Mariner Mission to VenusJet Propulsion Laboratory (U.S.)
Science
Mariner Mission to Venus
Jet Propulsion Laboratory (U.S.)
Project Mariner (U.S.)
At 11:59 a.m., PST, on December 14, 1962, Mariner’s radiometers began to
scan the planet Venus in a nodding motion at a rate of 0.1 degree per
second and reaching an angular sweep of nominally 120 degrees. The
radiometers had been switched on 6½ hours before the encounter with
Venus and they continued to operate for another hour afterward.
The microwave radiometer looked at Venus at a wavelength of 13.5
millimeters and 19 millimeters. The 13.5-millimeter region was the
location of a microwave water absorption band within the electromagnetic
spectrum, but it was not anticipated that it would detect any water
vapor on Venus. These measurements would allow determination of
atmospheric radiation, averaging the hot temperatures near the surface,
the warmer clouds at lower levels, and the lower temperatures found in
the high atmosphere. If the atmosphere were a strong absorber of
microwave energy at 13.5 millimeters, only the temperature of the upper
layers would be reported.
Unaffected by water vapor, 19-millimeter radiations could be detected
from deeper down into the cloud cover, perhaps from near or at the
planet’s surface. Large temperature differences between the 19- and 13.5
millimeter readings would indicate the relative amount of water vapor
present in the atmosphere. The 19-millimeter radiations would also test
the limb-brightening theory.
During its scanning operation, Mariner telemetered back to Earth about
18 digital data points, represented as voltage fluctuations in relation
to time. The first scan was on the dark side, going up on the planet:
the distance from the surface was 16,479 miles at midscan, and the
brightness temperature was 369 degrees F. The second scan nearly
paralleled the terminator (junction of light and dark sides) but crossed
it going down; it was made from 14,957 miles at midscan and showed a
temperature of 566 degrees F. The final scan, 13,776 miles at midpoint,
showed 261 degrees F as it swept across the sunlit side of Venus in an
upward direction.
The brightness temperature recorded by Mariner’s radiometer is not the
true temperature of the surface. It is derived from the amount of light
or radio energy reflected or emitted by an object. If the object is not
a perfect light emitter, as most are not, then the light and radio
energy will be some fraction of that returned from a 100% efficient
body, and the object is really hotter than the brightness measurement
shows. Thus, the brightness temperature is a minimum reading and in this
case, was lower than the actual surface temperature.
Mariner’s microwave radiometer showed no significant difference between
the light and dark sides of Venus and, importantly, higher temperatures
along the terminator or night-and-day line of the planet. These results
would indicate no ionosphere supercharged with electrons, but a definite
limb-darkening effect, since the edges were cooler than the center of
the planet.
Public-domain text, read in full here on John Shaqi.
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