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  #1 (permalink)  
Old 03-May-2007, 03:38 PM
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Default Interesting extrasolar planet discoveries

Gliese 581 c is not the only planet discovered recently.

* XO-2b: is a fairly typical transiting planet discovered by the XO telescope. It orbits one of the components of a wide binary star.
* HAT-2-b orbits the star HD 147506. It is by far the most massive and eccentric transiting planet discovered so far.
* Corot-exo-1b is the first planet discovered by the COROT telescope. Even though it is more massive than Jupiter, it seems to be one the most inflated planet discovered so far (radius 1.5-1.8 times that of Jupiter).

There are also been many regular radial velocity planet discoveries recently. So far in 2007 there have been almost as many discoveries as in the last year together (24 vs. 27). During the recent years and against predictions the number of new planets have been fairly constant between 26 and 34. Apparently that is changing, especially as lower-mass planets are being found more and more...
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Old 04-May-2007, 09:58 AM
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Two new yet-to-be announced transiting planets:
* TrES survey has found its third planet. TrES-3 is "a nearby, massive, transiting hot Jupiter in a 31-hour orbit". No further information available.
* XO-3b (not yet announced) resembles HAT-2-b in the sense it has an eccentric orbit (e ~ 0.2) and it is very massive (12 MJ, near the brown dwarf border). Since its host star is metal-poor, it is possible that it is actually a brown dwarf.
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Old 07-May-2007, 03:19 PM
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* HD 17092 b, a massive planet around the giant star HD 17092.
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Old 07-May-2007, 03:50 PM
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This is one of my favorite exoplanet sites
http://www.oklo.org/

Some other interesting ones that happened some time back

the Genesis planet - PSR B1620-26, it is thought to be almost 13 billion years old, discovery made thanks to Hubble

Keck Observatory has confirms the existence of Jupiter-sized planet, spotted by a network of astronomers using regular backyard telescopes, planet named TrES-1

2M1207b a direct image of an extra solar planet ?

A bit off-topic but Sporally has a vote going when Earth-II will be found
When will we find exoEarth
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Old 07-May-2007, 05:12 PM
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The nickname of PSR B1620-26c is Methuselah, not "Genesis".
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Old 10-May-2007, 11:24 AM
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The torrent continues...

* Two Jovian planets around the ancient (10 Ga) star HD 155358. It is the most metal-deficient star (20% of Sun's metallicity) known to have planets.
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Old 11-May-2007, 11:33 AM
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Nature news article about the flood of recent discoveries.
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Old 14-May-2007, 03:19 PM
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That's weird... WASP-1, the parent star of the very large planet WASP-1b, appears to be very similar to HD 149026, whose super-hot planet is anomalously dense. Apparently HD 149026 b's properties cannot be explained simply by the star's excessive metallicity.
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Old 15-May-2007, 08:51 AM
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Title: TrES-3: A Nearby, Massive, Transiting Hot Jupiter in a 31-Hour Orbit
Authors: Francis T. O'Donovan, David Charbonneau, Gáspár Á. Bakos, Georgi Mandushev, Edward W. Dunham, Timothy M. Brown, David W. Latham, Guillermo Torres, Alessandro Sozzetti, Géza Kovács, Mark E. Everett, Nairn Baliber, Márton G. Hidas, Gilbert A. Esquerdo, Markus Rabus, Hans J. Deeg, Juan A. Belmonte, Lynne A. Hillenbrand, Robert P. Stefanik.

We describe the discovery of a massive transiting hot Jupiter with a very short orbital period (1.30619 d), which we name TrES-3. From spectroscopy of the host star GSC 03089-00929, we measure T_eff = 5720 ± 150 K, logg=4.6 ± 0.3, and vsini < 2 km/s, and derive a stellar mass of 0.90 ± 0.15 M_sun. We estimate a planetary mass of 1.92 ± 0.23 M_Jup, based on the sinusoidal variation of our high-precision radial velocity measurements. This variation has a period and phase consistent with our transit photometry. Our spectra show no evidence of line bisector variations that would indicate a blended eclipsing binary star. From detailed modelling of our B and z photometry of the 2.5%-deep transits, we determine a stellar radius 0.802 ± 0.046 R_sun and a planetary radius 1.295 ± 0.081 R_Jup. TrES-3 has one of the shortest orbital periods of the known transiting exoplanets, facilitating studies of orbital decay and mass loss due to evaporation, and making it an excellent target for future studies of infrared emission and reflected starlight.

