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4217 Engelhardt
Asteroid
Asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 4217 Engelhardt |
| background | #D6D6D6 |
| discovery_ref | |
| discovered | 24 January 1988 |
| discoverer | C. Shoemaker |
| discovery_site | Palomar Obs. |
| mpc_name | (4217) Engelhardt |
| alt_names | 1944 RL |
| 1970 AA | |
| named_after | Wolf von Engelhardt |
| (German mineralogist) | |
| mp_category | main-beltPhocaea |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 72.73 yr (26,563 days) |
| aphelion | 2.8045 AU |
| perihelion | 1.8246 AU |
| semimajor | 2.3145 AU |
| eccentricity | 0.2117 |
| period | 3.52 yr (1,286 days) |
| mean_anomaly | 272.23° |
| mean_motion | / day |
| inclination | 23.129° |
| asc_node | 355.44° |
| arg_peri | 348.79° |
| satellites | 1 (P: 36.03 h) |
| dimensions | km |
| km | |
| km | |
| 9.24 km (derived) | |
| rotation | h |
| h | |
| albedo | |
| 0.2489 (derived) | |
| spectral_type | S |
| abs_magnitude | 12.2012.312.50 |
1970 AA (German mineralogist) km km 9.24 km (derived) h
0.2489 (derived)
4217 Engelhardt, provisional designation , is a stony Phocean asteroid and a potentially binary system from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 24 January 1988, by American astronomer Carolyn Shoemaker at Palomar Observatory in California, and later named after German mineralogist Wolf von Engelhardt.
Classification and orbit
Engelhardt is a stony S-type asteroid and a member of the Phocaea family (701). It orbits the Sun in the inner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,286 days). Its orbit has an eccentricity of 0.21 and an inclination of 23° with respect to the ecliptic.
It was first identified as at Turku Observatory in 1944, extending the body's observation arc by 44 years prior to its official discovery observation at Palomar. It will pass about 0.0017 AU from Earth threatening asteroid in 2736.
Physical characteristics
Lightcurves
In November 2004, a rotational lightcurve of Engelhardt was obtained from photometric observations by American astronomer Brian Warner at this Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation period of 3.066 hours with a brightness amplitude of 0.16 magnitude ().
In December 2011, a follow-up observation by Warner gave a period of 3.0661 hours with 0.18 amplitude (). Due to a couple of supposed occultation and eclipsing events, Warner also suspects that Engelhardt might by a binary system with a minor-planet moon orbiting it every 36.03 hours. The result, however, is far from conclusive.
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, Engelhardt measures between 7.34 and 9.16 kilometers in diameter and its surface has an albedo between and 0.231 and 0.37. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2489 and a diameter of 9.24 kilometers with on an absolute magnitude of 12.3.
Naming
Baltic German geologist and mineralogist Wolf von Engelhardt (1910–2008), expert on impact craters and related mineral metamorphism. He was a professor at the University of Tübingen and a longtime director of its Institute of Mineralogy and Petrography. The approved naming citation was published by the Minor Planet Center on 27 June 1991 (M.P.C. 18456).
Notes
References
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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