The asteroid orbits the Sun at a distance of 0.9–1.3 AU once every 13 months (408 days). Its orbit has an eccentricity of 0.20 and an inclination of 7° with respect to the ecliptic.
Between 2002 and 2006, 1997 XR2 was considered to have about a 1 in 10,000 chance of colliding with Earth on 1 June 2101, based on a 27-day observation arc following its discovery.[4] With an estimated mass of 1.7×1010 kilograms, it was ranked at level 1 on the Torino scale (0–10) of impact risk, and was the only near-Earth object to be ranked higher than zero until it was joined by 2004 VD17 at level 1 in November 2004, and then when 99942 Apophis – then known only by its provisional designation2004 MN4 – was temporarily assessed at level four in December 2004. Both 2004 VD17 and 99942 Apophis are now rated at level zero.
Recovery
On 24 February 2006, 1997 XR2 was observed by the Mount Lemmon Survey after being lost for more than 8 years.[2] The refinement of its orbit eliminated the possibility of impact in 2101. It is now known that on 20 November 2101, the asteroid will be 0.0392 AU (5,860,000 km) from Earth.[5]
Physical characteristics
According to a generic conversion of absolute magnitude to diameter, 1997 XR2 measures 200 to 230 meters.[3][4]
