Literature DB >> 22077375

Properties of an Earth-like planet orbiting a Sun-like star: Earth observed by the EPOXI mission.

Timothy A Livengood1, L Drake Deming, Michael F A'hearn, David Charbonneau, Tilak Hewagama, Carey M Lisse, Lucy A McFadden, Victoria S Meadows, Tyler D Robinson, Sara Seager, Dennis D Wellnitz.   

Abstract

NASA's EPOXI mission observed the disc-integrated Earth and Moon to test techniques for reconnoitering extrasolar terrestrial planets, using the Deep Impact flyby spacecraft to observe Earth at the beginning and end of Northern Hemisphere spring, 2008, from a range of ∼1/6 to 1/3 AU. These observations furnish high-precision and high-cadence empirical photometry and spectroscopy of Earth, suitable as "ground truth" for numerically simulating realistic observational scenarios for an Earth-like exoplanet with finite signal-to-noise ratio. Earth was observed at near-equatorial sub-spacecraft latitude on 18-19 March, 28-29 May, and 4-5 June (UT), in the range of 372-4540 nm wavelength with low visible resolving power (λ/Δλ=5-13) and moderate IR resolving power (λ/Δλ=215-730). Spectrophotometry in seven filters yields light curves at ∼372-948 nm filter-averaged wavelength, modulated by Earth's rotation with peak-to-peak amplitude of ≤20%. The spatially resolved Sun glint is a minor contributor to disc-integrated reflectance. Spectroscopy at 1100-4540 nm reveals gaseous water and carbon dioxide, with minor features of molecular oxygen, methane, and nitrous oxide. One-day changes in global cloud cover resulted in differences between the light curve beginning and end of ≤5%. The light curve of a lunar transit of Earth on 29 May is color-dependent due to the Moon's red spectrum partially occulting Earth's relatively blue spectrum. The "vegetation red edge" spectral contrast observed between two long-wavelength visible/near-IR bands is ambiguous, not clearly distinguishing between the verdant Earth diluted by cloud cover versus the desolate mineral regolith of the Moon. Spectrophotometry in at least one other comparison band at short wavelength is required to distinguish between Earth-like and Moon-like surfaces in reconnaissance observations. However, measurements at 850 nm alone, the high-reflectance side of the red edge, could be sufficient to establish periodicity in the light curve and deduce Earth's diurnal period and the existence of fixed surface units.

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Year:  2011        PMID: 22077375     DOI: 10.1089/ast.2011.0614

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  11 in total

1.  The dependence of the ice-albedo feedback on atmospheric properties.

Authors:  P von Paris; F Selsis; D Kitzmann; H Rauer
Journal:  Astrobiology       Date:  2013-10-10       Impact factor: 4.335

2.  Nonphotosynthetic pigments as potential biosignatures.

Authors:  Edward W Schwieterman; Charles S Cockell; Victoria S Meadows
Journal:  Astrobiology       Date:  2015-05-05       Impact factor: 4.335

Review 3.  Exoplanet Biosignatures: Observational Prospects.

Authors:  Yuka Fujii; Daniel Angerhausen; Russell Deitrick; Shawn Domagal-Goldman; John Lee Grenfell; Yasunori Hori; Stephen R Kane; Enric Pallé; Heike Rauer; Nicholas Siegler; Karl Stapelfeldt; Kevin B Stevenson
Journal:  Astrobiology       Date:  2018-06       Impact factor: 4.335

4.  Spectral fingerprints of Earth-like planets around FGK stars.

Authors:  Sarah Rugheimer; Lisa Kaltenegger; Andras Zsom; Antígona Segura; Dimitar Sasselov
Journal:  Astrobiology       Date:  2013-03       Impact factor: 4.335

5.  Geology and photometric variation of solar system bodies with minor atmospheres: implications for solid exoplanets.

Authors:  Yuka Fujii; Jun Kimura; James Dohm; Makiko Ohtake
Journal:  Astrobiology       Date:  2014-09       Impact factor: 4.335

Review 6.  Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life.

Authors:  Edward W Schwieterman; Nancy Y Kiang; Mary N Parenteau; Chester E Harman; Shiladitya DasSarma; Theresa M Fisher; Giada N Arney; Hilairy E Hartnett; Christopher T Reinhard; Stephanie L Olson; Victoria S Meadows; Charles S Cockell; Sara I Walker; John Lee Grenfell; Siddharth Hegde; Sarah Rugheimer; Renyu Hu; Timothy W Lyons
Journal:  Astrobiology       Date:  2018-05-04       Impact factor: 4.335

7.  The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants.

Authors:  Victoria S Meadows; Giada N Arney; Edward W Schwieterman; Jacob Lustig-Yaeger; Andrew P Lincowski; Tyler Robinson; Shawn D Domagal-Goldman; Russell Deitrick; Rory K Barnes; David P Fleming; Rodrigo Luger; Peter E Driscoll; Thomas R Quinn; David Crisp
Journal:  Astrobiology       Date:  2018-02-12       Impact factor: 4.335

Review 8.  Exoplanet Biosignatures: A Framework for Their Assessment.

Authors:  David C Catling; Joshua Krissansen-Totton; Nancy Y Kiang; David Crisp; Tyler D Robinson; Shiladitya DasSarma; Andrew J Rushby; Anthony Del Genio; William Bains; Shawn Domagal-Goldman
Journal:  Astrobiology       Date:  2018-04-20       Impact factor: 4.335

Review 9.  Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment.

Authors:  Victoria S Meadows; Christopher T Reinhard; Giada N Arney; Mary N Parenteau; Edward W Schwieterman; Shawn D Domagal-Goldman; Andrew P Lincowski; Karl R Stapelfeldt; Heike Rauer; Shiladitya DasSarma; Siddharth Hegde; Norio Narita; Russell Deitrick; Jacob Lustig-Yaeger; Timothy W Lyons; Nicholas Siegler; J Lee Grenfell
Journal:  Astrobiology       Date:  2018-05-10       Impact factor: 4.335

10.  Moonshine: Diurnally varying hydration through natural distillation on the Moon, detected by the Lunar Exploration Neutron Detector (LEND).

Authors:  T A Livengood; G Chin; R Z Sagdeev; I G Mitrofanov; W V Boynton; L G Evans; M L Litvak; T P McClanahan; A B Sanin; R D Starr; J J Su
Journal:  Icarus       Date:  2015-07-15       Impact factor: 3.508

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