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Beyond the horizon of the 2020 missions and
the search for biosignatures lie two other lofty
and longstanding Red Planet objectives: returning
rock and soil samples to Earth, and, eventually,
sending humans to explore Mars in person. These
goals have been stated and reiterated by space
agencies, planetary scientists and space enthusiasts
for decades, including in a NASA authorization
bill signed by President Trump in March that
reaffirmed the agency’s goal of sending humans to
Mars in the 2030s.
Past missions, particularly landers, have collected
valuable data related to entry, descent and landing
through the atmosphere, as well as weather and
radiation conditions at the surface, all of which could
broadly inform more ambitious sample return or
manned missions. To date, though, little headway
has been made in directly addressing the particularchallenges of these missions. Some of the 2020
efforts, if successful, may change this.
In addition to continuing studies of weather and
entry, descent and landing conditions, one of the
main tasks for NASA’s 2020 rover will be to not
only drill and analyze rocks, as Curiosity did, but also
to stow, or cache, up to about 30 15-gram samples
in secure containers that could be retrieved and
returned to Earth by a future mission. Although both
NASA’s rover and the ExoMars rover are equipped
with sensitive instrumentation for hunting for signs
of life, remotely determining whether a biosigna-
ture on Mars represents unequivocal evidence of
extraterrestrial life would be extremely difficult, and
likely controversial. “The reality is that the burden
of proof for the detection of life outside of Earth is
enormously high, and it’s unlikely that the instru-
ments we have on board will overcome that burden,”
Farley says. “By bringing samples back to Earth, we
can apply the whole arsenal of instrumentation that3&&MWIZEPYEXMRKXLVIIGERHMHEXIPERHMRKWMXIWJSVMXWȶȉȶȉVSZIV/I^IVS(VEXIVERH3]VXMW2ENSVMRXLIRSVXLIVRLIQMWTLIVI
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