Press Release

Subaru Telescope Discovers a New Extremely Distant Solar System Object During Hunt for Planet X

October 3, 2018

Using Hyper Suprime-Cam (HSC) on the Subaru Telescope, 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 an even-farther-out Super-Earth, or larger Planet X.


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Figure 1: Movie of the discovery images of 2015 TG387. Two images were taken about 3 hours apart on October 13, 2015 at the Subaru Telescope. 2015 TG387 can be seen moving between the images near the center, while the more distant background stars and galaxies remain stationary. (Credit: Dave Tholen, Chad Trujillo, Scott Sheppard)



The discovery of the newly found object, called 2015 TG387, was made by Carnegie Institution for Sciences' Scott Sheppard, Northern Arizona University's Chad Trujillo, and the University of Hawai'i Institute for Astronomy's David Tholen. 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 is around 34 au, so 2015 TG387 is about two and a half times further away from the Sun than Pluto is right now.

"The objects we're looking for are both faint and can be pretty much anywhere in the sky, so the ability to reach a faint limiting magnitude (large aperture) and cover a large amount of sky (wide field) is crucial for this work. The Subaru Telescope with its wide-field imaging camera Hyper Suprime-Cam is the facility best suited for this work," says Tholen.

The new 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 2300 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 of the 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."


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Figure 2: The orbits of the new extreme object 2015 TG387 and its fellow Inner Oort Cloud objects 2012 VP113 and Sedna, as compared with the rest of the Solar System. The of 2015 TG387 orbit has a larger semi-major axis than both 2012 VP11 and Sedna, so it travels much farther from the Sun, out to 2,300 au. (Credit: Roberto Molar Candanosa and Scott Sheppard / Carnegie Institution for Science)


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 or Planet 9 -- orbiting the Sun, well beyond Pluto at hundreds of au.

"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."

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 -- discovery that would redefine our knowledge of the Solar System's evolution," Sheppard added.

It took the team a few years of observations to obtain a good orbit for 2015 TG387 because it moves so slowly and has such a long orbital period. They first observed 2015 TG387 in October of 2015 at the Subaru Telescope. 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 determine 2015 TG387's orbit.

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 pushing 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. 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.


2015 TG387 was announced in the Minor Planet Electronic Circular issued by the International Astronomical Union's Minor Planet Center on October 1, 2018 (Tholen, D., Sheppard, S., and Trujillo, C. 2018, MPEC, 2018-T05). The research paper with the full details of the discovery is available as a preprint (Scott S. Sheppard, Chadwick A. Trujillo, David J. Tholen, Nathan Kaib 2018, arXiv:1810.00013, "A New High Perihelion Inner Oort Cloud Object"), and has also been submitted to The Astronomical Journal.



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