488 Kreusa
| Discovery[1] | |
|---|---|
| Discovered by |
Max Wolf Luigi Carnera |
| Discovery site | Heidelberg |
| Discovery date | 26 June 1902 |
| Designations | |
|
1902 JG, 1947 KH, 1977 YD, A901 CA, A905 XA[1] | |
| Asteroid belt | |
| Orbital characteristics[1][2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 115.18 yr (42068 d) |
| Aphelion | 3.67325 AU (549.510 Gm) |
| Perihelion | 2.66507 AU (398.689 Gm) |
| 3.16916 AU (474.100 Gm) | |
| Eccentricity | 0.15906084 |
| 5.64 yr (2060.7 d) | |
| 197.66463° | |
| 0° 10m 28.913s / day | |
| Inclination | 11.517875° |
| 84.23348° | |
| 71.36554° | |
| Earth MOID | 1.70236 AU (254.669 Gm) |
| Jupiter MOID | 1.5227 AU (227.79 Gm) |
| Jupiter Tisserand parameter | 3.152 |
| Physical characteristics | |
Mean radius |
75.065±3.2 km[1] 81.16 ± 4.77 km[3] |
| Mass | (2.48 ± 1.14) × 1018 kg[3] |
Mean density | 1.10 ± 0.54 g/cm3[3] |
| 32.666 h (1.3611 d)[1] | |
| 0.0589±0.005[1] | |
|
C (Tholen)[1] B−V=0.691±0.06[1] U−B=0.368±0.030[1] | |
| 7.81[1] | |
|
| |
488 Kreusa is an asteroid orbiting the Sun in the asteroid belt.
In 2002, Kreusa was detected by radar from the Arecibo Observatory at a distance of 1.67 AU. The resulting data yielded an effective diameter of 150±21 km.[4]
References
- 1 2 3 4 5 6 7 8 9 10 "488 Kreusa (1902 JG)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
- ↑ AstDys-2 on (488) Kreusa Retrieved 2012-01-03
- 1 2 3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336
, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009.See Table 1. - ↑ Magri, Christopher; et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999 2003" (PDF), Icarus, 186 (1): 126–151, Bibcode:2007Icar..186..126M, doi:10.1016/j.icarus.2006.08.018, retrieved 2015-04-14.
External links
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