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1335 Demoulina

Stony Florian asteroid from the inner regions of the asteroid belt


Stony Florian asteroid from the inner regions of the asteroid belt

FieldValue
minorplanetyes
name1335 Demoulina
background#D6D6D6
image001335-asteroid shape model (1335) Demoulina.png
captionShape model of *Demoulina* from its lightcurve
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered7 September 1934
mpc_name(1335) Demoulina
alt_names1934 RE1954 RA
named_afterProf. Demoulin
(Belgian astronomer)
mp_categorymain-belt(inner)
Florabackground
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc82.66 yr (30,191 days)
aphelion2.5854 AU
perihelion1.8955 AU
semimajor2.2404 AU
eccentricity0.1540
period3.35 yr (1,225 days)
mean_anomaly255.64°
mean_motion/ day
inclination2.5472°
asc_node172.62°
arg_peri198.89°
dimensionskm
7.47 km (calculated)
km
km
rotationh (poor)
h
albedo
0.24 (assumed)
spectral_typeS (assumed)
abs_magnitude12.812.913.06

(Belgian astronomer) Florabackground 7.47 km (calculated) km km h

0.24 (assumed)

1335 Demoulina, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. Discovered by Karl Reinmuth at Heidelberg Observatory in 1934, the asteroid was named after Prof. Demoulin, a Belgian astronomer at Ghent University. It has a slower-than average spin rate of nearly 75 hours.

Discovery

Demoulina was discovered on 7 September 1934, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. Six nights later, it was independently discovered by Belgian astronomer Eugène Delporte at Uccle Observatory on 13 September 1934. The Minor Planet Center only recognizes the first discoverer.

Orbit and classification

Demoulina is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the asteroid belt. However, it is a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements.

It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,225 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.15 and an inclination of 3° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Heidelberg in 1934.

Physical characteristics

Demoulina is an assumed S-type asteroid.

Rotation period

In February 2006, a rotational lightcurve of Demoulina was obtained from photometric observations by American astronomers Lawrence Molnar and Melissa Haegert at the Calvin–Rehoboth Observatory in New Mexico. Lightcurve analysis gave a rotation period of 74.86 hours with a brightness amplitude of 0.78 magnitude (). While not being a slow rotator, Demoulinas period is significantly longer than that for most asteroids. Its high brightness amplitude also indicates that it has an irregular or elongated shape.

Other photometric lightcurves which are based on a single night of observation are rated poorly ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Demoulina measures between 6.35 and 7.684 kilometers in diameter and its surface has an albedo between 0.2073 and 0.26.

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family, and calculates a diameter of 7.47 kilometers based on an absolute magnitude of 12.8.

Naming

This minor planet was named after Prof. Demoulin, a Belgian astronomer at Ghent University. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 121).

References

Info: 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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