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3822 Segovia

Asteroid


Asteroid

FieldValue
minorplanetyes
name3822 Segovia
background#D6D6D6
image003822-asteroid shape model (3822) Segovia.png
captionShape model of *Segovia* from its lightcurve
discovery_ref
discovered21 February 1988
discovererT. Seki
discovery_siteGeisei Obs.
mpc_name(3822) Segovia
alt_names1962 ST
1979 UP
named_afterAndrés Segovia
(classical guitarist)
mp_categorymain-beltFlora
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc54.18 yr (19,789 days)
aphelion2.5360 AU
perihelion2.0033 AU
semimajor2.2697 AU
eccentricity0.1173
period3.42 yr (1,249 days)
mean_anomaly159.41°
mean_motion/ day
inclination2.5596°
asc_node335.91°
arg_peri280.43°
mean_diameter(calculated)
rotation
albedo0.24 (assumed)
spectral_typeS
abs_magnitude13.7

1979 UP

(classical guitarist)

3822 Segovia (prov. designation: ) is a stony Flora asteroid from the inner regions of the asteroid belt. It was discovered by Japanese astronomer Tsutomu Seki at Geisei Observatory in Kōchi, Japan, on 21 February 1988. The presumed S-type asteroid has a rotation period of 11.0 hours and measures approximately 5 km in diameter. It was later named after Spanish guitarist Andrés Segovia.

Orbit and classification

The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,249 days). Its orbit has an eccentricity of 0.12 and an inclination of 3° with respect to the ecliptic. It was first observed as at the Karl Schwarzschild Observatory in 1962, extending the body's observation arc by 26 years prior to its official discovery observation.

Naming

This minor planet was named for world-famous virtuoso classical guitarist Andrés Segovia (1893–1987). In 1959, the discoverer attended one of his concerts in Japan and became inspired to play the guitar. The was published by the Minor Planet Center on 21 April 1989 (M.P.C. 14481).

Physical characteristics

In March 2016, a rotation period of Segovia was published using data from the Lowell Photometric Database (LPD). Using lightcurve inversion and convex shape models, as well as distributed computing power and the help of individual volunteers, a period of hours could be obtained for this asteroid from the LPD's sparse-in-time photometry data (). The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 4.9 kilometers with an absolute magnitude of 13.7.

References

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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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