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Summary
| DescriptionA very hungry planet (potw2534a).jpg |
English: What appears to be a ripple in space, is today’s Picture of the Week depicting a newborn planet eating its way through its dusty cradle as it orbits its host star. This image, taken with ESO’s Very Large Telescope (VLT) in Chile, is the first clear detection of a baby planet in a disc with multiple rings.
These so-called protoplanetary discs surround young stars and appear as disc-shaped structures of gas and dust, often with rings like the one in this image. They are the birthplace of planets, and the rings are thought to indicate the presence of (hungry) planets in the disc. Initially, little particles in the spinning disc begin to accumulate and grow as gravity takes over, stealing more material from the native disc until they evolve into embryo planets. The clear detection of the planet WISPIT 2b in this image is an important step forward in our understanding of how planets form. It’s about 5 times the mass of Jupiter, and its host star is a younger version of our Sun. It also reinforces the idea that gaps can be created by newly formed planets — a prediction only made in theory that has now been verified observationally. While looking for stars hosting young planets, the team of researchers were lucky enough to find a planet so young that is still embedded in its birth disc. This discovery was published in a paper led by Richelle van Capelleveen at the University of Leiden, Netherlands, in collaboration with an international team of astronomers from the University of Galway and the University of Arizona. It was made possible through the precise observations of the planet-hunting SPHERE instrument on the VLT. SPHERE blocks the light of the central star and corrects atmospheric turbulence with adaptive optics, delivering crisp images of the surroundings of the star. The University of Arizona's MagAO-X AO system on the 6.5m Magellan telescope in Chile detected hydrogen gas falling onto the planet, confirming that it is accreting matter from its surroundings. Further observations of this system might reveal new insights about how our own Solar System may have looked in its early days. Links |
| Date | |
| Source | https://www.eso.org/public/images/potw2534a/ |
| Author | ESO/R. F. van Capelleveen et al. |
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Captions
26 August 2025
744,986 byte
2,040 pixel
2,044 pixel
image/jpeg
a3320f3effe07829c38f8e0c1b776ed07d093438
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:18, 26 August 2025 | 2,044 × 2,040 (728 KB) | Meli thev | Uploaded a work by ESO/R. F. van Capelleveen et al. from https://www.eso.org/public/images/potw2534a/ with UploadWizard |
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| Credit/Provider | ESO/R. F. van Capelleveen et al. |
|---|---|
| Source | European Southern Observatory |
| Short title |
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| Image title |
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| Usage terms |
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| Date and time of data generation | 12:00, 26 August 2025 |
| JPEG file comment | What appears to be a ripple in space, is today’s Picture of the Week depicting a newborn planet eating its way through its dusty cradle as it orbits its host star. This image, taken with ESO’s Very Large Telescope (VLT) in Chile, is the first clear detection of a baby planet in a disc with multiple rings. These so-called protoplanetary discs surround young stars and appear as disc-shaped structures of gas and dust, often with rings like the one in this image. They are the birthplace of planets, and the rings are thought to indicate the presence of (hungry) planets in the disc. Initially, little particles in the spinning disc begin to accumulate and grow as gravity takes over, stealing more material from the native disc until they evolve into embryo planets. The clear detection of the planet WISPIT 2b in this image is an important step forward in our understanding of how planets form. It’s about 5 times the mass of Jupiter, and its host star is a younger version of our Sun. It also reinforces the idea that gaps can be created by newly formed planets — a prediction only made in theory that has now been verified observationally. While looking for stars hosting young planets, the team of researchers were lucky enough to find a planet so young that is still embedded in its birth disc. This discovery, published in a paper led by Richelle van Capelleveen at the University of Leiden, Netherlands, was made possible through the precise observations of the planet-hunting SPHERE instrument on the VLT. SPHERE blocks the light of the central star and corrects atmospheric turbulence with adaptive optics, delivering crisp images of the surroundings of the star. The University of Arizona's MagAO-X AO system on the 6.5m Magellan telescope in Chile detected hydrogen gas falling onto the planet, confirming that it is accreting matter from its surroundings. Further observations of this system might reveal new insights about how our own Solar System may have looked in its early days. Links VLT paper by R. F. van Capelleveen et al., accepted for publication in Astrophysical Journal Letters. Magellan paper by L. M. Close, accepted for publication in Astrophysical Journal Letters. |
| Software used | Adobe Photoshop 26.9 (Windows) |
| File change date and time | 09:41, 20 August 2025 |
| Date and time of digitizing | 13:18, 19 August 2025 |
| Date metadata was last modified | 11:41, 20 August 2025 |
| Unique ID of original document | xmp.did:4b6b435c-a0a2-8946-ba0e-2574885d20ae |
| Keywords | WISPIT 2b |
| Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
| IIM version | 4 |