When observing Kuiper Belt objects from the ground, we can only observe them at small solar phase angles (the angle between the sun, the object, and the observer). On the other hand, when observing a Kuiper Belt object from a spacecraft in the Kuiper Belt, the same object can be observed at various phase angles and its reflection characteristics can be used to estimate the surface properties of the object. This is something only New Horizons can do.

However, the camera on the spacecraft has a narrow field-of-view and cannot discover Kuiper Belt objects on its own. This is where the Subaru Telescope comes in. The Subaru Telescope uses its wide-field camera to find many Kuiper Belt objects and then narrow down the list of objects that the spacecraft can fly by and observe. This collaboration between New Horizons and the Subaru Telescope began in 2004.

For observations conducted during 2004–2005 with Subaru Telescope's prime focus camera (Suprime-Cam), due to the orbital relationship between Pluto and the spacecraft, an area near the center of the Milky Way galaxy got caught in the background of the search area for Kuiper Belt objects.

Although it was extremely difficult to search for solar system objects with many background stars, the research team was able to find 24 Kuiper Belt objects.

Unfortunately, the Kuiper belt objects so far found during this observation require too much fuel for the spacecraft to flyby, but new ones at great distance may fall within the available fuel reach of New Horizons. In 2020, deeper observations began with Hyper Suprime-Cam (HSC) on the Subaru Telescope, and by 2023, there had been 239 Kuiper Belt objects discovered.

"The most exciting part of the HSC observations was the discovery of 11 objects at distances beyond the known Kuiper Belt," says team member Dr. Fumi Yoshida, from the University of Occupational and Environmental Health Sciences and the Planetary Exploration Research Center, Chiba Institute of Technology.

Many of the objects discovered with HSC are located at distances of 30–55 astronomical units (au) from the sun (1 au corresponds to the distance between the sun and Earth) and are thought to be within the known Kuiper Belt.

On the other hand, the team was not expecting what appears to be a cluster of objects in the 70–90 au region and a valley between 55 au and 70 au (where only a small number of objects are distributed, see figure below). Such a valley had not been reported in other observations.

There may be a new population of Kuiper Belt objects at 70–90 au. "If this is confirmed, it would be a major discovery. The primordial solar nebula was much larger than previously thought, and this may have implications for studying the planet formation process in our solar system," says Dr. Yoshida.

New Horizons mission Principal Investigator Dr. Alan Stern says, "This is a groundbreaking discovery revealing something unexpected, new, and exciting in the distant reaches of the solar system; this discovery probably would not have been possible without the world-class capabilities of the Subaru observatory."

To determine the exact orbits of the objects discovered in this study, the research team is continuing observations with HSC. "I think the discovery of distant objects and the determination of their orbital distribution are important as a stepping stone to understanding the formation history of the solar system, comparing it with exoplanetary systems, and understanding universal planet formation," Dr. Yoshida says of the significance of the study.

New Horizons is currently traveling further out, 60 au from the sun. There must be many more distant objects that we have not yet discovered. The research team is excited to see what the Subaru Telescope and the New Horizons spacecraft will discover beyond the Kuiper Belt.

These results will be published in two papers in the Planetary Science Journal. They are currently available on the arXiv preprint server.

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