419 Aurelia
Discovery | |
---|---|
Discovered by | Max Wolf |
Discovery date | 7 September 1896 |
Designations | |
1896 CW | |
Main belt | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 117.23 yr (42819 d) |
Aphelion | 3.2498 AU (486.16 Gm) |
Perihelion | 1.94613 AU (291.137 Gm) |
2.59798 AU (388.652 Gm) | |
Eccentricity | 0.25091 |
4.19 yr (1529.5 d) | |
Average orbital speed | 18.49 km/s |
297.81° | |
0° 14m 7.332s / day | |
Inclination | 3.9247° |
229.14° | |
44.326° | |
Earth MOID | 0.932056 AU (139.4336 Gm) |
Jupiter MOID | 1.87283 AU (280.171 Gm) |
Jupiter Tisserand parameter | 3.368 |
Physical characteristics | |
Dimensions |
±4.1 km 129.01[1] 124.47 ± 3.08 km[2] |
Mass | (1.72 ± 0.34) × 1018 kg[2] |
Mean density | 1.70 ± 0.35 g/cm3[2] |
16.784 h (0.6993 d)[1][3] | |
±0.003 0.0455 | |
F | |
8.42 | |
|
419 Aurelia is a main-belt asteroid that was discovered by German astronomer Max Wolf on September 7, 1896, in Heidelberg. It is classified as an F-type asteroid.
Photometric observations of this asteroid made during 2008 at the Organ Mesa Observatory in Las Cruces, New Mexico gave a "somewhat irregular" light curve with a period of 16.784 ± 0.001 hours and a brightness variation of 0.07 ± 0.01 in magnitude. When allowing for varying aspect angles and changes in mean motion, this result is consistent with past studies.[3]
References
- 1 2 3 Yeomans, Donald K., "419 Aurelia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 10 May 2016.
- 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.
- 1 2 Pilcher, Frederick (September 2008), "Period Determinations for 26 Proserpina, 34 Circe 74 Galatea, 143 Adria, 272 Antonia, 419 Aurelia, and 557 Violetta", The Minor Planet Bulletin, 35 (3), pp. 135–138, Bibcode:2008MPBu...35..135P.
External links
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