The Voyagers' OdysseyBY STAMATIOS M. KRIMIGIS, ROBERT B. DECKER [NS]
THIS ARTICLE FROM ISSUE JULY-AUGUST 2015 VOLUME 103, NUMBER 4 PAGE 284 DOI: 10.1511/2015.115.284
A mission intended to last a mere four years has extended into a decades-long journey to interstellar space.
Both Voyager 1 and Voyager 2 flew by Saturn, in 1980 and 1981, respectively, returning unprecedented images of that planet before continuing farther into space. Voyager 1 became the first craft in interstellar space in 2012; Voyager 2 will soon follow. Image courtesy of NASA/JPL-Caltech.When the two Voyager spacecraft were launched in 1977, they followed a legacy of space exploration that was only two decades old, but which had accomplished much in that time. The first spacecraft to orbit Earth, Sputnik 1, was launched in 1957, and NASA’s Mariner 2 spacecraft passed Venus on December 14, 1962. Mariner 4, which swung by Mars on July 15, 1965—some 50 years ago—was the first to carry a camera. Pioneer 10 and 11’s flybys of Jupiter in the early 1970s, and Pioneer 11’s continuation to Saturn in 1979, gave a first glimpse of the complexity of these two planetary systems. The outer planets (Jupiter, Saturn, Uranus, and Neptune) as a group, however, remained basically unexplored until the two Voyager spacecraft arrived.
https://www.americanscientist.org/article/the-voyagers-odysseyVoyager 1 Nears Jupiter RendezvousBy John Noble Wilford Feb. 27, 1979
BEYOND the orbit of Mars and the asteroid belt, out where sunlight is diminished and the worlds are large and virtually unexplored, Voyager 1 is moving swiftly toward a rendezvous next Mon- day with Jupiter and several of the moons in its mighty embrace.
PASADENA, Calif.
After a journey of 18 months, the 1,800‐pound American spacecraft is more than 400 million miles from Earth and within five million miles of Jupiter. All is reported to be in readiness for the . most comprehensive close‐up ‘investigation ever undertaken of Jupiter, the solar system's largest planet, and its major Satellites, two of which are bigger than the planet Mercury.
Voyager is approaching the planet at a rate ofinore than 600,000 miles a day, gathering speed from the pull of Jovian gravity. This Is a powerful attraction, for Jupiter is big enough to contain 1,200 Earths and, although it is primarily a gaseous body, It has a mass 317.9 times that of Earth.
Spacecraft on Target
Voyager is on target, after a brief rocket maneuver last week “trimmed” its‐trajectory. The spacecraft crossed the orbit of Sinope, the most distant of Jupiter's 13 known moons, on Feb. 10 and will spend more than six weeks swinging through the Jovian system. Its course was selected carefully so that it could fly within safe distances of Jupiter and five Jovian moons — Amalthea, lo, Europa, Ganymede and Callisto — then be able to proceed on a 20month cruise to Saturn.
Despite some nagging malfunctions early in flight, Voyager is “working very normally,” according to Robert J. Parks, the project manager at the Jet Propulsion Laboratory here. The spacecraft is a large drum‐shaped structure dominated by a 12‐foot‐wide dish antenna and bristling with other antennas and booms carrying the scientific instruments and two slowscan television cameras. For nearly two months, Voyager has been studying the puzzling radio emissions from Jupiter and returning Increasingly spectacular photographs of the planet's multicolored bands of upper‐atmosphere clouds and the familiar Great Red Spot. Earlier this month, the photography began surpassing in resolution and clarity the pictures taken by Pioneers 10 and 11, which flew by Jupiter in 1973 and 1974. Voyager 1 will be observing Jupiter longer and in greater detail than the Pioneers did.
As the moment of closest encounter approaches, project scientists exude the excitement of anticipated discovery. Dr. Bradford A. Smith of the University of Arizona, the leader of the imaging science team, remarked that he had worked on many photographic missions to the planets but “to me, this is unquestionably the most exciting one of all.”
“We're extending our eyes into the outer solar system and into the unknown,” Dr. Smith said. “Not since Mariner 4 to Mars, some 15 years ago, have we been less prepared, less certain of what we expect to see. The next couple of weeks will be great.”
