Download The Grand Tour of Voyager An historic event occurred on August 25

The Grand Tour of Voyager
An historic event occurred on August 25, 2012, and no one was aware of what had even
happened. As Voyager 1 slipped out of the Sun’s sphere of influence and into interstellar space,
even the researchers studying data the probe was sending back to Earth were unsure a
momentous event had occurred: The Dawn of the Interstellar Age. Not until April of 2013 would
researchers at the Jet Propulsion Laboratory (JPL) in Pasadena, California prove that their
longest working probe had finally left the Sun’s harbor. The probes are now venturing into deep
space, opening yet another chapter in the decades spanning Voyager Mission. Launched in 1977,
the Voyager 1 and Voyager 2 space probes are the longest serving machines operated by NASA.
Through these machines humanity was able to truly see the outer solar system for the first time
and discover more than we ever dreamed we would. The Voyager flybys provided humanity with
most of the information we know now about the outer solar system. The Voyager Mission laid
the foundation of our knowledge about the Gas Giants, their moons, and interstellar space.
The “Grand Tour”, as the Voyager Mission became known, began in the mid-1960s as a
theorized trajectory path created by graduate student Gary Flandro. “I was looking for ways to
reach the outer solar system efficiently, making practical missions possible.” (Swift) Flandro was
exploring the possibility of gravity assisted flight paths into the outer solar system at the request
of his supervisor. Flandro quickly discovered in his research that all four of the outer planets
would be in a rare alignment in the late 1970s that favored gravity assisted trajectories. The next
occurrence of this alignment wouldn’t happen for another 175 years. After sharing his results
with his superiors, everyone was in agreement that a well-timed opportunity had been presented
to them. The benefits of gravity assist, when a probe uses the gravity of a large celestial body
such as a moon or planet to accelerate, was too much to overlook. By using gravity assist,
spacecraft could reach the outer limits of the solar system years before fuel propulsion
spacecraft. After quickly putting together a plan, the prospect was presented to the upper
echelons in NASA as well as congress.
The initial plan was gigantic in scope. Four probes would be sent, each equipped with
cutting edge technology that generated an expected cost much larger than the government was
willing to pay. The plan wasn’t shot down, however. As mission manager Harris Schurmeier
recalls, “They told us, ‘If you guys can come up with something less grandiose, we’ll consider
it.’” (Bell). After a revision, they had dropped the expected $900 million cost by more than two
thirds, to $250 million. For NASA, having a plan that saved money was critical to getting
ambitious, large-scale projects like Voyager through congress. (Butrica) This new plan was
approved.
Officially known as Mariner Jupiter Saturn ’77 (MSJ-77), the new project had been
drastically scaled back. Only two probes would be built, with substantially fewer instruments
than their first conceptualizations. Jupiter and Saturn remained the targets of observation for the
flybys, but Uranus and Neptune had to be left out, cutting the Grand Tour into “a less ambitious
mission, a mini-Grand Tour.” (Lakdawalla) The planners of the project weren’t completely
crestfallen about the loss in scope. Because of newly emerging technology, researchers would be
able to send commands to the probes to extend the mission if possible, brilliant foresight that
allowed Voyager 2 to continue to Uranus and Neptune, and to allow both probes to continue
functioning as they traveled towards interstellar space.
Voyager 2 was launched first, on August 20, 1977, followed by Voyager 1 on September
5, due to the different trajectories each probe was planned to undertake. By the time the probes
had passed the asteroid belt, Voyager 1 had achieved a lead over its twin, and has remained
further away from Earth ever since.
Traveling close to 35,000 miles an hour, Voyager 1 descended upon the Jovian system on
March 5, 1979. Scientists from around the world gathered at JPL to watch this momentous
occasion in person and became ecstatic as high resolution photos began to trickle in. Pictures of
distant Io started to raise questions. What were the colored splotches on its surface? The
questions quickly turned to panic as incoming photos became terribly smeared, making them
worthless.
A behemoth, Jupiter contains more mass than every other object in the solar system
combined, excluding the Sun. Because of its size, Jupiter emits harsh radiation that can affect the
computer components of the probes sent to it. As Voyager 1 approached, this intense field of
radiation was able to bypass the probe’s shielding, slightly altering the clocks between the
camera and the main computer, putting them out of sync. The computer began moving the
camera before it had closed its shutter, ruining pictures that scientists and researchers had been
waiting years to see. The problem was discovered quickly, and the probe was able to resume its
mission before leaving Jupiter and its moons behind.
