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Water vapor detected in the atmosphere of a distant
exoplanet
Red dwarfs
Red dwarfs (or M dwarfs) are the tiniest, coolest and the most long living of
all stars. Don’t look for them on the night sky, they are too faint to be seen
with the unaided eye. Red Dwarfs are very abundant in all galaxies. In the
Milky Way, for example, they make up around ¾ of all stars. In old elliptical
galaxies almost all stars are red dwarfs! Scientist think that 40% of all red
dwarfs have small planets around them. Are these planets good places to
search for alien life? Well, unfortunately, red dwarfs are not very “life-
friendly”. First, they are quite active. Superflares, similar to the solar
flares only much more powerful, erupt on red dwarfs while they are young,
i.e. at the time when planets potentially form around them. Second, they are
small and therefore their habitable zone, an area where liquid water can
exist, is very close to the star itself. Finally, planets around red dwarfs are
expected to be tidally locked. If they indeed have the same side always
facing their star, there might be a huge temperature variation between “day
side” and “night side” of these planets. For life as we know it all these
factors are bad news. For a long time now astronomers thought that planets
around red dwarfs are the least likely places to host life. But more recent
studies suggest that these worlds might not be quite as bad after all!
K2-18b
Planet K2-18b was discovered back in 2015 by Kepler Space
Telescope. This “Super-Earth ” is 8.6 times as massive as our
home planet and 3 times its size. K2-18b’s density is lower than
that of the Earth, so scientists don’t know what the planet is like
and whether it has a solid surface. The exoplanet orbits its star
once every 33 days at an uncomfortably close distance of
0.14AU. One astronomical unit, or AU, is equal to the Earth-Sun
distance, or 149.6 million kilometers.
Although K2-18b is so close to the host star, its equilibrium
temperature is similar to that of the Earth. That means it is
possible that liquid water and organics are present out there.
Now, equilibrium temperature is not the same as mean
temperature or surface temperature. The actual temperature on
any planet might be much higher than its equilibrium
temperature if there is an atmosphere and if the tidal effects
caused by the proximity to the host star heat the planet up from
within. Both are likely to be the cases with K2-18b.
Observations and water discovery
Hubble Space Telescope observed the planet K2-18b for
3 years between 2015 and 2017. Over that time scientists
recorded 8 transits, i.e. passages of the planet in front of
its star. Later, they added the data from two transits
observed by Kepler Space Telescope mission and 3
transits observed by the Infra Red space telescope
Spitzer.
As a result, astronomers were able to detect water vapor
in the thick hydrogen-rich atmosphere of K2-18b. What’s
more, the temperature on the planet seems to be low
enough to allow water condensation. That means the
water vapor probably condenses into droplets in K2-18b’s
middle-atmosphere, falls as rain and later evaporates in
the lower thicker atmospheric layers. Whether or not there
is liquid water on the actual surface of this planet, we don’t
know.
What’s next?
Scientists cannot wait to learn more about this amazing
planet. K2-18b is a great target candidate for the
upcoming NASA James Webb Telescope mission as well
as for ESA ARIEL mission. Who knows what else they will
discover!
Meanwhile, stay tuned and read our space blog. And don’t
forget to visit our inflatable planetarium to learn more
about exoplanets and search for life in the Universe!

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Water vapor detected in the atmosphere of a distant exoplanet

  • 1. Water vapor detected in the atmosphere of a distant exoplanet
  • 2. Red dwarfs Red dwarfs (or M dwarfs) are the tiniest, coolest and the most long living of all stars. Don’t look for them on the night sky, they are too faint to be seen with the unaided eye. Red Dwarfs are very abundant in all galaxies. In the Milky Way, for example, they make up around ¾ of all stars. In old elliptical galaxies almost all stars are red dwarfs! Scientist think that 40% of all red dwarfs have small planets around them. Are these planets good places to search for alien life? Well, unfortunately, red dwarfs are not very “life- friendly”. First, they are quite active. Superflares, similar to the solar flares only much more powerful, erupt on red dwarfs while they are young, i.e. at the time when planets potentially form around them. Second, they are small and therefore their habitable zone, an area where liquid water can exist, is very close to the star itself. Finally, planets around red dwarfs are expected to be tidally locked. If they indeed have the same side always facing their star, there might be a huge temperature variation between “day side” and “night side” of these planets. For life as we know it all these factors are bad news. For a long time now astronomers thought that planets around red dwarfs are the least likely places to host life. But more recent studies suggest that these worlds might not be quite as bad after all!
  • 3. K2-18b Planet K2-18b was discovered back in 2015 by Kepler Space Telescope. This “Super-Earth ” is 8.6 times as massive as our home planet and 3 times its size. K2-18b’s density is lower than that of the Earth, so scientists don’t know what the planet is like and whether it has a solid surface. The exoplanet orbits its star once every 33 days at an uncomfortably close distance of 0.14AU. One astronomical unit, or AU, is equal to the Earth-Sun distance, or 149.6 million kilometers. Although K2-18b is so close to the host star, its equilibrium temperature is similar to that of the Earth. That means it is possible that liquid water and organics are present out there. Now, equilibrium temperature is not the same as mean temperature or surface temperature. The actual temperature on any planet might be much higher than its equilibrium temperature if there is an atmosphere and if the tidal effects caused by the proximity to the host star heat the planet up from within. Both are likely to be the cases with K2-18b.
  • 4. Observations and water discovery Hubble Space Telescope observed the planet K2-18b for 3 years between 2015 and 2017. Over that time scientists recorded 8 transits, i.e. passages of the planet in front of its star. Later, they added the data from two transits observed by Kepler Space Telescope mission and 3 transits observed by the Infra Red space telescope Spitzer. As a result, astronomers were able to detect water vapor in the thick hydrogen-rich atmosphere of K2-18b. What’s more, the temperature on the planet seems to be low enough to allow water condensation. That means the water vapor probably condenses into droplets in K2-18b’s middle-atmosphere, falls as rain and later evaporates in the lower thicker atmospheric layers. Whether or not there is liquid water on the actual surface of this planet, we don’t know.
  • 5. What’s next? Scientists cannot wait to learn more about this amazing planet. K2-18b is a great target candidate for the upcoming NASA James Webb Telescope mission as well as for ESA ARIEL mission. Who knows what else they will discover! Meanwhile, stay tuned and read our space blog. And don’t forget to visit our inflatable planetarium to learn more about exoplanets and search for life in the Universe!