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Cool science stuff.

Brightest star in Galaxy has competition


URL to an interesting article in Science Daily News
_http://www.sciencedaily.com/releases/2008/07/080715131623.htm_
(http://www.sciencedaily.com/releases/2008/07/080715131623.htm)

I wonder how close a star could be to one of these monsters before the
radiation would make it impossible for life to form - 10 ly, 100ly?  I know 
that
when it blows up it will sterilize nearby systems, but what about during 
its
normal lifespan?

First few paragraphs
"
ScienceDaily (July 15, 2008) — A contender  for the title of brightest star
in our Milky Way galaxy has been unearthed in  the dusty metropolis of the
galaxy's center.

____________________________________
 See also:
_Space &  Time_ (http://www.sciencedaily.com/news/space_time/)
    *   _Stars_ (http://www.sciencedaily.com/news/space_time/stars/)
    *   _Nebulae_ (http://www.sciencedaily.com/news/space_time/nebulae/)
    *   _Astronomy_ (http://www.sciencedaily.com/news/space_time/astronomy/)

    *   _Galaxies_ (http://www.sciencedaily.com/news/space_time/galaxies/)
    *   _Extrasolar Planets_
(http://www.sciencedaily.com/news/space_time/extrasolar_planets/)
    *   _Astrophysics_
(http://www.sciencedaily.com/news/space_time/astrophysics/)
_Reference_ (http://www.sciencedaily.com/articles/)
    *   _Supergiant_ (http://www.sciencedaily.com/articles/s/supergiant.htm)

    *   _Star  cluster_
(http://www.sciencedaily.com/articles/s/star_cluster.htm)
    *   _Orion  Nebula_
(http://www.sciencedaily.com/articles/o/orion_nebula.htm)
    *   _Cepheid  variable_
(http://www.sciencedaily.com/articles/c/cepheid_variable.htm)

Nicknamed the "Peony nebula star," the bright stellar bulb was revealed by
NASA's Spitzer Space Telescope and other ground-based telescopes. It blazes
with  the light of an estimated 3.2 million suns.
The reigning "brightest star" champion is Eta Carina, with a whopping solar
wattage of 4.7 million suns. But according to astronomers, it's hard to pin
down  an exact brightness, or luminosity, for these scorching stars, so they
could  potentially shine with a similar amount of light.
"The Peony nebula star is a fascinating creature. It appears to be the
second-brightest star that we now know of in the galaxy, and it's located 
deep
into the galaxy's center," said Lidia Oskinova of Potsdam University in 
Germany.
"There are probably other stars just as bright if not brighter in our galaxy
that remain hidden from view." Oskinova is principal investigator for the
research and second author of a paper appearing in a future issue of the 
journal
 Astronomy and Astrophysics.
Scientists already knew about the Peony nebula star, but because of its
sheltered location in the dusty central hub of our galaxy, its extreme 
luminosity
was not revealed until now. Spitzer's dust-piercing infrared eyes can  see
straight into the heart of our galaxy, into regions impenetrable by visible
light. Likewise, infrared data from the European Southern Observatory's New
Technology Telescope in Chile were integral in calculating the Peony nebula
star's luminosity.
"Infrared astronomy opens extraordinary views into the environment of the
central region of our galaxy," said Oskinova.
The brightest stars in the universe are also the biggest. Astronomers
estimate the Peony nebula star kicked off its life with a hefty mass of 
roughly  150
to 200 times that of our sun. Stars this massive are rare and puzzle
astronomers because they push the limits required for stars to form. Theory 
predicts
that if a star starts out too massive, it can't hold itself together  and
must break into a double or multiple stars instead.
Not only is the Peony nebula star hefty, it also has a wide girth. It is a
type of giant blue star called a Wolf-Rayet star, with a diameter roughly 
100
times that of our sun. That means this star, if placed where our sun is, 
would
 extend out to about the orbit of Mercury.
With so much mass, the star barely keeps itself together. It sheds an
enormous amount of stellar matter in the form of strong winds over its 
relatively
short lifetime of a few million years. This matter is pushed so hard  by 
strong
radiation from the star that the winds speed up to about 1.6 million
kilometers per hour (one million miles per hour) in only a few hours.
Ultimately, the Peony nebula star will blow up in a fantastic explosion of
cosmic proportions called a supernova. In fact, Oskinova and her colleagues 
say
 that the star is ripe for exploding soon, which in astronomical terms mean
anytime from now to millions of years from now.
"When this star blows up, it will evaporate any planets orbiting stars in 
the
 vicinity," said Oskinova. "Farther out from the star, the explosion could
actually trigger the birth of new stars."
In addition to the star itself, the astronomers noted a cloud of dust and
gas, called a nebula, surrounding the star. The team nicknamed this cloud 
the
Peony nebula because it resembles the ornate flower.
"The nebula was probably created from the spray of dust leaking off the
massive Peony nebula star," said Andreas Barniske of Potsdam University, 
lead
author of the study."





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