2867 Šteins

Features on Å teins

On 11 May 2012, IAU's Working Group for Planetary System Nomenclature announced a naming system for geographical features on Å teins.^[15] Inspired by the asteroid's gem-like shape, its crater are given the English-language names of precious stones, with the largest being named Diamond crater (see below).

Except for the montes of Mercury and the lunar maria (and proposed for 2 Pallas and 7 Iris), the craters of Å teins are the only features in the Solar System whose names are not derived from proper nouns.^[16] In addition, a distinct region on the asteroid has been named Chernykh Regio after the discoverer, Nikolai Chernykh.^[17]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and observations by the Spitzer Space Telescope, Å teins measures 5.16 and 4.92 kilometers in diameter and its surface has an albedo of 0.30 and 0.34, respectively.^[6][7] Its overall Bond albedo is 0.24 ± 0.01.^[21] In 2012, the photographs of Å teins taken by Rosetta using stereophotoclinometry allowed scientists to determine that the asteroid's dimensions are 6.83 × 5.70 × 4.42 kilometers, which equates to a mean diameter in volume of 5.26 km.^[5] The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.34 and a diameter of 4.9 kilometers with an absolute magnitude of 13.36.^[8]

Rotation

Studying the asteroid with Rosetta spacecraft onboard OSIRIS cameras shortly before its flyby showed via a lightcurve analysis that Šteins has a rotation period of 6.052±0.007 hours.^[22][20] The results of the rotational lightcurve agree with ground-based photometric observations of Šteins with a period of 6.049 hours and a brightness amplitude between 0.18 and 0.31 magnitude (U=3/3).^{[8][10][12][13][23][24][a]}

A lightcurve inversion also modeled a concurring sidereal period of 6.04681 hours and determined a spin axis at (250.0°, −89.0°) in ecliptic coordinates (λ, β). The modeling was done by compiling a set of 26 previously obtained visible lightcurves.^[25]

Rosetta flyby

On 5 September 2008, the Rosetta space probe flew by Å teins at a distance of 800 km and a relatively slow speed of 8.6 km/s. Despite the short duration of this encounter (approximately 7 minutes in total), a great amount of data was obtained by the 15 scientific instruments operating on board the Rosetta spacecraft.^[26] This was the first of two planned asteroid flybys performed by the probe, with the second being to the much larger 21 Lutetia in 2010.^[27] The timing of the flyby meant that the asteroid was illuminated by the Sun from the perspective of the spacecraft, making the transmitted images clear. The European Space Operations Centre streamed a press conference on Å teins later that day.^[28]