Paydirt in the Outer Solar System

Rings around a Centaur
and the Discovery of a New Dwarf Planet

If you go outside really tonight or early tomorrow morning and look at the eastern horizon around midnight or thereafter, you’ll spot the planet Saturn low in the southeastern part of the sky. Look at it with binoculars or a small telescope and you should be able to make out its gorgeous ring system. Saurn, along with Jupiter, Uranus, and Neptune have ring systems. They were created when smaller bodies (perhaps one or more of their moons) collided and the pieces scattered in orbit around the planets. Until now, no one expected to see rings around anything smaller than a planet.

Well, that’s all changed now. Astronomers have just found a set of rings around a little world called Chariklo (which was discovered in 1997). It’s the first set of rings detected in the solar system since Neptune’s were found late in the 20th century. What makes them MORE unusual is that they’re orbiting a very small world. Chariklo is a member of of a class of small solar system bodies called the Centaurs (which have characteristics similar to both asteroids and comets) and it orbits between Saturn and Uranus. It’s about 250 kilometers in diameter, a small world by any definition.

To learn more about this distant mini-world, astronomers used a new high-resolution camera developed by the Niels Bohr Institute and attach to the Danish telescope at European Southern Observatory’s La Silla Observatory in Chile, to focus on Chariklo just as it was about to pass in front of a star.  Observers at six other locations in South America, including the 1.54-meter Danish and TRAPPIST telescopes at ESO’s La Silla Observatory in Chile, were able to watch the star apparently vanish for a few seconds as its light was blocked by Chariklo. They all expected to see a dip in the star’s brightness as Chariklo moved along through space. What they got was a tiny little dip just before the star disappeared completely from view for a few moments. That little dip was totally unexpected. And, what’s more, it showed up again just after the star reappeared from behind Chariklo.

The data were good enough that even though the entire occultation lasted only five seconds, astronomers figured out the cause for the tiny dip: a set of narrow, thin rings surrounding Chariklo. The team found that the ring system consists of two sharply confined rings only seven and three kilometers wide, likely made largely of chunks of ice and rocky pebbles, both separated by a clear gap of nine kilometers. 

The rings came as a total surprise to the science teams. “We weren’t looking for a ring and didn’t think small bodies like Chariklo had them at all, so the discovery — and the amazing amount of detail we saw in the system — came as a complete surprise,” said Felipe Braga-Ribas (Observatorio Nacional/MCTI, Rio de Janeiro, Brazil). He planned the observation campaign and is publishing a paper today in the journal Nature on the astonishing finding.

So, how did Chariklo get two rings? Probably the same way that Earth got a ring a few billion years ago, and Saturn got a ring sometime in the distant past: through collisions. Two smaller bodies may have collided, or perhaps something crashed into Chariklo, and the debris formed a pair of rings.

This is an amazing discovery, folks. It tells us that collisions are at work in our solar system, forming things as cool as ring systems.

A New World Redefines the Frontier of the Solar System

Chariklo and its rings aren’t the only big news from the distant reaches of the solar system today. Gemini Observatory planetary scientist Chad Trujillo and Carnegie Institution for Science planetary scientist Scott Sheppard announced that the dwarf planet 2012 VP113 is the newest outermost world of the solar system. It orbits even farther from the Sun than Sedna. Both Sedna and 2012 VP113 are part of a huge group of objects that make up the Inner Oort Cloud, part of the outermost reaches of the solar system.   And, there may be even more (and larger) worlds out there yet to be detected! The two scientists’ observations are described in a paper also appearing in Nature today.

Sheppard and Trujillo used the new Dark Energy Camera (DECam) on the NOAO 4-meter telescope in Chile for their work. DECam has the largest field of view of any 4-meter or larger telescope, giving it the ability to search large areas of sky for faint objects. The Magellan 6.5-meter telescope at Carnegie’s Las Campanas Observatory was used to determine the orbit of 2012 VP113 and obtain detailed information about its surface properties.

The fact that this distant world lies so far away from the Sun tells astronomers not just that there are more worlds out there to explore, but that some may be even larger than Earth!  How can this be?

Both Sedna and 2012 VP113 were found at points in their orbits when they were closest to the Sun. The point of closest approach for 2012 VP113 is 80 times the distance between Earth and the Sun, or 80 AU (astronomical unit). Sedna’s closest approach is 76 AU. The most distant parts of their orbits actually stretch out to hundreds of AU.

Both 2012 VP113 and Sedna have similar type orbits, as do a few other objects near the edge of the Kuiper Belt (a region that stretches out beyond the orbit of Neptune). The similarities of all these orbits suggests that there is at least one unknown massive world out there perturbing the orbits of Sedna, 2012 VP113 and other known objects into their current orbital configurations. Sheppard and Trujillo suggest a super Earth or an even larger object that lies perhaps hundreds of AU even farther out could create the shepherding effect seen in the orbits of these objects (which are too distant to be perturbed significantly by any of the known planets).

The Oort Cloud and Kuiper Belt regions of the outer solar system are giving us some of the most exciting finds in solar system exploration. The Inner Oort Cloud is the focus of intense observation now because it can give hints about the history of our solar system’s formative period. Some scientists think that a rogue planet was ejected from the giant planet region of the solar system and plunged through the Inner Oort Cloud on its way out, disturbing the orbits of objects that “live” there. It’s also possible that the gravitational effect of a passing star might have sent some objects racing into the inner Oort Cloud. And, another theory suggests that objects in this region of space used to be planets around stars that were once closer to the Sun in the solar birth cloud.

It has only been in the past few decades that terms like “inner Oort Cloud” came into use by planetary scientists. We knew of the larger Oort Cloud, which is the outermost region that surrounds the rest of the solar system like a large shell. It contains a reservoir of icy objects. Now, with new discoveries like this one, astronomers can further refine specific regions based on characteristics of the objects they contain, such as the Inner Oort Cloud, which stretches about the orbit of Sedna out to a distance of 1,500 AU.  At that point, the Outer Oort Cloud begins and stretches out to at least a quarter of the distance between the Sun and Proxima Centauri (its nearest stellar neighbor). The difference between Inner and Outer? The Outer Oort Cloud is more susceptible to gravitational influences from nearby or passing stars, whereas the objects in the Inner Oort Cloud have more stable orbits and are much less likely to be disturbed by traffic outside the solar system.

The outer solar system has often been called the “final frontier” in terms of our ability to explore it. We keep finding more things out there the more we refine our instruments and search strategies. I can’t wait to see what Trujillo, Sheppard and others find the next time they aim their scopes out that way!