It orbits the Sun at a distance of 4.9–5.5 AU once every 11 years and 11 months (4,345 days; semi-major axis of 5.21 AU). Its orbit has an eccentricity of 0.06 and an inclination of 12° with respect to the ecliptic.[4] The body's observation arc begins with a precovery taken at Lowell Observatory in February 1931, more than 52 years prior to its official discovery observation at Nauchnij.[1]
However this family is not included in David Nesvorný's HCM-analysis from 2014.[14][15] Instead, Makhaon is listed as a non-family asteroid of the Jovian background population on the Asteroids Dynamic Site (AstDyS) which based on another analysis by Milani and Knežević.[7]
In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Makhaon is a dark D-type asteroid, the most common spectral type among the Jupiter trojans.[13][15] It is also an assumed C-type asteroid with a V–I color index of 0.83, lower than most larger D-types. It has a B–R magnitude of 1.23 –the difference in magnitude between the blue and red filter – indicating a spectra redder than that of the Sun, which has a B–R mag of 1.03.[5]
Rotation period
Several rotational lightcurves of Makhaon have been obtained since its first photometric observation by Richard Binzel in 1988. It gave a rotation period of 17.3 hours (U=2).[17] In November 2009, French amateur astronomer René Roy measured a period of 2.6 hours from a fragmentary lightcurve based on a single-night observation.(U=1).[18]
Italian astronomer Stefano Mottola reported a period of 8.6354 and 8.648 taken from observation at La Silla Observatory, Chile, in June 1994, and from Calar Alto Observatory, Spain, in December 2009 with a low brightness variation of 0.06 and 0.09, respectively (U=2/2).[19]
In December 2010 and April 2014, follow-up observations by Daniel Coley in collaboration with Robert Stephens at the Center for Solar System Studies and the Goat Mountain Astronomical Research Station (G79) rendered a period of 8.64 and 8.45 hours and an amplitude of 0.15 magnitude (U=2/2-). The result shows that Binzel's first measurement was probably an alternative period solution (i.e. twice the actual period).[5][20][12][a]
In February 2013, Michael Alkema at the Elephant Head Observatory (G35) in Arizona reported a concurring period of 8.639 hours with a brightness variation of 0.08 magnitude (U=2).[21]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Makhaon measures between 111.65 and 116.14 kilometers in diameter and its surface has an albedo between 0.0476 and 0.056.[9][10][11] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0569 and a diameter of 116.35 kilometers based on an absolute magnitude of 8.4.[5]
100+ largest Jupiter trojans
Largest Jupiter Trojans by survey(A) (mean-diameter in kilometers; YoD: Year of Discovery)
Note: missing data was completed with figures from the JPL SBDB (query) and from the LCDB (query form) for the WISE/NEOWISE and SIMPS catalogs, respectively. These figures are given in italics. Also, listing is incomplete above #100.
Notes
^ abLightcurve plots of (3063) Makhaon from Dec 2010 and Apr 2014 by Daniel Coley at the Center for Solar System Studies (U80) and (U81). Quality code is 1/3 (lightcurve rating at CS3). Summary figures at the LCDB and CS3.
^ abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
^ abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 15 June 2018.