511 Davida

511 Davida
Discovery
Discovered byR. S. Dugan
Discovery dateMay 30, 1903
Designations
Designation
(511) Davida
Pronunciation/dəˈvdə/,[1] Latin Dāvīda
Named after
David Peck Todd
1903 LU
main-belt · (outer)
Meliboea[2]
AdjectivesDavidian /dəˈvɪdiən/[3]
Orbital characteristics[4]
Epoch July 01, 2021
(JD 2459396.5, heliocentric)
Aphelion3.759 AU
Perihelion2.569 AU
3.163 AU
Eccentricity0.188
5.626 yr (2055 d)
113°
Inclination15.94°
107.6°
337.2°
Physical characteristics
Dimensions(357 ± 2) × (294 ± 2) × (231 ± 50) km[6][a]
298±4 km[7]
Flattening0.30[b]
Mass(26.6±7.3)×1018 kg[7]
(38±2)×1018 kg[c][5]
Mean density
1.92±0.53 g/cm3[7]
2.97±1.30 g/cm3[5]
0.2137 d (5.130 h)
Albedo0.076±0.007 geometric (0.717±0.013 BV, 0.363±0.020)[4]
Temperature~160 K
Spectral type
C
9.50[8] to 12.98
6.43[4]

511 Davida is a large C-type asteroid in the asteroid belt. It is one of the largest asteroids; approximately tied for 7th place, to within measurement uncertainties, and the 5th or 6th most massive. It was discovered by R. S. Dugan in 1903. Davida is named after David Peck Todd, an astronomy professor at Amherst College.

  1. ^ John Daintith & William Gould, eds. (2006) The Facts On File Dictionary of Astronomy. 5th edition. Infobase Publishing.
  2. ^ Cite error: The named reference Ferret was invoked but never defined (see the help page).
  3. ^ "Davidian". Merriam-Webster.com Dictionary. Merriam-Webster.
  4. ^ a b c JPL data Retrieved 2021-09-29
  5. ^ a b c James Baer, Steven Chesley & Robert Matson (2011) "Astrometric masses of 26 asteroids and observations on asteroid porosity." The Astronomical Journal, Volume 141, Number 5
  6. ^ Conrad (2007), as cited in Baer et al. (2011).[5]
  7. ^ a b c d P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
  8. ^ "Bright Minor Planets 2003". Minor Planet Center. Retrieved May 21, 2008.[permanent dead link]


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