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
| Spacecraft | Agency | Arrived | Mission |
|---|---|---|---|
| JWST | NASA/ESA/CSA | 2022 | Infrared space telescope — 6.5 m mirror |
| Gaia | ESA | 2014 | Mapping 2 billion stars in 3D |
| Euclid | ESA | 2023 | Dark energy and dark matter survey |
| Planck | ESA | 2009–2013 | Cosmic microwave background (retired) |
| WMAP | NASA | 2001–2010 | CMB mapping (retired) |