Voyager 1 and 2 - UPDATE Narrated Documentary.

Carol Meier Narrator - revoeciov
14 Sept 201819:48

Summary

TLDRThe Voyager spacecrafts, launched in 1977, embarked on an ambitious mission to explore the outer planets during a rare alignment. Voyager 2, the only probe to visit Uranus and Neptune, and Voyager 1, the farthest human-made object, continue to send data from beyond the solar system. Equipped with scientific instruments, they have studied planets, moons, rings, and magnetic fields, and now venture into interstellar space, with their signals expected to fade by 2025.

Takeaways

  • 🚀 The Grand Tour was a proposed mission in the 1960s to take advantage of a rare planetary alignment for a comprehensive study of the outer planets.
  • 🛰️ The Voyager spacecrafts, launched in 1977, were designed to explore Jupiter, Saturn, Uranus, Neptune, and Pluto, using gravitational assists to extend their trajectories.
  • 🔭 Voyager 2 holds the record for visiting the most planets, having explored Jupiter, Saturn, Uranus, and Neptune, while Voyager 1 is the farthest human-made object from Earth.
  • 🌌 Both Voyagers have provided invaluable data on the outer planets, their moons, rings, and magnetic fields, contributing to our understanding of the solar system.
  • 🛠 Voyagers were remotely reprogrammed to enhance their capabilities beyond their initial design, showcasing adaptability in space exploration.
  • 🔋 The spacecrafts are powered by radioisotope thermoelectric generators (RTGs), which will eventually deplete, ceasing all operations around 2025-2027.
  • 📡 Communication with Voyagers is maintained through the Deep Space Network, which uses large antennas to send and receive signals that have significantly weakened by the time they reach Earth.
  • 🛂 The Voyagers carry scientific instruments that have been crucial for their exploration, with some still active, studying cosmic rays, plasma waves, and magnetic fields.
  • 🛑 Some instruments have been shut down to conserve power, and non-essential heaters have also been systematically turned off to extend the spacecrafts' operational life.
  • 🌐 Voyager 1's exit from the solar system was determined by measuring the change in plasma density and the shift in particle sources from solar wind to galactic wind.
  • 🌠 The Voyagers are destined to continue their journey through interstellar space, potentially outliving the solar system and carrying a message from humanity into the cosmos.

Q & A

  • What was the purpose of the Grand Tour proposed in the 1960s?

    -The Grand Tour was an ambitious plan to send unmanned probes to the outer planets of the solar system to study them, taking advantage of a rare alignment of the planets Jupiter, Saturn, Uranus, Neptune, and Pluto in the late 1970s.

  • Why were the Voyager spacecrafts launched in 1977?

    -The Voyager spacecrafts were launched in 1977 to take advantage of the rare planetary alignment that would not occur again for 176 years, allowing them to visit the outer planets using a gravitational slingshot effect.

  • What was the primary mission of the Voyager spacecrafts?

    -The primary mission of the Voyager spacecrafts was the exploration of Jupiter and Saturn, with the mission later being extended to include the exploration of Uranus and Neptune by Voyager 2.

  • How did the Voyager spacecrafts use Jupiter for their mission?

    -The Voyager spacecrafts used Jupiter as a gravitational slingshot to extend their trajectory to the other planets further out in the solar system.

  • Which Voyager spacecraft holds the record for visiting the most planets?

    -Voyager 2 holds the record for visiting the most planets, being the only spacecraft to have visited Uranus and Neptune.

  • What was the Voyager 1's speed when it became the most distant human-made object in outer space?

    -Voyager 1 was traveling at a speed of 39,000 miles per hour when it passed Pioneer 10 to become the most distant human-made object in outer space.

  • What is the Voyager Interstellar Mission?

    -The Voyager Interstellar Mission is the designation given to the Voyager project in January 1990, after the completion of their primary mission, focusing on exploring beyond the solar system.

  • How many instruments are still working on Voyager 1 and Voyager 2?

    -There are four instruments still working on Voyager 1 and five instruments still working on Voyager 2.

  • What is the purpose of the low energy charged particle detector on the Voyager spacecrafts?

