Astronomers have captured an image of a "baby" planet, or protoplanet, for the first time, orbiting around its star in a ring-shaped gap. WISPIT 2b, a massive gas giant about five times larger than Jupiter, was directly detected by researchers using the Magellan Telescope in Chile and the Large Binocular Telescope in Arizona.
This discovery is significant because it provides the first direct evidence of a growing planet clearing material from a disk gap, as scientists had long predicted. Protoplanetary disks are made up of gas and dust that surround young stars and serve as the birthplace for new planets. The rings and gaps in these disks can form due to the gravitational influence of forming planets.
The team used advanced technology, including the MagAO-X extreme adaptive optics system, which captures direct images of exoplanets. They also studied WISPIT 2b in different wavelengths of infrared light using the LMIRcam detector. These observations revealed a clear dot in one of the ring gaps, which was identified as the protoplanet.
The discovery of WISPIT 2b is not only fascinating for its size and age but also provides insights into the formation process of planets. The planet appears to have formed where it is located, suggesting that it did not form elsewhere and then moved into the gap. This finding highlights the complexities of planetary formation and the need for further research.
In addition to WISPIT 2b, the team detected a second candidate planet in another ring gap, which will be investigated in future studies. The discovery of these planets is an exciting step forward in understanding the process of planetary formation and the diversity of celestial bodies in our galaxy.
The researchers involved in this study are from various institutions, including the University of Arizona and Leiden Observatory in the Netherlands. Their findings were published in two papers in August 2025.
This discovery is significant because it provides the first direct evidence of a growing planet clearing material from a disk gap, as scientists had long predicted. Protoplanetary disks are made up of gas and dust that surround young stars and serve as the birthplace for new planets. The rings and gaps in these disks can form due to the gravitational influence of forming planets.
The team used advanced technology, including the MagAO-X extreme adaptive optics system, which captures direct images of exoplanets. They also studied WISPIT 2b in different wavelengths of infrared light using the LMIRcam detector. These observations revealed a clear dot in one of the ring gaps, which was identified as the protoplanet.
The discovery of WISPIT 2b is not only fascinating for its size and age but also provides insights into the formation process of planets. The planet appears to have formed where it is located, suggesting that it did not form elsewhere and then moved into the gap. This finding highlights the complexities of planetary formation and the need for further research.
In addition to WISPIT 2b, the team detected a second candidate planet in another ring gap, which will be investigated in future studies. The discovery of these planets is an exciting step forward in understanding the process of planetary formation and the diversity of celestial bodies in our galaxy.
The researchers involved in this study are from various institutions, including the University of Arizona and Leiden Observatory in the Netherlands. Their findings were published in two papers in August 2025.