Almost every clear night, Avi Loeb, chairman of Harvard’s Astronomy Department, steps
onto his porch and looks up at the Milky Way. The gleaming stars could be the
lights of a giant space ship.
Back inside, Loeb tells his wife what he’s seen. She
tells him it would be OK to leave with the aliens — under certain conditions.
“If there is an extraterrestrial, just make sure they
leave the car keys with me,” Loeb’s wife tells him. “And don’t wake the dog in
the backyard.”
Absent a late-night visit from aliens, how might we
discover if the universe is teeming with life? What tools exist to help the
search?
Loeb, the Frank B. Baird Jr. Professor of Science and
director of the Institute for
Theory and Computation, touched on those questions and others Tuesday at the
Science Center during an hourlong talk titled “New Search Methods for Primitive
and Intelligent Life Far from Earth.” The talk was the latest in a monthly
series that connects the public with insights from scientific research. Mallinckrodt Professor of Physics
Melissa Franklin served as moderator.
The question of whether we’re alone has the potential
to reshape almost every facet of human knowledge, with implications in biology,
history, linguistics, politics, and much more. Our religious beliefs would be
challenged.
Many scientists assume that Earth is the center of the
biological universe and that other galaxies are lifeless, but assumptions
impede discovery, Loeb noted.
“It was once common sense that heavy objects fell
faster than light ones,” he said. “We should simply check our assumptions
rather than make them, especially in the search for intelligent life.”
One such assumption: that objects of the Kuiper belt,
a region of the solar system beyond the orbit of Neptune, emit natural light
reflected by the sun. It could be artificial light, Loeb said. A city the size
of Tokyo could radiate light seen from that distance — if we looked for it,
according to Loeb.
Light could be the key to detecting life beyond the
solar system, Loeb said. Planets have a habitable zone: the right distance from
a star to be warm enough for liquid water. Scientists using powerful telescopes
should be able to view the starlight passing through a planet’s atmosphere to
detect the fingerprints of oxygen and methane, Loeb said.
Such telescopes have already discovered candidates for
observation. The deep-space Kepler satellite has found 3,500 objects. But Loeb
said that the Hubble Space Telescope’s successor, the James Webb Space
Telescope, set to be launched in 2018, will be an even more powerful
investigative tool.
“If we want to detect biological molecules of life in
the next decade, this is the best instrument,” he said.
There are also low-frequency observatories poised to
eavesdrop on RADIO signals from
extraterrestrial civilizations (while our signals head out into space to be
captured). What would we do if we detected such a signal and made contact with
a civilization billions of years older than our own?
“We could ask, ‘What is the nature of dark matter and
dark energy?’” Loeb said. “But it would feel like cheating on an exam.”
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