    -The low energy charged particle detector measures the number of low-energy particles hitting the spacecraft and determines their speed, studying cosmic radiation and particles from the Sun, planets, and interstellar space.

  • How do the Voyager spacecrafts communicate with Earth?

    -The Voyager spacecrafts communicate with Earth via a 3.7-meter diameter high gain antenna, sending and receiving radio waves through the Deep Space Network stations on Earth.

  • What is the expected timeline for the Voyager spacecrafts to cease operations?

    -The Voyager spacecrafts are expected to cease operations around 2025 due to the decay of the radioactive Plutonium 238 that powers them, but with careful power management, they may function through 2027.

  • How do scientists determine that Voyager 1 has entered interstellar space?

    -Scientists determined that Voyager 1 entered interstellar space by measuring the density of plasma surrounding the spacecraft using sound wave information from solar flares, and observing changes in the abundance of particles from the Sun and interstellar space.

  • What is the Voyager 1's expected encounter with a star in the future?

    -Voyager 1 is expected to encounter a star in 40,000 years when it flies about 1.7 light-years away from an obscure star in the constellation Camelopardalis called AC + 79 3888.

  • How long will it take for Voyager 1 to complete one orbit around the center of the Milky Way?

    -It will take Voyager 1 approximately 225 million years to complete one orbit around the center of the Milky Way.

Outlines

00:00

🚀 The Grand Tour and Voyager Missions

The script discusses the ambitious 'Grand Tour' space mission of the 1960s, aimed at exploring the outer planets during a rare alignment in the late 1970s. The Voyager 1 and 2 spacecrafts were launched in 1977 to leverage this alignment, using gravitational assists to visit Jupiter, Saturn, Uranus, and Neptune. The missions discovered 48 moons and studied planetary rings and magnetic fields. Voyager 1 holds the record for the farthest human-made object, while Voyager 2 is the only spacecraft to have visited Uranus and Neptune. The spacecrafts were equipped with various scientific instruments that are still active, contributing to our understanding of our solar system and interstellar space.

05:02

🛰️ Voyager Spacecraft's Instruments and Communication

This paragraph delves into the instruments aboard the Voyager spacecrafts, including the low energy charged particle detector, cosmic ray instrument, plasma wave subsystem, and magnetometers. These tools have been instrumental in studying solar wind, cosmic radiation, and the transition between interplanetary and interstellar media. The spacecrafts communicate with Earth via the Deep Space Network, using a high-gain antenna and radio waves. Despite their age, the Voyagers' signals are still strong enough to be detected, although the transmitter on Voyager 2 has been using a backup since 1978. The spacecrafts' power comes from radioisotope thermoelectric generators, which are expected to cease functioning around 2025.

10:02

🌌 Voyager 1's Entry into Interstellar Space

The script explains how scientists determined that Voyager 1 had entered interstellar space by measuring the density of plasma and the change in solar wind versus galactic wind. Despite the failure of Voyager 1's plasma detector in 1980, the analysis of sound wave information from solar flares allowed for the measurement of plasma density. This data, along with the increase in galactic cosmic rays and decrease in solar particles, confirmed Voyager 1's position in interstellar space. The spacecraft is now surrounded by cosmic rays from outside our solar system.

15:05

🌠 Voyagers' Journey Through the Milky Way

The final paragraph outlines the long-term trajectory of the Voyager spacecrafts as they continue their journey through the cosmos. It details the time it will take for each spacecraft to pass various celestial bodies, including the Oort cloud and nearby stars, and the estimated time for completing an orbit around the Milky Way's center. The paragraph also contemplates the ultimate fate of the Voyagers, which could include surviving a collision of galaxies and continuing their eternal journey through space, potentially outliving the solar system and the Milky Way itself.

Mindmap

Keywords

💡Voyager spacecrafts

The Voyager spacecrafts, Voyager 1 and Voyager 2, are the main subjects of the video. Launched in 1977, they were designed to take advantage of a rare planetary alignment to explore the outer planets of our solar system. These twin spacecrafts have since traveled beyond the solar system and continue to send data back to Earth. The script describes their mission, the instruments they carry, and their current status as they venture into interstellar space.

