Astrophysics
A diamond heavier than the Sun
Pierre Bergeron, a Professor in the Department of Physics
at Université de Montréal, and a team of
researchers from the United States , have just discovered
a very massive white dwarf star named LHS 4033 which confirms
a hypothesis put forward more than 70 years ago by the
American astrophysicist Subrahmanyan Chandrasekhar, winner
of the 1983 Nobel Prize for physics. “What makes
this discovery important is that the mass of the object
we discovered is below the limit between a white dwarf
and a neutron star,” the Québec astronomer
explains.
To achieve these results, published in the April 2004
issue of The Astrophysical Journal, Mr. Bergeron
used data he had gathered himself in an observing session
in Arizona last October. He compared his calculations with
photometric data obtained by his colleagues in three series
of observations in Arizona and Hawaii .
The large majority of white dwarfs observed to date have
a mass equivalent to 60% of the Sun’s mass. Back
in the 1930s, the Indian-born scientist had predicted that
if a white dwarf reached 1.4 times the mass of the Sun,
the balance between its pressure and gravity would be upset.
The modern value of this limit mass is 1.36 times the mass
of the Sun. The mass of the star discovered by the astrophysicists
is 1.33 times the mass of the Sun, still within the mass
range corresponding to a white dwarf. The existence of
LHS 4033 would appear to provide confirmation of the “Chandrasekhar
mass.”
The discovery is especially meaningful for the Québec
researcher, since he used a method for analyzing spectroscopic
observations of his own invention. Published in his 1992
after his post-doctorate, the “Bergeron method” is
now widely used.
This white dwarf also exhibits a feature that makes it
even more exotic, the researcher points out. “Physical
models of this star tell us that matter will reorganize
itself, at very low temperature and very high pressure.
As a result, a gigantic crystalline network of carbon seems
to be forming—a veritable diamond in the sky! Warning
to prospectors: in case you are thinking of mining it,
the mass of this diamond is larger than the Sun’s
mass!
Researcher: |
Pierre Bergeron |
Email: |
bergeron@astro.umontreal.ca |
Telephone: |
(514) 343-6678 |
Funding: |
Natural Sciences and
Engineering Research Council of Canada, Fonds québécois
de la recherche sur la nature et les technologies,
Canada Foundation for Innovation |
|