Fermi Gamma-ray Space Telescope
    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)