💡Gravitational slingshot

A gravitational slingshot, also known as a gravity assist, is a method used by the Voyager spacecrafts to gain speed and change their trajectory by using the gravity of a planet like Jupiter. This technique allowed the spacecrafts to extend their reach to other outer planets without using additional fuel. The script mentions how the Voyagers used Jupiter as a gravitational slingshot to continue their journey to Saturn, Uranus, and Neptune.

💡Planetary alignment

The planetary alignment refers to the rare and favorable positioning of the outer planets in the late 1970s, which allowed the Voyager spacecrafts to travel to multiple planets in an efficient and time-saving manner. The script explains that this alignment would not occur again for another 176 years, making the Voyager missions time-sensitive and opportunistic.

💡Interstellar space

Interstellar space is the region between star systems, beyond the influence of the Sun's solar wind. The script details how Voyager 1 entered interstellar space in 2012, becoming the first human-made object to do so. It discusses the scientific significance of this achievement and the data collected by the spacecrafts as they explore this uncharted territory.

💡Radioisotope thermoelectric generators (RTGs)

RTGs are power sources used by the Voyager spacecrafts. They generate electricity from the heat produced by the radioactive decay of Plutonium-238. The script explains that these generators are crucial for the continued operation of the spacecrafts' instruments, despite being far from the Sun and unable to use solar power.

💡Deep Space Network (DSN)

The Deep Space Network is a system of large antennas located around the globe that NASA uses to communicate with distant spacecraft, including the Voyagers. The script describes how the DSN's global positioning allows for constant communication with the Voyagers, despite their vast distances from Earth.

💡Magnetic fields

Magnetic fields are discussed in the context of the Voyager spacecrafts' exploration of the outer planets and their current mission in interstellar space. The script mentions how magnetometers on the Voyagers were used to study the magnetic fields of the planets and are now helping scientists understand the transition from the solar wind's influence to interstellar space.

💡Plasma waves

Plasma waves are oscillations in the charged particles that make up plasma, which is a state of matter found in stars and interstellar space. The script explains how the plasma wave subsystem on the Voyagers was used to measure electrical field components at the outer planets and is now providing information about plasma wave changes as the spacecrafts enter interstellar space.

💡Cosmic rays

Cosmic rays are high-energy particles originating from outside our solar system. The script discusses how the cosmic ray instrument on the Voyagers is detecting particles from inside the solar system's influence bubble and from interstellar space, helping scientists determine when Voyager 1 entered interstellar space.

💡Oort cloud

The Oort cloud is a theoretical sphere of icy objects that surrounds the Sun at great distances, considered the outermost region of the solar system. The script mentions that Voyager 1 will not be considered to be in pristine interstellar space until it has passed through the Oort cloud, which could take another 300 years.

💡Interstellar medium

The interstellar medium refers to the matter and radiation that exists in the space between star systems. The script describes how the Voyager spacecrafts are now exploring the interstellar medium, studying the transition from the solar system's influence to the broader galaxy.

Highlights

The Grand Tour was a proposed planetary tour in the 1960s to study the outer planets using unmanned probes.

A rare alignment of Jupiter, Saturn, Uranus, Neptune, and Pluto in the late 1970s was the basis for the Voyager mission timing.

Voyager spacecrafts were launched in 1977 to utilize the planetary alignment for a more efficient exploration trajectory.

Voyager 2 was the only spacecraft to visit Uranus and Neptune, expanding the mission beyond Jupiter and Saturn.

Remote control programming enhanced the Voyagers' capabilities beyond their initial launch capabilities.

Voyagers explored 48 moons and the unique ring and magnetic field systems of the outer planets.

Voyager 1 overtook Voyager 2 in the asteroid belt in December 1977, becoming the faster spacecraft.

Voyager 1 became the most distant human-made object in outer space in February 1998.

Voyager 1 left the solar system in 2002, marking a significant milestone in space exploration.

Voyager 2 holds the record for visiting more planets than any other man-made object in history.

Voyagers were equipped with scientific instruments to study the solar system and beyond, with some still active today.

The low energy charged particle detector and cosmic ray instrument are active on both Voyager 1 and Voyager 2, studying cosmic radiation.

The plasma wave subsystem and magnetometers continue to provide data on plasma waves and magnetic fields.

Voyager 1's plasma detector malfunctioned in 1980, necessitating alternative methods to study plasma.

Voyager 1's location in interstellar space was determined by measuring the density of plasma using sound wave data from solar flares.

Voyager 1 will encounter the star AC + 79 3888 in 40,000 years, while Voyager 2 will pass by Sirius in 296,000 years.

The Voyagers are expected to orbit the Milky Way galaxy for billions of years before a potential collision with the Andromeda galaxy.

The Voyagers' communication systems, including an 8-track tape recorder and thrusters, have been crucial for maintaining contact with Earth.

NASA's Deep Space Network enables continuous communication with the Voyagers despite their immense distance.

The Voyagers are equipped with radioisotope thermoelectric generators as a power source, expected to last until around 2025.

Transcripts

play00:01

In the 1960s a grand planetary tour to

play00:05

study the outer planets was proposed. It

play00:08

was an ambitious plan to send unmanned

play00:11

probes to the outer planets of the outer

play00:13

solar system. The Grand Tour could

play00:16

exploit a rare unusual and favorable

play00:19

alignment of the planets Jupiter Saturn

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Uranus Neptune and Pluto. This planetary

play00:25

alignment would occur in the late 1970s

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and would not occur again for a hundred

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and seventy-six years. So the twin

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Voyager spacecrafts one and two were

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launched in 1977 to take advantage of

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this special planetary alignment. It

play00:42

would allow a probe to be sent to

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Jupiter and use that planet as a

play00:45

gravitational slingshot to extend the

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trajectory to the other planets further

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out in the solar system. The primary

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mission of the Voyager spacecrafts was

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the exploration of Jupiter and Saturn.

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After making a series of outstanding

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discoveries the mission was extended.

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Voyager 2 went on to explore Uranus and

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Neptune and is still the only spacecraft

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to have visited those outer planets.

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Remote control programming was used to

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endowed the voyagers with greater

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capabilities than they had when they

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left the earth. Eventually

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Voyager 1 and Voyager 2 explored all the

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giant outer planets of our solar system,

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48 of their moons and the unique system

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of rings and magnetic fields that those

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planets possess. In December 1977 Voyager 2

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entered the asteroid belt. Nine days

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later

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Voyager 1 traveling at a greater speed

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overtook Voyager 2. In February 1998

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Voyager 1 passed pioneer 10 to become

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the most distant human-made object in

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outer space. In 2002

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Voyager 1 left the solar system rising

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above the ecliptic plane at an angle of

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35 degrees

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and at a speed of 39,000 miles per hour.

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Voyager 2 also left the solar system

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diving below the ecliptic plane at an

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angle of 48 degrees and a speed of 30

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4,500 miles per hour . Voyager 2 still

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holds the record of traveling to more

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planets than any other man-made object

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in history. And Voyager 1 holds the

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record as the Explorer from Earth that

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has traveled farthest from home. Voyager

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1 and 2 completed their exploration of

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the outer planets in the first dozen

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years of their mission. Having completed

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their primary mission in 1989 the

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Voyagers were ready to begin exploring

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outside the solar system. In January 1990

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with voyagers new destinations outside

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the solar system the project's

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designation was changed to Voyager

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Interstellar Mission. Both voyagers

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continue exploring where nothing from

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Earth has flown before. In order to

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explore the solar system and beyond,

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Voyager 1 and Voyager 2 were equipped

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with a large number of special

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scientific instruments, suites and

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subsystems. Most of the instruments are

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located on the body of the spacecraft.