Early results, reported last week, suggest what is in store. Voyager cameras and other instruments have detected what appears to be a persistent jet stream of frozen ammonia moving at a speed of 350 miles an hour above the Jovian clouds. Hydrogen and helium are known to be the principal constituents of the planet.
Sequences of time‐lapse pictures disclose the curious phenomenon of dark orange “hot spots” traveling through the upper cloud layers. Sometimes, one spot overtakes another and seems to gobble it up; at other times two spots merge for as long as 12 days, then break apart.
Although the Great Red Spot has been observed through ground‐based telescopes for more than three centuries, Voyager photographs show that it undergoes striking changes. Dr. Smith said the color of the huge, hurriCane‐like feature seems to have faded, becoming more dark brown, since the Pioneer. pictures in 1974. There also appear to be “atmospheric currents swirling around it that weren't there before.”
“We have found,” Dr. Smith concluded, “that Jupiter is far more complex in atmospheric motions than we had ever imagined.”
Voyager is also beginning to return some distant photographs of the larger Jovian moons. Dark reddish polar re gions are visible on lo. Europa appears to be coated with ice. Bright equatorial areas are visible on Callisto's dark face.
During the encounter phase of the mission, Voyager will fly within 258,000 miles of Amalthea, the innermost moon, early on March 5. Then it will fly within 174,000 miles of Jupiter's southern hemisphere at 7:05 A.M. New York time on the same day. Its closest approach to a Jovian body will be at lo, 12,752 miles away. The spacecraft will swing within 71,500 miles of Ganymede, the largest moon, and 455,000 miles of Europa — both on March 5. Early the next day, it will fly within 78,359 miles of Callisto and then begin searching for any heretofore undiscovered Jovian moons. There has been a sighting from
Earth, as yet unconfirmed, of a 14th moon.
All of Voyager's scientific instruments have been turned on and are working. In addition to wide‐angle and narrow‐angle television cameras, Voyager carries a cosmic‐ray detector, an infrared interferometer‐spectrometer‐radiometer, a low‐energy chargedparticle detector, magnetometers, a photopolarimeter, a planetary radioastronomy instrument, plasma and plasma‐wave experiments and an ultraviolet spectrometer.
These instruments were selected and designed for three broad areas of study of Jupiter: atmospheric sciences, satellite observations and investigations of magnetic fields and the trapped radiation environment.
With the ultraviolet and infrared sensors, for example, project scientists expect to learn much about the composi tion, temperature and structure of Jupiter's turbulent atmosphere. This should give them answers to such questions as: Why are the bands of light zones and dark belts so well‐defined? What gives them their colors? What lies beneath the upper clouds?
The dynamics of the atmosphere will be studied through photography. Dr. Edward C. Stone, a physics professor at the California Institute of Technology and the project's chief scientist, said that the time‐lapse photography shows mass motions of the Jovian clouds and enables scientists to measure velocities of small features and flow patterns and perhaps to identify the physical processes that cause the multi‐colored belts, zones and spots.
“Up to now, we have been working with pictures that are like one frame out of a movie,” Dr. Stone explained. “Now we have a movie, if you will, and can see flow patterns.”
From the pictures already taken at a distance, Dr. Stone said, scientists are identifying regions of high interest “so we can zoom in on them during the close approach.” Close‐up shots of the Great Red Spot should produce pictures of sufficient detail that objects five miles across can be distinguished.
Voyager should return data on the temperatures, composition, surface texture and general nature of Jupiter's four major satellites. The two largest ones, Ganymede and Callisto, are thought to be almost entirely ice, although there is a hypothesis that they possess oceans of liquid water covered by a thick crust of ice. Voyager has already detected ice covering Europa, but no one knows the depth of the ice or much of anything else about the satellite.
“These are objects unlike anything we have photographed in a solar system before,” Dr. Stone remarked.
Voyager will be concentrating much of its attention on lo, the most puzzling of the satellites. The closest large one to Jupiter, lo is blanketed with salts of various kinds and may be pocked with fresh,lunar‐like craters. It is ringed by a cloud of sodium vapor, perhaps generated by intense radiation bombardment of the satellite's surface. Voyager's photopolarimeter will analyze the composition of the sodium cloud, as well as study the density of satellite atmospheres, if there are any, and determine the texture and composition of the satellites’ surfaces.
