Rare image of Super-Jupiter sheds light on planet formation

Nov 19, 2012
False color, near infrared (wavelength 3.8 micrometers) image of the κ And ("Kappa Andromedae") system, generated from data collected in July 2012 with the Subaru Telescope in Hawai'i. Almost all of the light of the host star, on which the image is centered, has been removed through image processing; the host star is covered by the dark, software-generated disk in the center. The speckled pattern surrounding the software-generated mask at the center represents the residuals from the starlight subtraction. The Super-Jupiter κ And b is clearly visible to the upper left. It has a projected separation of 1.8 times the distance between Neptune and the Sun. Credit: NAOJ / Subaru / J. Carson (College of Charleston) / T. Currie (University Toronto)

Astronomers using infrared data from the Subaru Telescope in Hawaii have discovered a "super-Jupiter" around the bright star Kappa Andromedae, which now holds the record for the most massive star known to host a directly imaged planet or lightweight brown dwarf companion.

Designated Kappa Andromedae b (Kappa And b, for short), the new object has a mass about 12.8 times greater than Jupiter's. This places it teetering on the dividing line that separates the most massive planets from the lowest-mass brown dwarfs. That ambiguity is one of the object's charms, say researchers, who call it a super-Jupiter to embrace both possibilities.

"According to conventional models of planetary formation, Kappa And b falls just shy of being able to generate energy by fusion, at which point it would be considered a brown dwarf rather than a planet," said Michael McElwain, a member of the discovery team at NASA's Goddard Space Flight Center in Greenbelt, Md. "But this isn't definitive, and other considerations could nudge the object across the line into brown dwarf territory."

Massive planets slowly radiate the heat leftover from their own formation. For example, the planet Jupiter emits about twice the energy it receives from the sun. But if the object is massive enough, it's able to produce energy internally by fusing a heavy form of hydrogen called deuterium. (Stars like the sun, on the other hand, produce energy through a similar process that fuses the lighter and much more common form of hydrogen.) The theoretical mass where deuterium fusion can occur—about 13 Jupiters—marks the lowest possible mass for a brown dwarf.

"Kappa And b, the previously imaged planets around HR 8799 and Beta Pictoris, and the most massive planets discovered by non-imaging techniques likely all represent a class of object that formed in much the same way as lower-mass exoplanets," said lead researcher Joseph Carson, an astronomer at the College of Charleston, S.C., and the Max Planck Institute for Astronomy in Heidelberg, Germany.

The discovery of Kappa And b also allows astronomers to explore another theoretical limit. Astronomers have argued that large stars likely produce large planets, but experts predict that this stellar scaling can only extend so far, perhaps to stars with just a few times the sun's mass. The more massive a young star is, the brighter and hotter it becomes, resulting in powerful radiation that could disrupt the formation of planets within a circumstellar disk of gas and dust.

"This object demonstrates that stars as large as Kappa And, with 2.5 times the sun's mass, remain fully capable of producing planets," Carson adds.

The "super-Jupiter" Kappa Andromedae b, shown here in an artist's rendering, circles its star at nearly twice the distance that Neptune orbits the sun. With a mass about 13 times Jupiter's, the object glows with a reddish color. Credit: Credit: NASA's Goddard Space Flight Center/S. Wiessinger

The research is part of the Strategic Explorations of Exoplanets and Disks with Subaru (SEEDS), a five-year effort to directly image extrasolar planets and protoplanetary disks around several hundred nearby stars using the Subaru Telescope on Mauna Kea, Hawaii. Direct imaging of exoplanets is rare because the dim objects are usually lost in the star's brilliant glare. The SEEDS project images at near-infrared wavelengths using the telescope's adaptive optics system, which compensates for the smearing effects of Earth's atmosphere, in concert with its High Contrast Instrument for the Subaru Next Generation Adaptive Optics and Infrared Camera and Spectrograph.

Young star systems are attractive targets for direct exoplanet imaging because young planets have not been around long enough to lose much of the heat from their formation, which enhances their brightness in the infrared. The team focused on the star Kappa And because of its relative youth—estimated at the tender age of 30 million years, or just 0.7 percent the age of our solar system, based on its likely membership in a stellar group known as the Columba Association. The B9-type star is located 170 light-years away in the direction of the constellation Andromeda and is visible to the unaided eye.

Kappa And b orbits its star at a projected distance of 55 times Earth's average distance from the sun and about 1.8 times as far as Neptune; the actual distance depends on how the system is oriented to our line of sight, which is not precisely known. The object has a temperature of about 2,600 degrees Fahrenheit (1,400 Celsius) and would appear bright red if seen up close by the human eye.

Carson's team detected the object in independent observations at four different infrared wavelengths in January and July of this year. Comparing the two images taken half a year apart showed that Kappa And b exhibits the same motion across the sky as its host star, which proves that the two objects are gravitationally bound and traveling together through space. Comparing the brightness of the super-Jupiter between different wavelengths revealed infrared colors similar to those observed in the handful of other gas giant planets successfully imaged around stars.

A paper describing the results has been accepted for publication in The Astrophysical Journal Letters and will appear in a future issue.

The SEEDS research team is continuing to study Kappa And b to better understand the chemistry of its atmosphere, constrain its orbit, and search for possible secondary planets.

Coincidentally, the stellar association that hosts Kappa And also includes another famous high-mass star, HR 8799, which is one of the first where astronomers directly imaged an extrasolar planet. The system hosts several gas giant planets with masses and infrared colors similar to Kappa And b.

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More information: The work described here will be published as J. Carson et al., "Direct Imaging Discovery of a 'Super-Jupiter' Around the late B-Type Star Kappa Andromedae" in the Astrophysical Journal Letters. arxiv.org/abs/1211.3744

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Sonhouse
5 / 5 (1) Nov 19, 2012
Kappa is about 170 ly away, and the distance of its planet is about 9E9km or about 6 E9 miles, so the separation is not that big a deal, about 0.8 arc seconds.
Birger
5 / 5 (1) Nov 19, 2012
A separation of 60 AU ?
Sonhouse
5 / 5 (2) Nov 19, 2012
Yep,about twice the distance to Neptune. Pretty far out so the angular separation isn't that great, just under one arc second.
JRi
1.5 / 5 (2) Nov 19, 2012
Would love to see a movie made of series of these images which would show how the planet circles around the star.
GSwift7
3.7 / 5 (6) Nov 19, 2012
Would love to see a movie made of series of these images which would show how the planet circles around the star


With that orbit distance, it's going to orbit once every few hundred years, so good luck with that.
Torbjorn_Larsson_OM
5 / 5 (4) Nov 19, 2012
So there could really be a mass overlap between core accretion planets and gas collapse stars.

If we are really unlucky the degeneracy is spectroscopic to boot. Oh well, not much of a problem for astrobiology (except as a hinder to understand system formation). :-)

On the movie, when we have a part arc of 2-3 images and a reasonable orbit estimate we can cheat and "paint" arcs along the projected orbit. I hear it is a beta feature of Astroshop.

Lurker2358
1 / 5 (1) Nov 24, 2012
A separation of 60 AU ?


60 A.U. is relatively small as orbiting bodies go.

Most of the "objects" orbiting the Sun are actually much farther away than that, including most of the known "dwarf planets".