The asteroid orbits the Sun in the central main-belt at a distance of 2.0–3.2 AU once every 4 years and 1 month (1,489 days). Its orbit has an eccentricity of 0.23 and an inclination of 13° with respect to the ecliptic.[4] The first identification of this asteroid was made at the Japanese Geisei Observatory in 1990. However the observation was excluded from the asteroid's orbit determination and did not extend its observation arc prior to its discovery.[1]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Myroncope measures 10.8 kilometers in diameter and its surface has an albedo of 0.08.[7][8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a smaller diameter of 6.2 kilometers based on an absolute magnitude of 13.4.[6]
Rotation period and poles
In 2016, the asteroid's lightcurve has been modeled using data from Lowell photometric database, which gave a sidereal rotation period of 7.43019 hours, as well as two spin axes of (72.0°, −64.0°) and (288.0°, −55.0°) in ecliptic coordinates (λ, β) (Q=n.a.).[9]
^ abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68.