1388 Aphrodite
1388 Aphrodite is an asteroid of the Eos family from the outer regions of the asteroid belt, approximately in diameter. It was discovered on 24 September 1935, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. The likely elongated K-type asteroid has a rotation period of 11.9 hours. It was named after the Greek goddess Aphrodite from Greek mythology.
Orbit and classification
Aphrodite is a core member of the Eos family, the largest asteroid family in the outer main belt consisting of nearly 10,000 asteroids. It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months. Its orbit has an eccentricity of 0.09 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins at Johannesburg Observatory in September 1939, just four nights after its official discovery observation at Uccle.Naming
This minor planet was named from Greek mythology after Aphrodite, the Greek goddess of love, beauty, and sexuality, and daughter of Zeus and the Titaness Dione. The asteroid's name was proposed by the German Astronomisches Rechen-Institut. The official was mentioned in The Names of the Minor Planets by Paul Herget in 1955.Physical characteristics
While the asteroid's spectral type is unknown, Aphrodite, with a geometric albedo of around 0.15 , is likely a K-type asteroid, which is typically associated with members of the Eos family.Rotation period and poles
In May 2007, a rotational lightcurve of Aphrodite was obtained from photometric observations by Julian Oey at the Kingsgrove Observatory in Australia in collaboration with other observatories. Lightcurve analysis gave a well-defined rotation period of hours and a brightness variation of 0.65 magnitude, indicative for an elongated, non-spherical shape. Alternative period determinations by Alvaro Alvarez-Candal in 2004, René Roy in 2006, and Kevin Ivarsen in 2003, received a lower rating.A modeled lightcurve using photometry obtained from public databases and through a large collaboration network as well as sparse-in-time individual measurements from a few sky surveys was published in 2016 and 2018. Most recent results gave a concurring sidereal period of hours, as well as two spin axes at and in ecliptic coordinates.