A giant stride has been
made in the study of the age of stars. Astronomers find that the actual age of
a star can be calculated by the speed of its spin. It is found that younger
stars spin faster than the older stars.
For the first time,
a US team has now measured the spin speed of stars that are more than one
billion years old - and it matches what they predicted.
The finding
resolves a long-standing challenge, allowing astronomers to estimate a star's
age to within 10%.
The work was
presented in Seattle at a meeting of the American Astronomical Society and also appears in the journal Nature.
This is applicable to the “cool starts” –
suns about the size of our own sun, or even smaller. They are mostly available in
our galaxy.
Dr. Meibom from
the Harvard-Smithsonian Center for Astrophysics called them the lamp posts
"They act as lamp
posts, lighting up even the oldest parts of our galaxy."
Cool stars also host
the vast majority of earth-like planets that we have spotted in the distance.
The study of star spins
dates back to 1970 with the name, Gyrochronology.
"A cool star spins very fast when it's young, but just
like a top on a table it gets slower and slower as the star grows older,"
Dr Meibom said.
Granted is the fact that it is difficult
to see a star spin. Astronomers takes recourse to the sun spots on the stars to
tell the spinning.
Measuring the younger stars is easier
because they have larger sun spots; older ones smaller sun spots. These makes
studying their spinning more problematic.
A Young Star with Large Sun Spots
Kepler space telescope,
which has been trailing Earth around the Sun since 2009 got images used
by this team in measuring about 30 stars in a cluster of 2.5 billion years.
Older Stars have Smaller Sun Spots
A PhD student, Ruth Angus who researches
gyrochronology at the University of Oxford, said the results were "a
really big deal" for the field.
"More
evidence has been slowly accumulating that lots of stars do seem to follow this
pattern, but how reliably stars fall onto this relation is a bit of an
unknown," Ms Angus told the BBC.
"This
cluster will certainly help with our understanding of how good gyrochronology
is as a method, and how valid it is.
"It shows
that these stars are doing what they're expected to do, and everything's
peachy."
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