Spaceflightpedia
Mission · 1977–9999

Voyager 1 — beyond the heliosphere

Two probes launched in 1977 transformed our view of the outer planets and still study interstellar space. Explore their engineering, discoveries and long journey towards one light-day from Earth.

Voyager program mission insignia.
Mission patch
Reading time
6 min
Level
Advanced
Sources
8 cited
Updated
26 Sept 2026

Original 3D reconstruction of a Voyager spacecraft in interstellar space.Official illustration · Vlastní 3D model a render, Blender · CC-BY-SA-4.0

A day still to come

Voyager 1 is expected to reach a striking milestone on 18 November 2026: a radio signal from Earth will take roughly a full day to reach it. A reply will need another day. The exact moment shifts with the positions of Earth and the spacecraft; the probe is not crossing a physical boundary.

Launched 49 years ago, Voyager 1 is the most distant human-made object and still returns measurements from beyond the heliosphere. Its twin, Voyager 2, flies in a different direction and remains the only spacecraft to have visited Uranus and Neptune.

Talking across billions of kilometres

This diagram links transmitter power, the dish and the very slow data link. The figures are approximate and depend on the communication mode.
This diagram links transmitter power, the dish and the very slow data link. The figures are approximate and depend on the communication mode.

One light-day

Distances and signal travel times for November 2026 are approximate; the spacecraft and Earth keep moving.
Distances and signal travel times for November 2026 are approximate; the spacecraft and Earth keep moving.

Video: Voyager 1 And one light-day

Spaceflightpedia video about Voyager 1 approaching a distance of one light-day.

A once-in-175-years opportunity

In 1965, JPL’s Gary Flandro showed that the outer planets’ late-1970s alignment could let one spacecraft visit several worlds. A planetary flyby bends its path and, in the heliocentric frame, transfers some of the planet’s orbital energy to it. A comparable alignment recurs roughly once in 175 years.

The original Grand Tour was too costly. NASA approved two probes for Jupiter and Saturn, but the engineers preserved Voyager 2’s option to continue. The twins shared a spacecraft design, not a trajectory.

The machine at scale

The dimensions show why the booms keep sensitive instruments away from the electronics and radioisotope sources.
The dimensions show why the booms keep sensitive instruments away from the electronics and radioisotope sources.

The Grand Tour of both probes

Flyby paths are simplified; planet sizes are not to scale.
Flyby paths are simplified; planet sizes are not to scale.

Anatomy of Voyager

A ten-sided aluminium bus houses the electronics. A 3.66-metre dish dominates the spacecraft and must remain accurately pointed towards Earth. Separate booms carry three radioisotope generators, a science platform and a magnetometer as far as 13 metres from the bus.

Behind the seemingly simple shape are three computer systems for commands, science data and attitude control. Their combined memory amounts to only tens of kilobytes. After nearly half a century, every bit and every watt matters.

Anatomy of Voyager

Original procedural 3D reconstruction based on NASA/JPL, PDS and NASM references; this is not a manufacturing drawing.
Original procedural 3D reconstruction based on NASA/JPL, PDS and NASM references; this is not a manufacturing drawing.

Ten bays, three computers

Ten bays around the bus protect the electronics. The CCS executes commands, the FDS prepares telemetry, and the AACS controls the pointing of the antenna and instruments. An eight-track tape recorder stored data for later transmission when a direct Earth link was unavailable.

The cutaway draws on the known arrangement and public photographs. A complete map of every internal bay is not publicly documented, so unlabeled modules in the reconstruction are schematic.

Inside the spacecraft bus

Technical reconstruction of the electronics bays. Some cabinet placements are illustrative.
Technical reconstruction of the electronics bays. Some cabinet placements are illustrative.

Electricity from fading heat

Solar panels would not provide enough power at the outer planets. Each Voyager therefore carries three radioisotope thermoelectric generators. Decaying plutonium-238 produces heat that thermocouples convert into electricity. At launch they supplied roughly 470 W of electrical power.

Output declines gradually, by roughly four watts a year. The ground team therefore switches off instruments and finds savings in heaters. The 1977 figure is not the spacecraft’s current power.

How a radioisotope generator works

The MHW-RTG cutaway traces the path from decay heat to electrical power.
The MHW-RTG cutaway traces the path from decay heat to electrical power.

Number two launched first

Voyager 2 launched on a Titan IIIE–Centaur rocket on 20 August 1977. Voyager 1 followed on 5 September. The latter took a shorter, faster path, overtook its twin by December 1977 and reached Jupiter first.

Follow us

Follow us on social media

New plates, trivia and behind-the-scenes updates as soon as they are ready.

After launch, the booms deployed and the instruments were readied for work. The probes were built for several years of exploration; the following decades depended on design margins and continuous work by the ground team.

