Exo-Earth yield of a 6 m space telescope in the near-infrared

Rhonda Morgan, Dmitry Savransky, Mario Damiano, Doug Lisman, Bertrand Mennesson, Eric E. Mamajek, Tyler D. Robinson, Michael Turmon

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The Astro2020 Decadal Survey recommended a “future large IR/O/UV telescope optimized for observing habitable exoplanets and general astrophysics” that would “search for biosignatures from a robust number of about 25 habitable zone [exo]planets,”1 now dubbed the Habitable Worlds Observatory (HWO). The search for biosignatures requires high quality spectra over a broad bandwidth and sufficient signal-to-noise. The combination of wavelength, spectral resolution, bandwidth, and signal-to-noise-ratio impacts the number of exo-Earths that can be spectrally characterized. Previous work (Morgan et al. 2022)2 evaluated the number of Earth-size, habitable zone exoplanets (denoted here as yield) that could be spectrally characterized over the wavelength range of 500-1000 nm for a 6-m diameter exoplanet direct imaging mission for coronagraph-only and hybrid coronagraph-starshade architectures for three prior knowledge cases: the nominal case of a blind-search survey, the upper-bound case of perfect prior knowledge, which is useful to determine if target depletion occurs, and the partial prior knowledge case of a hypothetical extreme precision radial velocity survey. In this paper, we extend previous exoplanet yields to include wavelengths out to 1.8 microns. Because the IWA for coronagraphs is proportional to wavelength, the achievable spectral coverage will be different for every planet detected. We present the spectral coverage achieved across individual target stars, as well as the ensemble target set, for a coronagraph-only architecture and a hybrid coronagraph + starshade architecture. We use the three prior knowledge cases. The coronagraph spectral characterization is simulated in the near-infrared for each of the 10% sub-bands individually, as if it were the only spectral characterization performed during the mission, and then as a broadband spectral characterization performed in sequence over the sub-bands. The starshade achieves the broadband spectral equivalent simultaneously. We also examine the capabilities of the 60 m starshade point design and investigate the benefits of refueling.

Original languageEnglish (US)
Title of host publicationTechniques and Instrumentation for Detection of Exoplanets XI
EditorsGarreth J. Ruane
PublisherSPIE
ISBN (Electronic)9781510665743
DOIs
StatePublished - 2023
Externally publishedYes
EventTechniques and Instrumentation for Detection of Exoplanets XI 2023 - San Diego, United States
Duration: Aug 21 2023Aug 24 2023

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume12680
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceTechniques and Instrumentation for Detection of Exoplanets XI 2023
Country/TerritoryUnited States
CitySan Diego
Period8/21/238/24/23

Keywords

  • coronagraph
  • exoplanets
  • extreme precision radial velocity
  • Future Great Observatory
  • HabEx
  • HWO
  • LUVOIR
  • starshade

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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