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Scintillation

Collier's New Encyclopedia (1921)

a twinkling of the stars; a familiar phenomenon to all who have directed their attention to the firmament above us. Under ordinary atmospheric conditions this flickering is possessed only by the so-called fixed stars. A planet shines steadily and by this mark can readily be picked out. When near the horizon, however, planets have been observed to scintillate slightly; while stars at low altitudes invariably twinkle more vigorously than stars overhead. This at once points to the atmosphere as an important factor, since the phenomenon is more pronounced when the light has to traverse a greater depth of air. Again, when viewed through sufficiently large telescopes stars cease twinkling altogether. The action of the telescope is to concentrate on the eye a much larger pencil of rays than could naturally enter it. Instead of one slender ray the eye receives the integral effect of a great number of rays, whose individual features are lost in the general average. In the case of a planet, again, the rays which fall on the retina converge from all parts of a disk of sensible size; and in the integral effect of this pencil the individual half of the 4th century B. C. One of his earliest works was the temple of Athena Alea at Tegea in Arcadia, on the site of a previous one burned down in 395 b. c. Some 15 years or so later he settled in Athens, where for more than a quarter of a century he labored at his profession. Toward the end of his life he was associated with Leochares and others in preparing sculpture for the great mausoleum of Halicarnassus in Asia Minor. A large composition, representing Achilles being convoyed to Leucæ by Poseidon, Thetis, and the Nereids, preserved for some time in the temple of Neptune at Rome, was accounted one of his masterpieces. He excelled also in statues of single gods and goddesses. SCORBUTUS. See SCURVY.

What Has Changed in the Last Century

Collier's explanation in 1921 — that twinkling comes from starlight crossing a great depth of air, that planets show steady disks, and that a large telescope averages the flicker away — is still what astronomers teach, now framed in terms of turbulent cells of differing air density refracting the beam. What has moved is the response to it: telescopes above the atmosphere (Hubble, launched 1990) escape the problem entirely, and since the 1990s big ground-based instruments have used adaptive optics, deformable mirrors flexing hundreds of times a second to cancel the atmosphere's distortion. The word itself has also acquired meanings Collier's would not recognize: scintillation counters, which detect particles by the tiny flashes they produce in a crystal, and radio scintillation, whose study at Cambridge led Jocelyn Bell Burnell and Antony Hewish to the first pulsar in 1967.

Written for this edition, 2026.