Earthshine observation of vegetation and implication for life detection on other planets -.pdf
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Space Science Reviews manuscript No.
(will be inserted by the editor)
Luc Arnold
Earthshine observation of vegetation
and implication for life detection on
other planets
A review of 2001 - 2006 works
Received: 23 Feb 2007 - Revised: 26 Jun 2007
Abstract The detection of exolife is one of the goals of very ambitious future
space missions that aim to take direct images of Earth-like planets. While
associations of simple molecules present in the planet’s atmosphere (O2, O3,
CO2 etc.) have been identified as possible global biomarkers, we review here
the detectability of a signature of life from the planet’s surface, i.e. the green
vegetation. The vegetation reflectance has indeed a specific spectrum, with
a sharp edge around 700 nm, known as the ”Vegetation Red Edge” (VRE).
Moreover vegetation covers a large surface of emerged lands, from tropical
evergreen forest to shrub tundra. Thus considering it as a potential global
biomarker is relevant.
Earthshine allows to observe the Earth as a distant planet, i.e. without
spatial resolution. Since 2001, Earthshine observations have been used by
several authors to test and quantify the detectability of the VRE in the
Earth spectrum. The vegetation spectral signature is detected as a small
’positive shift’ of a few percents above the continuum, starting at 700 nm.
This signature appears in most spectra, and its strength is correlated with
the Earth’s phase (visible land versus visible ocean). The observations show
that detecting the VRE on Earth requires a photometric relative accuracy
of 1% or better. Detecting something equivalent on an Earth-like planet will
therefore remain challenging, moreover considering the possibility of mineral
artifacts and the question of ’red edge’ universality in the Universe.
Keywords Earthshine · Earth’s spectrum · biosignature · vegetation red
edge · global biomarker · extrasolar planet
Observatoire de Haute Provenc
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