Summary for : (48) Doris

DynT.TT.BT T.L B T.DDensity (g/cm^3)Δρ/ρDiameter (km)ΔD/DMass (kg)ΔM/MRefAvg.M
MBACGCh- | -Ch1.43 ± 0.73   (D)51 %217.1 ± 11.75.4 %7.69e+18 ± 3.70e+1848 %SEVM
MBACGCh- | -Ch1.59 ± 2.20   (E)138 %210.2 ± 9.44.5 %7.74e+18 ± 1.06e+19137 %Sw.avg
MBACh1.23 ± 0.62   (D)50 %211.7 ± 10.95.1 %6.12e+18 ± 2.96e+1848 %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)

Object is a Gaia target for mass determination !

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
(48) Doris221.80 ± 7.503.4 % STM2004D93 0.39 1
(48) Doris211.30 ± 16.017.6 % STM2010D64 0.13 2
(48) Doris238.79 ± 9.213.9 % NEATM2010D64 5.53 3
(48) Doris200.27 ± 2.751.4 % STM2011D832 37.55 4
(48) Doris223.42 ± 4.171.9 % NEATM2011D72 2.28 5

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 = (217.1 ± 11.73) km   (ΔD/D = 5%, SNR = 18.50) Derived bulk density ρ = (1.43 ± 0.73) g/cm3   (Δρ/ρ = 51%, SNR = 2.0)


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.
D72(2011):Masiero, J.R., Mainzer, A.K., Grav, T., Bauer, J.M., Cutri, R.M., Dailey, J., Eisenhardt, P.R.M., McMillan, R.S., Spahr, T.B., Skrutskie, M.F., Tholen, D., Walker, R.G., Wright, E.L., DeBaun, E., Elsbury, D., Gautier, IV, T., Gomillion, S., Wilkins, A., 2011. Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters. Astrophysical Journal 741, 68.
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.

Mass estimates

DesignationMass / Err (kg)ΔM/MMethodYearRefNχ2Use
(48) Doris1.21e+19 ± 5.97e+1849 %Deflec 2004M420.55 1
(48) Doris4.00e+19 ± 2.98e+1974 %Ephem 2010M93121.18 2
(48) Doris5.89e+18 ± 4.84e+1882 %Deflec 2011M970.14 3
(48) Doris3.78e+18 ± 3.74e+1899 %Deflec 2011M971.09 4
(48) Doris3.84e+18 ± 3.69e+1896 %Deflec 2011M971.09 5
(48) Doris7.94e+18 ± 6.39e+1880 %Deflec 2011M970.00 6
(48) Doris2.40e+19 ± 6.83e+1828 %Ephem 2011M100125.70 7
(48) Doris7.76e+18 ± 5.97e+178 %OrbFitN 2014M1230.01 8
(48) Doris8.86e+18 ± 3.44e+1839 %Ephem 2019M1260.12 9

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).

Deflec : Orbital deflection (close encounter) of one or several test asteroids (classical LSQ). Ephem : Planetary ephemeris solution. OrbFitN : Simultaneous multi-asteroid astrometric orbit solution (similar to 'Ephem').


EVM mass average M = (7.688 ± 3.705) × 1018 kg   (ΔM/M = 48%, SNR = 2.1) Derived bulk density ρ = (1.43 ± 0.73) g/cm3   (Δρ/ρ = 51%, SNR = 2.0)


References
M42(2004):Kochetova, O.M., 2004. Determination of Large Asteroid Masses by the Dynamical Method. Solar System Research 38, 66–75.
M93(2010):Fienga, A., Manche, H., Kuchynka, P., Laskar, J., Gastineau, M., 2010. INPOP10a. Scientific Notes.
M97(2011):Zielenbach, W., 2011. Mass Determination Studies of 104 Large Asteroids. Astronomical Journal 142, 120–128.
M100(2011):Fienga, A., Kuchynka, P., Laskar, J., Manche, H., Gastineau, M., 2011. Asteroid mass determinations with INPOP planetary ephemerides. EPSC-DPS Joint Meeting 2011 , 1879.
M123(2014):Goffin, E., 2014. Astrometric asteroid masses: a simultaneous determination. Astronomy & Astrophysics, Volume 565, id.A56, 8 pp.
M126(2019):Fienga, A., et. al, 2019. INPOP19a planetary ephemeris. Notes Scientifiques et Techniques de l'Institut de mécanique céleste,