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Each spacecraft is comprised of 65,000

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individual parts. Of the dozens of

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working instruments that the voyagers

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left earth with, there are only four

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instruments still working on Voyager 1

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and five instruments still working on

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Voyager 2. The low energy charged

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particle detector and its three sets of

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particle sensors measure how many

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low-energy particles hit it and

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determine the speed of those particles.

play03:59

It studies cosmic radiation and

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particles that emanate from the Sun, the

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planets and interstellar space. It is

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active on both Voyager 1 and Voyager 2

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The cosmic ray instrument looks for very

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high energetic particles from the Sun

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and other galactic sources. It currently

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is detecting the abundance of particles

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from inside the bubble of our sun's

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influence and also particles that

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emanate outside of the bubble in

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interstellar space.

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These readings help scientists determine

play04:33

when Voyager 1 entered interstellar

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space. It is still active on both Voyager 1

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and Voyager 2. The plasma wave

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subsystem uses the 2 long antennas on

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the spacecraft which stretch at right

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angles to one another. It was used to

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measure the electrical field components

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of possible waves at the outer planets

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but now the instrument is providing

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information about the changes to plasma

play05:01

waves as they enter interstellar space,

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It is still active on both Voyager 1 and

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Voyager 2. The magnetometers job was to

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investigate the magnetic fields of the

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outer planets but now its primary job is

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to search for the transition region

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between the interplanetary and

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interstellar media. They investigate the

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magnetic characteristics of the

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transition region at the solar wind

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boundary where the sun's magnetic

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influence interacts with and gives way

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to the magnetic field of interstellar

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space. This instrument is still working

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on both Voyager 1 and Voyager 2. Finally

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the plasma science instrument looks for

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the lowest energy particles in plasma. It

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also has the ability to look for

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particles moving at particular speeds

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and to a limited extent to determine the

play05:54

direction from which they come. This is

play05:57

important as the spacecraft enters

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interstellar space. The instrument is now

play06:02

active only on Voyager 2. The other

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instruments have either stopped working

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on their own or have been shut down to

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preserve power. NASA has also

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systematically shut down heaters on both

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crafts to save power. In 1998, 21 years

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after launch,

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non-essential instruments were

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permanently shut off. The power source on

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each spacecraft is a group of three

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radioisotope thermoelectric generators

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The RTGS give off heat by the decay of

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radioactive Plutonium 238 and turning it

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into electricity.

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Eventually the plutonium 238 will have

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decayed completely and will no longer be

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able to provide power, at which time all

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instrumentation will cease to operate.

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This should occur around 2025 but with

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careful power management the Voyager

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team hopes to keep both spacecraft

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functioning through 2027, the 50th

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anniversary of their launch. The voyagers

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are each equipped with a pair of

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thrusters which are not used for

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propelling the craft forward, but for

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reorienting the probe so that it's

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antenna is always pointing at the earth.

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Otherwise we would not be able to

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communicate with it. These thrusters fire

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in tiny pulses or puffs lasting mere

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milliseconds to subtly rotate the

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spacecraft so that its antenna points at

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the earth. Since the primary thrusters on

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Voyager 1 had degraded, scientists fired

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up the backup thrusters in November 2017

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so that Voyager 1 could keep its lock on

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the earth. They had not been activated in

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almost 40 years but they came to life to

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reorient the spacecraft's antennae.

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Voyager 2, whose primary thrusters were

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still working, was able to also keep its

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orientation toward the earth.

play08:02

The voyagers communicate with earth via

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a 3.7 meter diameter high gain antenna

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which sends and receives radio waves via

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three Deep Space Network stations on the

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earth. Voyagers main transmitter radiates

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about 20 watts which is comparable to a

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typical refrigerator light bulb.

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By the time Voyagers’ signal reaches

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Earth its strength has diminished to

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about 20 billion times weaker than a

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digital watch battery. Your iPhone has

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100,000 times more memory than the

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Voyager spacecraft,

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Although state-of-the-art at the time

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Voyagers computer systems are vintage

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1974-75, causing NASA to look for

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programmers who understand decades-old

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software. In fact Voyager is equipped

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with an 8-track tape recorder which it

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uses to store information for

play08:55

transmission to Earth. In 1978 the

play09:00

transmitter failed on Voyager 2 so the

play09:03

backup transmitter has been used ever

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since. The voyagers signal however is

play09:08

bright when compared to most natural

play09:10

objects studied by radio telescopes.

