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1691 Oort

Rare-type carbonaceous Themistian asteroid


Rare-type carbonaceous Themistian asteroid

FieldValue
minorplanetyes
name1691 Oort
background#D6D6D6
image1691Oort (Lightcurve Inversion).png
caption
discovery_ref
discovered9 September 1956
discovererK. Reinmuth
I. Groeneveld
discovery_siteHeidelberg Obs.
mpc_name(1691) Oort
alt_names1956 RB1945 TD
1947 DA1950 PZ
1950 RU1951 XW
1955 MW1956 SD
1964 DAA917 TD
named_afterJan Oort (astronomer)
mp_categorymain-beltThemis
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc71.42 yr (26,086 days)
aphelion3.7153 AU
perihelion2.6084 AU
semimajor3.1618 AU
eccentricity0.1750
period5.62 yr (2,054 days)
mean_anomaly240.25°
inclination1.0860°
asc_node174.55°
arg_peri232.69°
dimensions27.13 km (calculated)
km
km
rotationh
h
albedo
0.10 (assumed)
spectral_typeTholen = CUCU
B–V = 0.682
U–B = 0.316
abs_magnitude10.95

I. Groeneveld 1947 DA1950 PZ 1950 RU1951 XW 1955 MW1956 SD 1964 DAA917 TD km

km h

0.10 (assumed) B–V = 0.682 U–B = 0.316

1691 Oort, provisional designation , is a rare-type carbonaceous Themistian asteroid from the outer region of the asteroid belt, approximately 33 kilometers in diameter.

It was discovered on 9 September 1956, by German astronomer Karl Reinmuth and Dutch astronomer Ingrid van Houten-Groeneveld at Heidelberg Observatory in south-west Germany. It was later named after Dutch astronomer Jan Oort.

Orbit and classification

is a member of the Themis family, a dynamical family of outer-belt asteroids with nearly coplanar ecliptical orbits. Oort orbits the Sun at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,054 days). Its orbit has an eccentricity of 0.18 and an inclination of 1° with respect to the ecliptic.

It was first identified as at Turku in 1945, extending body's observation arc by 14 years prior to its official discovery observation. Information about an earlier 1917-identification, , is not available.

Physical characteristics

The dark C-type asteroid, classified as a rare intermediate CU-type in the Tholen taxonomy.

Rotation period

In February 2009, a rotational lightcurve of Oort was obtained from photometric observations taken by French amateur astronomer René Roy. It gave a well-defined rotation period of 10.2705 hours with a brightness variation of 0.38 magnitude (). An international study from 2013, published a concurring, modeled period of 10.2684 hours (n.a.).

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Oort measures 33.64 and 37.37 kilometers in diameter, and its surface has an albedo of 0.065 and 0.053, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and calculates a diameter of 27.13 kilometers with an absolute magnitude of 10.95.

Naming

This minor planet was named in honor of Dutch astronomer Jan Oort (1900–1992), director of the Leiden Observatory (1945–1970), president of the International Astronomical Union (1958–1961), and a well-known authority on stellar statistics and galactic structure.

He overturned the idea that the Sun was at the center of the Milky Way. The Oort cloud, the outermost gravitationally bound region of the Solar System, was also named after him. The official was published by the Minor Planet Center on 15 February 1970 (M.P.C. 3023).

References

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