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Findings of outer Solar System revealed using information gathered from the Subaru Telescope on Hawaiʻi Island and New Horizons spacecraft

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Survey observations using the Subaru Telescope’s ultra-widefield prime focus camera have revealed that there may be a population of small bodies further out in the Kuiper Belt waiting to be discovered. The results, which are important for understanding the formation of the Solar System, were obtained through an international collaboration between the Subaru Telescope on Hawaiʻi Island and the New Horizons spacecraft traveling through the outer Solar System.

The Subaru Telescope (left) and New Horizons spacecraft (right). (Credit: NAOJ/Southwest Research Institute)

NASA’s New Horizons spacecraft was launched in 2006 with the critical mission of observing the surface of outer Solar System bodies up close for the first time in human history. It successfully completed a flyby of the Pluto system in 2015, and in 2019 it made a flyby of one of the Kuiper Belt objects, (486958) Arrokoth. There have been five spacecraft that have flown to the outer Solar System (including New Horizons), but New Horizons is the only spacecraft that has flown through the Kuiper Belt while observing Kuiper Belt objects, according to a news release from the National Astronomical Observatory of Japan.

The Kuiper Belt is a ring-shaped region of asteroids and other celestial bodies (small objects) located beyond Neptune, about 30 to 55 au from the Sun. Scientists explain that small objects distributed in the Kuiper Belt are called “Kuiper Belt Objects.”

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 according to the NAOJ release.

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.

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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 (see Buie et al. 2024 “The New Horizons Extended Mission Target: Arrokoth Search and Discovery“).

Unfortunately, the Kuiper belt objects so far found during this observation require too much fuel for the spacecraft to fly past, 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 241 Kuiper Belt objects discovered (see Fraiser et al. 2024 “Candidate Distant Trans-Neptunian Objects Detected by the New Horizons Subaru TNO Survey“).

“The most exciting part of the HSC observations was the discovery of 11 objects at distances beyond the known Kuiper Belt,” said team member Dr. Fumi Yoshida (University of Occupational and Environmental Health Sciences; 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). Such a valley had not been reported in other observations.

Figure 2: Distance distribution of Kuiper Belt objects discovered by HSC. The horizontal axis represents the distance from the Sun to the objects, measured in astronomical units (au; the distance between the Earth and the Sun). The vertical axis represents the number of objects. (Credit: Fraser et al. 2024)
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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,” said Dr. Yoshida.

New Horizons mission Principal Investigator Dr. Alan Stern said, “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 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. Researchers say there must be many more distant objects that 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.

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These results were published in two scientific papers in the Planetary Science Journal.

The Subaru Telescope is a large optical-infrared telescope located on Maunakea in Hawaiʻi and operated by the National Astronomical Observatory of Japan, National Institutes of Natural Sciences with the support of the MEXT Project to Promote Large Scientific Frontiers.

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