A New High Perihelion Trans-Plutonian Inner Oort Cloud Object: 2015 TG387

Journal Article · Mon Apr 01 04:00:00 EDT 2019 · The Astronomical Journal (Online)

DOI:https://doi.org/10.3847/1538-3881/AB0895· OSTI ID:22897336

Sheppard, Scott S. ^[1]; Trujillo, Chadwick A. ^[2]; Tholen, David J. ^[3]; Kaib, Nathan ^[4]

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1. Department of Terrestrial Magnetism, Carnegie Institution for Science, 5241 Broad Branch Road NW, Washington, DC 20015 (United States)
2. Northern Arizona University, Flagstaff, AZ 86011 (United States)
3. Institute for Astronomy, University of Hawai’i, Honolulu, HI 96822 (United States)
4. HL Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 (United States)

Inner Oort cloud objects (IOCs) are trans-Plutonian for their entire orbits. They are beyond the strong gravitational influences of the known planets, yet close enough to the Sun that outside forces are minimal. Here we report the discovery of the third known IOC after Sedna and 2012 VP113, called 2015 TG387. This object has a perihelion of 65 ± 1 au and semimajor axis of 1170 ± 70 au. The longitude of perihelion angle, ω-bar , for 2015 TG387 is between that of Sedna and 2012 VP113 and thus similar to the main group of clustered extreme trans-Neptunian objects (ETNOs), which may be shepherded into similar orbital angles by an unknown massive distant planet called Planet X, or Planet Nine. The orbit of 2015 TG387 is stable over the age of the solar system from the known planets and Galactic tide. When including outside stellar encounters over 4 Gyr, 2015 TG387's orbit is usually stable, but its dynamical evolution depends on the stellar encounter scenarios used. Surprisingly, when including a massive Planet X beyond a few hundred au on an eccentric orbit that is antialigned in longitude of perihelion with most of the known ETNOs, we find that 2015 TG387 is typically stable for Planet X orbits that render the other ETNOs stable as well. Notably, 2015 TG387's argument of perihelion is constrained, and its longitude of perihelion librates about 180° from Planet X’s longitude of perihelion, keeping 2015 TG387 antialigned with Planet X over the age of the solar system.

• OSTI ID: 22897336
• Journal Information: The Astronomical Journal (Online), Journal Name: The Astronomical Journal (Online) Journal Issue: 4 Vol. 157; ISSN 1538-3881
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ASTEROIDS
COMETS
COSMIC DUST
PLANETS
SATELLITES
SOLAR SYSTEM