Retired star found with planets and debris disc

Apr 09, 2013
An image of the star Kappa Coronae Borealis, based on observations with the PACS instrument on the Herschel Space Observatory. North is up and east is left. The star is in the centre of the frame (not visible in this graphic) with an excess of infrared emission detected around it, interpreted as a dusty debris disc containing asteroids and/or comets. The inclination of the planetary system is constrained at an angle of 60º from face-on. Credit: ESA/Bonsor et al (2013).

(Phys.org) —ESA's Herschel space observatory has provided the first images of a dust belt – produced by colliding comets or asteroids – orbiting a subgiant star known to host a planetary system. The team of scientists who made the discovery publishes their results in the Oxford University Press journal Monthly Notices of the Royal Astronomical Society.

After billions of years steadily burning hydrogen in their cores, like our Sun exhaust this central fuel reserve and start burning it in shells around the core. They swell to become subgiant stars, before later becoming .

At least during the subgiant phase, planets, asteroids and comet belts around these 'retired' stars are expected to survive, but observations are needed to measure their properties. One approach is to search for discs of dust around the stars, generated by collisions between populations of asteroids or comets.

Thanks to the sensitive far-infrared detection capabilities of the , astronomers have been able to resolve bright emission around the star Kappa Borealis (κ CrB, or Kappa Cor Bor), indicating the presence of a dusty debris disc. This star is a little heavier than our own Sun at 1.5 , is around 2.5 billion years old and lies at a distance of roughly 100 light years.

From ground-based observations, it is known to host one giant planet roughly twice the mass of Jupiter orbiting at a distance equivalent to the in our own . A second planet is suspected, but its mass is not well constrained.

Herschel's detection provides rare insight into the life of planetary systems orbiting subgiant stars, and enables a detailed study of the architecture of its planet and disc system.

"This is the first 'retired' star that we have found with a debris disc and one or more planets," says Amy Bonsor of the Institute de Planétologie et d'Astrophysique de Grenoble, and lead author of the study.

'The disc has survived the star's entire lifetime without being destroyed. That's very different to our own Solar System, where most of the debris was cleared away in a phase called the Late Heavy Bombardment era, around 600 million years after the Sun formed."

Dr Bonsor's team used models to propose three possible configurations for the disc and planets that fit Herschel's observations of Kappa Cor Bor.

The first model has just one continuous dust belt extending from 20 AU to 220 AU (where 1 AU, or Astronomical Unit, is the distance between Earth and Sun). By comparison, the icy debris disc in our Solar System – known as the Kuiper Belt – spans a narrower range of distances, 30–50 AU from the Sun. In this model, one of the planets orbits at a distance of greater than 7 AU from the star, and its gravitational influence may sculpt the inner edge of the disc.

A variation on this model has the disc being stirred by the gravitational influence of both companions, mixing it up such that the rate of dust production in the disc peaks at around 70–80 AU from the star.

In another interesting scenario, the dust disc is divided into two narrow belts, centred on 40 AU and 165 AU, respectively. Here, the outermost companion may orbit between the two belts between a distance of about 7 AU and 70 AU, opening the possibility of it being rather more massive than a planet, possibly a substellar brown dwarf.

"It is a mysterious and intriguing system: is there a planet or even two planets sculpting one wide disc, or does the star have a brown dwarf companion that has split the disc in two?" says Dr Bonsor.

As this is the first known example of a subgiant star with planets and a debris disc orbiting it, more examples are needed to determine whether Kappa Cor Bor is unusual or not.

"Thanks to Herschel's sensitive far-infrared capabilities and its rich dataset, we already have hints of other subgiant stars that may also have dusty discs. More work will be needed to see if they also have ," says Göran Pilbratt, ESA's Herschel project scientist.

Explore further: Hubble sees 'ghost light' from dead galaxies

More information: Bonsor et al. Spatially Resolved Images of Dust Belt(s) Around the Planet-hosting Subgiant κ CrB, Monthly Notices of the Royal Astronomical Society, April 2013. mnras.oxfordjournals.org/conte… 29/mnras.stt367.full

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User comments : 3

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Husky
1 / 5 (2) Apr 09, 2013
if there is a giant planet/sub brown dividing the two dustdiscs we shall name it Occams razer.
geokstr
1 / 5 (4) Apr 09, 2013
OMG! We simply have to institute a 100% marginal tax rate on all income over $11,369.47 and a transfer of all individual rights to algore and the UN immediately. There is a 97% consensus in the scientific community that there is only about 5 billion years to prepare for this.
katesisco
1 / 5 (2) Apr 10, 2013
I am thinking it is not gravity that keeps out the dirty gas but electromagnetism. Perhaps it first keeps the dirty gas confined to a tight flattened ring like our Saturn. Then the strength makes a jet or lesser, planets. Would this system then have had an early cessation of the EM field?

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