Laser Interferometer Space Antenna (LISA)

The Laser Interferometer Space Antenna (LISA) is a planned ESA-led space observatory, developed with NASA collaboration, designed to detect gravitational waves. Three spacecraft will fly in a triangular formation and use laser interferometry to measure changes in their separations caused by passing waves. Its launch is planned for 2035.

Last updated
8 November 2026
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Moderate (80%)
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Mission concept

LISA is a space-based observatory dedicated to studying gravitational waves—minute distortions of spacetime produced by accelerating massive objects, including pairs of black holes as they orbit and merge. The mission is led by the European Space Agency (ESA), with NASA as a collaborative partner. Its three spacecraft will follow Earth around the Sun in a vast triangular formation. The mission is designed to observe low-frequency gravitational waves that are difficult or impossible to measure with ground-based detectors.

How the observatory works

Laser beams exchanged between the spacecraft will measure changes in the distances between free-floating test masses carried inside them. Passing gravitational waves are expected to stretch and compress the triangle's arms by extremely small amounts. Combining measurements from all three spacecraft will allow researchers to identify signals and infer information about their sources. The mission's planned arm length is about 2.5 million kilometres. Its measurement approach builds on earlier space technology demonstrations, including ESA's LISA Pathfinder mission.

Scientific aims

LISA is intended to study sources such as massive black-hole binaries and compact stellar remnants, including binary white dwarfs, neutron stars and black holes in the Milky Way. Gravitational waves provide information complementary to light: they can reveal the motion and properties of systems whose signals may be hidden or difficult to observe electromagnetically. The observations could help scientists investigate black-hole growth and evolution, test aspects of gravity, and search for signals from sources not yet known. These are research goals, not guaranteed discoveries.

International mission and schedule

ESA describes LISA as its first space-based observatory dedicated to gravitational-wave science. NASA's stated contributions include laser and telescope systems, charge-management devices for the test masses, data-analysis systems, and scientific and engineering expertise. ESA currently lists the launch as planned for 2035, from Europe's Spaceport in French Guiana on an Ariane 6 rocket. The date and mission plans are scheduled targets and may change as development continues.

Key facts

Full name
Laser Interferometer Space Antenna (LISA).
Purpose
A space-based observatory designed to detect and study gravitational waves.
Lead agency
European Space Agency (ESA), with NASA as a collaborative partner.
Spacecraft configuration
Three spacecraft in a triangular formation following Earth around the Sun.
Planned arm length
Approximately 2.5 million kilometres.
Planned launch
2035; ESA lists Europe's Spaceport in French Guiana and Ariane 6.

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Answers use only “Laser Interferometer Space Antenna (LISA)” and its references, with citations.

References

  1. 1.
    LISA

    European Space Agency · other · reliability: unverified · retrieved 8 November 2026

    Supports: Mission's scientific purpose, planned launch year, location and launch vehicle.

  2. 2.
    LISA - NASA Science

    NASA · other · reliability: unverified · retrieved 8 November 2026

    Supports: Three-spacecraft formation, laser interferometry and test masses, gravitational-wave science goals, and NASA contributions.

  3. 3.
    LISA – the Laser Interferometer Space Antenna

    LISA Consortium · other · reliability: unverified · retrieved 8 November 2026

    Supports: Mission overview, gravitational-wave observatory concept and approximate arm length.

References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.

Article history

  1. Version 18 November 2026 · EditorCreated by Zapia