From the April 2006 issue

Does Pluto have rings?

Planetary scientist Alan Stern fills us in on the possibility.
By | Published: April 21, 2006 | Last updated on May 18, 2023
New Horizons
The New Horizons mission, which launched January 19, is on its way to Pluto. It is scheduled to arrive in the Pluto system in 2015.
NASA / JPL
After our team discovered Pluto’s small moons, we realized impacts on them might generate ejecta that gets into orbit around Pluto, creating rings around the planet. Rings have so far been discovered only around our solar system’s gas-giant planets.

The reason Pluto’s small moons might generate rings, but its large moon Charon would not, is that Charon’s gravity requires an escape speed of almost 1,100 mph (1,800 kilometers/hour). This means Charon is large enough to hold on to virtually all ejecta that would result from impacts on its surface. In contrast, P1 and P2 have escape speeds about 10 times smaller, allowing much of the ejecta produced in impact events on their surfaces to get into orbit around Pluto. We’ve also predicted that such rings might occur around large Kuiper Belt objects (KBOs) that have small — P1- and P2-size — satellites.

Hal Weaver, myself, and the rest of our research team wrote about this possibility in scientific papers published in the February 22, 2006, issue of the scientific journal Nature. Our calculations show that such rings would be tenuous, like Jupiter’s ring system. Also, both the occurrence frequency and how much material surrounds Pluto should vary in time — owing to the random nature of impacts on the small moons and the still-uncertain rate in which material from impacts would dissipate.

Any plutonian rings would be almost impossible to spot from Earth, even with the best equipment. However, future stellar occultation events — when Pluto obscures the light from a distant star, allowing astronomers to study the planet carefully — might present opportunities for such a discovery.

The New Horizons mission, which launched January 19, is on its way to Pluto. Once the spacecraft arrives in mid-2015, we plan to use it to look for dust rings or dust sheets in the Pluto system. With exquisitely sensitive cameras and a dust detector, New Horizons is probably the best way to determine if Pluto has rings.

Updated diagram and caption from “How we discovered Pluto’s new worlds”
Pluto and Earth
Each member of the Pluto quadruple system is smaller than the United States. While the distance between San Francisco and Washington is roughly 2,850 miles (4,590 kilometers), Pluto is about one-half this size with a diameter of 1,454 miles (2,340 km). P1 and P2 are tiny in comparison – possibly as small as 29 miles (46 km) across.
Astronomy: Roen Kelly
Updated diagram and caption from “How we discovered Pluto’s new worlds”
Pluto and Earth
Each member of the Pluto quadruple system is smaller than the United States. While the distance between San Francisco and Washington is roughly 2,850 miles (4,590 kilometers), Pluto is about one-half this size with a diameter of 1,454 miles (2,340 km). P1 and P2 are tiny in comparison – possibly as small as 29 miles (46 km) across.
Astronomy: Roen Kelly