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Astronomers Sniff A Super-Earth’s Atmosphere

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This artist’s impression shows the super-Earth 55 Cancri e in front of its parent star. Using observations made with the NASA/ESA Hubble Space Telescope and new analytic software scientists were able to analyse the composition of its atmosphere. It was the first time this was possible for a super-Earth. Credit: ESA/Hubble, M. Kornmesser
This artist’s impression shows the super-Earth 55 Cancri e in front of its parent star, 55 Cancri in the constellation Cancer the Crab, 40 light years from Earth. Using observations made with the Hubble Space Telescope and new analytic software scientists were able to analyse the composition of its atmosphere. It was the first time this was possible for a super-Earth. Credit: ESA/Hubble, M. Kornmesser

Smells like teen spirit, er, I mean like hydrogen and helium laced with bitter almonds. Using data gathered with the Hubble Space Telescope and new analysis techniques, the exoplanet 55 Cancri e was found to have a dry atmosphere bereft of water vapor but rich in the simplest elements that are also the most common in the universe. It orbits its host star 55 Cancri so closely that a year there lasts 18 hours, and the temperature cooks at around 3,600° F (2,000° C). Hot! No, the livin’ ain’t easy on this extrasolar planet, but it’s the first super-Earth to have its atmosphere analyzed.

A super-Earth is a planet more massive than our own but considerably less than the ice-giants Uranus and Neptune. As instrumentation and measurement have become ever more precise since the first extrasolar planet discovery in 1995, we’ve gone from detecting only the most massive, Jupiter-like worlds down to super-Earths and even a few Earth-mass planets. Astronomers find planets beyond our solar system primarily by measuring the drop in light as they transit their host suns or by the gravitational wobble they induce in those same stars.

Illustration of the inferred size of the super-Earth COROT-7b (center) in comparison with Earth and Neptune. Credit: Aldaron/Wikipedia
Illustration of the inferred size of the super-Earth COROT-7b (center) in comparison with Earth and Neptune. Credit: Aldaron/Wikipedia

The next step after nailing down size and orbit is to determine atmospheric and surface conditions with the goal of finding planets that might be habitable. 55 Cancri b is one of five planets orbiting its parent sun, all of which formed from a cloud of gas and dust similar to the one that birthed our own solar system and sun. Eight times more massive than Earth, it held onto the nebula’s lighter gases hydrogen and helium much like Jupiter and Saturn did.

Super-Earths like 55 Cancri e are thought to be the most common type of planet in our galaxy, though this one’s unusual in orbiting its sun-like star so closely. Traces of the bitter almond-smelling gas hydrogen cyanide found in its air is a marker for carbon-rich atmospheres.

This artist's conception compares a hypothetical solar system centered around a tiny "sun" (top) to a known solar system centered around a star, called 55 Cancri, which is about the same size as our sun. NASA's Spitzer Space Telescope, in combination with other ground-based and orbiting telescopes, discovered the beginnings of such a miniature solar system 500 light-years away in the Chamaeleon constellation. The tiny system consists of an unusually small "failed" star, or brown dwarf, called Cha 110913-773444, and a surrounding disk of gas and dust that might one day form planets. At a mass of only eight times that of Jupiter, the brown dwarf is actually smaller than several known extrasolar planets. The largest planet in the 55 Cancri system is about four Jupiter masses. Astronomers speculate that the disk around Cha 110913-773444 might have enough mass to make a small gas giant and a few Earth-sized rocky planets, as depicted here around the little brown dwarf.
Artist’s conception of 55 Cancri, a double star in Cancer with a larger sun-like star orbited by at least five planets (four shown here) and a red dwarf companion star. Credit: Credit: NASA/JPL-Caltech/T. Pyle (SSC)

“If the presence of hydrogen cyanide and other molecules is confirmed in a few years time by the next generation of infrared telescopes, it would support the theory that this planet is indeed carbon rich and a very exotic place,” concludes Jonathan Tennyson of University College London, who was part of the team making the discovery. “Although hydrogen cyanide, or prussic acid, is highly poisonous, so it is perhaps not a planet I would like to live on!”


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