(129327) Davehamara Main-belt Asteroid

Discovered on 10 October 2005 by CSS at Catalina.

Dave Hamara (b. 1960) served as lead electronic designer for the Camera Control Module on the OSIRIS-REx Asteroid Sample Return Mission OCAMS camera. He worked with gamma ray and neutron instruments and data on Mars Odyssey, Mars Phoenix, Messenger and Lunar Reconnaissance Orbiter missions.Naming citation (WGSBN Bull. 5, #17, 6), IAU / Minor Planet Center, via NASA/JPL

Where Davehamara is today

MercuryVenusEarthEarthMarsMarsDavehamaraDavehamara

Seen from above the solar system on 2026-10-14: Davehamara is 3.21 au from the Sun and 2.34 au from Earth. Computed from JPL's orbital elements.

Facts

Number129327
Provisional designation2005 TG134
Orbit classMain-belt Asteroid
Diameter4.43 km (#11,779 largest of 17,440 named asteroids with a measured size)
Albedo0.0900
Absolute magnitude (H)15.11
Orbital period4.31 years
Semi-major axis2.65 au
Perihelion – aphelion2.08 – 3.21 au
Eccentricity0.212
Inclination12.2°
Closest distance between its orbit and Earth's (MOID)1.10 au

Data: NASA/JPL Small-Body Database and the IAU Minor Planet Center.

Also named after someone called Dave

Also discovered on 10 October 2005

More named asteroids discovered by CSS