Astronomers find a precise rotation of the Milk Way
Pulsating stars enabled this new determination of our galaxy's rotation.
September 22, 2008
Provided by ESO, Garching, Germany
September 22, 2008
This artist's impression shows the local neighborhood of the Sun and its setting within our galaxy (see insert above). The figure shows the positions of some bright stars (in white) in the sky as well as the eight Cepheids used in the investigation (in blue). After the rotation of the Milky Way had been accounted for (red arrow), it seemed that the Cepheids were all falling towards the Sun (blue arrows; these are not to scale: in reality the blue velocities are typically a factor one hundred smaller than the velocity around the Milky Way).
Photo by ESO
New, vry precise measurements show that the rotation of the Milky Way is simpler than previously thought. A remarkable result from High Accuracy Radial Velocity Planet Searcher (HARPS), the most successful European Southern Observatory (ESO) instrument, shows that a much debated, apparent fall of neighborhood Cepheid stars towards our Sun stems from an intrinsic property of the Cepheids themselves.
The result, obtained by a group of astrophysicists led by Nicolas Nardetto, will soon appear in the journal Astronomy & Astrophysics.
Since Henrietta Leavitt's discovery of their unique properties in 1912, the class of bright, pulsating stars known as Cepheids has been used as a distance indicator. Combined with velocity measurements, the properties of Cepheids are also an extremely valuable tool in investigations of how our galaxy rotates.
"The motion of Milky Way Cepheids is confusing and has led to disagreement among researchers," says Nardetto. "If the rotation of the galaxy is taken into account, the Cepheids appear to fall towards the Sun with a mean velocity of about 2 kilometers per second."
A debate has raged for decades as to whether this phenomenon was truly related to the actual motion of the Cepheids and, consequently, to a complicated rotating pattern of our galaxy, or if it was the result of effects within the atmospheres of the Cepheids.
Nardetto and his colleagues observed eight Cepheids with the high precision HARPS spectrograph, attached to the 3.6-meter ESO telescope at La Silla, 7,874 feet (2,400 meters) up in the mountains of the Chilean Atacama Desert. HARPS is best known as a very successful planet hunter, but it can also be used to resolve other complicated cases, where its ability to determine radial velocities — the speed with which something is moving towards or away from us — with phenomenally high accuracy is invaluable.
"Our observations show that this apparent motion towards us almost certainly stems from an intrinsic property of Cepheids," says Nardetto.
The astronomers found that the deviations in the measured velocity of Cepheids were linked to the chemical elements in the atmospheres of the Cepheids considered.
"This result, if generalized to all Cepheids, implies that the rotation of the Milky Way is simpler than previously thought, and is certainly symmetrical about an axis," concludes Nardetto.