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1010 Marlene

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1010 Marlene
background#D6D6D6
image001010-asteroid shape model (1010) Marlene.png
captionModelled shape of Marlene from its lightcurve
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered12 November 1923
mpc_name(1010) Marlene
alt_names1923 PF
1950 CJ1950 EY
A903 UDA908 VA
1923 PF
named_afterMarlene Dietrich
(German actress and singer)
mp_categorymain-belt(outer)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc113.61 yr (41,495 days)
aphelion3.2329 AU
perihelion2.6278 AU
semimajor2.9303 AU
eccentricity0.1033
period5.02 yr (1,832 days)
mean_anomaly265.92°
mean_motion/ day
inclination3.9070°
asc_node98.747°
arg_peri279.74°
dimensions43.38 km (derived)
km
km
km
km
km
km
rotationh
h
h
h
albedo
0.0540 (derived)
spectral_typeC
abs_magnitude10.4010.6010.7

1950 CJ1950 EY A903 UDA908 VA 1923 PF (German actress and singer) km km km km km km h h h

0.0540 (derived)

1010 Marlene (prov. designation: or ) is a carbonaceous background asteroid from the outer regions of the asteroid belt, approximately 47 kilometers in diameter. It was discovered on 12 November 1923, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named after German actress and singer Marlene Dietrich.

Classification and orbit

Marlene is not a member of any known asteroid family. It orbits the Sun in the outer main-belt at a distance of 2.6–3.2 AU once every 5.02 years (1,832 days). Its orbit has an eccentricity of 0.10 and an inclination of 4° with respect to the ecliptic.

The asteroid was first identified as at the discovering observatory in October 1903. The body's observation arc begins at Heidelberg in January 1924, more than two months after its official discovery observation.

Naming

This minor planet was named after German-born Marlene Dietrich (1901–1992), actor, singer and high-profile entertainer during World War II. The name was proposed by astronomer Gustav Stracke. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 97).

Physical characteristics

Marlene is an assumed carbonaceous C-type asteroid.

Rotation period

Photometric measurements of Marlene – made by American astronomer Brian Warner at the Palmer Divide Observatory (716), Colorado, in February 2005 – showed a lightcurve with a longer-than average rotation period of hours and a brightness variation of in magnitude (). Most asteroids have periods shorter than 20 hours.

Another lightcurve, obtained by French amateur astronomer René Roy, gave a period of 29.0 hours and an amplitude of 0.17 magnitude ().

Spin axis

In 2013 and 2016, an international study modeled a lightcurve with a concurring period of 31.0651 and 31.066 hours, respectively. The study also determined two spin axis of (299.0°, 42.0°) and (106.0°, 47.0°) 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, Marlene measures between 43.47 and 51.085 kilometers in diameter and its surface has an albedo between 0.03 and 0.0647.

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.054 and a diameter of 43.38 kilometers based on an absolute magnitude of 10.6.

Notes

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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