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914 Palisana

Main-belt asteroid


Summary

Main-belt asteroid

FieldValue
minorplanetyes
background#D6D6D6
name914 Palisana
mpc_name(914) Palisana
alt_names1919 FNA904 PB
A916 WC
pronounced
named_afterJohann Palisa
(Austrian astronomer)
mp_categorymain-beltPhocaea
discovererM. F. Wolf
discovered4 July 1919
discovery_siteHeidelberg Obs.
orbit_ref
epoch31 July 2016 (JD 2457600.5)
uncertainty0
observation_arc84.07 yr (30,706 days)
aphelion2.9857 AU
perihelion1.9300 AU
semimajor2.4578 AU
eccentricity0.2148
period3.85 yr (1,407 days)
mean_anomaly71.191°
mean_motion/ day
inclination25.206°
asc_node255.80°
arg_peri49.144°
dimensionskm
km
km
km
km
mass(2.35 ± 0.24) × 1018 kg
density8.36 ± 1.85 g/cm3
rotation15.922 h
albedo
spectral_typeB–V = 0.741
U–B = 0.368
Tholen = CU
C
abs_magnitude8.76

A916 WC (Austrian astronomer) km km km km

U–B = 0.368 Tholen = CU C

914 Palisana, provisional designation , is a Phocaean asteroid from the inner regions of the asteroid belt, approximately 77 kilometers in diameter. It was discovered by German astronomer Max Wolf at Heidelberg Observatory on 4 July 1919.

Description

The carbonaceous asteroid is classified as a CU-type on the Tholen taxonomic scheme. It orbits the Sun at a distance of 1.9–3.0 AU once every 3 years and 10 months (1,407 days). Its orbit has an eccentricity of 0.21 and an inclination of 25° with respect to the ecliptic.

Measurements using the adaptive optics at the W. M. Keck Observatory give a diameter estimate of 76 km. The size ratio between the major and minor axes is 1.16. During 2004, the asteroid was observed occulting a star. The resulting chords were used to determine a diameter estimate of 91.2 km. This is a poor match to the diameter determined by other means.

The minor planet is named after the Austrian astronomer Johann Palisa (1848–1925), who has discovered many asteroids himself between 1874 and 1923.

References

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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