Variation in brightness and the position of stars due to atmospheric refraction
For other uses, see Twinkle (disambiguation) and Scintillation.
The twinkling of the brightest star in the night sky Sirius (apparent magnitude of -1.1), shortly before upper culmination at the meridian, at 20° above the southern horizon. In 29 seconds, Sirius appears to move 7.5 arcminutes from left to right.
Twinkling, also called scintillation, is a generic term for variations in apparent brightness, colour, 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; for objects within the atmosphere, the phenomenon is termed terrestrial scintillation.[2] As one of the three principal factors governing astronomical seeing (the others being light pollution and cloud cover), atmospheric scintillation is defined as variations in illuminance only.
In simple terms, twinkling of stars is caused by the passing of light through different layers of a turbulent atmosphere. Most scintillation effects are caused by anomalous atmospheric refraction caused by small-scale fluctuations in air density usually related to temperature gradients.[3][4] Scintillation effects are always much more pronounced near the horizon than near the zenith (directly overhead),[5] since light rays near the horizon must penetrate a denser layer of and have longer paths through the atmosphere before reaching the observer. Atmospheric twinkling is measured quantitatively using a scintillometer.[6] The effects of twinkling are reduced by using a larger receiver aperture; this effect is known as aperture averaging.[7][8]
While light from stars and other astronomical objects is likely to twinkle,[9] twinkling usually does not cause images of planets to flicker appreciably.[10][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. 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]
^Wang, Ting-I; Williams, Donn; "Scintillation technology bests NIST". Archived 2013-10-04 at the Wayback Machine, InTech, May 1, 2005.
^"NASA Aerospace Science and Technology Dictionary", NASA.gov.
^Sofieva, V. F.; Dalaudier, F.; Vernin, J. (2013-01-13). "Using stellar scintillation for studies of turbulence in the Earth's atmosphere". Philosophical Transactions of the Royal Society. 371 (1982). The Royal Society: 20120174. doi:10.1098/rsta.2012.0174. ISSN 1364-503X.
^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.
^Perlot, N.; Fritzsche, D. "Aperture-Averaging – Theory and Measurements", elib – Electronic Library.
^Andrews, C.; Phillips, R. L.; Hopen, C. (2000). "Aperture averaging of optical scintillations". Waves in Random Media. 10 (1). Taylor & Francis: 53–70. doi:10.1088/0959-7174/10/1/305. S2CID 120797868.
^Wheelon, Albert D. (2003). Electromagnetic Scintillation: Volume 2, Weak Scattering. Cambridge University Press. ISBN 978-1-139-43960-2.
^Kenyon, S. L.; Lawrence, M. et al; "Atmospheric Scintillation at Dome C, Antarctica", Astronomical Society of the Pacific118, 924–932.
^Ellison, M. W. (1952). "Why do Stars Twinkle?". Irish Astronomical Journal. 2 (1): 5–8. Bibcode:1952IrAJ....2....5E.
^Graham, John A. "Why do stars twinkle?" Scientific American, October 2005.
^Byrd, Deborah; "Why don’t planets twinkle as stars do?", Earthsky, October 24, 2005.
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