Sharing Life Could Be Easy
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How could life be shared between planets in close proximity to one
another? This question has received a greater insight thanks to new
analytics based on previously known and new calculations. The findings
from this new research are helping scientists understand how likely
life would be on a given planet in such tight-knit systems if that world
shows signs of habitability. This approach began with a blasphemous-at-the-time idea: that life
exists throughout the universe and can travel without supernatural
interference. Anaxagoras, a 5th-century B.C. Greek philosopher, called
this concept "panspermia."
Kelvin, Helmholtz and Arrhenius advanced the idea in the 19th and 20th
centuries by examining how life could be carried to and from Earth. In
2009, Stephen Hawking went beyond our solar system with the idea when he
suggested that "life could spread from planet to planet or from stellar
system to stellar system, carried on meteors." [5 Bold Claims of Alien Life] Dimitri Veras, an astrophysicist at the University of Warwick in
England and lead author of a recent paper on the subject, said, "Within
the last century, [panspermia] has been focused on life transport within
the solar system, including Earth." The TRAPPIST-1 solar system,
which is 39 light-years from Earth and includes seven planets packed
into an orbit smaller than Mercury's, changes this Earth-centric idea.
This system's sun is an ultracool red dwarf. So, even though the seven
nearby planets orbit closely, they are possibly all still in the
habitable zone, to varying degrees depending upon the makeup of their
atmospheres. That makes this system a perfect model for exploring the
idea of panspermia, per Hawking, anywhere in the universe.
use and are general enough to be applicable to a wide variety
of systems." [Exoplanet Discovery: The 7 Earth-Size Planets of TRAPPIST-1 in Pictures] But back to our solar system, where the "foundation for
panspermia-related processes has been established," Veras' paper said.
That includes evidence that life can survive the three stages of
traveling from one planet to another: initial ejection, the journey
through space between planets and impact onto a new planet. Each stage presents challenges to the survival of life.
Veras wanted to create an analytical system to quantify each of these
parts to create a better understanding of the probability of the whole
process occurring.
He had some information to start with: Microbes can survive ejection
from a planet with life on it, as per previous studies, and even a
voyage through interplanetary space, if shielded from the radiation and
cold. Less is known about how well a microbe that endured space travel
could survive impact on a new planet, which would be necessary for life
to complete the voyage from one planet to another.
Because impact includes more unknowns than ejection and transit between
planets, Veras had less-detailed information to work with in this area
of his calculations.
"The physics of re-entry features complexities that are not present
with the ejection and voyage phases through space," he said. "For
example, frictional heating during re-entry can lead to the formation of
a fusion crust [the outer layer of the meteorite that melts and ablates
during atmospheric entry] on the surface of the meteorite."
To figure out how to calculate the tricky physics of atmospheric entry
onto a new planet, Veras turned to some already-available math. He told
Astrobiology Magazine that "Equations regarding the physics of impact
have already been established and used for solar system applications,
[so] we converted those for use in a general extrasolar system."
To understand the probability of ejected material traveling from one
planet to another, Veras combined his equations into analytics. This
way, he could figure out the whole system of panspermia, not just parts
of it.
"Usually, the dynamics of panspermia is studied with numerical
simulations. However, these can be slow to run and must be tailored to
an individual system," Veras said. "Alternatively, analytics are much
faster to use and are general enough to be applicable to a wide variety of systems."
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