(142091) Omerblaes Main-belt Asteroid

Discovered on 29 August 2002 by S. F. Hoenig at Palomar.

Omer Michael Blaes (b. 1961) is an astrophysicist at the University of California Santa Barbara, working on the theory of accretion onto compact objects. He is best known for his contributions to the hydrodynamics of accretion disks, including analysis of shear instabilities and the magnetorotational instability.Naming citation (MPC batch dated 2013-07-22), IAU / Minor Planet Center, via NASA/JPL

Where Omerblaes is today

MercuryVenusEarthEarthMarsMarsOmerblaesOmerblaes

Seen from above the solar system on 2026-10-14: Omerblaes is 2.40 au from the Sun and 3.17 au from Earth. Computed from JPL's orbital elements.

Facts

Number142091
Provisional designation2002 QW52
Orbit classMain-belt Asteroid
Absolute magnitude (H)16.79
Orbital period3.76 years
Semi-major axis2.42 au
Perihelion – aphelion2.12 – 2.71 au
Eccentricity0.121
Inclination6.32°
Closest distance between its orbit and Earth's (MOID)1.15 au

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

Also named after someone called Omer

Also discovered on 29 August 2002

More named asteroids discovered by S. F. Hoenig