Outer solar system more populated than we thought

Observations of the outer Solar System with the Subaru Telescope have discovered new bodies where none were expected. The new objects are likely members of a much larger population waiting to be discovered. This discovery has profound implications for our understanding of the structure and history of the Solar System. First and foremost, it suggests that the Solar System has more in common with other planetary systems, which in turn has implications on our search for life outside of the Solar System.

The Subaru Telescope has been conducting observations of the outer Solar System to help support NASA’s New Horizons spacecraft, the first mission to observe the Kuiper Belt on the outer edge of the Solar System beyond Neptune while flying through it. The Subaru Telescope has been looking for interesting Kuiper Belt Objects (KBO) for New Horizons to observe up close since before the spacecraft was launched in 2006. These ongoing observations have already discovered 263 KBOs. Among them, 11 objects lay out beyond the accepted edge of the Kuiper Belt.

There has been mounting evidence in recent years for objects beyond the outer edge of the known Kuiper Belt, but this study is significant in that the large number of objects found in a relatively small search area can’t be dismissed as flukes or false positives. The 11 objects discovered this time appear to represent a new class of objects orbiting in a “ring” separated from the known Kuiper Belt by an empty “gap” where very few objects are found. This kind of ring and gap structure has been well documented on the outskirts of many nascent planetary systems observed by the ALMA (Atacama Large Millimeter/submillimeter Array) radio telescope array in Chile.

Dr. Fumi Yoshida (University of Occupational and Environmental Health Sciences; Planetary Exploration Research Center, Chiba Institute of Technology) comments on the possibility of a second ring of KBOs beyond the known one, “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."

Dr. Wes Fraser of the National Research Council of Canada, a co-investigator on the New Horizons mission science team and the study’s lead author, explains, “Our Solar System’s Kuiper Belt long appeared to be very small in comparison with many other planetary systems, but our results suggest that idea might just have arisen due to an observational bias.” He adds, “So maybe, if this result is confirmed, our Kuiper Belt isn’t all that small and unusual after all compared to those around other stars.”

Our search for life in the Universe is hindered by the fact that we have only one confirmed example of a planet where life arose: Earth in the Solar System. With only one example, we can not determine which idiosyncrasies were important for the appearance of life, and which were irrelevant. So anything we can do to rule out a possible prerequisite moves us closer to finding the true prerequisites for life. If it is confirmed that the Solar System formed from a solar nebula that was much larger, and therefore much less unusual than we thought, it not only eliminates “small parent nebula” from the list of possible prerequisites, it greatly increases the possibilities of finding another planetary system that meets all of the true prerequisites for life, thus increasing the probability of finding alien life.

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 Subaru Telescope.”

The number and distribution of objects at the edge of the Solar System is a question for future study. But at the very least, Subaru Telescope’s results indicate that new discoveries await in what was thought to be a cold, empty, boring void beyond the known Kuiper Belt.

Observations of the outer Solar System with the Subaru Telescope have discovered new bodies where none were expected. The new objects are likely members of a much larger population waiting to be discovered. This discovery has profound implications for our understanding of the structure and history of the Solar System. First and foremost, it suggests that the Solar System has more in common with other planetary systems, which in turn has implications on our search for life outside of the Solar System.

The Subaru Telescope has been conducting observations of the outer Solar System to help support NASA’s New Horizons spacecraft, the first mission to observe the Kuiper Belt on the outer edge of the Solar System beyond Neptune while flying through it. The Subaru Telescope has been looking for interesting Kuiper Belt Objects (KBO) for New Horizons to observe up close since before the spacecraft was launched in 2006. These ongoing observations have already discovered 263 KBOs. Among them, 11 objects lay out beyond the accepted edge of the Kuiper Belt.

There has been mounting evidence in recent years for objects beyond the outer edge of the known Kuiper Belt, but this study is significant in that the large number of objects found in a relatively small search area can’t be dismissed as flukes or false positives. The 11 objects discovered this time appear to represent a new class of objects orbiting in a “ring” separated from the known Kuiper Belt by an empty “gap” where very few objects are found. This kind of ring and gap structure has been well documented on the outskirts of many nascent planetary systems observed by the ALMA (Atacama Large Millimeter/submillimeter Array) radio telescope array in Chile.

Dr. Fumi Yoshida (University of Occupational and Environmental Health Sciences; Planetary Exploration Research Center, Chiba Institute of Technology) comments on the possibility of a second ring of KBOs beyond the known one, “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."

Dr. Wes Fraser of the National Research Council of Canada, a co-investigator on the New Horizons mission science team and the study’s lead author, explains, “Our Solar System’s Kuiper Belt long appeared to be very small in comparison with many other planetary systems, but our results suggest that idea might just have arisen due to an observational bias.” He adds, “So maybe, if this result is confirmed, our Kuiper Belt isn’t all that small and unusual after all compared to those around other stars.”

Our search for life in the Universe is hindered by the fact that we have only one confirmed example of a planet where life arose: Earth in the Solar System. With only one example, we can not determine which idiosyncrasies were important for the appearance of life, and which were irrelevant. So anything we can do to rule out a possible prerequisite moves us closer to finding the true prerequisites for life. If it is confirmed that the Solar System formed from a solar nebula that was much larger, and therefore much less unusual than we thought, it not only eliminates “small parent nebula” from the list of possible prerequisites, it greatly increases the possibilities of finding another planetary system that meets all of the true prerequisites for life, thus increasing the probability of finding alien life.

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 Subaru Telescope.”

The number and distribution of objects at the edge of the Solar System is a question for future study. But at the very least, Subaru Telescope’s results indicate that new discoveries await in what was thought to be a cold, empty, boring void beyond the known Kuiper Belt.