English

Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission

Earth and Planetary Astrophysics 2022-08-10 v4 Instrumentation and Methods for Astrophysics

Abstract

One of the long-term goals of exoplanet science is the atmospheric characterization of dozens of small exoplanets in order to understand their diversity and search for habitable worlds and potential biosignatures. Achieving this goal requires a space mission of sufficient scale. We seek to quantify the exoplanet detection performance of a space-based mid-infrared nulling interferometer that measures the thermal emission of exoplanets. For this, we have developed an instrument simulator that considers all major astrophysical noise sources and coupled it with Monte Carlo simulations of a synthetic exoplanet population around main-sequence stars within 20 pc. This allows us to quantify the number (and types) of exoplanets that our mission concept could detect over a certain time period. Two different scenarios to distribute the observing time among the stellar targets are discussed and different apertures sizes and wavelength ranges are considered. Within a 2.5-year initial search phase, an interferometer consisting of four 2 m apertures with a total instrument throughput of 5% covering a wavelength range between 4 and 18.5 μ\mum could detect up to ~550 exoplanets with radii between 0.5 and 6 R_\oplus with an integrated SNR\ge7. At least ~160 of the detected exoplanets have radii \le1.5 R_\oplus. Depending on the observing scenario, ~25-45 rocky exoplanets (objects with radii between 0.5 and 1.5 _{\oplus}) orbiting within the empirical habitable zone (eHZ) of their host stars are among the detections. With an aperture size of 3.5 m, the total number of detections can increase to up to ~770, including ~60-80 rocky, eHZ planets. With 1 m aperture size, the maximum detection yield is ~315 exoplanets, including \le20 rocky, eHZ planets. In terms of predicted detection yield, such a mission can compete with large single-aperture reflected light missions. (abridged)

Keywords

Cite

@article{arxiv.2101.07500,
  title  = {Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission},
  author = {S. P. Quanz and M. Ottiger and E. Fontanet and J. Kammerer and F. Menti and F. Dannert and A. Gheorghe and O. Absil and V. S. Airapetian and E. Alei and R. Allart and D. Angerhausen and S. Blumenthal and L. A. Buchhave and J. Cabrera and Ó. Carrión-González and G. Chauvin and W. C. Danchi and C. Dandumont and D. Defrère and C. Dorn and D. Ehrenreich and S. Ertel and M. Fridlund and A. García Muñoz and C. Gascón and J. H. Girard and A. Glauser and J. L. Grenfell and G. Guidi and J. Hagelberg and R. Helled and M. J. Ireland and M. Janson and R. K. Kopparapu and J. Korth and T. Kozakis and S. Kraus and A. Léger and L. Leedjärv and T. Lichtenberg and J. Lillo-Box and H. Linz and R. Liseau and J. Loicq and V. Mahendra and F. Malbet and J. Mathew and B. Mennesson and M. R. Meyer and L. Mishra and K. Molaverdikhani and L. Noack and A. V. Oza and E. Pallé and H. Parviainen and A. Quirrenbach and H. Rauer and I. Ribas and M. Rice and A. Romagnolo and S. Rugheimer and E. W. Schwieterman and E. Serabyn and S. Sharma and K. G. Stassun and J. Szulágyi and H. S. Wang and F. Wunderlich and M. C. Wyatt and the LIFE collaboration},
  journal= {arXiv preprint arXiv:2101.07500},
  year   = {2022}
}

Comments

Accepted for publication by A&A - some typos corrected and affiliations updated; 14 pages main text (incl. 14 figures); first paper in the LIFE paper series; papers II (arXiv:2203.00471) and III (arXiv:2112.02054) are also available