Astronomy:419 Aurelia

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419 Aurelia
Discovery
Discovered byMax Wolf
Discovery date7 September 1896
Designations
(419) Aurelia
Pronunciation/ɒˈrliə/[1]
1896 CW
Minor planet categoryMain belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc117.23 yr (42819 d)
|{{{apsis}}}|helion}}3.2498 astronomical unit|AU (486.16 Gm)
|{{{apsis}}}|helion}}1.94613 AU (291.137 Gm)
2.59798 AU (388.652 Gm)
Eccentricity0.25091
Orbital period4.19 yr (1529.5 d)
Mean anomaly297.81°
Mean motion0° 14m 7.332s / day
Inclination3.9247°
Longitude of ascending node229.14°
44.326°
Physical characteristics
Mean diameter148.701±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 density1.70 ± 0.35 g/cm3[3]
1.74 ± 0.506/0.523 g/cm3[4][lower-alpha 1]
Rotation period16.784 h (0.6993 d)[2][5]
Geometric albedo0.034±0.008[2]
F
Absolute magnitude (H)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.

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 (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=aurelia  (Subscription or UK public library membership required.)
  2. 2.0 2.1 2.2 2.3 2.4 Yeomans, Donald K., "419 Aurelia", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=419, retrieved 10 May 2016. 
  3. 3.0 3.1 3.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73 (1): 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  4. 4.0 4.1 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. https://academic.oup.com/mnras/article/492/1/589/5658701. 
  5. 5.0 5.1 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, Bibcode2008MPBu...35..135P.