4029 Bridges

Orbit and classification

Bridges is a stony S-type asteroid that orbits the Sun in the middle main-belt at a distance of 2.2–2.9 AU once every 4.01 years (1,466 days). Its orbit has an eccentricity of 0.13 and an inclination of 5° with respect to the ecliptic. With a semi-major axis of 2.525 AU, Bridges is near the main-belt's Kirkwood gap at 2.5 AU, which corresponds to the 3:1 orbital resonance with the gas giant Jupiter. It is, however, not a member of the Alinda family due to its much lower eccentricity.

It was first identified as at the Chilean Cerro El Roble Observatory in 1974, extending the body's observation arc by 8 years prior to its official discovery observation at Palomar.

Physical characteristics

Primary

Rotation period

In May 2002, a first rotational lightcurve of Bridges was obtained from photometric observations by French amateur astronomers René Roy and Laurent Bernasconi. Lightcurve analysis gave a well-defined rotation period of 3.6941 hours with a brightness variation of 0.24 magnitude ().

A large number of observations have followed since 2006, when a satellite in orbit of Bridges was discovered (see below). Between 2007 and 2012, several observation by astronomers Petr Pravec and gave a period between 3.57459 and 3.5754 hours with an amplitude between 0.18 and 0.29 magnitude ().

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer (WISE) with its subsequent NEOWISE mission, Bridges measures 7.433 and 8.015 kilometers in diameter and its surface has an albedo of 0.265 and 0.2007, respectively. The Collaborative Asteroid Lightcurve Link adopts Petr Pravec's revised WISE-data, that is, an albedo of 0.1848 and a diameter of 7.91 kilometers with an absolute magnitude of 12.96.

Satellite

In April and May 2006, Bridges was observed by astronomers David Higgins at Hunters Hill Observatory (E14), Australia, Petr Pravec and Peter Kušnirák at Ondřejov Observatory Czech Republic, Walter R. Cooney Jr., John Gross and Dirk Terrell at Sonoita Research Observatory (G94), United States, and Robert Stephens at Santana Observatory (646), United States.

The observed mutual occultation/eclipsing events revealed, that Bridges is a binary asteroid, that is orbited every hours by a minor-planet moon. A refined orbital period of 16.317 hours was later published. Based on the system's secondary-to-primary mean-diameter ratio of , the satellite measures approximately kilometers in diameter. Johnston's Archive also estimates a semi-major axis of 13 kilometers for the moon's orbit.

Naming

This minor planet was named after Patricia M. Bridges, planetary cartographer with the United States Geological Survey. Bridges has created detailed maps of several planetary body's surface features, and has been an airbrushing expert for shaded lunar relief maps based on spacecraft images. The approved naming citation was published by the Minor Planet Center on 12 December 1989 (M.P.C. 15576).

Notes

• lightcurve plot porb

• lightcurve plot porb contacts

• lightcurve plot p1 Remarks: P_orb = 16.31 +/- 0.02 h, a lower limit on D_2/D_1 = 0.32 +/- 0.02. H_R estimated assuming G = 0.24 +/- 0.11

• lightcurve plot p1

• lightcurve plot porb

• lightcurve plot p1

• lightcurve plot porb

• lightcurve plot p1 (A)

• lightcurve plot porb (A)

• lightcurve plot p1 (B)

• lightcurve plot porb (B)

References