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NASA's Jet Propulsion Laboratory

play09:16

communicates with Voyager practically

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everyday via NASA's Deep Space Network

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but it takes someone with 1970s design

play09:24

experience to be able to understand

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Voyager . The Deep Space Network consists

play09:32

of three antenna complexes that are

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stationed around the globe approximately

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a hundred and twenty longitudinal

play09:38

degrees apart. They are located in Madrid

play09:42

Spain, Goldstone California and Canberra

play09:47

Australia. The global separation of the

play09:51

stations allows the spacecraft to have

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an uninterrupted line of sight

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with at least one station regardless of

play09:58

the time of day.

play09:59

These massive antennas have been

play10:02

upgraded several times to accommodate

play10:04

receiving signals from Voyager and other

play10:06

spacecraft Voyager 1 and Voyager 2

play10:10

signals can still be received by all

play10:12

three stations but Canberra is the only

play10:15

one with a powerful enough transmitter

play10:18

that can transmit to the Voyagers.

play10:22

Centers at each DSN site receive

play10:24

incoming information then send it to the

play10:27

Space Flight Operations facility at the

play10:29

Jet Propulsion Laboratory in Pasadena

play10:30

California. Due to the incredible

play10:34

weakness of the spacecraft's downlink, by

play10:37

the time it reaches Earth, large

play10:39

parabolic reflectors and hyperbolic sub

play10:41

reflectors collect the microwave

play10:43

radiation and focus it on a

play10:45

cryogenically cooled receiver at the

play10:47

base of the antenna. While one of the

play10:50

antennas is more than powerful enough to

play10:52

transmit to Voyager, a single 34 meter

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antenna does not collect enough

play10:57

electromagnetic radiation to detect

play11:00

Voyagers downlink. So antennas at each

play11:03

site are linked together so that they

play11:05

can simultaneously receive the signals

play11:08

from the spacecraft providing increased

play11:10

gain. It currently takes more than 19

play11:13

hours for Voyager to receive signals

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from Earth and 19 hours for earth to

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receive signals sent by Voyager. The

play11:21

massive antennas that comprise NASA's

play11:23

Deep Space Network will pick up a faint

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distant signal for the final time around

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2025. It will track the downlink signal

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from the spacecraft as it sputters into

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silence and becomes part of the

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background noise of the solar system,

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never to be heard from by humans again.

play11:49

So how do we know Voyager 1 is in the

play11:52

interstellar space. The most convenient

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way to determine the location of Voyager 1

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was to measure the temperature,

play12:00

pressure and density of plasma or

play12:02

ionized gas around the spacecraft.

play12:06

Everything inside the solar bubble or

play12:08

heliosphere should be exposed to plasma

play12:11

that streams from the Sun, whereas

play12:14

interstellar space is filled with denser

play12:16

plasma emanating from interstellar space

play12:18

as a result of the explosion of giant

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stars millions of years before.

play12:24

Unfortunately Voyager 1’s plasma

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detector stopped working in 1980 and

play12:29

hasn't functioned for almost 40 years. So

play12:33

scientists needed to examine the plasma

play12:36

or charged particles which fill the

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bubble encasing our solar system and

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compare that with the plasma or charged

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particles that occur in interstellar

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space, ithout the use of Voyager 1’s

play12:47

plasma detector. We needed to compare the

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solar wind versus the galactic wind each

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traveling in a different direction. Since

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July of 2012 the solar wind has

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decreased and the galactic wind has

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increased, placing the craft in what is

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known as the magnetic highway. Plasma

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consists of charged particles and is

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more prevalent in the extreme cold of

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interstellar space than in the bubble of

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solar wind that permeates our solar

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system. The plasma detector on Voyager 1

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had been designed to measure the

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composition of those two plasmas but

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without that instruments such

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measurements were not possible.

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Fortunately and by chance a pair of

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solar flares blasted charged particles

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in Voyagers direction in 2011 and 2012.

