Videos
Just a few weeks ago, ESO revealed a planetary system being born in a new, stunning VLT image. Now, the same telescope, using the same instrument, has taken the first direct image of a planetary system around a star like our Sun, located about 300 light-years away and known as TYC 8998-760-1.
“This discovery is a snapshot of an environment that is very similar to our Solar System, but at a much earlier stage of its evolution,” says Alexander Bohn, a PhD student at Leiden University in the Netherlands, who led the new research published today in The Astrophysical Journal Letters.
“Even though astronomers have indirectly detected thousands of planets in our galaxy, only a tiny fraction of these exoplanets have been directly imaged,” says co-author Matthew Kenworthy, Associate Professor at Leiden University, adding that “direct observations are important in the search for environments that can support life.” The direct imaging of two or more exoplanets around the same star is even more rare; only two such systems have been directly observed so far, both around stars markedly different from our Sun. The new ESO’s VLT image is the first direct image of more than one exoplanet around a Sun-like star. ESO’s VLT was also the first telescope to directly image an exoplanet, back in 2004, when it captured a speck of light around a brown dwarf, a type of ‘failed’ star.
“Our team has now been able to take the first image of two gas giant companions that are orbiting a young, solar analogue,” says Maddalena Reggiani, a postdoctoral researcher from KU Leuven, Belgium, who also participated in the study. The two planets can be seen in the new image as two bright points of light distant from their parent star, which is located in the upper left of the frame (click on the image to view the full frame). By taking different images at different times, the team were able to distinguish these planets from the background stars.
The two gas giants orbit their host star at distances of 160 and about 320 times the Earth-Sun distance. This places these planets much further away from their star than Jupiter or Saturn, also two gas giants, are from the Sun; they lie at only 5 and 10 times the Earth-Sun distance, respectively. The team also found the two exoplanets are much heavier than the ones in our Solar System, the inner planet having 14 times Jupiter’s mass and the outer one six times.
Bohn’s team imaged this system during their search for young, giant planets around stars like our Sun but far younger. The star TYC 8998-760-1 is just 17 million years old and located in the Southern constellation of Musca (The Fly). Bohn describes it as a “very young version of our own Sun.”
These images were possible thanks to the high performance of the SPHERE instrument on ESO’s VLT in the Chilean Atacama desert. SPHERE blocks the bright light from the star using a device called coronagraph, allowing the much fainter planets to be seen. While older planets, such as those in our Solar System, are too cool to be found with this technique, young planets are hotter, and so glow brighter in infrared light. By taking several images over the past year, as well as using older data going back to 2017, the research team have confirmed that the two planets are part of the star’s system.
Further observations of this system, including with the future ESO Extremely Large Telescope (ELT), will enable astronomers to test whether these planets formed at their current location distant from the star or migrated from elsewhere. ESO’s ELT will also help probe the interaction between two young planets in the same system. Bohn concludes: “The possibility that future instruments, such as those available on the ELT, will be able to detect even lower-mass planets around this star marks an important milestone in understanding multi-planet systems, with potential implications for the history of our own Solar System.”
This research was presented in the paper “Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1” to appear in The Astrophysical Journal Letters (https://doi.org/10.3847/2041-8213/aba27e).
The team is composed of Alexander J. Bohn (Leiden Observatory, Leiden University, The Netherlands), Matthew A. Kenworthy (Leiden Observatory), Christian Ginski (Anton Pannekoek Institute for Astronomy, University of Amsterdam, The Netherlands and Leiden Observatory), Steven Rieder (University of Exeter, Physics Department, UK), Eric E. Mamajek (Jet Propulsion Laboratory, California Institute of Technology, USA and Department of Physics & Astronomy, University of Rochester, USA), Tiffany Meshkat (IPAC, California Institute of Technology, USA), Mark J. Pecaut (Rockhurst University, Department of Physics, USA), Maddalena Reggiani (Institute of Astronomy, KU Leuven, Belgium), Jozua de Boer (Leiden Observatory), Christoph U. Keller (Leiden Observatory), Frans Snik (Leiden Observatory) and John Southworth (Keele University, UK).
For external comment on the paper, please contact ESO Astronomer Carlo Manara (cmanara@eso.org), who did not participate in the study.
ESO is the foremost intergovernmental
astronomy organisation in Europe and the world’s most productive
ground-based astronomical observatory by far. It has 16 Member States:
Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany,
Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden,
Switzerland and the United Kingdom, along with the host state of Chile
and with Australia as a Strategic Partner. ESO carries out an
ambitious programme focused on the design, construction and operation of
powerful ground-based observing facilities enabling astronomers to make
important scientific discoveries. ESO also plays a leading role in
promoting and organising cooperation in astronomical research. ESO
operates three unique world-class observing sites in Chile: La Silla,
Paranal and Chajnantor. At Paranal, ESO operates the Very Large
Telescope and its world-leading Very Large Telescope Interferometer as
well as two survey telescopes, VISTA working in the infrared and the
visible-light VLT Survey Telescope. Also at Paranal ESO will host and
operate the Cherenkov Telescope Array South, the world’s largest and
most sensitive gamma-ray observatory. ESO is also a major partner in two
facilities on Chajnantor, APEX and ALMA, the largest astronomical
project in existence. And on Cerro Armazones, close to Paranal, ESO is
building the 39-metre Extremely Large Telescope, the ELT, which will
become “the world’s biggest eye on the sky”.
Alexander Bohn
Leiden Observatory, University of Leiden
Leiden, The Netherlands
Tel: +31 (0)71 527 8150
Email: bohn@strw.leidenuniv.nl
Matthew Kenworthy
Leiden Observatory, University of Leiden
Leiden, The Netherlands
Tel: +31 64 172 0331
Email: kenworthy@strw.leidenuniv.nl
Maddalena Reggiani
Institute of Astronomy, KU Leuven
Leuven, Belgium
Tel: +32 16 19 31 99
Email: maddalena.reggiani@kuleuven.be
Carlo Manara (astronomer who did not participate in the study; contact for external comment)
European Southern Observatory
Garching bei München, Germany
Tel: +49 (0) 89 3200 6298
Email: cmanara@eso.org
Bárbara Ferreira
ESO Public Information Officer
Garching bei München, Germany
Tel: +49 89 3200 6670
Cell: +49 151 241 664 00
Email: pio@eso.org
