Merrifield and his colleagues derived new formulas and applied them to measurements of M77's carbon-monoxide-laced gas clouds (carbon monoxide molecules emit finely tuned radio waves, allowing astronomers to precisely measure the positions and line-of-sight velocities of interstellar matter). Spiral-shaped wave patterns that are just 3,000 light-years (20 arcseconds) from the galaxy's center whirl around the core three times as often as those 6,000 light-years out, says the team — all but guaranteeing that the galaxy's bright inner pinwheel is destined to wind itself up into an amorphous disk. "If this result turns out to apply commonly to other galaxies," the scientists write, "then intergalactic travelers would be well advised not to use the morphology of spiral structure to identify their homes."
But some experts are reserving judgment. Bruce G. Elmegreen (IBM Thomas J. Watson Research Center) cautions that the composition of M77's interstellar clouds may differ from place to place, possibly fooling Merrifield and his collaborators into thinking that the innermost parts of the galaxy's spiral pattern will outrace the outer parts after a few laps around the track. And while M77's inferred identity as a quick-change artist doesn't surprise John Kormendy (University of Texas, Austin), he doubts that M77's subtle inner spiral can shed much light on the longevity of simple but bold spirals seen in prominently barred galaxies like NGC 1300 and in closely interacting ones like M51.