Gravitational waves provide a laboratory for general relativity and a windo
w to energetic astrophysical phenomena invisible with electromagnetic radia
tion. Several terrestrial detectors are currently under construction, and a
space-based interferometer is envisioned for launch early next century to
detect test-mass motions induced by waves of relatively short wavelength. V
ery-long-wavelength gravitational waves can be detected using the plasma in
the early Universe as test masses; the motion induced in the plasma by a w
ave is imprinted onto the cosmic microwave background (CMB). While the sign
ature of gravitational waves on the CMB temperature fluctuations is not uni
que, the polarization pattern can be used to unambiguously detect gravitati
onal radiation. Thus, forthcoming CMB polarization experiments, such as the
Microwave Anisotropy Probe and Planck, will be the first space-based gravi
tational-wave detectors. [S0556-2821(99)01002-4].