How Many Earth-like Planets Are There? We Don't Know, But Soon. . .
Credit: J Barstow
As the light from the star passes through the Earth’s atmosphere
some of it is absorbed in the ozone layer. This results in a clear
feature that can be seen using telescopes like JWST. Venus,
however, has no ozone layer so the feature is absent.
In the third post on what scientists know about the possibility of life existing elsewhere, we take a look at another paper being presented at the at the 2015 National Astronomy Meeting in Wales during the second week of July, 2015.
Dr Joanna Barstow of the University of Oxford conducted a study of the new space telescope to be launched by the U.S. in 2018, examining its ability to distinguish Earth-like planets with conditions right for life from the many exo-planets we have found using the Hubble telescope.
Again, scientists have ideas and theories about life on other planets, but until verifiable data is obtained, ideas and theories remain just that. This is what separates speculation from science - hard data obtained from controlled observation.
Here's the report with a link to the original in the attribution:
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Eyeing up Earth-like planets
Almost 2000 exoplanets have been discovered to date, ranging from rocky Earth-like planets to hot-Jupiters, and orbiting every type of star. But how many of these distant worlds are habitable? Today's technology means that we currently have very little information about what exoplanets are like beyond their presence, size and distance from star. With the launch of the James Webb Space Telescope (JWST), we may have our first glimpses into atmospheres of Earth-like exoplanets, according to the results of a study by Dr Joanna Barstow presented at the 2015 National Astronomy Meeting in Llandudno (Thlandudno) Wales, UK.
"A planet's atmosphere provides a good guide to likely conditions on the surface," said Barstow, of the University of Oxford. "The Earth's atmosphere contains significant amounts of nitrogen, oxygen, ozone and water. By contrast, its inhospitable 'evil twin', Venus, has an atmosphere made mostly of carbon dioxide, which drives its surface temperature to a blistering 450 degrees Celsius."
A successor to the Hubble Space Telescope, JWST is due for launch in 2018 and will study the Universe in infrared wavelengths. Barstow's study shows that JWST may be able to differentiate between a planet with a clement, Earth-like atmosphere, and one with more hostile conditions such as are found on our neighboring planet Venus. JWST will have the capability to detect key markers that could indicate the presence of a climate like our own when looking at Earth-sized planets around stars that are smaller and redder than our Sun.
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"If we took the Earth and Venus, and placed them in orbit around a cool, red star that's not too far away, our study shows that JWST could tell them apart. Earth's ozone layer, 10 kilometers above the surface, is produced when light from the Sun interacts with molecules of oxygen in our atmosphere, and it produces an unmistakable signal that could be detected by JWST. Venus, without a substantial ozone layer, would look very different," said Barstow. "That's assuming that planets starting out like Earth and Venus would evolve in the same way around a cool star!"
However, JWST will be used for a wide range of astronomical applications, not just detecting exoplanets, and securing time on the telescope will be highly competitive. To make these detections, astronomers would need to observe the exoplanets at least 30 times, taking valuable telescope time.
"Future telescopes that are dedicated to observing the atmospheres of many rocky planets around different stars will be required to fully resolve the question of habitability on exoplanets. In the meantime, JWST will observe many other weird and wonderful planets in unprecedented detail," said Barstow.
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