between the two planets indicate that planetary size alone does not control geologic evolution. Earth's geology is dominated by plate tectonics, or active lid convection. The crater retention age of Venus demonstrates that the planet has been very geologically active …

2007 Geophysical Monograph Series
VenusExpress 13
Venus atmosphere dynamics: A continuing enigma
DOI: 10.1029/176GM07 Bibcode: 2007GMS...176..101S

Bougher, S. W.; Del Genio, A. D.; Limaye, S. S. +5 more

The dynamics of the Venus atmosphere presents a major unsolved problem in planetary science: the so-called superrotation of the lower atmosphere and its transition to a subsolar-to-antisolar circulation in the upper atmosphere. (In this paper we place the dividing line between the lower and upper atmosphere at 90-100 km altitude (pressure 0.39 to …

2007 Geophysical Monograph Series
VenusExpress 12
Surface evolution of Venus
DOI: 10.1029/176GM04 Bibcode: 2007GMS...176...23B

Basilevsky, Alexander T.; McGill, George E.

This chapter contains short descriptions of material units and structures observed on the surface of Venus as well as an abbreviated history of discoveries, that led to the current knowledge of this planet's geology. It is shown that observed units and structures are broadly similar and commonly exhibit similar age sequences in different regions o…

2007 Geophysical Monograph Series
VenusExpress 9
Venus upper atmosphere and plasma environment: Critical issues for future exploration
DOI: 10.1029/176GM09 Bibcode: 2007GMS...176..139R

Luhmann, J. G.; Russell, C. T.; Cravens, T. E. +2 more

This chapter briefly summarizes our state of knowledge about the upper atmosphere and plasma environment of Venus. This is followed by a discussion of some of the outstanding remaining issues in the field beginning with the Venus Express epoch and continuing to Planet C and beyond. We compare with other planets, especially Mars, and emphasize open…

2007 Geophysical Monograph Series
VenusExpress 7
Technology perspectives in the future exploration of Venus
DOI: 10.1029/176GM13 Bibcode: 2007GMS...176..207C

Cutts, James A.; Balint, Tibor S.; Chassefiere, Eric +1 more

Science goals to understand the origin, history and environment of Venus have been driving international space exploration missions for over 40 years. Today, Venus is still identified as a high priority science target in NASA's Solar System Exploration Roadmap, and clearly fits scientific objectives of ESA's Cosmic Vision Program in addition to th…

2007 Geophysical Monograph Series
VenusExpress 4
Experiencing Venus: Clues to the origin, evolution, and chemistry of terrestrial planets via in-situ exploration of our sister world
DOI: 10.1029/176GM11 Bibcode: 2007GMS...176..171B

Baines, Kevin H.; Crisp, David; Russell, Christopher T. +5 more

We review the current state of knowledge of (1) the origin and evolution of Venus and (2) the photochemical and thermochemical processes occurring in the middle and lower atmosphere there. For each, we review the promise of on-going and planned orbital observations by ESA's Venus Express and Japan's Venus Climate Orbiter missions. We review the ne…

2007 Geophysical Monograph Series
VenusExpress 2