Asteroids

Asteroid observations and imaging, including the asteroid (99862) "Kenlevin" named for Ken Levin. Tracking observations showing asteroid motion against background stars.

Asteroid (99862) Kenlevin

This asteroid was named for Ken Levin in recognition of his contributions to astronomy. The official citation reads:

"Ken Levin (b. 1953) is a physicist who works in the field of infrared optics and sensors for application in medicine, aerospace and astronomy. Levin is an avid amateur astronomer and operates two private observatories."

(99862) "Kenlevin" = 2002 OD2

Observation Statistics

40+
Discoveries
as of Jan 2011
5+
Light Curves
photometry studies
2100+
Recovery/Astrometry
as of Feb 2011
52+
Near-Earth Obs.
as of March 2008

Asteroid Images

(99862) Kenlevin - Asteroid Kenlevin

Asteroid (99862) Kenlevin, named in honor of Ken Levin for his contributions to asteroid observations.

(99862) Kenlevin

H85

Asteroid Kenlevin

2002 QF15 - Near-Earth Asteroid

Observation of near-Earth asteroid 2002 QF15 from Wise Observatory and Blackbird Observatory.

2002 QF15

BBO

Near-Earth Asteroid

MP 785 - Asteroid Light Curve

Light curve analysis of minor planet 785.

MP 785

H85

Asteroid Light Curve

WMAP - WMAP Probe

WMAP probe at 1.46 million km, observed on 2005 Nov. 12 following trajectory correction maneuver.

WMAP

H85

WMAP Probe

Recovery of Faint Asteroids

Asteroids that are only observed for a short time can have calculated orbits which have large uncertainties and may be in danger of being lost. Therefore, it is important to recover and observe these asteroids in order to refine their orbital parameters. While some asteroids have not been seen for years, others, although measured (even many times by the surveys), were never identified.

Adding these to the database of unidentified objects increases the amount of computer time needed for identification exponentially. Securing the orbit of these objects allows the assignment of still unidentified measurements, and assures that the asteroid will never be lost, and it probably will be numbered at the next opposition.

We perform targeted searches of faint objects (magnitude between 19 and 20 and beyond) with large uncertainties and in danger of being lost, using dedicated software by J.C. Pelle allowing a high confidence in the identification of the recovered object.

Observatories

H85
Silver Spring Observatory
Maryland
H08 (BBO)
Blackbird Observatory
Cloudcroft, New Mexico
G53
Alder Springs Observatory
Sierra Remote, California

Asteroid Discoveries (Sample)

DateObservatoryObjectMagnitude
2005/10/03H852005TT15 (242693)19.6
2005/11/06H852005 VL219.1
2006/01/30H082006 BN21220.4
2006/03/20H852006 FD19.6
2007/11/08H082007 VW12521.6
2008/12/07H082008 XW620.0
2009/01/15H082009 AT1621.2
2009/01/19H082009 BT921.4
2009/01/19H082009 BU921.8
2009/01/19H082009 BV921.9
2009/10/25H082009 UY9120.3
2009/10/25H082009 UP1919.7
2009/10/25H082009 UD2020.0
2009/11/16H082009 WU20.0
2010/11/30G532010 W73V21.3

Observer: K. Levin • Measurer: N. Teamo / J.C. Pelle