Flux Tube to Be Penetrated
As lo moves through Jupiter's strong magnetic field, it generates an electric current that flows along the magnetic field lines connecting the satellite and the planet. This cylindrical region .is called the “flux tube.” Voyager is aimed so that it can penetrate the flux tube for five minutes during the spacecraft's swing under Io's south pole.
Several days before the close encounter, Voyager will enter the general sphere of Jupiter's magnetic field. As Pioneer 10 discovered, Jupiter has a powerful magnetic field and is surrounded by radiation belts similar to the Van Allen belts around Earth, but thousands of times more intense. This vast, rapidly spinning region makes Jupiter a major source of several types of radiation.
One of the mission's objectives will be to get a better understanding of the size and shape and nature of Jupiter's magnetic field. From the results of the two Pioneer missions, scientists believe the size and shape of the magnetic field changes periodically.
Voyager 1 is the first of two identical spacecraft in the $400‐million project of exploration. Only four months behind is Voyager 2, bound for an encounter with Jupiter on July 9. It will also go to Saturn and may even continue on to Uranus, with the encounter there occurring in January 1986.
This is possible because of a rare alignment at this time of all the outer planets, enabling a carefully aimed spacecraft to use the gravitational force of one planet to give it a boost of energy and a change of course toward the next planet. This shortens the flight time to the far outer planets and brings them within the range of present spacecraft capabilities.
There is also a possibility, albeit remote, that Voyager 2 could be targeted at Uranus to proceed on to Neptune, arriving there in September 1989. If that should happen, it would mean that history could say of the first 32 years of the space age, from 1957 to 1989, that vehicles of human design completed the initial reconnaissance of all the planets of the solar system, save Pluto, and of many of the planets’ fascinating moons.
NASA
https://www.nytimes.com/1979/02/27/archives/voyager-1-nears-jupiter-rendezvous-voyager-1-nears-jupiter.htmlVoyager l Finds Stunning Variety on Jupiter's MoonsBy John Noble Wilford June 5, 1979
AFTER three months of examining the photographs and data from Voyager l's rendezvous with Jupiter, scientists have concluded that they have never seen anything in the solar system to compare to the four major Jovian moons —Io. Europa. Ganvmede and Callisto — each a distinct world and a source of continuing surprise.
Reflecting the excitement of such a discovery, the Voyager photographic interpretation team, led by Dr. Bradford A. Smith of the University of Arizona, reported in the June 1 issue of the journal Science:
“The bodies in the Jupiter system explored by Voyager 1 do not resemble closely either the planets in the inner solar system or one another. The wide range of unexpected findings is due both to the real differences between the outer and the inner solar system and to the depth of our prior ignorance. The sense of novelty would probably not have been greater had we explored a different solar system.”
Before Voyager 1 cruised through the environs of Jupiter last March, the four largest of the 13 known Jovian moons had been little more than vague points of light in the sky. Galileo discovered them in 1610, which is why they are called the Galilean satellites. Other astronomers plotted their orbits and determined that Ganymede and Callisto were each as big as the planet Mercury and that Io and Europa were about the size of Earth's moon. But the nature and appearance of the moons were beyond the resolving power of pre‐Voyager science.
The report in Science and discussions by planetary specialists at the spring meeting of the American Geophysical Union in Washington last week painted this picture of the moons of Jupiter:
IO‐When scientists thought about it at all, they speculated that Io, the innermost of the Galilean satellites, would be a cold, essentially dead world resembling Earth's moon. Instead, Voyager found Io to be a diverse, colorful world (bright orange‐red mottled by irregular patches of white), devoid of lunar‐like impact craters and alive with spewing volcanoes. Finding the first active volcanoes elsewhere in the solar system was Voyager's most surprising and spectacular discovery.
Further analysis in recent weeks has led geologists to identify eight erupting volcanoes on Io. Some of the eruptions, greenish in color, sent plumes of gases and other material more than 150 miles above the surface at velocities of as much as 1,200 miles an hour. For unknown reasons, the volcanoes are distributed around the equatorial region.
