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412 Elisabetha

From Wikipedia, the free encyclopedia
Main-belt asteroid

412 Elisabetha
Lightcurve-base 3D-model of 412 Elisabetha.
Discovery
Discovered byMax Wolf
Discovery date7 January 1896
Designations
(412) Elisabetha
1896 CK
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc117.65 yr (42970 d)
Aphelion2.8841 AU (431.46 Gm)
Perihelion2.64290 AU (395.372 Gm)
2.7635 AU (413.41 Gm)
Eccentricity0.043648
4.59 yr (1,678.0 d)
1.07289°
0° 12m 52.344s / day
Inclination13.767°
106.47°
91.701°
Physical characteristics
Dimensions96.056±0.424 km[1]
Mass(1.843 ± 0.850/0.441)×1018 kg[2]
3.422 ± 1.578/0.819 g/cm3[2][a]
19.635 h (0.8181 d)
0.044±0.005[1]
9.17[1]
8.97[3]

412 Elisabetha is a largemain beltasteroid that was discovered by German astronomerMax Wolf on 7 January 1896 inHeidelberg. It may have been named after his mother, Elise Wolf (née Helwerth).[4] This minor planet is orbiting at a distance of2.76 AU from the Sun with aperiod of 4.59 years and anorbital eccentricity (ovalness) of 0.044. Theorbital plane isinclined at an angle of 13.8° to theplane of the ecliptic.[1]

This asteroid is rotating with a period of19.65618±0.00004 h. Shape models and stellaroccultations provide an estimated diameter of97+7
−14
 km
. Older diameter estimates range from76.38±2.114 to111.12±22.22 km.[5]

Notes

[edit]
  1. ^Assuming a diameter of 100.94 ± 1.4 km.

References

[edit]
  1. ^abcdeYeomans, Donald K.,"412 Elisabetha",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved10 May 2016.
  2. ^abFienga, A.; Avdellidou, C.; Hanuš, J. (February 2020)."Asteroid masses obtained with INPOP planetary ephemerides"(PDF).Monthly Notices of the Royal Astronomical Society.492 (1).doi:10.1093/mnras/stz3407.
  3. ^Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project",The Minor Planet Bulletin, vol. 34, pp. 113–119,Bibcode:2007MPBu...34..113W.
  4. ^Schmadel, Lutz D. (2012),Dictionary of Minor Planet Names, Springer, p. 47,ISBN 3642297188.
  5. ^Marciniak, A.; Ďurech, J.; Choukroun, A.; Hanuš, J.; Ogłoza, W.; Szakáts, R.; Molnár, L.; Pál, A.; Monteiro, F.; Frappa, E.; Beisker, W.; Pavlov, H.; Moore, J.; et al. (November 2023). "Scaling slowly rotating asteroids with stellar occultations".Astronomy & Astrophysics.679. id. A60.arXiv:2310.08995.Bibcode:2023A&A...679A..60M.doi:10.1051/0004-6361/202346191.

External links

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