1722 Goffin

Main-belt asteroid From Wikipedia, the free encyclopedia

1722 Goffin, provisional designation 1938 EG, is a stony asteroid from the central region of the asteroid belt, approximately 10.3 kilometers in diameter.

Discoverydate23 February 1938
(1722) Goffin
Quick facts Discovery, Discovered by ...
1722 Goffin
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date23 February 1938
Designations
(1722) Goffin
Named after
Edwin Goffin
(amateur astronomer)[2]
1938 EG Â· 1942 DJ
1950 HK Â· 1952 SW
1952 UQ Â· 1960 WB
1964 UF Â· 1964 VD1
main-belt Â· (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.09 yr (28,889 days)
Aphelion2.6369 AU
Perihelion2.3902 AU
2.5135 AU
Eccentricity0.0491
3.99 yr (1,456 days)
42.038°
0° 14m 50.28s / day
Inclination5.4668°
168.12°
283.20°
Physical characteristics
Dimensions10.290±0.118[4]
10.44 km (taken)[3]
10.442 km[5]
10.446±0.130 km[6]
28.8±1.0 h[a]
31 h[7]
0.2175[5]
0.2191±0.0165[6]
0.224±0.041[4]
S(est.)[7] Â· S[3]
B–V = 0.890[1]
12.18[3][5][6][a] Â· 12.30[1] Â· 12.34[7]
Close

It was discovered on 23 February 1938, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle, Belgium.[8] It was later named after Belgian amateur astronomer Edwin Goffin, following a suggestion by Jean Meeus.[2]

Orbit and classification

Minor planet 1722 Goffin orbits the Sun at a distance of 2.4–2.6 AU once every 3 years and 12 months (1,456 days). Its orbit has an eccentricity of 0.05 and an inclination of 5° with respect to the ecliptic.[1] The body's observation arc begins 6 days after its official discovery observation.[8]

Physical characteristics

It is an assumed S-type asteroid, one of the most common spectral types.[3][7] American astronomer Sherry Fieber-Beyer at NASA Infrared Telescope Facility obtained VNIR spectra on July 20, 2011. The resulting spectrum analysis showed an S-IV assemblage with a derived L-chondrite mineralogy.[9]

Lightcurves

(1722)'s first rotational lightcurve was obtained by American astronomer Richard P. Binzel at UT Austin in October 1984. It gave a rotation period of 31 hours and an brightness variation of 0.63 magnitude (U=2),[7] while Czech astronomers Petr Pravec and Adrián Galád at Ondřejov Observatory derived a period of 28.8 hours with and amplitude of 0.6 magnitude using Binzel's photmetric observations (U=n.a.).[a]

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Goffin measures 10.29 kilometers in diameter and its surface has an albedo of 0.224 (using the 2014-published revised near-infrared albedo fits),[4] superseding a preliminary published diameter of 10.446 kilometers.[6] The Collaborative Asteroid Lightcurve Link takes Petr Pravec's 2012-revised WISE data, that gave an albedo of 0.2175 and a diameter of 10.442 kilometers.[3][5]

Naming

This minor planet was named in honor of the Belgian amateur astronomer Edwin Goffin (born 1950), who has made extensive computations involving minor-planet orbits, and whose initials are indicated by the body's provisional designation, 1938 EG.[2] The official naming citation was published by the Minor Planet Center on 8 April 1982 (M.P.C. 6832).[10]

Notes

  1. Pravec (1984) web: rotation period 28.8±1.0 hours with a brightness amplitude of 0.6 mag. Quality code is not available. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (1722) Goffin and Pravec, P.; Wolf, M.; Sarounova, L. (1984)

References

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