Significant exoplanet finding announcement on Monday

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Re: Significant exoplanet finding announcement on Monday

Post by lodp on Tue Oct 20, 2009 8:14 pm

Cannot find anything on arXiv again tonight - where are the submissions? Also thinking that if sub stellar are given b designation when significantly > 13 Mj yet well below 80 Mj (ongoing fusion approx) how are they to be classified?

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Re: Significant exoplanet finding announcement on Monday

Post by Sirius_Alpha on Tue Oct 20, 2009 9:16 pm

The HD 40307 et al. systems announced last June took several months for their papers to show up.

lodp wrote:...if sub stellar are given b designation when significantly > 13 Mj
yet well below 80 Mj (ongoing fusion approx) how are they to be
classified?
That's a really good question

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Re: Significant exoplanet finding announcement on Monday

Post by Lazarus on Wed Oct 21, 2009 3:52 pm

I can't remember if it is COROT or SuperWASP that holds the record for longest time between press release and appearance of the discovery paper.

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Re: Significant exoplanet finding announcement on Monday

Post by Edasich on Wed Oct 21, 2009 4:19 pm

Surely COROT, which seems is going to announce the millennium discovery, the top-secret facts and then...hot jupiters as usual.

Except the one and only super-earth in tightest orbit.

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Re: Significant exoplanet finding announcement on Monday

Post by Sirius_Alpha on Sat Oct 24, 2009 3:55 am

In the original text-based table, four systems are listed as having a "curved drift", which may mean another planet: HD 44219, HD 148156, HIP 5158, and HD 104067.

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Re: Significant exoplanet finding announcement on Monday

Post by Lazarus on Sat Oct 24, 2009 2:41 pm

Steinn Siguršsson's take on this at Dynamics of Cats has some interesting musings about the implications of this for the planet-metallicity correlation.

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Re: Significant exoplanet finding announcement on Monday

Post by Sirius_Alpha on Sun Oct 25, 2009 9:55 am

Interesting read. Could it be that gas planets aren't actually preferentially formed around high-metallicity stars? Instead, could it be that high metallicity disks simply help to facilitate migration, leading to more easily detected planets?

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