The first moon to fall under scrutiny was Io. Craterless, covered in a palette of orange,
white, black, and red, the mystery of this tidally abused moon was answered by accident when
Voyager 1 had already passed by and had taken photos for navigation, not discovery. After
changing the color saturation of the navigation photos at a lab back on Earth to view the dim
stars past the moon to determine the probe’s position along its trajectory, Linda Morabito saw a
strange crescent off Io’s surface. When Morabito showed her finding to the leaders of the project
and explained that they were looking at plumes of material ejecting from the surface of Io, the
other scientists were skeptical. Additional data proved conclusive, and Io became the most
geologically active body in the solar system, surpassing Earth. Vicious tidal forces from Jupiter
and moons Europa and Ganymede place Io under immense stress, creating volcanism not seen
anywhere else in the solar system. These same tidal forces affect Europa, cracking its icy surface
to allow slushy water to seep over the surface, erasing craters and mountains and valleys,
creating a surprisingly fresh and young surface.
The Jovian system proved to be very interesting for the Voyager team as they discovered
the unexpected personalities and vastly different characteristics of each moon. Before the flybys,
it was widely believed that all moons in the solar system would be much like Earth’s; an ancient,
cratered rock with no atmosphere and no significant mysteries. Io shattered that perspective, and
Europa cemented the idea that many things in the outer solar system could not be predicted
accurately; humanity simply did not know enough about these distant worlds. Even Ganymede
and Callisto, appearing more like how a moon was thought to be, harbor evidence of
subterranean oceans.
The bar had been set for Voyager as it picked up speed from Jupiter’s massive gravity,
and eyes turned towards Saturn. On November 12, 1980, Voyager 1 descended upon the ringed
planet with a very specific goal that needed to be accomplished: the planet’s largest moon, Titan,
needed to be accurately photographed and measured. If the probe failed to obtain enough data,
Voyager 2’s trajectory would be altered to finish the measurements. The spacecraft would lose
the window needed to make it to Uranus and Neptune, effectively ending the Grand Tour.
Obtaining information on Titan was so crucial to the Voyager team at JPL they were prepared to
lose the rest of the Solar System.
Voyager 1 did not disappoint. A world larger than Mercury, Titan surprised the
researchers back on Earth with an atmosphere of methane and ethane almost 50% thicker than
Earth’s. Orange clouds covered the surface, making it impossible for the probes to snap pictures
of the surface, likely to have rivers, lakes, and oceans of liquid methane because of Titan’s frigid
temperatures that are only ninety degrees above absolute zero. After measuring the solar
system’s second largest moon, Voyager 1 continued through Saturn’s miniature solar system,
collecting readings on Saturn itself, with wind and storm belts raging across its atmosphere, and
shocking scientists and mathematicians with braided rings.
Having gathered enough information successfully during the short flyby, Voyager 1
opened the path for its twin to continue to Uranus, a planet completely unknown to astronomers.
The probe’s own Grand Tour was over, however. While possible for Voyager 1 to intercept Pluto
at one point, Titan had been deemed too important to observe at a distance. After the flyby of
Saturn, the probe was launched upward (relative to the disk or plane of the solar system) at ten
miles per second. The only purpose for Voyager 1 now was to serve as a practice dummy for
critical fixes Voyager 2 might need and to measure space as it approached the end of the sun’s
sphere of influence.
The wait time between the Jupiter and Saturn encounters had only been a year and a half;
Uranus would be a much longer wait. Almost five years passed between Voyager 2’s August 26,
1981 flyby of Saturn and the January 24, 1986 passing of Uranus. This giant planet proved no
less interesting than the two that proceeded it.
The turquoise planet is unique almost immediately: it rolls as it orbits the sun instead of
spinning. Many researchers were curious to see how this affected the magnetosphere the planet
emits. Observers were surprised to find, as Voyager 2’s magnetometer began relaying
measurements, that the magnetic fields were oriented much like every other planets’ (those that
do have them) magnetosphere. What was surprising about Uranus’ - and later Neptune’s –
magnetic field is that it isn’t generated by the core of the planet, but is instead off center. The
reason why wouldn’t be discovered until after Neptune was visited, but suspicions began to arise
that Uranus was a different class of planet than the gas giants of Jupiter and Saturn.
The Uranian moons continued the trend of providing new and unexpected characteristics
not thought to belong to satellites of massive planets. Hints of cryovolcanism, where liquid water
is magma instead of rock, appeared on Ariel, suggesting a geological past. Umbriel showed off a
very dark surface, perplexing researchers to this day. However, little Miranda, only 300 miles
across, stole the show. A world too small to have believed it had any geological past, Miranda
looks like chunks of different terrain all mashed together like patchwork. From flat vistas to
jagged terrain, the small moon has the most diverse set of geological features out of the Uranian
moons. Some of Miranda’s cliffs are more than ten miles high.
