The Current State of Space Debris

Debris and defunct launcher stages in the Geostationary ring. Aging satellites are known to release debris and explosions can occur due to residual energy sources. The resulting fragments can be thrown back and cross the Geostationary orbit. For this reason it’s fundamental to release residual energy once the nominal mission is completed. (Credit: ESA/ID&Sense/ONiRiXEL)

PARIS (ESA PR) — Swirling fragments of past space endeavours are trapped in orbit around Earth, threatening our future in space. Over time, the number, mass and area of these debris objects grows steadily, boosting the risk to functioning satellites.

ESA’s Space Debris Office constantly monitors this ever-evolving debris situation, and every year publishes a report on the current state of the debris environment.


First Laser Detection of Space Debris in Daylight

A visible green laser shone from ESA’s Optical Ground Station (OGS). Part of Teide Observatory, the OGS located 2400 m above sea level on the volcanic island of Tenerife, used for the development of optical communication systems for space as well as space debris and near-Earth orbject surveys and quantum communication experiments. (Credit: IAC– Daniel López)

Lasers on Earth are used to measure the position of space debris high above, providing crucial information on how to avoid in-space collisions. Until now, this technique has suffered from a fatal flaw.

For some time, lasers could only be used to measure the distance to space debris during the few twilight hours in which the ‘laser ranging’ station on Earth is in darkness, but debris objects high above are still bathing in the last of the Sun’s rays.