page_title: 2002 XV93
section_title: Orbit and rotation
hierarchical_section_title: 2002 XV93 / Orbit and rotation
caption_attribution_description: English: 90-minute exposure precovery image of 2002 XV93 taken by the Palomar Observatory in 28 September 1992. DSS precovery images are from DSS plate archive scans by the California Institute of Technology.
context_page_description: 2002 XV₉₃, also written as 2002 XV93, is a trans-Neptunian object with an absolute magnitude of 5.4. A 2:3 orbital resonance with Neptune makes it a plutino.
  It has been observed with precovery images back to 1990.
context_section_description: 2002 XV₉₃ is locked in 2:3 resonance with Neptune, which means that when it makes two revolutions around the Sun, Neptune makes exactly three.
  The rotation period of this object is not known.
caption: Precovery image of 2003 XV93 taken by the Palomar Observatory in 1992[7]