Aulis is an assumed C-type asteroid. Its V–I color index of 0.98 is typical for that of most Jovian D-types, the dominant spectral type among the larger Jupiter trojans.[10]
Rotation period
Italian astronomer Stefano Mottola obtained two concurring rotational lightcurves from photometric observations. In June 1994, together with astronomer Anders Erikson, he constructed a lightcurve from observations made with the 0.9-meter Dutch telescope at La Silla, showing a rotation period of 18.60±0.05 hours and a brightness variation of 0.09±0.01magnitude (U=2+). In September 2009, he used the 1.2-meter reflector at Calar Alto Observatory, Spain, and measured a refined period of 18.476±0.007 hours with an amplitude of 0.16±0.01 in magnitude (U=2+), confirming his previous result.[9][10]
Diameter and albedo
According to the space-based 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, Aulis measures between 59.57 and 81.92 kilometers in diameter and its surface has an albedo between 0.046 and 0.087.[6][7][8] The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.0553 from IRAS, and derives a similar diameter of 74.53 kilometers based on an absolute magnitude of 9.4.[9]
100+ largest Jupiter trojans
Largest Jupiter Trojans by survey(A) (mean-diameter in kilometers; RP: rotation period in hours; 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.
1234Tedesco, 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 17 June 2018.