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Patrick Dufour et un collègue américain découvrent une planète possiblement riche en calcaire
2016-06-13

Un groupe de chercheurs, utilisant le télescope de 10 mètres de l’Observatoire W.M. Keck (Hawaii), ont découvert un corps planétaire possiblement recouvert de calcaire et dont les couches superficielles sont érodées par son étoile désormais morte. En effet, en plus d’appliquer une méthode relativement nouvelle permettant de déterminer la composition chimique des planètes afin d’examiner leur structure interne, l’équipe a constaté que le matériel rocheux accrété par l’étoile morte pourrait être composé de minéraux qui sont généralement associés à des processus de la vie marine sur Terre. L’équipe - composée de Carl Melis de l’Université de Californie à San Diego, et Patrick Dufour du Centre de recherche en astrophysique du Québec (CRAQ) de l’Université de Montréal - annonce ses conclusions à l’occasion de la 228e rencontre de l’American Astronomical Society, qui se tient cette semaine à San Diego.

Pour en savoir plus.

PLANET-DEVOURING STAR REVEALS POSSIBLE LIMESTONE CRUMBS

A group of researchers using the W. M. Keck Observatory have discovered a planet-like body that may have been encrusted in limestone and is having its surface layers devoured by its deceased host star. In addition to extending a relatively new method of determining the chemical composition of planets to examine their internal structure, the team found that the rocky material being accreted by the star could be comprised of minerals that are typically associated with marine life processes here on Earth. The team -- comprised of Carl Melis of University of California, San Diego, and Patrick Dufour of the Université de Montréal -- is announcing their findings at the 228th meeting of the American Astronomical Society this week.

Building on past observations of the white dwarf called SDSS J1043+0855 (the dead core of a star that originally was a few times the mass of the Sun), which has been known to be gobbling up rocky material in its orbit for almost a decade, the team used Keck Observatory’s HIRES instrument fitted to the 10-meter Keck I telescope as well as data from the Hubble Space Telescope to measure and characterize the material being accreted by the star.

What they found is that the white dwarf appears to be accreting the outermost layers of a differentiated, rocky extrasolar body (i.e., the surface of a massive, planet-like object) from its extant planetary system.

“Spectroscopic observations of the white dwarf allowed us to measure the abundances of the rocky material as it is being accreted and filtered through the star’s atmosphere in real time,” Melis said. “We can see the material that used to make up this planet being accreted and replenished on a daily timescale. What we see is what the rock was made of.”

This may be the single best tool astronomers have to determine the chemical composition of planets, according to Luca Rizzi, Support Astronomer at Keck Observatory.

“We’ve known for some time that examining the accreted remains of rocky planets in the atmosphere of their host white dwarf star can give bulk chemical composition information, and now it looks like we can even hone in on specific layers of an accreted body in some fortuitous cases,” Melis said.

Determining the chemical composition or structure of planets outside of the solar system to date has been elusive at best. “It’s a huge issue in exoplanetology right now,” Melis said. “The major exoplanet identifying methods can’t tell you what a planet is made of or what it’s structure is.”

While the finding will provide a new angle for scientists to study the chemical composition and structure of rocky planets, the possibility that life may have contributed to the inferred mineralogy certainly intrigued the team.

The researchers’ finding shows that SDSS J1043+0855 is accreting the surface of a body that has large enhancements of carbon. This feature -- combined with mild enhancements of calcium and oxygen -- points to the possibility of the material coming in the form of calcium-carbonate, a mineral that is often associated with shelled marine organisms here on Earth. Calcium-carbonate is attractive as a mineral constituent of this planet-like body as incorporating and entraining carbon in rocky objects (especially their surfaces) is difficult. The terrestrial planets in our solar system are said to live in a “carbon desert” since they are so heavily depleted in this element -- the planetary surface being accreted by this white dwarf star could have as much as several hundred times more carbon than the surface of the Earth.

“This method allows us to truly get a glimpse of what aliens might be standing on,” Melis said. “In this particular case, the presence of such high levels of carbon is unique and really needs to be explained. Our choice of calcium-carbonate as a potential carrier of the carbon provides a natural way for it to be locked up in the planet and eventually delivered to the white dwarf star, is entirely consistent with the observations in hand, and of course is suggestive. That’s really the hidden subtext. When people think about finding extraterrestrial life, they think about Hollywood dramatizations. But the first evidence of life outside of our solar system will probably come in a much subtler form. More likely than not, it’s going to come as a nuanced signature that may not be immediately recognizable.”

Non-biological processes can produce calcium-carbonate too, so its presence isn’t necessarily a smoking gun, even if it is confirmed. “There’s a lot of hoops to jump through before we can settle on the conclusion that life was involved in what we are observing,” Dufour said.

Specifically, the inferred presence of calcium-carbonate came from examining the atomic leftovers of the planet accretion event in the atmosphere of the white dwarf star -- after the presumed dust from the planet’s demolished surface was consumed by the white dwarf. The next step will be to look at the dust in a mineral state before it falls into the star, to both confirm its composition and to measure its concentration.

“Future observations with the James Webb Space Telescope can confirm calcium-carbonate if it is present. If we are able to get to that point, then you have to ask: Is there enough there for it to be produced with natural processes?” Melis said.

While the presence of the calcium-carbonate is still in question, the paper shows strong evidence that the accreted material is almost certainly coming from the outer layers of a planet-like object and that white dwarf stars hold promise in informing on the structure of planets outside of the solar system.

Media Contact:
Steve Jefferson
W. M. Keck Observatory
+1 (808) 881-3827
sjefferson@keck.hawaii.edu

Science Contact:
Carl Melis
University of California, San Diego
+1 (858) 534-6627
cmelis@ucsd.edu

Patrick Dufour
Université de Montréal
(514) 343-7355
dufourpa@astro.umontreal.ca

Reference:
“The Surface of a Limestone-Rich World?” Carl Melis & Patrick Dufour, 2016 June, paper 201.03, 228th AAS meeting, San Diego, California [https://aas.org/meetings/aas228].


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