JPL Horizons data · calculated for current UTC

Where are Voyager 1 and Voyager 2 now?

Voyager 1 and Voyager 2 continue their journeys through interstellar space. Follow their calculated distances from Earth and the Sun, speed and signal travel time. The values are computed for the current UTC using stored NASA/JPL ephemerides.

Illustration of Voyager 1 in interstellar space
Current status

Beyond the heliosphere

The primary value is the geometric distance from the centre of Earth. Speed is explicitly relative to the Sun; the change in Earth distance is a separate radial quantity.

Interstellar mission

Voyager 1

Loading local ephemeris…
Distance from Earth— km— AU
From the Sun
— AU
Speed relative to the Sun
— km/s
Change in distance from Earth
— km/s
Signal to Earth
—
Round trip
—
Distance travelled today
— km
Relative to escape velocity
—×
Relativistic time difference
— s
Apparent magnitude of the Sun
— mag
Remaining Pu‑238
— %
Mission duration
—
Distance travelled since page load
0 km
Launch

Calculation for current UTC. The position is interpolated from daily geometric JPL vectors; it is not direct telemetry.

Interstellar mission

Voyager 2

Loading local ephemeris…
Distance from Earth— km— AU
From the Sun
— AU
Speed relative to the Sun
— km/s
Change in distance from Earth
— km/s
Signal to Earth
—
Round trip
—
Distance travelled today
— km
Relative to escape velocity
—×
Relativistic time difference
— s
Apparent magnitude of the Sun
— mag
Remaining Pu‑238
— %
Mission duration
—
Distance travelled since page load
0 km
Launch

Calculation for current UTC. The position is interpolated from daily geometric JPL vectors; it is not direct telemetry.

“Current” means interpolation for the present UTC from an ephemeris generated on 2026-08-11. This is neither GPS nor live spacecraft telemetry.

Voyager 1 today: distance, speed and mission

Voyager 1 followed a faster route than Voyager 2 and is now the more distant probe. Its distance from Earth changes as both the spacecraft and Earth move. The live values above distinguish that distance from its distance to the Sun and show how long a radio signal takes to reach Earth.

The Voyager 1 profile explains what the numbers mean, which instruments remain active, why its cameras are off and how its route led beyond the heliopause. It also brings together the Jupiter and Saturn encounters, the Pale Blue Dot image and the next distance milestone.

Voyager 1: current position and distance

The story behind the numbers

Where are Voyager 1 and Voyager 2?

Both NASA spacecraft are in interstellar space, beyond the heliosphere. Voyager 1 crossed this boundary in 2012 and Voyager 2 in 2018. They crossed at different locations, allowing their measurements to reveal the environment beyond the heliosphere in two different directions.

The trackers above show each spacecraft’s distance from Earth and from the Sun. These are separations between two bodies at a given moment, not the distance travelled since launch. The position-over-time page lets you explore earlier positions during the mission.

Voyager 1 · Voyager 2 · Explore positions over time

Distance map

The Solar System at a glance

The directions of both Voyagers come from JPL heliocentric vectors. Planetary orbits, planet positions, the Kuiper belt and the heliopause are schematic.

Logarithmic radial scale · Voyagers from local JPL data · planets, Kuiper belt and heliopause shown schematically

What does it mean to be in interstellar space?

The Sun emits a stream of particles called the solar wind. It forms a vast region around the Sun and planets: the heliosphere. Its outer boundary, the heliopause, separates the solar wind from the surrounding interstellar medium. Both spacecraft have crossed this boundary.

Leaving the heliosphere is not the same as leaving the entire Solar System. If its extent is defined by objects gravitationally bound to the Sun, it also includes the distant Oort Cloud, which still lies ahead of the Voyagers. “Interstellar space” describes the environment around the spacecraft, not the end of the Sun’s gravitational influence.

Distance over time

From the planets into interstellar space

The chart shows heliocentric distance from JPL’s 60-day overview series. It compares the long-term trend and is not intended for navigation during flybys.

Vertical: distance from the Sun in AU · horizontal: 1977–2036 · source: JPL Horizons

Table alternative to the chart
Heliocentric distance in AU at the nearest 60-day JPL node
YearVoyager 1Voyager 2
19771 AU1 AU
199039.9 AU31 AU
200076.2 AU59.7 AU
2010112.3 AU91 AU
2020148.1 AU122.7 AU
2030183.2 AU154.5 AU
2036204.8 AU173.3 AU
Understanding the tracker

Distances and trajectories in context

How can we picture the Voyagers’ distance?

One astronomical unit (AU) is exactly 149,597,870.7 km. Light in a vacuum covers that distance in approximately 8 minutes and 19 seconds. Kilometres can therefore be expressed as something easier to imagine: the time information takes to travel from a spacecraft.

The one-way signal time is the travel time from the spacecraft to Earth. The round-trip time includes both directions, without waiting for a command to be processed. The calculation accounts for the motion of Earth and the spacecraft during transmission; it is not simply twice the displayed one-way time.

Why is Voyager 1 farther away than Voyager 2?

Launch order was not decisive. Voyager 2 launched on 20 August 1977, while Voyager 1 followed on 5 September. Voyager 1 took a faster, shorter trajectory to Jupiter and Saturn, reaching both planets before Voyager 2.

Planetary flybys changed the spacecraft’s directions and speeds through gravity assists. Voyager 1’s path at Saturn took it past Titan and then out of the plane of the planets. Voyager 2 continued to Uranus and Neptune. Their different trajectories explain their present separation.

Compare trajectories and speeds →

Calculated milestones

The next frontiers

The date is found by locating the specified distance crossing in the local ephemeris, not by estimation.

Voyager 1 · 175 AU

Calculating…

Searching the ephemeris.

Voyager 2 · 150 AU

Calculating…

Searching the ephemeris.

The mission continues

Still listening to interstellar space

As of 11 August 2026, MAG and PWS operate on Voyager 1; Voyager 2 retains CRS, MAG and PWS.

Voyager 1

2 instruments

Magnetic fields and plasma waves

LECP was switched off in April 2026 because of limited power.

Voyager 1 details →
Voyager 2

3 instruments

Particles, magnetic fields and plasma

A power-saving change in 2026 extended science operations.

Voyager 2 details →
Since 1977

Selected timeline events

Full interactive timeline →
  1. Voyager 2 launches

    Voyager 2 was the first of the pair to launch and headed toward the outer planets.

  2. Voyager 1 launches

    A faster trajectory brought Voyager 1 to Jupiter before its twin.

  3. Voyager 1 at Jupiter

    The close flyby returned detailed images of the planet and its moons, including active volcanoes on Io.

  4. Voyager 2 at Jupiter

    A second set of measurements expanded the mapping of the Jovian system.

  5. Voyager 1 at Saturn

    The Titan flyby deflected the spacecraft's trajectory out of the plane of the planets.

  6. Voyager 2 at Saturn

    The spacecraft continued along its unique trajectory toward Uranus.

  7. First visit to Uranus

    Voyager 2 remains the only spacecraft to have visited Uranus up close.

Compare

Two spacecraft, two trajectories

Voyager 1 is farther away; Voyager 2 alone visited Uranus and Neptune.

Open comparison →
A message from Earth

Golden Record

Sounds, images and greetings stored on a gold-plated copper disc.

Explore the record →
Frequently asked questions

Questions about the Voyager spacecraft

How do the spacecraft generate electricity so far from the Sun?

Each Voyager has three radioisotope thermoelectric generators (RTGs). They convert heat from the radioactive decay of plutonium-238 into electricity. Available electrical power gradually declines, so the mission team switches off selected instruments and other systems.

Why do the Voyagers no longer send new photographs?

The cameras were switched off to free up power and memory for other scientific instruments. The software controlling the cameras was also removed from the spacecraft. Voyager 1 took its last images in 1990. You can view photographs from the mission in our gallery.

Why does the distance from Voyager to Earth sometimes decrease?

Earth orbits the Sun. During part of the year, its motion towards a spacecraft reduces their separation even while the spacecraft continues outwards from the Sun. A negative change in distance does not, by itself, indicate an error or a reversal of flight.

Is the displayed position a live message from the spacecraft?

No. This website loads locally stored trajectory data from NASA/JPL Horizons and interpolates between their time points to calculate the position for the current time. The numbers can therefore change continuously without a new connection to the spacecraft. Our methodology explains the process and its limitations.

Why does speed differ from the change in distance from Earth?

The tracker’s speed describes the spacecraft’s motion relative to the Sun. The change in distance from Earth describes how quickly the spacecraft and Earth move farther apart or closer together. These are different quantities, distinguished in our methodology.

All questions about the Voyager spacecraft

NASA/JPL

Stories Behind Voyager's Discoveries

Three original NASA images reveal what the spacecraft saw, what scientists could conclude, and where to find the primary sources.

01 / 03

Io: a volcanic plume beyond Earth

Voyager 1 photographed an eruption on Jupiter's moon Io in 1979. The image helped establish the first observed active volcanism beyond Earth.

Open article →
02 / 03

Triton: plumes above an icy moon

A sequence of Voyager 2 images from 1989 captured an active dark plume on Triton, Neptune's largest moon.

Open article →
03 / 03

Pale Blue Dot: Earth from Voyager 1

Voyager 1 looked back in 1990 and recorded Earth as less than a pixel. The familiar version shown here is a 2020 reprocessing of those data.

Open article →

Stories Behind Voyager's Discoveries →

NASA/JPL

Explore

How NASA repaired Voyager 1 from Earth

The 2023–2024 flight computer fault: unreadable data, damaged memory, relocated software and the return of science measurements.

How NASA repaired Voyager 1 from Earth →

Voyager for schools: worksheet

Four printable exercises using the live tracker: distances, astronomical units, signal delay and the spacecraft's different routes. Answers included.

Voyager for schools: worksheet →
NASA/JPL

Explore

What cosmic rays revealed at the heliopause

Read an original NASA graph comparing Voyager 1 and 2: galactic cosmic rays increased while lower-energy particles from inside the heliosphere decreased.

What cosmic rays revealed at the heliopause →

Voyager distances on a human scale

Imagine one astronomical unit as one metre: Earth is at 1 m, Neptune near 30 m, and one light-day is about 173 m on this model.

Voyager distances on a human scale →