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It took a year for the particles to

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reach the spacecraft but they did

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eventually and they provided sound wave

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information that could be used to

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determine how dense the plasma was in

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voyagers location. When that last wave

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reached Voyager it caused the plasma

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around Voyager to vibrate or oscillate

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in a certain particular tone. By

play14:02

measuring that soundwave we could

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measure the density of the plasma

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surrounding the spacecraft. Scientists

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knew then that Voyager 1 was in a place

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no spacecraft had ever been before. It

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was on the magnetic highway where all

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particles that were inside the

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heliosphere had streamed away and were

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now gone. What we now saw instead were

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cosmic rays from outside the heliosphere.

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The data showed a huge spike in the

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number of galactic cosmic rays from

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outside the solar system and a

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corresponding decrease in particles

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emanating from the Sun. All of the pink

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colored ions you see here were from the

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hot bubble of solar wind coming from our

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Sun and permeating our solar system. They

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were leaving the heliosphere along the

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magnetic highway. And at the same time

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the blue ions seen here are the cosmic

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ions moving at a higher speed coming in

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from interstellar space and from a

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different direction. Voyager 1 is now in

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a region where it is surrounded only by

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cosmic rays accelerated from elsewhere

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in the galaxy. Many scientists now

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declare that Voyager 1 is in

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interstellar space. There is a caveat

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that comes with our ones exit from the

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solar system however. Many scientists

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consider the term solar system to mean

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not only the planets in our solar system

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and the sun's influence beyond, but that

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the solar system extends up to the edge

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of the Oort cloud. If so it will take

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another 300 years for Voyager 1 to reach

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the inner edge of the vast Oort cloud.

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And the journey through the Oort cloud

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could take another 30,000 years. Only

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then will Voyager 1 be considered to be

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in pristine interstellar space.

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Voyager 1 is currently traveling at

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about 38,000 miles per hour, a million

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miles per day or about a billion miles

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every three years. That velocity will

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never change. It will go on forever.

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Having left the solar system, the next

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time it will encounter a star is in

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40,000 years when it flies about 1.7

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light-years away from an obscure star in

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the constellation Camelopardalis called

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AC + 79 3888

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It will be in the year 40,000 282. And in

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56,000 years Voyager 1 will pass out of

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the Oort cloud. After another 570

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thousand years Voyager 1 will brush past

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the stars GJ 686 & GJ 678.

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Voyager 2 traveling at 34,500

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miles per hour is

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also on course to enter interstellar

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space, likely late 2019 or 2020. Voyager 2

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is heading out of the solar system in

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another direction from Voyager 1. Voyager

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2 is not headed for any particular star

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but in about 61,000 years from now

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Voyager 2 will pass out of the Oort

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cloud. After 296 thousand years in the

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year two hundred and ninety eight

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thousand AD, Voyager will pass by the

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star Sirius at a distance of

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4.3 light-years. About one hundred

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thousand years after that, Voyager 2 will

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brush past two stars Delta pav and GJ 754.

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Beyond this both Voyagers will continue

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into the void passing through dust

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clouds and local bubbles of empty space

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blown upon by dying stars. The

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spacecrafts could be affected by dust

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clouds and the gravitational pull of

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rogues starless planets however.

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Ultimately like the stars in the Milky

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Way the Voyagers will orbit the center

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of the Milky Way galaxy. It will take 225

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million years to complete one orbit

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around the center of the Milky Way. And

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the voyagers will orbit for billions of

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years or until our neighboring galaxy

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Andromeda collides with the Milky Way.

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Due to the enormous distances between

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the stars, it is likely that the voyagers

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will survive this collision of galaxies

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however and continue their journey.

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Frozen in the vacuum of space both

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spacecraft and their contents need not

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fear decay.

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The ultimate death of the voyagers could

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come from thousands of micro meteorite

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impacts or one unforeseen collision.

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The Voyagers however will probably

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outlive the solar system long after our

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Sun dies and long after the Milky Way

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galaxy has been unalterably changed or

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disappeared. The voyagers are destined

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perhaps for all eternity to wander the

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cosmos carrying with them the only

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Связанные теги
Voyager MissionSpace ExplorationPlanetary TourGalactic JourneyOuter PlanetsSolar SystemInterstellar SpaceMagnetic FieldsCosmic RaysSpacecraft History
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