From Wikipedia, the free encyclopedia
  (Redirected from Scintillation (astronomy))
Jump to: navigation, search

Twinkling, or scintillation, is a generic term for variations in apparent brightness or position of a distant luminous object viewed through a medium.[1] If the object lies outside the Earth's atmosphere, as in the case of stars and planets, the phenomenon is termed astronomical scintillation; within the atmosphere, the phenomenon is termed terrestrial scintillation.[2] As one of the three principal factors governing astronomical seeing, atmospheric twinkling is defined as variations in illuminance only. In simple terms, twinkling of stars is caused by the passing of light through different layers of atmosphere. Twinkling does not cause images of planets to flicker.[3][4] Most scintillation effects are caused by anomalous refraction caused by small-scale fluctuations in air density usually related to temperature gradients.[5][6] Scintillation effects are always much more pronounced near the horizon than near the zenith (straight up).[7] Atmospheric twinkling is measured quantitatively using a scintillometer.[8] The effects of twinkling are reduced by using a larger receiver aperture. This effect is known as aperture averaging.[9][10]

Planetary scintillation[edit]

Light from planets, stars and other astronomical objects are also likely to twinkle.[11]

Stars twinkle because they are so far from Earth that they appear as point sources of light easily disturbed by Earth's atmospheric turbulence which acts like lenses and prisms diverting the light's path. Scintillation occurs because astronomical objects are points of light so small that they fall upon only one rod at a time in the human retina. As the point of light moves from rod to rod, the star will "twinkle". Large astronomical objects closer to Earth, like the Moon and other planets, encompass many points in space and can be resolved as objects with observable diameters. With multiple observed points of light traversing the atmosphere, their light's deviations average out and the viewer perceives less variation in light coming from them.[12][13]

See also[edit]


  1. ^ Wang,Ting-I; Williams, Donn; "Scintillation technology bests NIST", InTech, May 1, 2005
  2. ^ " NASA Aerospace Science and Technology Dictionary",
  3. ^ Kenyon, S.L.; Lawrence, M. et al; "Atmospheric Scintillation at Dome C, Antarctica", Astronomical Society of the Pacific 118 924-932
  4. ^ Ellison, M. W. (1952). "Why do Stars Twinkle?". Irish Astronomical Journal 2 (1): 5–8. Bibcode:1952IrAJ....2....5E. 
  5. ^ Sofieva, V. F.; Sofieva, A.S.; et al "Reconstruction of internal gravity wave and turbulence parameters in the stratosphere using GOMOS scintillation measurements" Journal of Geophysical Research 112
  6. ^ VanCleave, Janice; "Stellar Scintillation: Twinkling Stars" JVC's Science Fair Projects, May 2, 2010
  7. ^ "Scintillation or Atmospheric Boil",
  8. ^ Chun, M.; Avila, R; "Turbulence profiling using a scanning scintillometer", Astronomical Site Evaluation in the Visible and Radio Range, Astronomical Society of the Pacific 266:72-78
  9. ^ Perlot,.N.; Fritzsche, D. "Aperture-Averaging - Theory and Measurements", elib - Electronic Library
  10. ^ Andrews, C.; Phillips, R.L; Hopen, C. (2000). "Aperture averaging of optical scintillations". Waves in Random and Complex Media (Taylor & Francis) 10 (1): 53–70. 
  11. ^ Wheelon, Albert D. "Electromagnetic Scintillation: Volume 2, Weak Scattering", Cambridge University Press, Jul 31, 2003
  12. ^ Graham, John A. "Why do stars twinkle?" Scientific American, October 2005
  13. ^ Byrd, Deborah; "Why don’t planets twinkle as stars do?", Earthsky, October 24, 2005