| Minorplanet: | yes |
| Background: |
|
| Discovered: | 10 November 1998 |
| Mpc Name: | (23958) |
| Mp Category: | Jupiter trojan |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 30.86 yr (11,272 d) |
| Perihelion: | 4.7171 AU |
| Semimajor: | 5.2313 AU |
| Eccentricity: | 0.0983 |
| Period: | 11.97 yr (4,370 d) |
| Mean Motion: | / day |
| Inclination: | 24.901° |
| Asc Node: | 225.44° |
| Arg Peri: | 234.89° |
| Jupiter Moid: | 0.0976 AU |
| Tisserand: | 2.8050 |
| Mean Diameter: | |
| Albedo: | |
| Abs Magnitude: | 9.90 10.10 10.2 |
(provisional designation ) is a Jupiter trojan from the Greek camp, approximately 47km (29miles) in diameter. It was discovered on 10 November 1998, by astronomers with the LINEAR survey at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. The dark Jovian asteroid belongs to the 110 largest Jupiter trojans and shows an exceptionally slow rotation of 562 hours. It has not been named since its numbering in April 2001.
is a dark Jupiter trojan in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's Lagrangian point, 60° ahead of its orbit . It is also a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 4.7–5.7 AU once every 12 years (4,370 days; semi-major axis of 5.23 AU). Its orbit has an eccentricity of 0.10 and an inclination of 25° with respect to the ecliptic. The body's observation arc begins with its first observation as at the Kiso Observatory in November 1986, or 12 years prior to its official discovery observation at Socorro.
This minor planet was numbered by the Minor Planet Center on 8 April 2001 ., it has not been named.
is an assumed, carbonaceous C-type asteroid. Most Jupiter trojans are D-types, with the reminder being mostly C and P-type asteroids. It has a typical V–I color index of 0.99 and a BR-color of 1.15.
With a rotation period of 562 hours, this slow rotator belongs to the Top 100 slowest rotators known to exist. It is also the third-slowest rotator among the larger Jupiter trojans after 4902 Thessandrus (738 hours) and (7352) 1994 CO (648 hours). In August 2015, a rotational lightcurve of was obtained from photometric observations by the Kepler space observatory during its K2 mission. Lightcurve analysis gave an exceptionally long period of hours with a brightness amplitude of 0.45 magnitude, somewhat indicative of a non-spherical shape . A second, lower-rated lightcurve from Kepler gave an alternative, even longer period of hours .
These results supersede a poor period determination made at the Sierra Nevada Observatory in 2007, which gave a period 12.080 hours .
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Japanese Akari satellite, measures 46.00 and 47.91 kilometers in diameter and its surface has an albedo between 0.076 and 0.084, respectively. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a larger diameter of 50.77 kilometers based on an absolute magnitude of 10.2.