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A Remarkable Direct Image Of A Nearby Super-Jupiter
io9 ^ | George Dvorsky

Posted on 05/11/2015 1:38:31 PM PDT by SunkenCiv

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To: outofsalt

That was good ;)


21 posted on 05/11/2015 2:14:36 PM PDT by Norm Lenhart
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To: Norm Lenhart

Just that it’s not really close to being a star with only 11 Jupiter masses. But it is close to being a brown dwarf, which is a sort of transitional category between planet and star.


22 posted on 05/11/2015 2:21:34 PM PDT by Telepathic Intruder (The only thing the Left has learned from the failures of socialism is not to call it that)
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To: Norm Lenhart
Be a hell of a thing if we actually witnessed the ignition/birth of a star.

2010 Odyssey - Jupiter Ignition

23 posted on 05/11/2015 2:27:34 PM PDT by Talisker (One who commands, must obey.)
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To: Telepathic Intruder

I meant the actual fusion thing. What I am curious about is the timeframe.

I would assume the core being the highest pressure/temp is the starting point, but considering the sheer mass/size of a star, how fast does the entire ‘star’ become involved in the reaction? is it more a ‘slow burn’ or ‘blinding flash”?


24 posted on 05/11/2015 2:29:50 PM PDT by Norm Lenhart
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To: Talisker

I really need to watch that movie.


25 posted on 05/11/2015 2:34:59 PM PDT by Norm Lenhart
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To: itsahoot
You've filtered out the distortions now let's adjust the focus.

Toldja he didn't come from Earth.

26 posted on 05/11/2015 3:02:21 PM PDT by TigersEye (STONE COLD ZOMBIE SCOURGE)
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To: rjsimmon

Due to geometric considerations, 11x the mass (roughly volume) wouldn’t be that much bigger, diameter-wise.


27 posted on 05/11/2015 3:06:54 PM PDT by fwdude (The last time the GOP ran an "extremist," Reagan won 44 states.)
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To: SunkenCiv

Red Dwarf.

“It’s cold outside, no kind of atmosphere, I’m all alone, more or less....”


28 posted on 05/11/2015 3:11:46 PM PDT by Secret Agent Man (Gone Galt; Not averse to Going Bronson.)
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To: Norm Lenhart
I'm not exactly sure how it works in brown dwarfs fusing deuterium, which is only a tiny fraction of the total hydrogen, but stars only fuse elements in the core. When that's used up, the star dies. The more massive the star, the shorter the lifespan on the order of around mass to the power of -3.5. This is a lengthy topic, however, but the Wiki page should give you a decent overview:

http://en.wikipedia.org/wiki/Stellar_evolution
29 posted on 05/11/2015 3:33:50 PM PDT by Telepathic Intruder (The only thing the Left has learned from the failures of socialism is not to call it that)
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To: Telepathic Intruder

I’ll check it out, Thanks!


30 posted on 05/11/2015 3:36:33 PM PDT by Norm Lenhart
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To: KevinDavis; annie laurie; Knitting A Conundrum; Viking2002; Ernest_at_the_Beach; Mmogamer; ...
 
X-Planets
· join · view topics · view or post blog · bookmark · post new topic · subscribe ·
Google news searches: exoplanet · exosolar · extrasolar ·

31 posted on 05/11/2015 3:36:59 PM PDT by SunkenCiv (What do we want? REGIME CHANGE! When do we want it? NOW!)
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To: Norm Lenhart

Actually that’s mass^-2.5, but minor point. For example, a star twice the mass of our sun will last 18% as long, or 1.8 billion years. Half the mass, 5.6 times as long.


32 posted on 05/11/2015 3:40:54 PM PDT by Telepathic Intruder (The only thing the Left has learned from the failures of socialism is not to call it that)
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To: Norm Lenhart

Supernovas occur at the end of the life of really massive stars. Not itsy-bitsy ones.


33 posted on 05/11/2015 6:38:55 PM PDT by Sherman Logan
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To: SunkenCiv

That looks like my typical image of anything when I take a photo.


34 posted on 05/11/2015 7:49:14 PM PDT by minnesota_bound
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