Galactic data shore up a constant.The first galactic ga·lac·tic adj. 1. Relating to milk. 2. Promoting the flow of milk. galactic 1. pertaining to milk. 2. galactagogue. test for possible variations in a fundamental constant of nature has found no evidence for change. The new findings raise doubts about a 2001 report by quasar quasar (kwā`sär), one of a class of blue celestial objects having the appearance of stars when viewed through a telescope and currently believed to be the most distant and most luminous objects in the universe; the name is shortened from observers that alpha, a presumed constant that figures into the strength of the electromagnetic force electromagnetic force One of the four known basic forces in the universe. Electromagnetism is responsible for interactions between charged particles that occur because of their charge, and for the emission and absorption of photons (electromagnetic radiation). , actually varies over time, says Jeffrey Newman of Lawrence Berkeley (Calif.) National Laboratory. The earlier observations examined absorption of quasar emissions by clouds of gas deep in space, and the findings suggested that alpha, also called the fine-structure constant The fine-structure constant or Sommerfeld fine-structure constant, usually denoted , is the fundamental physical constant characterizing the strength of the electromagnetic interaction. , has grown slightly since the universe was young (SN: 10/6/01, p. 222). Any fluctuation FluctuationA price or interest rate change. could have big implications. For instance, a changing alpha might signify extra unseen dimensions. The new galaxy data gathered by Newman and his colleagues emerges from DEEP2, a nearly completed 5-year telescope survey of thousands of distant galaxies. To test alpha, DEEP2 scientists monitored light of two specific wavelengths coming from oxygen ions in 300 of the brightest galaxies in the survey. When the universe was about half its current age, ultraviolet An invisible band of radiation at the upper end of the visible light spectrum. With wavelengths from 10 to 400 nm, ultraviolet starts at the end of visible light and ends at the beginning of X-rays. The primary source of ultraviolet light is the sun. radiation from the galaxies' stars excited oxygen ions in gas clouds within the galaxies. Those ions then emitted the light now reaching Earth, Newman explains. If alpha had changed since the original emission, the wavelengths emitted by oxygen ions on Earth today would differ slightly from those coming from the faraway far·a·way adj. 1. Very distant; remote. 2. Abstracted; dreamy: a faraway look. faraway Adjective 1. very distant 2. galaxies. As it turns out, the observed wavelengths have remained the same--to a precision of one part in 30,000--according to a comparison of survey data with laboratory spectra of oxygen ions, Newman reports. However, it's too early to draw firm conclusions from the new study, he cautions. For one thing, the 2001 quasar study yielded an alpha variation of one part in 100,000--too subtle for the new galaxy study to detect or rule out. Moreover, quasar data like those in the earlier study have grown and still support a changing alpha, says astronomer Michael T. Murphy of the University of Cambridge in England. "Now, we have a sample of [quasar observations] nearly three times the sample in 2001," Murphy told Science News. |
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, is the fundamental physical constant characterizing the strength of the electromagnetic interaction.
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