| Discovery [1] | |
|---|---|
| Discovered by |
Max Wolf Luigi Carnera |
| Discovery site | Heidelberg |
| Discovery date | 26 June 1902 |
| Designations | |
| (488) Kreusa | |
| Pronunciation | /kriːˈuːsə/ [2] |
| 1902 JG, 1947 KH, 1977 YD, A901 CA, A905 XA [1] | |
| Asteroid belt | |
| Orbital characteristics [1] [3] | |
| 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° | |
| Physical characteristics | |
| 75.065±3.2
km
[1] 81.16 ± 4.77 km [4] | |
| Mass | (2.48 ± 1.14) × 1018 kg [4] |
Mean
density | 1.10 ± 0.54 g/cm3 [4] |
| 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] | |
Kreusa ( minor planet designation: 488 Kreusa) is a C-type asteroid orbiting the Sun in the asteroid belt, with the type indicating a surface with a low albedo and high carbonaceous content. The spectra of the asteroid displays evidence of aqueous alteration. [5]
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. [6]
- ^ a b c d e f g h i j "488 Kreusa (1902 JG)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 6 May 2016.
- ^ "Creüsa". Dictionary.com Unabridged (Online). n.d.
- ^ AstDys-2 on (488) Kreusa Retrieved 2012-01-03
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv: 1203.4336, Bibcode: 2012P&SS...73...98C, doi: 10.1016/j.pss.2012.03.009.See Table 1.
- ^ Fornasier, S.; et al. (February 1999), "Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites", Astronomy and Astrophysics Supplement, 135: 65−73, Bibcode: 1999A&AS..135...65F, doi: 10.1051/aas:1999161.
- ^ 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 14 April 2015.
- 488 Kreusa at AstDyS-2, Asteroids—Dynamic Site
- 488 Kreusa at the JPL Small-Body Database
_mathilde.jpg){kind=small} | This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |
| Discovery [1] | |
|---|---|
| Discovered by |
Max Wolf Luigi Carnera |
| Discovery site | Heidelberg |
| Discovery date | 26 June 1902 |
| Designations | |
| (488) Kreusa | |
| Pronunciation | /kriːˈuːsə/ [2] |
| 1902 JG, 1947 KH, 1977 YD, A901 CA, A905 XA [1] | |
| Asteroid belt | |
| Orbital characteristics [1] [3] | |
| 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° | |
| Physical characteristics | |
| 75.065±3.2
km
[1] 81.16 ± 4.77 km [4] | |
| Mass | (2.48 ± 1.14) × 1018 kg [4] |
Mean
density | 1.10 ± 0.54 g/cm3 [4] |
| 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] | |
Kreusa ( minor planet designation: 488 Kreusa) is a C-type asteroid orbiting the Sun in the asteroid belt, with the type indicating a surface with a low albedo and high carbonaceous content. The spectra of the asteroid displays evidence of aqueous alteration. [5]
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. [6]
- ^ a b c d e f g h i j "488 Kreusa (1902 JG)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 6 May 2016.
- ^ "Creüsa". Dictionary.com Unabridged (Online). n.d.
- ^ AstDys-2 on (488) Kreusa Retrieved 2012-01-03
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv: 1203.4336, Bibcode: 2012P&SS...73...98C, doi: 10.1016/j.pss.2012.03.009.See Table 1.
- ^ Fornasier, S.; et al. (February 1999), "Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites", Astronomy and Astrophysics Supplement, 135: 65−73, Bibcode: 1999A&AS..135...65F, doi: 10.1051/aas:1999161.
- ^ 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 14 April 2015.
- 488 Kreusa at AstDyS-2, Asteroids—Dynamic Site
- 488 Kreusa at the JPL Small-Body Database
|
| This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |