Home Library Glossary Deep Space & Astrophysics L2
🔭 Deep Space & Astrophysics

L2 (Sun–Earth Lagrange Point 2)

Also known as: Lagrange Point 2, Sun-Earth L2, Second Lagrange Point, SEL2

📘 Definition
The Sun–Earth L2 (second Lagrange) point is one of five gravitational equilibrium positions in the Sun–Earth system. Located about 1.5 million km from Earth in the anti-sunward direction, it allows a spacecraft to orbit the Sun with the same 365.25-day period as Earth, maintaining a roughly constant distance. L2 is a saddle point — not truly stable — so spacecraft orbit around it in halo or Lissajous orbits rather than sitting exactly at the point, performing small station-keeping burns every 21 days. The position offers three critical advantages: constant cold conditions (the Sun, Earth, and Moon are always behind the sunshield), thermal stability (no heating/cooling cycles), and uninterrupted sky coverage.
1.5 million km
Distance from Earth
151.1 million km
Distance from Sun
365.25 days (same as Earth)
Orbital Period
2–4 m/s per year
Station-keeping Δv

Understanding L2

Why L2 Is Perfect for Telescopes

At L2, a spacecraft's sunshield can simultaneously block sunlight, Earthlight, and moonlight while keeping the telescope pointed at deep space. This maintains instruments at temperatures below 40 K (−233 °C) — essential for infrared observations. Unlike LEO telescopes like Hubble, which experience heating/cooling every 90 minutes as they pass in and out of Earth's shadow, L2 provides a thermally stable environment 24/7.

Halo Orbits Around L2

No spacecraft sits exactly at L2 — the point is gravitationally unstable (like balancing a ball on a hilltop). Instead, spacecraft like JWST trace large halo orbits around L2, with amplitudes of roughly 250,000–800,000 km. These orbits are chosen to avoid Earth's shadow (which would cut solar power) and to maintain continuous communication with ground stations.

Spacecraft at L2

SpacecraftAgencyArrivedMission
JWSTNASA/ESA/CSA2022Infrared space telescope — 6.5 m mirror
GaiaESA2014Mapping 2 billion stars in 3D
EuclidESA2023Dark energy and dark matter survey
PlanckESA2009–2013Cosmic microwave background (retired)
WMAPNASA2001–2010CMB mapping (retired)
🛰️ Track JWST at L2 Live
See JWST's real-time position at L2 — distance from Earth, current observation target, and image gallery.
Open JWST Tracker →
📖 Learn More

Frequently Asked Questions

Approximately 1.5 million kilometres (about 1 million miles), or roughly 4 times the distance to the Moon. Light takes about 5 seconds to travel from L2 to Earth.
Not currently. L2 is far beyond the reach of any crewed spacecraft or robotic servicing mission. Unlike Hubble in LEO, which was serviced 5 times by Space Shuttle crews, JWST and other L2 spacecraft must work flawlessly for their entire mission — there is no repair option.
Not quite. Spacecraft at L2 orbit in halo orbits specifically designed to avoid Earth's shadow cone. If JWST entered Earth's shadow, its solar panels would lose power and its instruments would warm up, potentially causing permanent damage.