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(8201) 1994 AH2
Near-Earth asteroid
Near-Earth asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| name | |
| background | #FFC2E0 |
| discovery_ref | |
| discovered | 5 January 1994 |
| discoverer | G. J. Garradd |
| discovery_site | Siding Spring Obs. |
| mpc_name | |
| alt_names | |
| mp_category | ApolloNEO |
| Alinda group | |
| orbit_ref | |
| epoch | 4 September 2017 (JD 2458000.5) |
| uncertainty | 0 |
| observation_arc | 34.86 yr (12,731 days) |
| aphelion | 4.3322 AU |
| perihelion | 0.7436 AU |
| semimajor | 2.5379 AU |
| eccentricity | 0.7070 |
| period | 4.04 yr (1,477 days) |
| mean_anomaly | 285.46° |
| mean_motion | / day |
| inclination | 9.5538° |
| asc_node | 164.12° |
| arg_peri | 25.120° |
| moid | 0.1012 AU39.4 LD |
| jupiter_moid | 0.6611 AU |
| dimensions | km |
| 2.17 km (calculated) | |
| km | |
| rotation | h |
| h | |
| albedo | 0.15 (estimated) |
| 0.18 (assumed) | |
| spectral_type | |
| abs_magnitude | 15.816.3 |
Alinda group 2.17 km (calculated) km h
0.18 (assumed)
**** is a highly eccentric, rare-type asteroid, classified as near-Earth object of the Apollo group of asteroids, approximately 2 kilometers in diameter. It was discovered on 5 January 1994, by Australian amateur astronomer Gordon Garradd during the AANEAS survey at the Siding Spring Observatory, Australia. It has an Earth minimum orbit intersection distance of 0.1 AU and is associated with the Beta Taurids daytime meteor shower.
Orbit and classification
The asteroid orbits the Sun at a distance of 0.7–4.3 AU once every 4.04 years (1,477 days). Its orbit has an eccentricity of 0.71 and an inclination of 10° with respect to the ecliptic. It is a member of the Alinda group of asteroids with a 3:1 resonance with Jupiter that has excited the eccentricity of the orbit over the eons. As an Alinda asteroid it makes approaches to Jupiter, Earth, and Venus.
has an Earth minimum orbital intersection distance of 0.1012 AU, which corresponds to 39.4 lunar distances. Due to its elongated orbit, it also approaches the orbit of Jupiter within 0.1022 AU. On 4 January 2079, it will pass 0.3595 AU from the Earth.
A first precovery was taken at the discovering observatory in 1981, extending the asteroid's observation arc by 13 years prior to its discovery.
Physical characteristics
In the SMASS classification, is characterized as a rare O-type asteroid.
Rotation period
In the late 1990s, Czech astronomer Petr Pravec obtained two rotational lightcurves for this asteroid from photometric observations taken at the Ondřejov Observatory, Czech Republic. They gave a longer-than average rotation period of and 24 hours with a brightness variation of 0.27 and 0.3 magnitude, respectively ().
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 1.86 kilometers in diameter and its surface has an albedo of 0.154. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.18 and calculates a diameter of 2.17 kilometers, based on an absolute magnitude of 15.8. American astronomer Richard Binzel gives a diameter of 2.2 kilometers.
Naming
As of 2017, remains unnamed.
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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