419 Aurelia

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419 Aurelia
419 Aurelia.png
Lightcurve-base 3D-model of Aurelia on the top with an image of the asteroid on the bottom.
Discovery
Discovered by Max Wolf
Discovery date7 September 1896
Designations
(419) Aurelia
Pronunciation /ɒˈrliə/ [1]
1896 CW
Main belt
Orbital characteristics [2]
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)
297.81°
0° 14m 7.332s / day
Inclination 3.9247°
229.14°
44.326°
Physical characteristics
148.701±1.611  km [2]
124.47 ± 3.08 km [3]
Mass (1.72±0.34)×1018 kg [3]
(1.654 ± 0.481/0.497)×1018 kg [4]
Mean density
1.70 ± 0.35 g/cm3 [3]
1.74 ± 0.506/0.523 g/cm3 [4] [a]
16.784  h (0.6993  d) [2] [5]
0.034±0.008 [2]
F
8.59 [2]

    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.

    Contents

    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. [5]

    Notes

    1. Assuming a diameter of 122 ± 3 km.

    References

    1. "aurelia" . Oxford English Dictionary (Online ed.). Oxford University Press.(Subscription or participating institution membership required.)
    2. 1 2 3 4 5 Yeomans, Donald K., "419 Aurelia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory , retrieved 10 May 2016.
    3. 1 2 3 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, S2CID   119226456. See Table 1.
    4. 1 2 Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides". Monthly Notices of the Royal Astronomical Society. 492 (1): 589–602. doi: 10.1093/mnras/stz3407 .
    5. 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): 135–138, Bibcode:2008MPBu...35..135P.