PREFIRE Mission

Context

  • Recently, NASA launched one of two climate satellites as part of the PREFIRE (Polar Radiant Energy in
    the Far-InfraRed Experiment) Mission.

PREFIRE Satellites

  • The PREFIRE satellites are 6U CubeSats, measuring around 90 cm in height and nearly 120 cm in width
    when their solar panels are deployed.
  • Two 6U CubeSats aim to orbit at an altitude of about 525 kilometres in a near-polar orbit.
  • Each satellite carries a miniaturised infrared spectrometer, covering the 0-45 µm range at 0.84 µm spectral
    resolution.
  • Operating for one seasonal cycle (approximately a year), PREFIRE aims to provide unprecedented data on
    far-infrared emissions from Earth’s poles.

PREFIRE’s Objectives

  • Quantifying Far-Infrared Emission: PREFIRE aims to document the variability in spectral fluxes from 5
    µm to 45 µm, shedding light on the energy radiated by Earth’s polar regions.
  • Nearly 60% of Arctic emission occurs at wavelengths > 15 µm (FIR), which has remained uncharted
    territory until now.
  • Anchoring Climate Predictions: By measuring far-infrared radiation, PREFIRE improves Arctic climate
    predictions.
  • It provides critical data for understanding Arctic warming, sea ice loss, ice sheet melt, and sea level rise.
  • Earth’s Thermostat: The Arctic acts as Earth’s thermostat, regulating the climate by venting excess energy
    received in the tropics.
  • PREFIRE’s insights into Arctic heat emissions contribute to a more accurate understanding of our planet’s
    climate dynamics.

Significance: Earth’s Energy Budget

  • Understanding Earth’s energy balance is crucial for predicting climate changes, as incoming solar radiation
    and outgoing heat determines our planet’s temperature and climate.
  • However, a significant portion of heat radiated from the Arctic and Antarctica occurs as far-infrared
    radiation (wavelengths of 3 µm to 1,000 µm), which has never been systematically measured.
  • PREFIRE aims to bridge this gap in knowledge by capturing spectral fluxes from 5 µm to 45 µm on hourly
    to seasonal timescales.