Candidate protoplanet spotted inside its stellar womb
Astronomers using ESO’s Very Large Telescope have obtained what is likely the first direct observation of a forming planet still embedded in a thick disc of gas and dust. If confirmed, this discovery will greatly improve our understanding of how planets form and allow astronomers to test the current theories against an observable target.
This artist’s impression shows the formation of a gas giant planet in the ring of dust around the young star HD 100546. This system is also suspected to contain another large planet orbiting closer to the star. The newly-discovered object lies about 70 times further from its star than the Earth does from the Sun. This protoplanet is surrounded by a thick cloud of material so that, seen from this position, its star almost invisible and red in color because of the scattering of light from the dust. Image Credit: ESO/L. Calçada
An international team led by Sascha Quanz (ETH Zurich, Switzerland) has studied the disk of gas and dust that surrounds the young star HD 100546, a relatively nearby neighbour located 335 light-years from Earth. They were surprised to find what seems to be a planet in the process of being formed, still embedded in the disk of material around the young star. The candidate planet would be a gas giant similar to Jupiter.
“So far, planet formation has mostly been a topic tackled by computer simulations,” says Sascha Quanz. “If our discovery is indeed a forming planet, then for the first time scientists will be able to study the planet formation process and the interaction of a forming planet and its natal environment empirically at a very early stage.”
HD 100546 is a well-studied object, and it has already been suggested that a giant planet orbits about six times further from the star than the Earth is from the Sun. The newly found planet candidate is located in the outer regions of the system, about ten times further out .
This composite image shows a view from the NASA/ESA Hubble Space Telescope (left) and from the NACO system on ESO’s Very Large Telescope (right) of the gas and dust around the young star HD 100546. The Hubble visible-light image shows the outer disc of gas and dust around the star. The new infrared VLT picture of a small part of the disk shows a candidate protoplanet. Both pictures were taken with a special coronagraph that suppresses the light from the brilliant star. The position of the star is marked with a red cross in both panels. Image Credit: ESO/NASA/ESA/Ardila et al.
The planet candidate around HD 100546 was detected as a faint blob located in the circumstellar disk revealed thanks to the NACO adaptive optics instrument on ESO’s VLT, combined with pioneering data analysis techniques. The observations were made using a special coronagraph in NACO, which operates at near-infrared wavelengths and suppresses the brilliant light coming from the star at the location of the protoplanet candidate .
According to current theory, giant planets grow by capturing some of the gas and dust that remains after the formation of a star . The astronomers have spotted several features in the new image of the disk around HD 100546 that support this protoplanet hypothesis. Structures in the dusty circumstellar disk, which could be caused by interactions between the planet and the disk, were revealed close to the detected protoplanet. Also, there are indications that the surroundings of the protoplanet are potentially heated up by the formation process.
Adam Amara, another member of the team, is enthusiastic about the finding. “Exoplanet research is one of the most exciting new frontiers in astronomy, and direct imaging of planets is still a new field, greatly benefiting from recent improvements in instruments and data analysis methods. In this research we used data analysis techniques developed for cosmological research, showing that cross-fertilisation of ideas between fields can lead to extraordinary progress.”
This video fly-through show the dusty environment around the star HD 100546. A gas giant planet appears to be forming in the ring of dust around the young star. This system is also thought to probably contain another large planet orbiting closer to the star. The protoplanet candidate lies about 70 times further from its star than the Earth does from the Sun and the inner planet lies about ten times closer in. Video Credit: ESO/L. Calçada
Although the protoplanet is the most likely explanation for the observations, the results of this study require follow-up observations to confirm the existence of the planet and discard other plausible scenarios. Among other explanations, it is possible, although unlikely, that the detected signal could have come from a background source. It is also possible that the newly detected object might not be a protoplanet, but a fully formed planet which was ejected from its original orbit closer to the star. When the new object around HD 100546 is confirmed to be a forming planet embedded in its parent disk of gas and dust, it will become an unique laboratory in which to study the formation process of a new planetary system.
This research was presented in a paper “A Young Protoplanet Candidate Embedded in the Circumstellar disc of HD 100546”, by S. P. Quanz et al., to appear online in the 28 February 2013 issue of Astrophysical Journal Letters.
 The protoplanet candidate orbits about 70 times further from its star than the Earth does from the Sun. This distance is comparable to the size of the orbits of outer Solar System dwarf planets such as Eris and Makemake. This location is controversial, as it does not fit well with current theories of planet formation. It is unclear at present whether the newfound planet candidate has been in its current position for the whole time since it formed or whether it could have migrated from the inner regions.
 To study planet formation, astronomers cannot look at the Solar System, as all the planets in our neighborhood were formed more than four billion years ago. But for many years, theories about planet formation were strongly influenced by what astronomers could see in our local surroundings, as no other planets were known. Since 1995, when the first exoplanet around a Sun-like star was discovered, several hundred planetary systems have been found, opening up new opportunities for scientists studying planetary formation. Up to now however, none have been “caught in the act” in the process of being formed, whilst still embedded in the disk of material around their young parent star.
Source: The European Southern Observatory (ESO)