From Cosmic Birth to Living Earths: The Future of UVOIR Space Astronomy
arXiv:1507.04779
Abstract
For the first time in history, humans have reached the point where it is possible to construct a revolutionary space-based observatory that has the capability to find dozens of Earth-like worlds, and possibly some with signs of life. This same telescope, designed as a long-lived facility, would also produce transformational scientific advances in every area of astronomy and astrophysics from black hole physics to galaxy formation, from star and planet formation to the origins of the Solar System. The Association of Universities for Research in Astronomy (AURA) commissioned a study on a next-generation UVOIR space observatory with the highest possible scientific impact in the era following JWST. This community-based study focuses on the future space-based options for UV and optical astronomy that significantly advance our understanding of the origin and evolution of the cosmos and the life within it. The committee concludes that a space telescope equipped with a 12-meter class primary mirror can find and characterize dozens of Earth-like planets and make fundamental advances across nearly all fields of astrophysics. The concept is called the High Definition Space Telescope (HDST). The telescope would be located at the Sun-Earth L2 point and would cover a spectral range that, at a minimum, runs from 0.1 to 2 microns. Unlike JWST, HDST will not need to operate at cryogenic temperatures. HDST can be made to be serviceable on orbit but does not require servicing to complete its primary scientific objectives. We present the scientific and technical requirements for HDST and show that it could allow us to determine whether or not life is common outside the Solar System. We do not propose a specific design for such a telescope, but show that designing, building and funding such a facility is feasible beginning in the next decade - if the necessary strategic investments in technology begin now.
177 pages, 47 figures. Full resolution report and executive summary are available at http://www.hdstvision.org/report . Version 2 fixes several typographical errors
References in corpus (4)
- A Statistical Reconstruction of the Planet Population Around Kepler Solar-Type Stars
- Lower Limits on Aperture Size for an ExoEarth-Detecting Coronagraphic Mission
- Apodized Pupil Lyot Coronagraphs for Arbitrary Apertures. IV. Reduced Inner Working Angle and Increased Robustness to Low-Order Aberrations
- Phase-Occultation Nulling Coronagraphy
Cited by in corpus (26)
- Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment
- Tidal Locking of Habitable Exoplanets
- Identifying Planetary Biosignature Impostors: Spectral Features of CO and O4 Resulting from Abiotic O2/O3 Production
- Organic Haze as a Biosignature in Anoxic Earth-like Atmospheres
- Sulfur Hazes in Giant Exoplanet Atmospheres: Impacts on Reflected Light Spectra
- Observational biases for transiting planets
- Inferring Planetary Obliquity Using Rotational & Orbital Photometry
- The Pale Green Dot: A Method to Characterize Proxima Centauri b using Exo-Aurorae
- Active correction of aperture discontinuities - optimized stroke minimization II: optimization for future missions
- Detectors and cooling technology for direct spectroscopic biosignature characterization
- Focal plane wavefront sensor achromatization : The multireference self-coherent camera
- SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
- High-contrast imager for Complex Aperture Telescopes (HiCAT): 3. first lab results with wavefront control
- Polynomial Apodizers for Centrally Obscured Vortex Coronagraphs
- The direct imaging search for Earth 2.0: Quantifying biases and planetary false positives
- Impact of EDGES 21cm Global Signal on Primordial Power Spectrum
- Valuing life detection missions
- Active correction of aperture discontinuities (ACAD) for space telescope pupils: a parametic analysis
- ATLAST detector needs for direct spectroscopic biosignature characterization in the visible and near-IR
- Exoplanet Atmosphere Measurements from Direct Imaging
- Improved performance of semiconductor laser tracking frequency gauge
- Capabilities of ACAD-OSM, an active method for the correction of aperture discontinuities
- The Astrobiology of the Anthropocene
- Exoplanet Exploration Program Analysis Group (ExoPAG) Report to Paul Hertz Regarding Large Mission Concepts to Study for the 2020 Decadal Survey
- A Response to Elvis' 2015 Critique of the AURA Report "From Cosmic Birth to Living Earths"
- SUPERSHARP - Segmented Unfolding Primary for Exoplanet Research via Spectroscopic High Angular Resolution Photography