Demoulina is an assumed
S-type asteroid.
Rotation period In February 2006, a rotational
lightcurve of
Demoulina was obtained from photometric observations by American astronomers
Lawrence Molnar and Melissa Haegert at the
Calvin–Rehoboth Observatory in New Mexico. Lightcurve analysis gave a
rotation period of 74.86 hours with a brightness amplitude of 0.78
magnitude (). While not being a
slow rotator,
Demoulinas period is significantly longer than that for most asteroids. Its high brightness amplitude also indicates that it has an irregular or elongated shape. Other photometric lightcurves which are based on a single night of observation are rated poorly ().
Diameter and albedo According to the survey carried out by the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer,
Demoulina measures between 6.35 and 7.684 kilometers in diameter and its surface has an
albedo between 0.2073 and 0.26. The
Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from
8 Flora, the parent body of the Flora family, and calculates a diameter of 7.47 kilometers based on an
absolute magnitude of 12.8. == Naming ==