Summary for : (416) Vaticana

DynT.TT.BT T.L B T.DDensity (g/cm^3)Δρ/ρDiameter (km)ΔD/DMass (kg)ΔM/MRefAvg.M
MBASSl- | --3.26 ± 2.27   (D)70 %86.1 ± 3.74.2 %1.09e+18 ± 7.47e+1769 %SEVM
MBASSl- | --2.56 ± 5.03   (E)197 %86.7 ± 8.59.8 %8.72e+17 ± 1.70e+18195 %Sw.avg
MBAS9.44 ± 8.99   (D)95 %87.1 ± 2.63.0 %3.27e+18 ± 3.10e+1895 %C?

Average asteroid densities (g/cm^3):
C = 1.3 ± 0.6, B = 2.4 ± 0.5, S = 2.7 ± 0.5, M = 3.5 ± 1.0, P = 2.8 ± 1.6, X = 1.9 ± 0.8, Xc = 4.9 ± 0.9, Xk = 4.2 ± 0.7 (Ref)

Additional resources:
3D Model | JPL New Horizons | Minor Planet Center | Wikipedia (these auto-generated links might not work)

Note: The density estimates have been ranked from (A) to (E), corresponding to the relative error: (B) less than 20%, (C) between 20 and 50%, (D) between 50 and 100%, and (E) more than 100%. (A) stands for (presumably) reliable estimates (accuracy better than 20%), based on more than 5 mass estimates and 5 diameter estimates, or a spacecraft encounter. Apparently unrealistic densities (ρ > 8) are tagged with (X).

EVM: average by using the Expected Value Method (Ref). w.avg: weighted average (with w = 1/err^2).

T.T: Tholen Tax Class. T.B: Bus & Binzel Tax Class. T T.L: S3OS2 Lazarro (Tholen) Tax Class. T.L B: S3OS2 Lazarro (Bus & Binzel) Tax Class. T.D: DeMeo Tax Class.

Ref: S = SiMDA, C = Carry (2012)

Diameter estimates

DesignationDiameter / Err (km)ΔD/DMethodYearRefNχ2Use
(416) Vaticana85.44 ± 5.866.9 % STM2004D94 0.01 1
(416) Vaticana85.47 ± 1.702.0 % STM2004D93 0.13 2
(416) Vaticana83.56 ± 3.043.6 % STM2010D64 0.68 3
(416) Vaticana84.96 ± 1.411.7 % STM2010D64 0.62 4
(416) Vaticana92.14 ± 4.665.1 % NEATM2010D64 1.70 5
(416) Vaticana128.30 ± 22.8617.8 % NEATM2010D642 3.41 6
(416) Vaticana88.80 ± 1.261.4 % STM2011D83 4.69 7

plot, average diameter and derived density

All

Notes (N):
1: This estimate is discarded for the average diameter (and derived density) calculation in Carry (2012).
2: This estimate is discarded for the average diameter (and derived density) calculation in SiMDA (catalog).

NEATM : Near-Earth Asteroid Thermal Model. STM : Standard Thermal Model.


EVM diam. average D = (86.1 ± 3.65) km   (ΔD/D = 4%, SNR = 23.55) Derived bulk density ρ = (3.26 ± 2.27) g/cm3   (Δρ/ρ = 70%, SNR = 1.4)


References
D64(2010):Ryan, E.L., Woodward, C.E., 2010. Rectified Asteroid Albedos and Diameters from IRAS and MSX Photometry Catalogs. Astronomical Journal 140, 933–943.
D83(2011):Usui, F., Kuroda, D., Müller, T.G., Hasegawa, S., Ishiguro, M., Ootsubo, T., Ishihara, D., Kataza, H., Takita, S., Oyabu, S., Ueno, M., Matsuhara, H., Onaka, T., 2011. Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey. Publications of the Astronomical Society of Japan 63, 1117–1138.
D93(2004):Tedesco, E.F., Noah, P.V., Noah, M.C., Price, S.D., 2004. IRAS Minor Planet Survey. NASA Planetary Data System. IRAS-A-FPA-3-RDR-IMPS-V6.0.
D94(2004):Tedesco, E.F., Egan, M.P., Price, S.D., 2004. MSX Infrared Minor Planet Survey. NASA Planetary Data System. MSX-A-SPIRIT3-5-SBN0003-MIMPS-V1.0.

Mass estimates

DesignationMass / Err (kg)ΔM/MMethodYearRefNχ2Use
(416) Vaticana3.27e+18 ± 3.10e+1895 %Ephem 2010M9320.50 1
(416) Vaticana8.32e+17 ± 3.97e+1748 %Ephem 2019M1260.41 2

plot, average mass and derived density

All

Notes (N):
1: This estimate is discarded for the average mass (and derived density) calculation in Carry (2012).
2: This estimate is discarded for the average mass (and derived density) calculation in SiMDA (catalog).
3: This estimate is an average of individual solutions listed before under the same reference (e.g. M125).

Ephem : Planetary ephemeris solution.


EVM mass average M = (1.088 ± 0.747) × 1018 kg   (ΔM/M = 69%, SNR = 1.5) Derived bulk density ρ = (3.26 ± 2.27) g/cm3   (Δρ/ρ = 70%, SNR = 1.4)


References
M93(2010):Fienga, A., Manche, H., Kuchynka, P., Laskar, J., Gastineau, M., 2010. INPOP10a. Scientific Notes.
M126(2019):Fienga, A., et. al, 2019. INPOP19a planetary ephemeris. Notes Scientifiques et Techniques de l'Institut de mécanique céleste,