Mariner Mission to VenusJet Propulsion Laboratory (U.S.)
Science
Mariner Mission to Venus
Jet Propulsion Laboratory (U.S.)
Project Mariner (U.S.)
On its 109th day of travel, Mariner had approached Venus in a precarious
condition. Seven of the over-heated temperature sensors had reached
their upper telemetry limits. The Earth-sensor brightness reading stood
at 3 (0 was the nominal threshold) and was dropping. Some 149 watts of
power were being consumed out of the 165 watts still available from the
crippled solar panels.
At JPL’s Space Flight Operations Center, there was reason to believe
that the ailing CC&S might not command the spacecraft into its encounter
sequence at the proper time. Twelve hours before encounter, these fears
were verified.
Quickly, the emergency Earth-originated command was prepared for
transmission. At 5:35 a.m., PST, a radio signal went out from
Goldstone’s Echo Station. Thirty-six million miles away, Mariner II
responded to the tiny pulse of energy from the Earth and began its
encounter sequence.
After Mariner had “acknowledged” receipt of the command from the Earth,
the spacecraft switched into the encounter sequence as engineering data
were turned off and the radiometers began their scanning motion, taking
up-and-down readings across the face of the planet. As throughout the
long cruise, the four experiments monitoring the magnetic fields, cosmic
dust, charged particles, and solar plasma experiments continued to
operate.
[Illustration: _Mariner II approached Venus from the dark side,
crossed between the planet and the Sun while making three radiometer
scans of the disk._]
As Mariner approached Venus on its night side, it was travelling about
88,400 miles per hour with respect to the Sun. At the point of closest
approach, at 11:59.28 a.m., PST, the distance from the planet was 21,598
miles.
During encounter with Venus, three scans were made: one on the dark
side, one across the terminator dividing dark and sunlit sides, and one
on the sunlit side. Although the scan went slightly beyond the edge of
the planet, the operation proceeded smoothly and good data were received
on the Earth.
With encounter completed, the cruise condition was reestablished by
radio command from the Earth and the spacecraft returned to transmitting
engineering data, together with the continuing readings of the four
cruise scientific experiments.
After approaching closer to a planet and making more meaningful
scientific measurements than any man-made space probe, Mariner II
continued on into an orbit around the Sun.
December 27, 13 days after Venus encounter, marked the perihelion, or
point of Mariner’s closest approach to the Sun: 65,505,935 miles. The
Sun-related speed was 89,442 miles per hour. As Mariner began to pull
away from the Sun in the following months, its Sun-referenced speed
would decrease.
Public-domain text, read in full here on John Shaqi.
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