Particle.news

Download on the App Store

Newly Cataloged Extreme Trans-Neptunian Object Challenges Planet Nine Hypothesis

The International Astronomical Union's Minor Planet Center officially recognized 2017 OF201, a potential dwarf planet with a highly elongated orbit, on May 21, 2025.

Image
Orbits of 96 minor planets and extreme trans-Neptunian objects. Graphic: Nrco0e / Wikimedia Commons
Image
Image

Overview

  • 2017 OF201, a trans-Neptunian object with an estimated diameter of 470–820 km, has been officially added to the Minor Planet Center catalog.
  • Its extreme orbit ranges from 44–45 AU at perihelion to over 1,600 AU at aphelion, taking approximately 25,000 years to complete a full revolution around the Sun.
  • The object’s trajectory deviates from the clustering patterns of other extreme TNOs, raising questions about the validity of the Planet Nine hypothesis.
  • The discovery was made using archival data from telescopes, with researchers identifying the object in 19 exposures spanning seven years.
  • Astronomers suggest that hundreds of similar distant objects may exist, remaining undetected due to their vast distances from the Sun.