Constraining the orbit of the possible companion to Β pictoris

A. M. Lagrange, M. Kasper, A. Boccaletti, G. Chauvin, D. Gratadour, T. Fusco, D. Ehrenreich, D. Apai, D. Mouillet, D. Rouan

Research output: Contribution to journalArticle

35 Scopus citations

Abstract

Context.We recently reported on the detection of a possible planetary mass companion to β Pictoris at a projected separation of 8 AU from the star, using data taken in November 2003 with NaCo, the adaptive-optics system installed on the Very Large Telescope UT4. Even though no second epoch detection was available, there are strong arguments to favor a gravitationally bound companion rather than a background object. If confirmed and located at a physical separation of 8 AU, this companion would be the closest planet ever imaged, and above all, could have formed via core-accretion. Its apparent magnitude would indicate a typical temperature of ∼1500 K and a mass of ∼8 MJup. Interestingly, a planet with such characteristics would explain the main morphological and dynamical peculiarities of the β Pic system. Aims.Our goal was to re-observe β Pic five years later to again detect the companion or, in the case of a non-detection, constrain its orbit. Methods. Deep adaptive-optics L'-band direct images of β Pic as well as Ks-band Four Quadrant Phase Mask coronagraph images with were recorded with NaCo. Results. No point-like signal with the brightness of the companion candidate (apparent magnitudes L' = 11.2 or Ks ≃ 12.5) was detected at projected distances down to ≃6.5 AU in the present data from the star (by comparison, the same limit was reached at ≃5.5 AU in the better quality November 2003 data). As expected, the non detection does not allow us to rule out a background companion from an observational point of view. We show that the non detection is consistent with orbital motion. Using these data and previous Ks-band data obtained in 2004, we place strong constraints on the possible orbits of the companion.

Original languageEnglish (US)
Pages (from-to)927-934
Number of pages8
JournalAstronomy and astrophysics
Volume506
Issue number2
DOIs
StatePublished - Nov 1 2009

    Fingerprint

Keywords

  • Instrumentation: adaptive optics
  • Stars: early-type
  • Stars: individual: Β pictoris
  • Stars: planetary systems

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Lagrange, A. M., Kasper, M., Boccaletti, A., Chauvin, G., Gratadour, D., Fusco, T., Ehrenreich, D., Apai, D., Mouillet, D., & Rouan, D. (2009). Constraining the orbit of the possible companion to Β pictoris. Astronomy and astrophysics, 506(2), 927-934. https://doi.org/10.1051/0004-6361/200912098