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6489 Golevka

Mars-crossing asteroid


Mars-crossing asteroid

FieldValue
minorplanetyes
background#FFC2E0
name6489 Golevka
image6489 Golevka Radar.gif
captionRadar images of 6489 Golevka.
discovererEleanor F. Helin
discovered10 May 1991
mpc_name(6489) Golevka
alt_names1991 JX
mp_category{{Ubl
PHA&thinsp;<ref namejpldata/
epoch6 November 2001 (JD 2452219.5)
orbit_ref
observation_arc8968 days (24.55 yr)
uncertainty0
aphelion4.021663 AU
perihelion0.992813 AU
semimajor2.507238 AU
eccentricity0.604021
period3.97 yr (1450.1 d)
inclination2.278065°
asc_node211.596909°
arg_peri65.939347°
mean_motion/ day
mean_anomaly213.841234°
moid0.0288423 AU
jupiter_moid1.13922 AU
tisserand3.181
mean_diameter
mass
density
rotation6.026 h
spectral_typeQ
abs_magnitude19.2
albedo0.151 ± 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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