Anne-Marie Lagrange 1 et al 1 Laboratoire d’Astrophysique de Grenoble, France IAU276 – October,...
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Transcript of Anne-Marie Lagrange 1 et al 1 Laboratoire d’Astrophysique de Grenoble, France IAU276 – October,...
Anne-Marie Lagrange 1 et al
1Laboratoire d’Astrophysique de Grenoble, France
IAU276 – October, 11, 2010
The candidate companion around b Pictoris
HR8799 bcd (~7-10MJup; 24,38,64AU)Marois et al. (2008)
Formation process ??
Fomalhautb (<3MJup; 115AU)Kalas et al. (2008)
2M1207B (~5-8MJup; 50AU)Chauvin et al. (2004;2005)
ABPic b (~13MJup; 250AU)Chauvin et al. (2005a)
Planet candidate around beta Pictoris
Lagrange et al (2009a, 2009b)
400mas
N
E
Planet candidate . ΔL’ = 7.7 ± 0.3 => M~9MJup if bound. Sep = 411 ± 8 mas (~8 AU) proj. P.A. = 31.8 ± 1.3 deg (disk P.A. ~ 33 deg)Teff ~1500KAge ~12 Myr
VLT/NaCo2003
February 2009
Lagrange et al (2009); see also Fitzgerald and Kalas (2009)
6s limit( L_abs=9.8)
After quad.
Before quad.
Augereau et al. (2001b)
Planet on an inclined orbit, 10 AU
~ 80 UA
Augereau et al. (2001b)Augereau et al. (2001b)
Mouillet et al. (1997)
90’s: Falling Evaporating Bodies onb Pictoris=> indirect evidence for planet ?
Vidal-Madjar, Lagrange, Beust, Morbidelli…
A massive Giant Planet at ~10AU explains: The inner warp and other disk asymetries
The FEBs
Implications on planet formation scenari : Giant Planets form rapidly (< a few Myr) Formation process: could be core accretion (see Keenedy & Kenyon 08) Test of evolutionary model: unique test given its short period