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6489 Golevka
Mars-crossing asteroid
Mars-crossing asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #FFC2E0 |
| name | 6489 Golevka |
| image | 6489 Golevka Radar.gif |
| caption | Radar images of 6489 Golevka. |
| discoverer | Eleanor F. Helin |
| discovered | 10 May 1991 |
| mpc_name | (6489) Golevka |
| alt_names | 1991 JX |
| mp_category | {{Ubl |
| PHA <ref name | jpldata/ |
| epoch | 6 November 2001 (JD 2452219.5) |
| orbit_ref | |
| observation_arc | 8968 days (24.55 yr) |
| uncertainty | 0 |
| aphelion | 4.021663 AU |
| perihelion | 0.992813 AU |
| semimajor | 2.507238 AU |
| eccentricity | 0.604021 |
| period | 3.97 yr (1450.1 d) |
| inclination | 2.278065° |
| asc_node | 211.596909° |
| arg_peri | 65.939347° |
| mean_motion | / day |
| mean_anomaly | 213.841234° |
| moid | 0.0288423 AU |
| jupiter_moid | 1.13922 AU |
| tisserand | 3.181 |
| mean_diameter | |
| mass | |
| density | |
| rotation | 6.026 h |
| spectral_type | Q |
| abs_magnitude | 19.2 |
| albedo | 0.151 ± 0.023 |
| Alinda | Apollo | PHA | Mars-crosser
6489 Golevka is an Apollo, Mars-crosser, and Alinda asteroid discovered in 1991 by Eleanor F. Helin.
Its name has a complicated origin. In 1995, Golevka was studied simultaneously by three radar observatories across the world: Goldstone in California, Yevpatoria RT-70 radio telescope in Ukraine (Yevpatoria is sometimes romanized as Evpatoria) and Kashima in Japan. 'Golevka' comes from the first few letters of each observatory's name; it was proposed by the discoverer following a suggestion by Alexander L. Zaitsev.
Golevka is a small object, measuring 0.6 × 1.4 km. The radar observations revealed that it has a very strange, angular shape that looks different depending on the direction. In 2003 the Yarkovsky effect was first observed at work by high-precision radar observations of Golevka. Between 1991 and 2003, the small force of the Yarkovsky effect caused a shift of 15 km from what would be expected based on only gravitational interactions. This helped evaluate the asteroid's bulk density (2.7 ± 0.5 g/cm3) and mass (2.10 kg).
Golevka approaches Earth to 0.05 AU in 2046, 0.10 AU in 2069, and 0.11 AU in 2092. On the other hand, Golevka's collision probability with any planet is negligible for at least the next nine centuries. Its orbit is strikingly similar to that of 4179 Toutatis in eccentricity, semi-major axis, and inclination. However, Toutatis is better known due to a close approach to Earth in 2004.
References
|access-date=11 April 2016}}
|author-link = David Morrison (astrophysicist) |access-date = 2004-04-15 |url-status = dead |archive-url = https://web.archive.org/web/20051108142011/http://impact.arc.nasa.gov/news_detail.cfm?ID=132 |archive-date = November 8, 2005}}
|access-date=2009-03-16}}
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