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2019 van Albada

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name2019 van Albada
background#D6D6D6
discovery_ref
discovered28 September 1935
discovererH. van Gent
discovery_siteJohannesburg Obs.
(Leiden Southern Station)
mpc_name(2019) van Albada
alt_names1931 JN
1941 HS1964 DG
1971 HB1975 ND
1975 PLA911 KD
named_afterGale Bruno van Albada
(Dutch astronomer)
mp_categorymain-beltFlora
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc85.90 yr (31,374 days)
aphelion2.6116 AU
perihelion1.8701 AU
semimajor2.2409 AU
eccentricity0.1655
period3.35 yr (1,225 days)
mean_anomaly221.81°
mean_motion/ day
inclination4.0435°
asc_node252.20°
arg_peri24.949°
dimensionskm
km
km
9.41 km (calculated)
rotationh (R)
h
h
h
h (S)
albedo
0.24 (assumed)
spectral_typeSMASS = SS
abs_magnitude11.9 (R)12.2012.3 (S)

(Leiden Southern Station) 1941 HS1964 DG 1971 HB1975 ND 1975 PLA911 KD (Dutch astronomer) km km 9.41 km (calculated) h h h h (S)

0.24 (assumed)

2019 van Albada, provisional designation , is a stony Florian asteroid and former spacecraft target from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 28 September 1935, by Dutch astronomer Hendrik van Gent at Leiden Southern Station, annex to the Johannesburg Observatory in South Africa. The asteroid was later named after Gale Bruno van Albada.

Orbit and classification

van Albada is a member of the Flora family, one of the largest collisional populations of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,225 days). Its orbit has an eccentricity of 0.17 and an inclination of 4° with respect to the ecliptic.

In May 1911, the asteroid was first identified as at the discovering Johannesburg Observatory. The body's observation arc begins at Lowell Observatory in 1931, four years prior to its official discovery observation.

Former flyby target

van Albada was considered as a flyby target of the NEAR unmanned robotic spacecraft mission in the 1990s. NEAR eventually launched, but visited 253 Mathilde and 433 Eros. There is only a small number of minor planets formerly targeted for spacecraft visitation.

Physical characteristics

In the SMASS classification, van Albada is a common S-type asteroid. It has also been characterized as a stony asteroid by Pan-STARRS photometric survey.

Lightcurves

Between 2012 and 2015, several rotational lightcurves of van Albada were obtained from photometric observations by astronomers Pierre Antonini, Junda Liu, Raoul Behrend and Jean Strajnic, as well as by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a short rotation period between 2.72 and 2.73 hours with a brightness variation between 0.13 and 0.20 magnitude ().

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, van Albada measures between 7.53 and 8.009 kilometers in diameter and its surface has a high albedo between 0.411 and 0.496.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 9.41 kilometers based on an absolute magnitude of 12.3.

Naming

This minor planet was named in memory of Dutch astronomer Gale Bruno van Albada (1911–1972), who was director of the Bosscha Observatory and of the Astronomical Institute at Amsterdam. The approved naming citation was published by the Minor Planet Center on 28 April 1991 (M.P.C. 18135). The lunar crater Van Albada is also named in his honor.

References

Info: Wikipedia Source

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