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1170 Siva

Asteroid


Asteroid

FieldValue
minorplanetyes
name1170 Siva
background#FA8072
image001170-asteroid shape model (1170) Siva.png
captionModelled shape of *Siva* from its lightcurve
discovery_ref
discovered29 September 1930
discovererE. Delporte
discovery_siteUccle Obs.
mpc_name(1170) Siva
alt_names1930 SQ
named_afterShiva (Hindu deity)
mp_categoryMars-crosser
Phocaea
orbit_ref
epoch16 February 2017 (JD 2457800.5)
uncertainty0
observation_arc85.19 yr (31,116 days)
aphelion3.0245 AU
perihelion1.6291 AU
semimajor2.3268 AU
eccentricity0.2998
period3.55 yr (1,296 days)
mean_anomaly94.741°
mean_motion/ day
inclination22.184°
asc_node0.9218°
arg_peri59.391°
moid0.7263 AU
mars_moid0.3760 AU
dimensionskm
km (IRAS:2)
km
rotationh
h
h
albedo
(IRAS:2)
spectral_typeB–V = 0.864
U–B = 0.452
Tholen = SS
abs_magnitude12.0012.1812.43

Phocaea km (IRAS:2) km h h (IRAS:2)

U–B = 0.452 Tholen = SS

1170 Siva, provisional designation , is a stony Phocaea asteroid and large Mars-crosser from the innermost regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 29 September 1930, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium, and later named after the Hindu deity Shiva.

Orbit and classification

Siva is a Mars-crossing asteroid, as it crosses the orbit of Mars at 1.666 AU. It is also a member of the Phocaea family (701). It orbits the Sun at a distance of 1.6–3.0 AU once every 3 years and 7 months (1,296 days). Its orbit has an eccentricity of 0.30 and an inclination of 22° with respect to the ecliptic. Siva was first observed at the Japanese Kwasan Observatory, 3 days prior to is discovery. The body's observation arc begins at Uccle, two weeks after its official discovery observation.

Naming

This minor planet is named after Shiva, a Hindu deity often depicted with a third eye on his forehead and with a snake around his neck. Naming citation was first mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 109).

Physical characteristics

In the Tholen taxonomy, Siva is a stony S-type asteroid.

Rotation period

Only fragmentary lightcurves of Siva have been obtained since 2001. They gave a rotation period between 3.5 and 5.22 hours with a small change in brightness of 0.04 to 0.1 magnitude (). As of 2017, no secure period has been published.

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Siva measures between 7.68 and 12.13 kilometers in diameter, and its surface has an albedo between 0.128 and 0.40. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1751 and a diameter of 10.37 kilometers with an absolute magnitude of 12.43. Siva belongs to the brightest known Mars-crossers.

Notes

References

Info: Wikipedia Source

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