(Feature Image courtesy of ESA/Hubble, M. Kornmesser)
In the past week, the big news in astronomy was the first detection of gravitational waves, a phenomenon predicted by Albert Einstein in his general theory of relativity. No doubt within a few years students will be reading in textbooks about how the LIGO experiment measured the gravitational waves created from a collision of two black holes.
However, beneath the incredible news of LIGO’s success is another astronomical milestone. Just today, a team from University College London (UCL) was able to observe the atmosphere of a “super-Earth” for the first time. In short, super-Earths are planets larger than Earth and smaller than the gas giants of our Solar System. This class of planets is thought to be the most common in the Milky Way Galaxy, and therefore, our search for life on other planets has focused largely on extrasolar super-Earths.
Measuring Extrasolar Atmosphere
Using a new form of analysis, The UCL team was able to take Hubble data and determine the atmospheric structure of 55 Cancri e, an extrasolar planet about 40 light years away. An excerpt from the UCL article describes the analysis technique in more detail:
Observations were made by scanning WFC3 [Wide Field Camera 3] very quickly across the star to create a number of spectra. By combining these observations and processing through computer analytic ‘pipeline’ software, the researchers were able to retrieve the spectral fingerprints of 55 Cancri e embedded in the starlight.
As far as I can tell, the astrophysicists at UCL were able to analyze the atmosphere of a planet 40 light years away by setting the Hubble’s cameras to “burst mode.” Incredible!
What We Learned About 55 Cancri e
(Video courtesy of HubbleESA – The European Space Agency)
The analysis run by UCL found that the atmosphere is largely composed of Hydrogen and Helium, suggesting that the planet retained a lot of the material from the initial nebula that birthed the planet. Also interesting is the presence of Hydrogen Cyanide in the atmosphere, a chemical that is often an indicator for a carbon-rich atmosphere.
However, considering the average temperature of 55 Cancri e is about 3,600° F, even if we were to filter out the incredibly poisonous Hydrogen Cyanide from the atmosphere, we would probably find the planet a bit too toasty. In addition to obscenely hot temperatures and toxic gas, we would have to get used to the 18 hour year of 55 Cancri e. Yes, 55 Cancri e makes a full orbit around its star (55 Cancri) every 18 hours. Perhaps the planet’s small distance from its parent star explains those hot temperatures…
For all of the downsides to paying this planet a visit, there is one fantastic upside. The planet is known as “The Diamond Planet” because much of the carbon that forms the planet is in diamond form. Maybe some day, when we can travel light years at a time and land on planets with temperatures in the thousands of degree Fahrenheit, we will be able to stand on a planet made of diamonds.












