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1777 Gehrels

Asteroid


Summary

Asteroid

FieldValue
minorplanetyes
name1777 Gehrels
background#D6D6D6
discovery_ref
discovered24 September 1960
discovererC. J. van Houten
I. van Houten-G.
T. Gehrels
discovery_sitePalomar Obs.
mpc_name(1777) Gehrels
alt_names4007 P-L1937 GN
1941 BU1951 QB
1958 DAA905 UE
A923 AA
named_afterTom Gehrels (astronomer)
mp_categorymain-belt(middle)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc111.43 yr (40,699 days)
aphelion2.6705 AU
perihelion2.5810 AU
semimajor2.6258 AU
eccentricity0.0171
period4.25 yr (1,554 days)
mean_anomaly37.596°
mean_motion/ day
inclination3.1476°
asc_node334.69°
arg_peri131.12°
dimensions
km
km
12.67 km (taken)
km
rotationh
h
h
h
h
h
h
h
albedo
spectral_typeSMASS = SqS
abs_magnitude11.4211.611.78

I. van Houten-G. T. Gehrels 1941 BU1951 QB 1958 DAA905 UE A923 AA km km 12.67 km (taken) km h h h h h h h

1777 Gehrels, also designated , is a stony asteroid from the middle region of the asteroid belt, approximately 13 kilometers in diameter. It was discovered during the Palomar–Leiden survey in 1960, and named for astronomer Tom Gehrels, one of the survey's principal investigators and credited discoverer.

Discovery

Gehrels was discovered during the Palomar–Leiden survey by the Dutch astronomer couple Ingrid and Cornelis van Houten, in collaboration with Dutch–American astronomer Tom Gehrels at Palomar Observatory, California, on 24 September 1960.

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory, where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.

Orbit and classification

It orbits the Sun in the central main-belt at a distance of 2.6–2.7 AU once every 4 years and 3 months (1,554 days). Its orbit has an eccentricity of 0.02 and an inclination of 3° with respect to the ecliptic.

First observed as at Heidelberg Observatory in 1905, Gehrels first used observation was made at Goethe Link Observatory in 1958, extending the body's observation arc by 2 years prior to its official discovery at Palomar.

Physical characteristics

This S-type asteroid is characterized as a transitional Sq-type in the SMASS classification.

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer (WISE) with its subsequent NEOWISE mission, Gehrels measures between 11.860 and 13.14 kilometers in diameter and its surface has an albedo between 0.2212 and 0.277.

The Collaborative Asteroid Lightcurve Link adopts Petr Pravec's revised WISE-data and takes an albedo of 0.2151 with a diameter of 12.67 kilometers based on an absolute magnitude of 11.773.

Lightcurves

Several rotational lightcurve of Gehrels were obtained from photometric observations by astronomers Wiesław Wiśniewski, Petr Pravec, Pierre Antonini, Raoul Behrend, Donn Starkey, Laurent Bernasconi, Jacques Montier, Serge Heterier, Daniel Klinglesmith and Robert Stephens. Lightcurve analysis gave a rotation period between 2.83 and 2.840 hours with a brightness variation of 0.21 and 0.27 magnitude ().

Naming

This minor planet was named in honor of Dutch-born American astronomer Tom Gehrels (1925–2011), professor at the University of Arizona, staff member of the LPL research center at Tucson, a principal investigator in the Pioneer program, receiver of the Masursky Award, initiator of the Spacewatch project, and co-discoverer of thousands of minor planets in the Palomar–Leiden survey (see above). He was a pioneer in the field of photometric and polarimetric observations of Solar System bodies in the 1950s. The official was published by the Minor Planet Center on 25 September 1971 (M.P.C. 3185).

Notes

References

Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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