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520 Franziska

Main-belt asteroid


Summary

Main-belt asteroid

FieldValue
minorplanetyes
name520 Franziska
background#D6D6D6
discovery_ref
discovererM. F. Wolf
P. Götz
discovery_siteHeidelberg Obs.
discovered27 October 1903
mpc_name(520) Franziska
alt_names1903 MVA924 WH
pronounced
named_afterunknown (Franziska)
mp_categorymain-belt(outer)
Eos
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc112.81 yr (41,205 days)
aphelion3.3354 AU
perihelion2.6735 AU
semimajor3.0044 AU
eccentricity0.1102
period5.21 yr (1,902 days)
mean_anomaly291.42°
mean_motion/ day
inclination10.960°
asc_node34.295°
arg_peri21.772°
dimensions
28.61 km (derived)
rotation(superseded)
albedo0.1143 (derived)
spectral_typeTholen CGU
B–V 0.738
abs_magnitude10.6110.69

P. Götz Eos

28.61 km (derived)

B–V 0.738

520 Franziska, provisional designation , is an Eoan asteroid from the outer regions of the asteroid belt, approximately 27 kilometers in diameter. It was discovered on 27 October 1903, by astronomers Max Wolf and Paul Götz at the Heidelberg-Königstuhl State Observatory in southwest Germany. The origin of the asteroid's name is unknown.

Orbit and classification

Franziska is a member the Eos family (606), the largest outer-belt asteroid family consisting of nearly 10,000 known members. It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,902 days). Its orbit has an eccentricity of 0.11 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins one day after its official discovery observation at Heidelberg.

Physical characteristics

In the Tholen classification, Franziskas spectral type is ambiguous. It is closest to a common C-type, and somewhat similar to the rare and also carbonaceous G-type asteroids (CG). The spectrum has also been labelled as "unusual" by Tholen (U). For a carbonaceous asteroid, it has a relatively high albedo (see below).

Rotation period

In December 2013, a rotational lightcurve of Franziska was obtained from photometric observations by American astronomer Frederick Pilcher at the Organ Mesa Observatory in New Mexico. Lightcurve analysis gave a well-defined rotation period of 16.507 hours with a brightness variation of 0.35 magnitude (). The result supersedes Richard Binzel's previously obtained lightcurve from May 1985, which gave a period of 14.0 hours and an amplitude of 0.53 magnitude ().

Poles

Two lightcurves, published in 2016, using modeled photometric data from the Lowell Photometric Database (LPD) and other sources, gave a concurring period of 16.5044 and 16.5045 hours, respectively. Each modeled lightcurve also determined two spin axes of (122.0°, −50.0°) and (301.0°, −59.0°), as well as (282.0°, −79.0°) and (114.0°, −45.0°) in ecliptic coordinates (λ, β), respectively.

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, Franziska measures between 25.261 and 28.67 kilometers in diameter and its surface has an albedo between 0.1226 and 0.147.

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1143 and a diameter of 28.61 kilometers based on an absolute magnitude of 10.69.

Naming

Any reference of this minor planet's name to a person or occurrence is unknown. "Franziska" is a common German female name and was proposed by the second discoverer Paul Götz in 1905 (AN 169, 363).

Unknown meaning

Among the many thousands of named minor planets, Franziska is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between and and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.

References

References

  1. [https://www.germannames.de/wiki/Franziska (German Names)]
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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