Astronomy:9905 Tiziano

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9905 Tiziano
AnimatedOrbitOf9905Tiziano.gif
Orbit of Tiziano (blue), with the inner planets and Jupiter (outermost)
Discovery [1]
Discovered byC. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date24 September 1960
Designations
(9905) Tiziano
Pronunciation[titˈtsjaːno]
Named afterTitian – Tiziano Vecellio
(Renaissance painter)[2]
4611 P-L · 1990 TD10
Minor planet categorymain-belt [1][3] · (inner)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc56.35 yr (20,581 days)
|{{{apsis}}}|helion}}2.7157 AU
|{{{apsis}}}|helion}}2.0914 AU
2.4035 AU
Eccentricity0.1299
Orbital period3.73 yr (1,361 days)
Mean anomaly333.40°
Mean motion0° 15m 52.2s / day
Inclination12.723°
Longitude of ascending node9.1406°
130.73°
Physical characteristics
Dimensions5.239±0.040 km[4]
Geometric albedo0.099±0.016[4]
Absolute magnitude (H)14.4[1]


9905 Tiziano (Italian pronunciation: [titˈtsjaːno]), provisional designation 4611 P-L, is an asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. Discovered during the Palomar–Leiden survey in 1960, the asteroid was named after Italian Renaissance painter Titian.

Discovery

Tiziano was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten, as well as Dutch–American astronomer Tom Gehrels. The asteroid was spotted during the Palomar–Leiden survey by examining photographic plates taken at Palomar Observatory, California, United States.[3]

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[5]

Orbit and classification

Tiziano orbits the Sun in the inner main-belt at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,361 days). Its orbit has an eccentricity of 0.13 and an inclination of 13° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation at Palomar, as no precoveries were taken, and no prior identifications were made.[3]

Physical characteristics

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Tiziano measures 5.239 kilometers in diameter and its surface has an albedo of 0.099.[4] It has an absolute magnitude of 14.4[1]

Rotation period

As of 2017, the asteroid's rotation period, shape and spectral type remain unknown.[1][6]

Naming

This minor planet was named after Tiziano Vecellio (c. 1488–1576) known in English as Titian, who was an Italian Renaissance painter and the most important member of the Venetian school. His application and use of color, would exercise a profound influence not only on painters of the Italian Renaissance, but on future generations of Western art. Titian is famous for the Equestrian Portrait of Charles V and for the Portrait of Pope Paul III.[2] The official naming citation was published by the Minor Planet Center on 2 April 1999 (M.P.C. 34356).[7]

References

External links