Hot Venus

This false-color image is a near-infrared map of lower-levelclouds on

the night side of Venus, obtained by the Near InfraredMapping

Spectrometer (NIMS) aboard the Galileo spacecraft as itapproached the

planet's night side on February 10, 1990. Bright sliversof sunlit high clouds

are visible above and below the dark, glowing hemisphere.The spacecraft

is about 100,000 kilometers (60,000 miles) above the planet.An infrared

wavelength of 2.3 microns (about three times the longestwavelength

visible to the human eye) was used. The map shows the turbulent,cloudy

middle atmosphere some 50-55 kilometers (30-33 miles) abovethe surface,

10-16 kilometers or 6-10 miles below the visible cloudtops.The red

color represents the radiant heat from the lower atmosphere(about 400

degrees Fahrenheit) shining through the sulfuric acid clouds,which

appear as much as 10 times darker than the bright gapsbetween clouds.

This cloud layer is at about -30 degrees Fahrenheit, ata pressure about

1/2 Earths surface atmospheric pressure. Near the equator,the clouds

appear fluffy and blocky; farther north, they are stretchedout into

East-West filaments by winds estimated at more than 150mph, while the

poles are capped by thick clouds at this altitude.

 

This is the first image of a planet taken by NIMS duringits nine-year

mission. It is also the first near-infrared image everacquired of Venus from

a spacecraft, and reveals clouds details never seen before.orsince.

This is the only image ever taken which clearly shows theturbulent cloud

layer over the whole planet from pole to pole.

 

The Near Infrared Mapping Spectrometer (NIMS)on the Galileo

spacecraft is a combined mapping (imaging) and spectralinstrument. It can

sense 408 contiguous wavelengths from 0.7 microns (deepred) to 5.2 microns,

and can construct a map or image by mechanical scanning.It can

spectroscopically analyze atmospheres and surfaces andconstruct thermal and

chemical maps. Designed and operated by scientists andengineers at the Jet

Propulsion Laboratory, NIMS involves 15 scientists in theU.S., England, and

France. The Galileo Project is managed for NASA's Officeof Space Science and

Applications by JPL; its mission is to study the planetJupiter and its

satellites and magnetosphere after multiple gravity assistflybys at Venus and

the Earth.

Information provided to Chris Baines by Dr. Kevin Baines, Planetary Scientist,Jet Propulsion Laboratory, Pasadena, California.


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