2608 Seneca

Orbit

Seneca orbits the Sun at a distance of 1.1–4.0 AU once every 3 years and 12 months (1,457 days). Its orbit has an eccentricity of 0.57 and an inclination of 15° with respect to the ecliptic.

The body's observation arc begins with its official discovery observation in 1978, as no precoveries were taken, and no prior identifications were made.

Close approaches

Seneca has an Earth minimum orbital intersection distance of 0.1321 AU, which corresponds to 51.5 lunar distances. On 22 March 2062, it will pass 0.254 AU from the Earth.

Physical characteristics

In the Tholen taxonomy, Seneca is a stony S-type asteroid.

Photometry

In March 1978, a photometric observations taken by Degewij and Lebofsky at the Lunar and Planetary Laboratory, Arizona, using a 154-cm reflector, gave a rotational lightcurve with a rotation period of 8 hours and a brightness amplitude of 0.4 (0.5) magnitude ().

Radiometry

In addition, radiometric observations by L. and M. Lebofsky with the 71-cm reflector gave a mean-diameter of kilometers and albedo of .

Diameter and albedo

The Minor Planet Center classifies Seneca as an object larger than 1 kilometer ("1+ KM Near-Earth Object"), while Collaborative Asteroid Lightcurve Link derives an albedo of 0.20 and a diameter of 0.9 kilometers based on an absolute magnitude of 17.59. In 1994, astronomer Tom Gehrels published a diameter of 0.9 kilometers with an albedo of 0.21 in his Hazards Due to Comets and Asteroids.

Naming

This minor planet was named after Roman philosopher and statesman Lucius Annaeus Seneca (c. 4 BC – AD 65), also known as "Seneca the Younger" or simply "Seneca". The approved naming citation was published by the Minor Planet Center on 8 April 1982 (M.P.C. 6835). The lunar crater Seneca was also named in his honor.

References

References

1. {{OED. Seneca