Scientific American - February 2019

(Rick Simeone) #1
58 Scientific American, February 2019

PRECEDING PAGES: NASA AND JPL

Shortly afterward, though, scientists cobbled to -
geth er plans for a bargain-priced spacecraft ($680
million) made of leftover hardware and, miraculously,
saved the mission. In 1989 the Magellan orbiter launched
on a reconnaissance mission to Venus, and by 1990 it
was in orbit. Over the next five years the orbiter
returned near-global radar images, gravity data and a
topographic map of the second planet from the sun. It
was the latest in a long line of Soviet and U.S. missions
to our neighboring planet, but when Magellan
plunged to Venus’s surface in 1994, NASA’s support for
Venus spacecraft died with it. Since then, scientists
have submitted more than 25 proposals for return
missions to Venus, and although some of those
received high rankings from review boards, none were
approved. Decades-old data gathered by Magellan re-

main the foundation of Venus geoscience to this day.
But planetary scientists never give up, and we have
made progress in uncovering the secrets of this world
nonetheless. Since Magellan, the European and Japa-
nese space agencies have sent successful missions to
Venus, leading to breakthroughs in understanding its
atmosphere. Meanwhile scientists have been busy
rewriting the textbooks on our sister planet by per-
forming new analyses of Magellan data. We now think
that volcanoes are rampant on Venus, and we have
even found hints of the start of plate tectonics, which
scientists think is critical for a planet’s habitability.
New theoretical models also suggest Venus may have
had liquid water on its surface until relatively late in
its history—meaning that it may have been hospitable
to life much longer than we once thought.




N 1982 ALL ANYONE COULD TALK ABOUT IN THE PLANETARY SCIENCE DEPARTMENT AT THE
Massachusetts Institute of Technology was the cancellation of NASA’s latest flagship mis-
sion, the Venus Orbital Imaging Radar (VOIR). One of us (Dyar) was a graduate student
there at the time. (The other two were still in college and elementary school.) Graduate
students wept openly in the hallways, and veteran faculty shook their heads. The newly
elected Reagan administration had enacted sweeping cuts to space exploration, and VOIR
was one of the casualties.

M. Darby Dyar is a mineral spectroscopist who studies extraterrestrial
minerals and glasses from the moon, Mars, comets and asteroids.
She is a senior scientist at the Planetary Science Institute and Kennedy-
3Zr›šæ§«|0Í«{rÒÒ«Í«{ ÒÜÍ«§«¡ëDÜ$«æ§Ü«›ë«šr «››r†r»

Suzanne E. Smrekar ÒÜæf”rÒܐrf”|rÍr§Ür諛æܔ«§DÍëμDܐÒ
{«ÍÍ«Zšëμ›D§rÜÒdé”ܐ«ZZDҔ«§D›r›fé«ÍšDÜ諛ZD§«rÒ»
3r”ÒDÒr§”«ÍÍrÒrDÍZÒZ”r§Ü”ÒÜD§ffrμæÜëμ͔§Z”μD›”§èrÒܔ†DÜ«Í
of the InSight Mission at NASA’s Jet Propulsion Laboratory,
where the mountain biking is awesome.

Ü«Í

Stephen R. Kane is a planetary astrophysicist who has
f”ÒZ«èrÍrfæ§fÍrfÒ«{rê«μ›D§rÜÒD§fÒÜæf”rÒܐr”Íμ«Ür§Ü”D›
{«ÍDO”ÜDO”›”Üë»r”ÒD§DÒÒ«Z”DÜrμÍ«{rÒÒ«Í”§ܐrfrμDÍÜ¡r§Ü
«{rDÍܐÒZ”r§ZrÒDÜܐr7§”èrÍҔÜë«{ D›”{«Í§”Dd2”èrÍҔfr»

IN BRIEF

Venus and Ear th started out much the same,
but at some point, the planets diverged. Earth
went on to host oceans and an atmosphere.

Venus’s surface, meanwhile, became inhospitable
to life. Yet our neighboring planet still has active
volcanism and hints of nascent plate tectonics.

Learning why Venus evolved the way it did could illu-
minate the possibilities for life on the many Venus- like
exoplanets out there. A new mission to Venus is needed.

© 2019 Scientific American
Free download pdf