CoRoT detects oscillations in 3 distant stars 07/11/2008
CoRoT detects oscillations in 3 distant stars
CNES's CoRoT spacecraft has turned up 3 distant stars surprisingly similar to our own Sun. The discovery is the subject of an article this week in the prestigious American review Science.
CNES's CoRoT space telescope doesn't just hunt for exoplanets, since it recently found 3 distant stars hotter than the Sun but with similar physical characteristics.
How did it achieve this feat?
"CoRoT employs a method based on very-high-precision photometry," explains Eric Michel, from the LESIA space and astrophysics instrumentation research laboratory at the Observatoire de Paris.
"In each of the 3 stars it observed, CoRoT detected Sun-like oscillations and granulation."
Light curves of the 3 stars observed by CoRoT. Credits: LESIA.
This discovery is a major first, since oscillations have never been viewed before by photometry with such precision.
"These oscillations are periodic deformations in the star's structure revealed by extremely faint variations in its brightness," says Eric Michel.
Model of 4 types of oscillation in the stars. Credits: David B. Guenther.
Such faint variations are undetectable from Earth because scintillation in the atmosphere prevents ground telescopes from seeing as clearly as CoRoT.
Another feature the 3 stars share with the Sun is their granulation, with a roiling surface composed of bright granules (hot rising plasma) and darker spots (cooler plasma).
Granulation patterns on the surface of the Sun. A solar granule spans 1,000 km. Credits: Observatoire du Pic du Midi.
Learning about star shells
"This granulation reveals convection occurring just under the surface," says Eric Michel. "We saw solar-like granulation in all 3 stars."
The light curves obtained also confirm their ressemblance with the Sun.
"Analysis of the light curves clearly highlights solar-type pulsations with characteristic frequency profiles."
Astronomers will now look at each of the light curves in more detail to find out what is going on inside the stars. "Thanks to the photometric precision of the results obtained with CoRoT, we are going to learn more about the dynamics driving the shell, a region of stars that is still poorly understood," enthuses Eric Michel.
Convective movements take place in the convection zone, here in the Sun. Credits: Wikipedia Commons