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1484 Postrema

Main-belt carbonaceous asteroid


Main-belt carbonaceous asteroid

FieldValue
minorplanetyes
name1484 Postrema
background#D6D6D6
image001484-asteroid shape model (1484) Postrema.png
captionShape model of Postrema from its lightcurve
discovery_ref
discovererG. Neujmin
discovery_siteSimeiz Obs.
discovered29 April 1938
mpc_name(1484) Postrema
alt_names1938 HC1933 DH
A911 KC
pronounced
named_afterpostrēma
("the last of a group")
mp_categorymain-belt(middle)
Postrema
adjectivePostremian
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc84.61 yr (30,903 days)
aphelion3.2973 AU
perihelion2.1816 AU
semimajor2.7394 AU
eccentricity0.2036
period4.53 yr (1,656 days)
mean_anomaly194.22°
mean_motion/ day
inclination17.300°
asc_node72.767°
arg_peri126.82°
dimensionskm
km
km
km
km
km
km
43.42 km (derived)
km
rotationh
h
h
albedo
0.0409 (derived)
spectral_typeSMASS B
abs_magnitude10.8010.8810.9012.10

A911 KC ("the last of a group") Postrema km km km km km km 43.42 km (derived) km h h

0.0409 (derived)

1484 Postrema, provisional designation , is a carbonaceous Postremian asteroid and namesake of the Postrema family from the central regions of the asteroid belt, approximately 41 kilometers in diameter. It was discovered on 29 April 1938, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The name "Postrema" celebrates the astronomer's last minor planet discovery.

Orbit and classification

Postrema is the parent body and namesake of the Postrema family (541), a mid-sized central asteroid family of little more than 100 members.

It orbits the Sun in the central main-belt at a distance of 2.2–3.3 AU once every 4 years and 6 months (1,656 days). Its orbit has an eccentricity of 0.20 and an inclination of 17° with respect to the ecliptic.

The asteroid was first identified as at Johannesburg Observatory in May 1911. The body's observation arc begins with its identification as at Lowell Observatory in February 1933, more than 5 years prior to its official discovery observation at Simeiz.

Physical characteristics

Spectral type

In the SMASS classification, Postrema is a bright carbonaceous B-type asteroid, while the overall spectral type of the Postrema family has been described as that of C- and X-type.

Rotation period

In May 2006, two rotational lightcurves of Postrema were independently obtained from photometric observations. Lightcurve analysis gave a rotation period of 12.19 and 12.1923 hours with a brightness amplitude of 0.23 and 0.22 magnitude, respectively ().

Spin axis

The asteroids lightcurve has also been modeled, using photometric data from the Lowell Photometric Database and other sources. Modelling gave a concurring period of 12.18978 hours, as well as two spin axis of (19.0°, 44°) and (250.0°, 64°) in ecliptic coordinates (λ, β).

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Postrema measures between 34.696 and 47.00 kilometers in diameter and its surface has a notably low albedo between 0.0137 and 0.05.

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0409 and a diameter of 43.42 kilometers based on an absolute magnitude of 10.9.

Naming

This minor planet was named "Postrema", which means "the last of a group". It celebrates Grigory Neujmin's last numbered minor planet discovery. The official was published by the Minor Planet Center in June 1955 (M.P.C. 1252).

The citation only holds true at the time of publication. In retrospect, Postrema is not Neujmin's last discovery, neither by number nor by its discovery date. These would be the asteroids 4420 Alandreev (highest numbered) and 2536 Kozyrev, officially discovered on 15 August 1939, more than a year after Postrema.

References

Info: Wikipedia Source

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