Clio: A 5 micron camera for the detection of giant exoplanets

Melanie Freed, Philip M. Hinz, Michael R. Meyer, N. Mark Milton, Michael Lloyd-Hart

Research output: Contribution to journalConference article

31 Scopus citations

Abstract

We plan to take advantage of the unprecedented combination of low thermal background and high resolution provided by the 6.5m MMT's adaptive secondary mirror, to target the 3-5 micron atmospheric window where giant exoplanets are expected to be anomalously bright. We are in the process of building a 3-5 micron camera that we will use to carry out a survey to characterize the prevalence and distribution of giant planets around nearby, Sun-like stars. Sensitivity estimates show that for a 1 Gyr old GOV primary at 10 pc, we expect to detect 5 MJupiter and 15 MJupiter exoplanets at angular separations greater than 0.45-2.1" and 0.2-1.2" respectively. Monte Carlo simulations based on these sensitivity estimates and a sample of 80 young (<1 Gyr), nearby (<20 pc) MOV-FOV stars, predict the detection of 15±3 exoplanets with masses of 4-15 MJupiter and separations of 17-50 AU. Construction of the camera is currently underway and on-telescope testing is expected in the Fall 2004-Winter 2005.

Original languageEnglish (US)
Pages (from-to)1561-1571
Number of pages11
JournalProceedings of SPIE - The International Society for Optical Engineering
Volume5492
Issue numberPART 3
DOIs
StatePublished - Dec 24 2004
EventGround-based Instrumentation for Astronomy - Glasgow, United Kingdom
Duration: Jun 21 2004Jun 25 2004

Keywords

  • Adaptive optics
  • Exoplanets
  • Imaging
  • Thermal infrared

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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