Read more (39kb, PDF)
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Old 15-May-2007, 07:27 PM
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I just did an article on TrES-3. There are almost too many stories to keep up with now.

http://www.universetoday.com/2007/05...just-31-hours/
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Old 15-May-2007, 07:42 PM
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It seems like most of the papers are strongly emphasizing each exoplanet's unique characteristics to try and stand out in the crowd. I guess this is a consequence of there being so many discoveries recently.
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Old 15-May-2007, 08:23 PM
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Hum,
that would imply that they were aware of the other stories that were perhaps going to be released...and if true - that would mean that they released them together on purpose.

Motive: to stress out Fraser et al
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Old 16-May-2007, 12:32 AM
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I was talking with the researchers for TrES-3 and they said that there wasn't going to be a press release. So that confirms it. Extrasolar planets aren't important enough to warrant a press release any more.
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Old 16-May-2007, 08:26 AM
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Detection of transits of the nearby hot Neptune GJ 436 b

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This Letter reports on the photometric detection of transits of the Neptune-mass planet orbiting the nearby M-dwarf star GJ 436. It is by far the closest, smallest and least massive transiting planet detected so far. Its mass is slightly larger than Neptune's at M = 22.6 +- 1.9 M_earth. The shape and depth of the transit lightcurves show that it is crossing the host star disc near its limb (impact parameter 0.84 +- 0.03) and that the planet size is comparable to that of Uranus and Neptune, R = 25200 +- 2200 km = 3.95 +- 0.35 R_earth. Its main constituant is therefore very likely to be water ice. If the current planet structure models are correct, an outer layer of H/He constituting up to ten percent in mass is probably needed on top of the ice to account for the observed radius.
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Old 16-May-2007, 08:53 AM
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systemic blog:

Quote:
[...] It is Gl 436 b that’s transiting, and this is easily the biggest planet-related discovery so far this year. New results from the Swiss team have been coming so thick and fast that it’s hard to even keep them all straight. Let me be the first to offer my heartfelt — and let’s admit it, envious — congratulations.

[...]

Gl 436 should be placed under constant photometric surveillance. If you’re capable of doing sub-1% photometry, please get out there on the sky whenever the night is clear and Gl 436 is at low air mass. If there are additional planets in the system, then it’s completely possible that they are transiting as well.

In addition, it’s very important to collect the best possible time-series data for future Gl 436 transits. By timing when the transits occur, it will be possible to derive the orbital elements of significant additional perturbing bodies. This endeavor is within the reach of careful amateur and small-telescope observers.
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Old 16-May-2007, 09:02 AM
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Quote:
Originally Posted by Fraser View Post
I was talking with the researchers for TrES-3 and they said that there wasn't going to be a press release. So that confirms it. Extrasolar planets aren't important enough to warrant a press release any more.
Actually not true... there are certainly no less extrasolar planet press releases than before, there's no point to make press releases of similar discoveries. We already know 20 transiting planets, so TrES-3 is no longer as big news. Another reason is that TrES-3 doesn't have the magic words "habitable" and "water". That doesn't mean it isn't important, of course.

It is incredible if they don't make a press release about Gliese 436 b... *wink*
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Old 16-May-2007, 09:13 AM
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Default Hot Neptune GJ 436 b

Hum,
interesting diagram in their paper.

Quote:
Planetary mass-radius diagram (adapted from Fortney et al. 2007) comparing the position of Solar System planets, transiting hot Jupiters (diamonds), and GJ 436 b. The lines indicate the position of the Fortney et al. models for different compositions: pure iron, pure silicate, pure water ice (with thermal profiles from Solar System planets), and models for irradiated planets at 0.1 AU from a Solar-type star with a fraction of 10%, 50% and 100% of Hydrogen/Helium. The dotted lines show the models for a cold (a = 10 AU) and very hot (a = 0.02 AU) pure H/He gas giant.
(used under fair use policy)
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File Type: gif Image4.gif (21.6 KB, 44 views)
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Old 16-May-2007, 01:18 PM
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Wow...

I agree with the blogger...Gl 436b is one of the biggest discoveries of the year; we've been looking for a Neptune-sized transiting planet for a long time. This could go a ways towards refining models of planetary size, density, and composition.
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Old 16-May-2007, 01:23 PM
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Quote:
Originally Posted by Blob View Post
Hum,
interesting diagram in their paper.
Very interesting. I know humans love to look for patterns, even when none exist, but it seems to me that one could make a pretty nice curve connecting the points on that graph. I just don't know exactly what it would mean - maybe something about formation mechanisms?
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Old 16-May-2007, 02:49 PM
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