Extrasolar Visions II
Would you like to react to this message? Create an account in a few clicks or log in to continue.

Extrasolar Visions II

Extrasolar Planets.
 
HomeHome  SearchSearch  Latest imagesLatest images  RegisterRegister  Planet TablePlanet Table  Log in  

 

 G 196-3 B or b? - Revised mass

Go down 
AuthorMessage
Edasich
dK star
dK star
Edasich


Number of posts : 2292
Location : Tau Ceti g - Mid Latitudes
Registration date : 2008-06-02

G 196-3 B or b? - Revised mass Empty
PostSubject: G 196-3 B or b? - Revised mass   G 196-3 B or b? - Revised mass Empty23rd September 2011, 3:38 am

Not sure whether it goes to Unconfirmed Planets thread. In that case, shift this discussion there

Do you remember G 196-3 B in Extrasolar Vision I website? Previously classed as brown dwarf companion, but according to EPE's new planetary upper limit and Zapatero Osorio et al. (2010) new mass estimate, this objects well falls witihin massive planets' domain, with mass between 12 and 25 Jupiter masses (18.5 ± 6.5 Jupiter masses, I would say).

Paper Infrared and Kinematic Properties of the Substellar Object G 196-3 B

Quote :
We report unusual near- and mid-infrared photometric properties of G 196-3 B, the young substellar companion at 16'' from the active M2.5-type star G 196-3 A, using data taken with the IRAC and MIPS instruments onboard Spitzer. G 196-3 B shows markedly redder colors at all wavelengths from 1.6 up to 24 μm than expected for its spectral type, which is determined at L3 from optical and near-infrared spectra. We discuss various physical scenarios to account for its reddish nature and conclude that a low-gravity atmosphere with enshrouded upper atmospheric layers and/or a warm dusty disk/envelope provides the most likely explanations, the two of them consistent with an age in the interval 20-300 Myr. We also present new and accurate separate proper motion measurements for G 196-3 A and B confirming that both objects are gravitationally linked and share the same motion within a few mas yr-1. After integration of the combined spectrophotometric spectral energy distributions, we obtain the result that the difference in the bolometric magnitudes of G 196-3 A and B is 6.15 ± 0.10 mag. Kinematic consideration of the Galactic space motions of the system for distances in the interval 15-30 pc suggests that the pair is a likely member of the Local Association and that it lies near the past positions of young star clusters like α Persei less than 85 Myr ago, where the binary might have originated. At these young ages, the mass of G 196-3 B would be in the range 12-25 M Jup, close to the frontier between planets and brown dwarfs.


Emphasis mine.
Back to top Go down
 
G 196-3 B or b? - Revised mass
Back to top 
Page 1 of 1
 Similar topics
-
» Revised mass and orbit of Cha Hα b - Definitely not a planet
» Revised mass for 1RXS J1609-2105b
» FN Lyr - Low-mass companion?
» MOA-192 b's mass revisited?
» Revised Orbital Solutions for 94 Exoplanetary Systems

Permissions in this forum:You cannot reply to topics in this forum
Extrasolar Visions II :: Extrasolar Visions :: Extrasolar News and Discoveries-
Jump to: