
NASA
DOE
Active
Fermi Gamma-ray Space Telescope
Launched: June 11, 2008
Overview
The Fermi Gamma-ray Space Telescope (formerly GLAST) is designed to survey the sky in high-energy gamma rays, studying exotic astronomical objects such as black holes, neutron stars, and investigating dark matter and the early universe.
Primary Objectives
- Study gamma-ray sources such as active galaxies and pulsars
- Search for evidence of dark matter
- Study gamma-ray bursts
- Explore the high-energy universe
Notable Discoveries
- Detected over 5,000 gamma-ray sources including pulsars and blazars
- Discovered giant gamma-ray bubbles extending from the Milky Way's center
- Observed the highest-energy light ever seen from the sun during solar flares
- Found evidence of cosmic rays accelerated by supernova remnants
Technical Specifications
Size
2.9 m × 2.3 m
Weight
4,303 kg
Orbit
Low Earth Orbit, 550 km altitude
Mission Lifetime
10+ years (exceeded original plan)