New research led by Yale University scientists suggests that a rocky
planet twice Earth's size orbiting a nearby star is a diamond planet.
"This is our first glimpse of a rocky world with a fundamentally
different chemistry from Earth," said lead researcher Nikku Madhusudhan,
a Yale postdoctoral researcher in physics and astronomy. "The surface
of this planet is likely covered in graphite and diamond rather than
water and granite."
The paper reporting the findings has been accepted for publication in the journal Astrophysical Journal Letters.
The planet - called 55 Cancri e - has a radius twice Earth's, and a mass
eight times greater, making it a "super-Earth." It is one of five
planets orbiting a sun-like star, 55 Cancri, that is located 40 light
years from Earth yet visible to the naked eye in the constellation of
Cancer.
The planet orbits at hyper speed - its year lasts just 18 hours, in
contrast to Earth's 365 days. It is also blazingly hot, with a
temperature of about 3,900 degrees Fahrenheit, researchers said, a far
cry from a habitable world.
The planet was first observed transiting its star last year, allowing
astronomers to measure its radius for the first time. This new
information, combined with the most recent estimate of its mass, allowed
Madhusudhan and colleagues to infer its chemical composition using
models of its interior and by computing all possible combinations of
elements and compounds that would yield those specific characteristics.
Astronomers had previously reported that the host star has more carbon
than oxygen, and Madhusudhan and colleagues confirmed that substantial
amounts of carbon and silicon carbide, and a negligible amount of water
ice, were available during the planet's formation.
Astronomers also thought 55 Cancri e contained a substantial amount of
super-heated water, based on the assumption that its chemical makeup was
similar to Earth's, Madhusudhan said.
But the new research suggests the planet has no water at all, and
appears to be composed primarily of carbon (as graphite and diamond),
iron, silicon carbide, and, possibly, some silicates. The study
estimates that at least a third of the planet's mass - the equivalent of
about three Earth masses - could be diamond.
"By contrast, Earth's interior is rich in oxygen, but extremely poor in
carbon - less than a part in thousand by mass," says co-author and Yale
geophysicist Kanani Lee.
The identification of a carbon-rich super-Earth means that distant rocky
planets can no longer be assumed to have chemical constituents,
interiors, atmospheres, or biologies similar to those of Earth,
Madhusudhan said.
The discovery also opens new avenues for the study of geochemistry and
geophysical processes in Earth-sized alien planets. A carbon-rich
composition could influence the planet's thermal evolution and plate
tectonics, for example, with implications for volcanism, seismic
activity, and mountain formation.
"Stars are simple - given a star's mass and age, you know its basic
structure and history," said David Spergel, professor of astronomy and
chair of astrophysical sciences at Princeton University, who is not a
co-author of the study.
"Planets are much more complex. This 'diamond-rich super-Earth' is
likely just one example of the rich sets of discoveries that await us as
we begin to explore planets around nearby stars."
In 2011, Madhusudhan led the first discovery of a carbon-rich atmosphere
in a distant gas giant planet, opening the possibility of
long-theorized carbon-rich rocky planets (or "diamond planets").
The new research represents the first time that astronomers have
identified a likely diamond planet around a sun-like star and specified
its chemical make-up. Follow-up observations of the planet's atmosphere
and additional estimates of the stellar composition would strengthen the
findings about the planet's chemical composition.
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