At first glance, this story might not seem to have much of a
connection to the question of life in the universe, the planet I'm about to
discuss is probably about as hostile and uninhabitable as they get, but in fact
it answers a long-standing question about exoplanet atmospheres and just where
they can exist. That, in turn, has implications for where life, at least as we
know it here on earth, can arise.
GJ 1132b is an exoplanet discovered around a star located
about 39 light years away from us. It's a small planet, just a bit larger than
Earth and is thought to be rocky. It's been called a potential Venus twin due
likely having a very high surface temperature similar to Venus, though it's
probably even hotter. It was also thought to likely have some type of thick
atmosphere, though the composition was unknown. This atmosphere has now been
directly observed.
Scientists have observed the atmospheres of exoplanets
before, though up until now it was limited to gas giants and planets much
larger than earth. This is the first time they've directly observed a planet
with an atmosphere that is roughly in earth's class as far as size, but the
similarities end there.
John Southworth of Keele
University in the UK
and colleagues used the European Southern Observatory or ESO, a hotbed for
exoplanet discoveries as of late, to confirm the size of the planet by studying
it as it transited in front of its star. But they saw something else within the
data. One of the wavelengths of light they were studying seemed to be blocked
by an atmosphere of some type, though its composition isn't yet fully
understood.
This has an important implication regarding stars that can
have habitable planets in the universe. Stars fall into different classes, our
own sun being a G type yellow dwarf. GJ 1132b's star is an M-type dwarf, by far
the most common kind of star in the Milky Way, in fact Trappist - 1 is in that class.
GJ 1132, the parent star of the planet, is a type of star that tends to be
pretty active and, up until now, it was unclear if any planets orbiting very near
such a star could hold onto their atmospheres. For our kind of life here on
earth, obviously having an atmosphere is quite important.
GJ 1132b seemingly answers the question. Yes, planets
orbiting close to at least some M type stars can hold onto atmospheres. That
potentially opens up a huge amount of stars to the possibility of harboring
earth-like planets. But as far as GJ 1132b is concerned, it's not earth-like at
all.
But what might GJ 1132b's atmosphere look like? One
hypothesis based on the data is that it might be largely made up of water
vapor, basically a steam bath world, or a world high in methane. The planet is
close to its star, so it would probably be tidally locked, always presenting
the same face towards the star. That's about all that can be said though.
But in the future this world is set to be a priority for
study, especially with the James Webb Space Telescope. Other than Venus, this
is the first roughly earth-sized planet with an atmosphere that we can study.
As the facts about the planet come out, it will become a planet that we can
envision what it might be like better than most other exoplanets. Scientists
should eventually be able to work out the planet's color, what sort of winds it
has, and even what sunsets might look like on this world.
Thanks for listening! I am futurist and science fiction
author John Michael Godier currently hard at work preparing content for the new
channel and be sure to check out my books at your favorite online book retailer
and subscribe to my channel for regular, in-depth explorations into the
interesting, weird and unknown aspects of this amazing universe in which we
live
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