astro.wikisort.org - Asteroid

216 Kleopatra is a large M-type asteroid with a mean diameter of 120 kilometers (75 miles) and is noted for its elongate bone or dumbbell shape.[18][19][8][20] It was discovered on 10 April 1880 by Austrian astronomer Johann Palisa at the Austrian Naval Pola Observatory, in what is now Pula, Croatia, and was named after Cleopatra, the famous Egyptian queen.[1] It has two small minor-planet moons which were discovered in 2008 and later named Alexhelios and Cleoselene.

216 Kleopatra

Discovery [1]
Discovered by	J. Palisa
Discovery site	Pola Obs.
Discovery date	10 April 1880
Designations
MPC designation	(216) Kleopatra
Pronunciation	/ˌkliəˈpætrə/[2]
Named after	Cleopatra (Egyptian queen)[3]
Alternative designations	A880 GB · 1905 OA 1910 RA
Minor planet category	main-belt [1][4] · (central) [5] background [6]
Adjectives	Kleopatrian, Kleopatrean
Orbital characteristics [4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc	137.60 yr (50,259 d)
Aphelion	3.4951 AU
Perihelion	2.0931 AU
Semi-major axis	2.7941 AU
Eccentricity	0.2509
Orbital period (sidereal)	4.67 yr (1,706 d)
Mean anomaly	346.24°
Mean motion	0° 12m 39.6s / day
Inclination	13.113°
Longitude of ascending node	215.36°
Argument of perihelion	180.11°
Known satellites	2 (Alexhelios · Cleoselene)
Physical characteristics
Dimensions	c/a = 0.18±0.02[7] (276 × 94 × 78) ± 15% km[8]
Mean diameter	118±2 km[7] 122±30 km[8] 103±4 km[9] 121.6±1.6 km[10] 135±2 km[11]
Mass	(3.0±0.3)×1018 kg[7] (2.97±0.02)×1018 kg[12][8]
Mean density	3.45±0.41 g/cm3[7] ca. 4.5 g/cm3 (most likely between 3.6±0.4 g/cm3 for D = 135 km and 5.4±0.4 g/cm3 for D = 109 km)[8]
Synodic rotation period	5.385280±0.000001 h[8]
Geometric albedo	0.152 (calculated)[7] 0.1164±0.004[11] 0.170[13] 0.149±0.005[10] 0.1111±0.0336[14] 0.1068[15] 0.200±0.028[9]
Spectral type	M (Tholen)[4] · Xe (SMASS)[4] M [14][16] B–V = 0.713[4] U–B = 0.238[4]
Absolute magnitude (H)	7.30[4][9][11][10][14] 7.35±0.02[5][15][17] · 7.45[13]

Orbit and classification

Kleopatra is a non-family asteroid from the main belt's background population.[6] It orbits the Sun in the central asteroid belt at a distance of 2.1–3.5 AU once every 4 years and 8 months (1,706 days; semi-major axis of 2.79 AU). Its orbit has an eccentricity of 0.25 and an inclination of 13° with respect to the ecliptic.[4] The body's observation arc begins at Leipzig Observatory (534) on 20 April 1880, ten days after to its official discovery observation at Pola Observatory.[1]

Physical characteristics

Size and Shape

Kleopatra is a relatively large asteroid, with a mean (volume-equivalent) diameter of 120±2 km[8][20] and an unusually elongate shape.

