Earth as an Exoplanet: A Two-dimensional Alien Map
Abstract
Resolving spatially varying exoplanet features from single-point light curves is essential for determining whether Earth-like worlds harbor geological features and/or climate systems that influence habitability. To evaluate the feasibility and requirements of this spatial-feature resolving problem, we present an analysis of multi-wavelength single-point light curves of Earth, where it plays the role of a proxy exoplanet. Here, ~10,000 Deep Space Climate Observatory/Earth Polychromatic Imaging Camera frames collected over a two-year period were integrated over the Earth's disk to yield a spectrally dependent point source and analyzed using singular value decomposition. We found that, between the two dominant principal components (PCs), the second PC contains surface-related features of the planet, while the first PC mainly includes cloud information. We present the first two-dimensional (2D) surface map of Earth reconstructed from light curve observations without any assumptions of its spectral properties. This study serves as a baseline for reconstructing the surface features of Earth-like exoplanets in the future.
Additional Information
© 2019 The American Astronomical Society. Received 2019 July 1; revised 2019 August 5; accepted 2019 August 12; published 2019 August 27. This work was partly supported by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. Y.L.Y. and D.C. acknowledge support by the Virtual Planetary Laboratory at the University of Washington. We thank Lixiang Gu and Mimi Gerstell for proofreading the manuscript.Attached Files
Published - Fan_2019_ApJL_882_L1.pdf
Accepted Version - 1908.04350.pdf
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Additional details
- Eprint ID
- 98277
- Resolver ID
- CaltechAUTHORS:20190828-074526085
- NASA/JPL/Caltech
- University of Washington
- Created
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2019-08-28Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department, Division of Geological and Planetary Sciences