According to Dr. John C. Pearl of the Goddard Space Flight Center, reporting on Voyager's infrared measurements, Io's volcanoes seem to be cooler than had been expected. Most of Io's surface has temperatures of about 235 degrees below zero Fahrenheit. One of the volcanic plumes showed a temperature of about 80 degrees above zero. If the volcanoes were venting molten sulfur, as has been speculated, the ternperatures should have been about 230 degrees above zero.
The cause of Io's violent volcanoes has not been determined. But the report by Dr. Smith and his team said a “likely explanation” was tidal heating generated in Io's interior by the competing gravitational forces of Jupiter, in one direction, and Europa and Ganymede, in others.
In addition to the erupting volcanoes, Io photographs show signs of more than 100 huge depressions that resemble the craters, or calderas, of volcanoes on Earth and Mars. But in contrast to most terrestrial and Martian calderas, few of the ones on Io appear to be associated with high domes or other mountain structures. In fact, the only rugged mountains seen on Io thus far occur mainly in the polar regions.
Mother phenomenon found primarily in the polar regions is “blue snow,” the discovery of which was announced last week at the American Geophysical Union meeting. A recent re‐examination of Io photography disclosed 30 to 40 wisps of blue material, probably venting gases that condensed into snow,
EUROPA - Although Voyager 1 did not make a close approach to Europa, the cameras were able to see enough to show that it was a much different place than Io. The most distinctive features standing out in the moon's pale reflected light were long linear structures criss‐crossing the visible surface. Some are estimated to be more than 100 miles wide and 1,000 miles long. Geologists said the lines resemble faults and “are strongly suggestive” of globalscale processes that are moving and shaking Europa's crust.
Recent Earth‐based, near‐infrared observations indicate large amounts of water, probably in the form of ice, on the surface of Europa.
GANYMEDE - The largest of Jupiter's moons, Ganymede is also believed to be covered with water‐ice mixed with rock and, because of its low density compared to such rocky bodies as Earth, may be 50 percent water by weight.
Ganymede's surface, heavily marked with apparently ancient impact craters, bears some resemblance to Earth's moon. The photographs also show puzzling patterns of bright and dark grooves traversing the surface, suggesting some crustal movements on Ganymede, too.
But “a striking fact” about Ganymede, according to the report in Science, is the absence of major relief.
CALLISTO - The most impressive feature on Callisto is an enormous multi‐ring meteorite Impact basin with a central, circular patch of light-colored material about 180 miles wide. Radiating out from it are at least 8 to 10 bright discontinuous ridges more or less equally spaced, extending out about 850 miles.
“The flatness and unusual ring spacing,” the report in Science said, “are presumably due to the difference in material properties between an icerich crust and the silicate crusts of the moon and Mercury. Viscous flow during or subsequent to the impact event probably reduced the topographic relief.”
In early July, scientists expect to reap a new harvest of information about Jupiter and its moons. Voyager 2, an identical spacecraft, will fly by the moons on July 9 in such a way as to obtain high‐resolution photographs of the hemispheres not surveyed by Voyager 1.B.J. Poricbon
https://www.nytimes.com/1979/06/05/archives/voyager-1-finds-stunning-variety-on-jupiters-moons.htmlNASA’s Voyager Will Do More Science With New Power StrategyApril 26, 2023
(...) With those options now exhausted on Voyager 2, one of the spacecraft’s five science instruments was next on their list. (Voyager 1 is operating one less science instrument than its twin because an instrument failed early in the mission. As a result, the decision about whether to turn off an instrument on Voyager 1 won’t come until sometime next year.)
In search of a way to avoid shutting down a Voyager 2 science instrument, the team took a closer look at a safety mechanism designed to protect the instruments in case the spacecraft’s voltage – the flow of electricity – changes significantly. Because a fluctuation in voltage could damage the instruments, Voyager is equipped with a voltage regulator that triggers a backup circuit in such an event. The circuit can access a small amount of power from the RTG that’s set aside for this purpose. Instead of reserving that power, the mission will now be using it to keep the science instruments operating. (...)
https://www.jpl.nasa.gov/news/nasas-voyager-will-do-more-science-with-new-power-strategy