Voyager assembled

The exploded view shows the relation between the main dish, bus, booms and science platform.
The exploded view shows the relation between the main dish, bus, booms and science platform.

Jupiter, Saturn and the Titan decision

Voyager 1 flew past Jupiter in March 1979. Its pictures revealed complex storms and a faint ring. Linda Morabito identified a volcanic plume above the moon Io: the first observed active volcanism beyond Earth. Voyager 2 arrived in July and imaged Europa’s cracked ice in greater detail.

At Saturn in November 1980, Voyager 1 aimed for a close Titan flyby. It could study the moon’s atmosphere, but the encounter also bent its path far above the plane of the planets. Voyager 2 passed Saturn in August 1981 and continued to Uranus and Neptune.

Cameras and spectrometers on the platform

The movable scan platform let the cameras and spectrometers point at different targets during flybys.
The movable scan platform let the cameras and spectrometers point at different targets during flybys.

The twin’s journey to the ice giants

Voyager 2 reached Uranus on 24 January 1986 and Neptune on 25 August 1989. It remains the only spacecraft to have visited both planets at close range. At Uranus it found more moons and imaged Miranda; at Neptune it observed fast winds, the Great Dark Spot and plumes on Triton.

Meanwhile, on 14 February 1990, Voyager 1 took a distant portrait of the Solar System. Earth is barely a point in the famous Pale Blue Dot frame. The cameras were then switched off; the probes are no longer planetary photographers.

Beyond the heliosphere

Voyager 1 crossed the heliopause on 25 August 2012 and Voyager 2 on 5 November 2018. The heliopause marks the edge of the region dominated by the solar wind. It is neither the end of the Solar System nor a departure beyond the Oort Cloud. The probes measure particles, magnetic fields and plasma waves in local interstellar space.

Voyager 2 had a working plasma instrument at the crossing, providing a direct comparison on both sides. The two routes allow scientists to compare the heliosphere in different directions.

Which instruments still work

Status according to the September 2026 research pack: Voyager 1 has MAG and PWS, Voyager 2 MAG, PWS and CRS. Verify the status before a future update.
Status according to the September 2026 research pack: Voyager 1 has MAG and PWS, Voyager 2 MAG, PWS and CRS. Verify the status before a future update.

The twins today

Comparison as of September 2026. Distances and instrument status change over time.
Comparison as of September 2026. Distances and instrument status change over time.

Keeping a 1977 machine alive

In 2023, Voyager 1’s FDS computer stopped returning intelligible data. In 2024 engineers traced the fault to a memory chip and moved its code to other parts of memory. Engineering and then science data returned across tens of billions of kilometres.

In April 2026 the team switched off Voyager 1’s low-energy charged-particle detector, LECP. As of September 2026, its magnetometer (MAG) and plasma-wave receiver (PWS) remain. Voyager 2 also runs its cosmic-ray detector (CRS). NASA continues to plan power-saving changes; planned steps are not presented here as completed.

The power budget

The decline in electrical output explains successive instrument shutdowns. The chart uses approximate values and is not live telemetry.
The decline in electrical output explains successive instrument shutdowns. The chart uses approximate values and is not live telemetry.

A message for a possible finder

Both probes carry a gold-plated copper record with sounds of Earth, music, 115 images and greetings in 55 languages. Carl Sagan chaired the selection committee. The cover bears playback instructions, a pulsar map locating the Sun and a scale based on hydrogen.

One greeting is in Czech: “Dear friends, we wish you all the best.” The record is not a message transmitted by radio; it is a physical object for anyone who might one day find it. Long after contact ends, both probes will continue around the Galaxy.

The Golden Record

The record cover serves as a compact instruction sheet and a map of the probes’ place of origin.
The record cover serves as a compact instruction sheet and a map of the probes’ place of origin.

Article on the timeline

5 September 1977
Voyager 1 — beyond the heliosphere
Open the entry →

Check yourself

How can a probe launched in 1977 still talk to us?

Answer in your own words — everything you need is in the article above.

Sources & further reading

last verified · 26 September 2026

  1. NASA: joint mission history and planetary flybys.
  2. NASA: spacecraft design, antenna, power and instruments.
  3. NASA: the light-day distance and Voyager 1 milestone.
  4. NASA: LECP shutdown and remaining Voyager 1 instruments.
  5. NASA: FDS memory-chip fault and relocation of code.
  6. NASA: power savings and continued Voyager 2 science.
  7. JPL DESCANSO: technical description of radio communications.
  8. NASA/JPL: Golden Record contents and greetings.

Spaceflightpedia. (n.d.). Voyager 1 — beyond the heliosphere. Retrieved 9 October 2026, from https://spaceflightpedia.com/article/voyager-1

article text — CC-BY-SA · ◉ NASA photography — public domain · ✦ AI illustration — marked, generated from sources

Connections

Keep reading