Number 642 #3, June 19, 2003 by Phil Schewe, James Riordon, and Ben Stein
Star Out of Round
The Very Large Telescope Interferometer (VLTI), an array of 2 telescopes
which combine their light signals to achieve a higher angular resolution
than is possible with any one scope, has determined that the star Achernar
is the flattest star ever studied. The VLTI, which does not provide
an actual image of the star but can provide an accurate estimate of
the star's profile, has determined that Achernar's equatorial radius
is 50% larger than its polar radius. This is quite oblate compared to
most other celestial bodies, such as our Earth, whose equatorial radius
is only 0.3% larger than its polar radius. Theorists do not yet know
how to explain how a star like this could turn fast enough to adopt
with such a shape without flying apart. Achernar is about 145 light
years away from Earth in the southern sky and has a mass of about 6
solar masses. The telescopes used to make the interference map were
not the giant 8.2-m VLT telescopes, but more modest 40-cm reflectors
set at various configurations with separations as large as 140 m. (European
Southern Observatory press release, 11 June)