Spending less than a day with Uranus, Voyager 2 continued onward. The exciting new
information was quietly released several months later to the public, however. Four days after
Earth’s only visit to this distant planet, the space shuttle Challenger exploded, killing everyone
on board, placing space exploration under scrutiny. The go ahead was given for a flyby of
Neptune, however, and the next long wait began.
Voyager 2 completed its Grand Tour of the outer planets on August 25, 1989. The giant
azure planet confirmed what had been discovered at Uranus. These massive, gaseous planets had
a magnetosphere that was generated in the mantle of the planet, not the core. A new
classification of planet was created: the ice giant. Unlike Uranus, the atmosphere of Neptune was
chaotic, with dark storms racing across the surface, white clouds trailing at some of the fastest
speeds recorded in the solar system, with winds up to 1,300 miles per hour. Because of the
immense contrast between stormy Neptune and bland Uranus, it is widely believed the timing of
the Uranus flyby was during a lull in the weather patterns, when no storms were forming.
Neptune’s large moon Triton would be Voyager 2’s last object of observation. This moon
is unique even among such bizarre worlds as Io and Miranda: it orbits its planet opposite of
every other moon in the solar system. The leading theory for this is that Triton was actually
captured by the large planet, and has been stuck in Neptune’s grasp ever since. The moon proved
its uniqueness in more than one way; visually, it looks much like a cantaloupe, suggesting an
active geological past. As Voyager 2 sped away, in the last pictures taken of the moon, a very
thin atmosphere was discovered. In that atmosphere active geysers were found. One of the
coldest places in the solar system was spewing nitrogen gas out of the crust miles into the
atmosphere.
The Grand Tour was now complete. All that remained was the interstellar mission, to find
the true edge of the solar system, where the photons and plasma ejected from the sun lose their
strength and give way to the cosmic rays of interstellar space. Voyager 1 is believed to have
entered interstellar space on August 25, 2012. Unfortunately, an instrument that measures the
plasma around the probe was damaged during the flyby of Saturn, and so proof of the probe’s
interstellar status is not definitive, and has been met with criticism. While the current Voyager
team believes that humanity is now in interstellar space, they are waiting for Voyager 2 to
confirm the data, as the instruments on the spacecraft are working fine. Data is expected from
Voyager 2 any year now to verify the interstellar boundary, to once and for all proclaim
humanity as an interstellar species.
Before the probes had even begun construction, engineers were skeptical that spacecraft
capable of lasting longer than two years could be built. Thirty-nine years later, Voyager 1 and 2
are still sending signals back to Earth, letting us know that they are still determined to find new
discoveries. Without the spectacular journey these probes underwent, it would have been many
years before we discovered the extreme volcanism of Io. Saturn’s rings would’ve been counted
decades later. The ice giant classification of planet would still be unknown, as no manmade
spacecraft has been sent to Uranus and Neptune since Voyager. Mesmerizing photos of colorful
vistas, swirling cloud tops, and pale blue dots would never have been taken to capture the
imagination and drive the inspiration of many of today’s scientists and future scientists. Voyager
is one of the grandest projects attempted by mankind, accumulating over 11,000 years of work
time. (NASA) The information and photos sent back to Earth have been seen by millions of
people, if not billions. Earth isn’t the only planet these two probes might share information with,
either. On each probe is a golden record, containing songs, photos, and information about a
young species just beginning to explore space. The final mission of Voyager, after the power
supply is long dead, is to bear this message to the universe: we were here.
Works Cited
Bell, Jim. The Interstellar Age. New York City: Dutton, 2015. Print.
Butrica, Andrew J. From Engineering Science to Big Science. 22 March 2007.
http://www.history.nasa.gov/SP-4219/Chapter11.html. 2 October 2016.
Lakdawalla, Emily. "Historical PDF: "The Voyager Flights to Jupiter and Saturn" The Planetary
Society Blog. The Planetary Society, 20 Apr. 2011. Web. 26 Sept. 2016.
<http://www.planetary.org/blogs/emily-lakdawalla/2011/3007.html>.
"NASA Spacecraft Embarks on Historic Journey Into Interstellar Space." NASA. NASA, 12
Sept.
2013. Web. 25 Sept. 2016. <http://www.jpl.nasa.gov/news/news.php?release=2013277>.
Swift, David W. Voyager Tales: Personal Views of the Grand Tour. Reston: American Institute
of
Aeronautics and Astronautics, 1997.