The initial mapping of its elongated shape was indicated by stellar occultation observations from eight distinct locations on 19 January 1991.[21] Subsequent observations with the ESO 3.6 m Telescope at La Silla, run by the European Southern Observatory, were interpreted to show a double source with two distinct lobes of similar size.[22] These results were disputed when radar observations at the Arecibo Observatory showed that the two lobes of the asteroid are connected, resembling the shape of a ham-bone. The radar observations provided a detailed shape model that appeared on the cover of Science Magazine.[18] Later models suggested that Kleopatra was more elongate and the most recent models using radar delay-Doppler imaging, adaptive optics, and stellar occultations provide dimensions of 267 × 61 × 48 km.[23][8][20]

Moons

In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty.[24] In September 2008, Franck Marchis and his collaborators announced that by using the Keck Observatory's adaptive optics system, they had discovered two moons orbiting Kleopatra.[25] In February 2011, the minor-planet moons were named Alexhelios /ˌælɪksˈhiːliɒs/ (outer) and Cleoselene /ˌkliːoʊsɪˈliːniː/ (inner), after Cleopatra's children Alexander Helios and Cleopatra Selene II.[1] The outer and inner satellites are about 8.9 ± 1.6 and 6.9 ± 1.6 km in diameter, with periods of 2.7 and 1.8 days, respectively.[26]

Mass, Bulk Density, and Composition

The presence of two moons provides a way to estimate Kleopatra's mass, although its irregular shape makes the orbital modeling a challenge.[26] The most recent adaptive-optics observations and modeling provides a mass of Kleopatra of (1.49±0.16)×10⁻¹² M_⊙, or (2.97±0.32)×10¹⁸ kg, which is significantly lower than previously thought.[12] When combined with the best volume estimate for Kleopatra, this indicates a bulk density of 3.38±0.50 g/cm³.[20]

These recent bulk density results call into question the canonical view of Kleopatra as a pure metallic object.[18] Kleopatra's radar albedo suggests a high metal content in the southern hemisphere, but is similar to the more common S- an C-class asteroids along the equator.[8] One way to reconcile these observations is to hypothesize that Kleopatra is a rubble-pile asteroid with significant porosity in dynamic equilibrium.[20]

Origin

One possible origin that explains Kleopatra's shape, rotation, and moons is that it was created by an oblique impact perhaps 100 million years ago. The increased rotation would have elongated the asteroid and caused Alexhelios to split off. Cleoselene may have split off later, around 10 million years ago. Kleopatra is a contact binary – if it were spinning much faster, the two lobes would separate from each other, making a true binary system.[12][20]

See also

• List of exceptional asteroids

References

External links

• Lightcurve plot of 216 Kleopatra, Palmer Divide Observatory, B. D. Warner (2006)
• Triplicity and physical characteristics of Asteroid (216) Kleopatra
• Astronomers Catch Images of Giant Metal Dog Bone Asteroid – NASA article, May 2000 (archived)
• An Asteroid for the Dogs, August 2000 (archived)
• Dictionary of Minor Planet Names, Google books
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• 216 Kleopatra at AstDyS-2, Asteroids—Dynamic Site
  • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
• 216 Kleopatra at the JPL Small-Body Database
  • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

На других языках

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[de] (216) Kleopatra

(216) Kleopatra ist einer der größten Asteroiden des Asteroiden-Hauptgürtels. Mit einem mittleren Durchmesser von 122 km gehört Kleopatra zu den größeren Asteroiden des Hauptgürtels. Kleopatra hat zwei Monde: Alexhelios und Cleoselene mit Durchmessern von etwa 9 bzw. 7 km.

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- [en] 216 Kleopatra

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[es] (216) Kleopatra

(216) Kleopatra es un asteroide perteneciente al cinturón de asteroides descubierto el 10 de abril de 1880 por Johann Palisa desde el observatorio de Pula, Croacia.[2] Está nombrado en honor de la reina egipcia Cleopatra[3] (c.69 a. C.-30 a. C.).[4]

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[ru] (216) Клеопатра

(216) Клеопатра (лат. Kleopatra) — крупный астероид главного пояса. Открыт 10 апреля 1880 года австрийским астрономом Иоганном Пализой в Венской обсерватории и назван в честь Клеопатры VII, последней царицы эллинистического Египта из македонской династии Птолемеев[3]. Название было предложено венскими астрономами.

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