In the
SMASS classification,
Savo is an Sa-subtype that transitions from the stony
S-type to the
A-type asteroids.
Rotation period In August 2006, a rotational
lightcurve of
Savo was obtained from photometric observations by Czech astronomer
Petr Pravec at
Ondřejov Observatory. Lightcurve analysis gave a well-defined
rotation period of 5.35011 hours with a brightness amplitude of 0.52
magnitude (), indicative for a non-spherical shape. Follow up observations at the Calvin College Observatory () in 2007 and 2008, gave three nearly identical periods of 5.35020, 5.35031 and 5.35062 hours with an amplitude between 0.44 and 0.63 ().
Poles The asteroid's lightcurve has also been modeled twice. In 2011, the first modelling used photometric data from the AstDyS database and the Uppsala Asteroid Photometric Catalogue, and found two spin axis of (248.0°, −68.0°) and (83.0°, −66.0°) in
ecliptic coordinates (λ, β). A refined modeling in 2016, using the
Lowell Photometric Database gave two poles of (50.0°, −65.0°) and (233.0°, −68.0°) in ecliptic coordinates. Also, both studies found a concurring period of 5.35059 hours.
Diameter and albedo According to the surveys carried out by the Japanese
Akari satellite and the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer,
Savo measures between 7.80 and 9.23 kilometers in diameter and its surface has an
albedo between 0.173 and 0.349. The
Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 10.30 kilometers based on an
absolute magnitude of 12.3. == Naming ==