Spatially resolved spectroscopy of the exoplanet HR 8799 c

Jan, 2010
4 pages
Published in:
  • Astrophys.J.Lett. 710 (2010) L35
e-Print:

Citations per year

2010201120122013131097
Abstract: (arXiv)
HR 8799 is a multi-planet system detected in direct imaging, with three companions known so far. Here, we present spatially resolved VLT/NACO 3.88--4.10 micron spectroscopy of the middle planet, HR 8799 c, which has an estimated mass of ~10 Mjup, temperature of ~1100 K and projected separation of 38 AU. The spectrum shows some differences in the continuum from existing theoretical models, particularly longwards of 4 microns, implying that detailed cloud structure or non-equilibrium conditions may play an important role in the physics of young exoplanetary atmospheres.