Properties of an Earth-Like Planet Orbiting a Sun-Like Star: Earth Observed by the EPOXI Mission

被引:63
|
作者
Livengood, Timothy A. [1 ,2 ]
Deming, L. Drake [1 ]
A'Hearn, Michael F. [3 ]
Charbonneau, David [4 ]
Hewagama, Tilak [1 ,3 ]
Lisse, Carey M. [5 ]
McFadden, Lucy A. [1 ]
Meadows, Victoria S. [6 ]
Robinson, Tyler D. [6 ]
Seager, Sara [7 ]
Wellnitz, Dennis D. [3 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Natl Ctr Earth & Space Sci Educ, Capital Hts, MD USA
[3] Univ Maryland, College Pk, MD 20742 USA
[4] Harvard Univ, Cambridge, MA 02138 USA
[5] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[6] Univ Washington, Seattle, WA 98195 USA
[7] MIT, Cambridge, MA 02139 USA
关键词
Atmospheric composition; Biomarkers; Life detection; Habitability; Extrasolar terrestrial planets; EPOXI mission; Light curves; Exoplanets; DISK-AVERAGED SPECTRA; DEEP IMPACT; SYNTHETIC SPECTRA; LIGHT-CURVES; EXTRASOLAR; PHOTOSYNTHESIS; DETECTABILITY; NUCLEUS; SEARCH; OCEANS;
D O I
10.1089/ast.2011.0614
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 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 372-4540nm wavelength with low visible resolving power (lambda/Delta lambda=5-13) and moderate IR resolving power (lambda/Delta lambda=215-730). Spectrophotometry in seven filters yields light curves at similar to 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.
引用
收藏
页码:907 / 930
页数:24
相关论文
共 50 条
  • [21] An Earth-sized planet with an Earth-like density
    Francesco Pepe
    Andrew Collier Cameron
    David W. Latham
    Emilio Molinari
    Stéphane Udry
    Aldo S. Bonomo
    Lars A. Buchhave
    David Charbonneau
    Rosario Cosentino
    Courtney D. Dressing
    Xavier Dumusque
    Pedro Figueira
    Aldo F. M. Fiorenzano
    Sara Gettel
    Avet Harutyunyan
    Raphaëlle D. Haywood
    Keith Horne
    Mercedes Lopez-Morales
    Christophe Lovis
    Luca Malavolta
    Michel Mayor
    Giusi Micela
    Fatemeh Motalebi
    Valerio Nascimbeni
    David Phillips
    Giampaolo Piotto
    Don Pollacco
    Didier Queloz
    Ken Rice
    Dimitar Sasselov
    Damien Ségransan
    Alessandro Sozzetti
    Andrew Szentgyorgyi
    Christopher A. Watson
    Nature, 2013, 503 : 377 - 380
  • [22] An Earth-sized planet with an Earth-like density
    Pepe, Francesco
    Cameron, Andrew Collier
    Latham, David W.
    Molinari, Emilio
    Udry, Stephane
    Bonomo, Aldo S.
    Buchhave, Lars A.
    Charbonneau, David
    Cosentino, Rosario
    Dressing, Courtney D.
    Dumusque, Xavier
    Figueira, Pedro
    Fiorenzano, Aldo F. M.
    Gettel, Sara
    Harutyunyan, Avet
    Haywood, Raphaelle D.
    Horne, Keith
    Lopez-Morales, Mercedes
    Lovis, Christophe
    Malavolta, Luca
    Mayor, Michel
    Micela, Giusi
    Motalebi, Fatemeh
    Nascimbeni, Valerio
    Phillips, David
    Piotto, Giampaolo
    Pollacco, Don
    Queloz, Didier
    Rice, Ken
    Sasselov, Dimitar
    Segransan, Damien
    Sozzetti, Alessandro
    Szentgyorgyi, Andrew
    Watson, Christopher A.
    NATURE, 2013, 503 (7476) : 377 - +
  • [23] Venus as a more Earth-like planet
    Svedhem, Hakan
    Titov, Dmitry V.
    Taylor, Fredric W.
    Witasse, Olivier
    NATURE, 2007, 450 (7170) : 629 - 632
  • [24] Spectral evolution of an Earth-like planet
    Kaltenegger, Lisa
    Traub, Wesley A.
    Jucks, Kenneth W.
    ASTROPHYSICAL JOURNAL, 2007, 658 (01): : 598 - 616
  • [25] Venus as a more Earth-like planet
    Håkan Svedhem
    Dmitry V. Titov
    Fredric W. Taylor
    Olivier Witasse
    Nature, 2007, 450 : 629 - 632
  • [26] Polarization of Planet Earth and model Earth-like planets
    Wolstencroft, Ramon D.
    Breon, Francois-Marie
    Astronomical Polarimetry: Current Status and Future Directions, 2005, 343 : 211 - 212
  • [27] Most Earth-like planet yet
    不详
    SCIENCE, 2015, 349 (6247) : 457 - 457
  • [28] What makes a planet 'Earth-like'?
    Robinson, Brian
    NEW SCIENTIST, 2015, 227 (3037) : 54 - 54
  • [29] Looking for earth-like planets with the SIM planet quest light mission
    Goullioud, R.
    Catanzarite, J. H.
    2008 IEEE AEROSPACE CONFERENCE, VOLS 1-9, 2008, : 1729 - 1737
  • [30] Analysis of Planet Effect of Reference Star On Searching for Earth-like Planets
    Pan, Xiaopei
    Shao, Michael
    OPTICAL AND INFRARED INTERFEROMETRY, 2008, 7013