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About the project Overall mission Voyager Spacecraft Navigation Science The future |
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on a per-capita basis, this is only 20 cents per U.S. resident per year, or
roughly half the cost of one candy bar each year since project inception.
the daily interest on the U.S. national debt is a major fraction of the entire
cost of Voyager.
A total of five trillion bits of scientific data will have been returned to Earth by both Voyager spacecraft at the completion of the Neptune encounter. This represents enough bits to encode over 6000 complete sets of the Encyclopedia Brittanica, and is equivalent to about 1000 bits of information provided to each person on Earth.
The sensitivity of our deep-space tracking antennas located around the world is truly amazing. The antennas must capture Voyager information from a signal so weak that the power striking the antenna is only 10-16 watts (1 part in 10 quadrillion). A modern-day electronic digital watch operates at a power level 20 billion times greater than this feeble level.
Both Voyagers were specifically designed and protected to withstand the large
radiation dosage during the Jupiter swing-by. This was accomplished by
selecting radiation-hardened parts and by shielding very sensitive parts.
An unprotected human passenger riding aboard Voyager 1 during its Jupiter
encounter would have received a radiation dose equal to one thousand times
the lethal level.
The Voyager spacecraft can point its scientific instruments on the scan
platform to an accuracy of better than one-tenth of a degree. This is
comparable to bowling strike-after-strike ad infinitum, assuming that you must
hit within one inch of the strike pocket every time. Such precision is ecessary
to properly center the narrow-angle picture whose square field-of-view would
be equivalent to the width of a bowling pin.
To avoid smearing in Voyager's television pictures, spacecraft angular rates
must be extremely small to hold the cameras as steady as possible during the
exposure time. Each spacecraft is so steady that angular rates are typically
15 times slower than the motion of a clock's hour hand. But even this will not
be quite steady enough at Neptune, where light levels are 900 times fainter
than those on Earth. Spacecraft engineers have already devised ways to make
Voyager 30 times steadier than the hour hand on a clock.
The electronics and heaters aboard each nearly one-ton Voyager spacecraft can
operate on only 400 watts of power, or roughly one-fourth that used by an
average residential home in the western United States.
A set of small thrusters provides Voyager with the capability for attitude
control and trajectory correction. Each of these tiny assemblies has a thrust
of only three ounces. In the absence of friction, on a level road, it would
take nearly six hours to accelerate a large car up to a speed of 48 km/h using
one of the thrusters.
The Voyager scan platform can be moved about two axes of rotation.
A thumb-sized motor in the gear train drive assembly (which turns 9000
revolutions for each single revolution of the scan platform) will have rotated
five million revolutions from launch through the Neptune encounter. This is
equivalent to the number of automobile crankshaft revolutions during a trip of
2725 km (1700 mi).
The Voyager gyroscopes can detect spacecraft angular motion as little as one
ten-thousandth of a degree. The Sun's apparent motion in our sky moves over
40 times that amount in just one second.
The tape recorder aboard each Voyager has been designed to record and playback
a great deal of scientific data. The tape head should not begin to wear out
until the tape has been moved back and forth through a distance comparable to
that across the United States. Imagine playing a two-hour video cassette on
your home VCR once a day for the next 22 years, without a failure.
The Voyager magnetometers are mounted on a frail, spindly, fiberglass boom
that was unfurled from a two-foot-long can shortly after the spacecraft left
Earth. After the boom telescoped and rotated out of the can to an extension of
nearly 13 meters, the orientations of the magnetometer sensors were controlled
to an accuracy better than two degrees.
Voyager's fuel efficiency (in terms of mpg) is quite impressive.
Even though most of the launch vehicle's 700 ton weight is due
to rocket fuel, Voyager 2's great travel distance of 7.1 billion
km (4.4 billion mi) from launch to Neptune results in a fuel economy
of about 13,000 km per liter (30,000 mi per gallon). As Voyager
2 streaks by Neptune and coasts out of the solar system, this
economy will get better and better!
See "places visited" for information about what the Voyager`s has visited
Barring any serious spacecraft subsystem failures, the Voyagers may survive until the early twenty-first century, when diminishing power and hydrazine levels will prevent further operation. Were it not for these dwindling consumables and the possibility of losing lock on the faint Sun, our tracking antennas could continue to talk with the Voyagers for another century or two, or maby we can!

Each Voyager is equipped with computer programming
for autonomous fault protection. The Voyager system is one of the most
sophisticated ever designed for a deep-space probe. There are seven top-level
fault protection routines, each capable of covering a multitude of possible
failures.
The spacecraft can place itself in a safe state in a matter of only seconds or
minutes, an ability that is critical for its survival when round-trip
communication times for Earth stretch to several hours as the spacecraft
journeys to the remote outer solar system.
The resolution of the Voyager narrow-angle television cameras
is sharp enough to read a newspaper headline at a distance of
1 km (0.62 mi).
The solar system does not end at the orbit of Pluto, the ninth
planet. Nor does it end at the heliopause boundary, where the
solar wind can no longer continue to expand outward against the
interstellar wind. It extends over a thousand times farther out
where a swarm of small cometary nuclei, termed Oort's Cloud, is
barely held in orbit by the Sun's gravity, feeble at such a great
distance. Voyager 1 passed above the orbit of Pluto in May 1988,
and Voyager 2 passed beneath Pluto's orbit in august 1990.
But even at speeds of over 35,000 mph, it will take nearly 20,000
years for the Voyagers to reach the middle of the comet swarm,
and possibly twice this long for them to pass the outer boundaries
of cometary space. By this time, they will have traveled a distance
of two light-years, equivalent to half of the distance to Proxima
Centauri, the nearest star.Module
Mass
(Kg)
Usable propellant mass
Computer memory
limit
Instrument payload
Payload mass
Electric power
Voyager
?Kg
?Kg
1700 words
10 instruments
?Kg
3 RTGs