Elucidating the rate of volcanism on venus: Detection of lava eruptions using near-infrared observations

Joji Hashimoto, Takeshi Imamura

Research output: Contribution to journalArticle

29 Citations (Scopus)

Abstract

Lava eruptions can be observed remotely on Venus' nightside using a near-infrared window at a 1.0-micrometer wavelength, i.e., radiation at this wavelength emitted from the planetary surface traverses through the thick Venus atmosphere and clouds. Due to the strong dependence of the intensity of thermal emission on temperature, a hot surface produced by a lava eruption emits intense radiation, with the intensity of the excess radiation depending on the surface area and temperature of the lava flow. The excess emission from the hot surface is blurred by clouds, yet a 1-km2 1500-K basaltic lava lake and a 50-km2 1000-K lava flow are readily detected using this technique. Rapid cooling of exposed lava results in excess surface radiation that is detectable for just one Earth day after the end of an eruption; hence short-term eruptions are only detectable on the side of the planet where night is occurring. Eruptions lasting more than half a Venus day (i.e., more than about 60 Earth days), however, are detectable across the globe as nighttime occurs sometime during this period for every such event. Due to limited observational geometries, a complete global survey of active volcanos cannot be achieved from Earth, and in fact, only about 10% of short-lived major volcanic eruptions are observable. Alternatively, a satellite orbiting high above Venus (∼6 Venus radii) could detect virtually all short-lived nighttime volcanic events, or about half the events expected to occur across the globe.

Original languageEnglish
Pages (from-to)239-243
Number of pages5
JournalIcarus
Volume154
Issue number2
DOIs
Publication statusPublished - 2001
Externally publishedYes

Fingerprint

Venus (planet)
lava
Venus
volcanic eruptions
volcanism
near infrared
volcanic eruption
hot surfaces
globes
radiation
lava flow
Venus clouds
Venus atmosphere
infrared windows
wavelength
planetary surfaces
planetary surface
thermal emission
lakes
wavelengths

Keywords

  • Geological processes
  • Radiative transfer
  • Venus
  • Venus, surface
  • Volcanism

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Elucidating the rate of volcanism on venus : Detection of lava eruptions using near-infrared observations. / Hashimoto, Joji; Imamura, Takeshi.

In: Icarus, Vol. 154, No. 2, 2001, p. 239-243.

Research output: Contribution to journalArticle

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