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While Seeking Planet X, Astronomers Find a Distant Solar System Object

OCTOBER 2, 2018

Contacts:


Dr. David Tholen
UH Institute for Astronomy
tholen@hawaii.edu
Office: +1 808-956-6930

Dr. Scott Sheppard
Carnegie Institution for Science
ssheppard@carnegiescience.edu
Cell: +1 202-478-8854

Dr. Chad Trujillo
Northern Arizona University
chad.trujillo@nau.edu

Dr. Roy Gal
Media Contact
UH Institute for Astronomy
roygal@hawaii.edu
Cell: +1 808-388-8690

 

 

 

Maintained by RRG

Orbit of newly discovered solar system object 2015 TG387
High Res JPG
Additional versions can be found here.

The orbits of the new extreme dwarf planet 2015 TG387 and its fellow Inner Oort Cloud objects 2012 VP113 and Sedna, as compared with the rest of the Solar System. 2015 TG387 was nicknamed "The Goblin" by its discoverers, since its provisional designation contains "TG", and the object was first seen around Halloween. Its orbit has a larger semi-major axis than both 2012 VP11 and Sedna, so it travels much farther from the Sun, out to 2300 AU.

Credit: Roberto Molar Candanosa and Scott Sheppard / Carnegie Institution for Science

Astronomers have discovered a new object at the edge of our Solar System. The new extremely distant object far beyond Pluto has an orbit that supports the presence of a larger Planet X.

The newly found object, called 2015 TG387, was announced by the International Astronomical Union's Minor Planet Center on Monday, October 1, 2018. A paper with the full details of the discovery has also been submitted to The Astronomical Journal. The discovery was made by Carnegie Institution for Sciences' Scott Sheppard, Northern Arizona University's Chad Trujillo, and Dave Tholen of the University of Hawaiʻi Institute for Astronomy (IfA). Sheppard and Trujillo both completed their doctoral degrees at the IfA.

2015 TG387 was discovered about 80 astronomical units (AU) from the Sun. One AU is the distance between the Earth and Sun. For context, Pluto's distance is around 34 AU, so 2015 TG387 is about two and a half times further away from the Sun than Pluto is right now.

"We think there could be thousands of small bodies like 2015 TG387 out on the Solar System's fringes, but their distance makes finding them very difficult," Tholen said. "Currently we would only detect 2015TG387 when it is near its closest approach to the Sun. For some 99 percent of its 40,000-year orbit, it would be too faint to see, even with today's largest telescopes."

Tholen first observed 2015 TG387 in October of 2015 at the Japanese Subaru 8-meter telescope on Maunakea, Hawaiʻi. The team's software detected the unusual moving object, which led Tholen to more carefully measure the object's position and determine where to point other telescopes for follow-up observations.

It took the team a few years of observations to obtain a good orbit for 2015TG387 because it moves slowly, over a large orbit, so it has a very long orbital period. Follow-up observations at the Magellan telescope at Carnegie's Las Campanas Observatory in Chile, and the Discovery Channel Telescope in Arizona, were obtained in 2015, 2016, 2017 and 2018, to measure 2015 TG387's orbit.

With these data in hand, they determined that the newly found object is on a very elongated orbit and the closest it ever gets to the Sun, a point called perihelion, is about 65 AU. Only 2012 VP113 and Sedna, at 80 and 76 AU respectively, have more distant perihelia than 2015 TG387. Even though 2015 TG387 has the third-most-distant perihelion, its orbital semi-major axis is larger than that of both 2012 VP113 and Sedna, meaning it travels much farther from the Sun than they do. At its furthest point, it reaches all the way out to about 2,300 AU. 2015 TG387 is one of the few known objects that never comes close enough to the Solar System's giant planets, like Neptune and Jupiter, to have significant gravitational interactions with them.

"These so-called Inner Oort Cloud objects like 2015 TG387, 2012 VP113, and Sedna are isolated from most ofthe Solar System's known mass, which makes them immensely interesting," Sheppard explained. "They can be used as probes to understand what is happening at the edge of our Solar System."

The object with the most distant orbit at perihelion, 2012 VP113, was also discovered by Sheppard and Trujillo, in 2014. The discovery of 2012 VP113 led Sheppard and Trujillo to notice similarities of the orbits of several extremely distant Solar System objects, and they proposed the presence of an unknown planet several times larger than Earth - sometimes called Planet X - orbiting the Sun, well beyond Pluto at hundreds of AU.

The object was discovered as part of the team's ongoing hunt for unknown dwarf planets and Planet X. It is the largest and deepest survey ever conducted for distant Solar System objects.

"These distant objects are like breadcrumbs leading us to Planet X. The more of them we can find, the better we can understand the outer Solar System and the possible planet that we think is shaping their orbits - a discovery that would redefine our knowledge of the Solar System's evolution," Sheppard added.

2015 TG387 is likely on the small end of being a dwarf planet, since it has a diameter of roughly 300 kilometers. The location in the sky where 2015 TG387 reaches perihelion is similar to 2012 VP113, Sedna, and most other known extremely distant trans-Neptunian objects, suggesting that something is pulling them into similar types of orbits.

Trujillo and University of Oklahoma's Nathan Kaib ran computer simulations to see how different hypothetical Planet X orbits would affect the orbit of 2015 TG387. The simulations included a super-Earth-mass planet at several hundred AU on an elongated orbit, as proposed by Caltech's Konstantin Batygin and Michael Brown in 2016, building on earlier work by Sheppard and Trujillo. Most of the simulations showed that not only was 2015 TG387's orbit stable for the age of the Solar System, but it was actually shepherded by Planet X's gravity, which keeps the smaller 2015 TG387 away from the massive planet. This gravitational shepherding could explain why the most distant objects in our Solar System have similar orbits. These orbits keep them from ever approaching the proposed planet too closely, similar to how Pluto never gets too close to Neptune even though their orbits cross.

"What makes this result really interesting is that Planet X seems to affect 2015 TG387 the same way as all the other extremely distant Solar System objects. These simulations do not prove that there is another massive planet in our Solar System, but they are further evidence that something big could be out there," Trujillo concludes.

Discovery Images for distant solar system object 2015 TG387

Discovery Images of 2015 TG387

Movie of the discovery images of 2015 TG387. Two images were taken about 3 hours apart on October 13, 2015 at the Subaru Telescope on Maunakea, Hawaiʻi. 2015 TG387 can be seen moving between the images near the center, while the more distant background stars and galaxies remain stationary.

Credits: Dave Tholen, Chad Trujillo, Scott Sheppard

This research was funded by NASA Planetary Astronomy grant NNX15AF44G.

Based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. These results made use of the Discovery Channel Telescope at Lowell Observatory. Lowell is a private, non-profit institution dedicated to astrophysical research and public appreciation of astronomy and operates the DCT in partnership with Boston University, the University of Maryland, the University of Toledo, Northern Arizona University and Yale University. These results used the Large Monolithic Imager, which was built by Lowell Observatory using funds provided by the National Science Foundation (AST-1005313). This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile.


Founded in 1967, the Institute for Astronomy at the University of Hawaiʻi at Mānoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakalā and Maunakea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaiʻi.